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<v Speaker 4>Hey, welcome to Ologies. I'm your Alie Warren the host.

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<v Speaker 4>Now each week I sit down with an ologist, I

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<v Speaker 4>ask why do they love what they do? What is

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<v Speaker 4>your deal? What should we know about it? And this

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<v Speaker 4>week we cover the whole fucking universe which has existed

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<v Speaker 4>and it's expanding in your floating in it, and you're

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<v Speaker 4>made out of particles and matter and forces we don't

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<v Speaker 4>even understand, and maybe there are multiverses and is this reality?

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<v Speaker 4>And what are you doing here and does anything matter?

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<v Speaker 4>And of course it does. But should you be afraid

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<v Speaker 4>of wearing bright lipstick or dancing in public? Probably not. No,

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<v Speaker 4>in the scope of things, and the scope of things

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<v Speaker 4>is really it's giant. It's called cosmology. Now, if you

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<v Speaker 4>think that you listen to this episode already because you

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<v Speaker 4>learn some stuff about beard care and face wash, think again, suckers.

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<v Speaker 4>That was cosmetology. This week is cosmology, the study of

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<v Speaker 4>the cosmos. And so when I say this episode is

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<v Speaker 4>like everything, it's actually everything. It's the whole universe. It's

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<v Speaker 4>a lot, it's a lot, it's so much. It's a

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<v Speaker 4>two parter, it's a two fur So this week we'll

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<v Speaker 4>get the nuts and bolts of what astrophysics is, and

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<v Speaker 4>after about an hour you will walk away cocktail party

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<v Speaker 4>literate on goddamn astrophysics. Kind of. I don't know. I'm

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<v Speaker 4>learning here with you. Of all the episodes I've done,

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<v Speaker 4>this was probably the one I need the least about.

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<v Speaker 4>So let's learn together, shall we? Part two of this

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<v Speaker 4>next week are your questions submitted via Patreon and the

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<v Speaker 4>Ologies Podcast Facebook group. Y'all had good ones. Next week

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<v Speaker 4>will address them. Now, the etymology of cosmology. Cosmos with

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<v Speaker 4>a K is the kicky little Greek word for world

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<v Speaker 4>or order. So cosmology is a study of planets and such, sure,

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<v Speaker 4>but also why and what and how where? What's huh?

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<v Speaker 4>It's the study of what. This week's cosmologist is someone

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<v Speaker 4>I've had a fawning Twitter fascination with for a while,

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<v Speaker 4>and I met through a group of science friends I love,

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<v Speaker 4>known to some as the nerd Brigade or kind of

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<v Speaker 4>like a gang but with a website. But I was

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<v Speaker 4>always kind of intimidated by her because she is, in

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<v Speaker 4>her own words, an academic nomad, and she continent hops

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<v Speaker 4>while studying particle physics and black holes and gravitational waves,

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<v Speaker 4>and she hangs out with Stephen Hawking. So when I

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<v Speaker 4>met her through friends, I usually just sat at brunch

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<v Speaker 4>like a barnacle and tried to look away when she

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<v Speaker 4>caught me staring at her, So I asked her to

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<v Speaker 4>be on the podcast. She said yes, and I immediately

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<v Speaker 4>started perspiring. So she came to my apartment. We sat down,

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<v Speaker 4>and my usual hour interview stretched to almost two, hence

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<v Speaker 4>the two parter. Hours before she politely reminded me that

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<v Speaker 4>we were supposed to be meeting people for a movie

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<v Speaker 4>and we should stop. I'm so so glad we did

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<v Speaker 4>this podcast because I got to know her even better

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<v Speaker 4>as a friend, which, y'all, I'm going to be cheesy

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<v Speaker 4>and say it's a true honor. So in this episode,

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<v Speaker 4>you'll learn about the things that make you you and

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<v Speaker 4>the stars that exploded to make the things that make

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<v Speaker 4>you you, and the scale of our existence in space,

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<v Speaker 4>and what it feels like to be heckled by Stephen

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<v Speaker 4>Hawking and if this is real life, and if astrophysicists

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<v Speaker 4>are just like making bullshit up that the rest of

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<v Speaker 4>us just accept because we're like, man, I don't even

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<v Speaker 4>know how to read these equations. So okay. So you'll

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<v Speaker 4>get at the very least a loose grasp on just

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<v Speaker 4>the whole of existence and maybe steel yourself to be

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<v Speaker 4>the biggest you you ought to be, and more importantly,

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<v Speaker 4>get to know better one of the world's finest voices

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<v Speaker 4>in cosmology. You know her as astro Katie on Twitter

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<v Speaker 4>aka astrophysicist Katie mac. So take me back to defining

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<v Speaker 4>some stuff because as a layman, as a lay woman

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<v Speaker 4>over here, a lay human, yes, I don't know that

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<v Speaker 4>difference between a physicist, an astrophysicist, a particle physicist, an experimentalist,

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<v Speaker 4>a cosmologist, and an astronomer. I don't know what those are,

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<v Speaker 4>and I'm either going to have to Wikipedia this or

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<v Speaker 4>I can have you give me a rundown.

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<v Speaker 5>So these things are, they're a little bit like fluid,

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<v Speaker 5>these definitions. So astronomer is basically somebody who studies space

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<v Speaker 5>in some way. And usually when people say astronomer versus astrophysicists,

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<v Speaker 5>usually astronomer is like more on the observational side or

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<v Speaker 5>sort of describing stuff in space. Astrophysicist is more about

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<v Speaker 5>like trying to understand how the physics of the thing

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<v Speaker 5>in space works. So you can be an astrophysicist trying

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<v Speaker 5>to understand how galaxies form, for example, and so you're

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<v Speaker 5>applying physics to this stuff in space. If you're a

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<v Speaker 5>particle physicist, you're working on like how particle interactions work,

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<v Speaker 5>so like you know atoms, fasters and things. Large Hadron

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<v Speaker 5>collider exposon usually I mean the like classic particle experiment,

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<v Speaker 5>does you take two particles and you smash them together

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<v Speaker 5>and you see what comes out. Huh, that's what the

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<v Speaker 5>Large Hadron Collider is doing now.

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<v Speaker 4>The LHC. That's what you call the Large Hadron Collider

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<v Speaker 4>when y'all are tight, So you've maybe heard of it,

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<v Speaker 4>you kind of know, like it's a thing in Europe,

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<v Speaker 4>maybe has something to do with atoms. I looked into it.

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<v Speaker 4>The Large Hadron Collider is located near the France Switzerland border,

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<v Speaker 4>and it's a circular tunnel. It's over five hundred feet

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<v Speaker 4>deep in some parts, and it's seventeen miles around. It

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<v Speaker 4>is the largest machine in the world. So this thing

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<v Speaker 4>consists of over twelve hundred magnets and they're cooled to

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<v Speaker 4>a temperature colder than outer space, and then the magnets

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<v Speaker 4>accelerate protons to almost the speed of light, and then

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<v Speaker 4>the protons are bashed together. It's very punk rock, very expense.

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<v Speaker 4>The LHC was mostly completed in two thousand and eight.

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<v Speaker 4>Over ten thousand scientists and engineers worked on it. Now

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<v Speaker 4>in photos it looks kind of like a giant, well

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<v Speaker 4>lit subway tunnel, but with less p and rats. If

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<v Speaker 4>you're like, I can't remember what a proton is because

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<v Speaker 4>I'm not required to anymore. I'm not in school, don't worry.

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<v Speaker 4>Neither did I I had to google, like, how does

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<v Speaker 4>an atom work? I forgot, so I'll brush you up.

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<v Speaker 4>So matter is stuff, and molecules are some atoms stuck together.

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<v Speaker 4>Atoms are made of a nucleus, which is a little

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<v Speaker 4>cluster of neutrons and protons. Protons have a positive charge,

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<v Speaker 4>pro electrons have an equal negative charge, and electrons are

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<v Speaker 4>bebopping zooming around whirling dervish style outside of the nucleus.

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<v Speaker 4>So the neutrons and protons, which are the ones that

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<v Speaker 4>are just cuddling in the nucleus, those are made of

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<v Speaker 4>smaller powder called quarks. And the quarks come in a

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<v Speaker 4>couple different varieties. So what gives these particles their mass?

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<v Speaker 4>What are they? Where do they come from? We've got

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<v Speaker 4>all these little tiny things that make up matter. Okay,

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<v Speaker 4>So I heard it explained that there's a field called

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<v Speaker 4>the Higgs field. It's named after one alive and well

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<v Speaker 4>Scotsman physicist named Peter Higgs. And how a particle interacts

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<v Speaker 4>with the Higgs field gives it its mass, kind of

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<v Speaker 4>like drag and water. So Higgs bosons are particles. They're

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<v Speaker 4>an excitation of the Higgs field. It's kind of like

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<v Speaker 4>a drop of water. Splashing from an ocean. So the

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<v Speaker 4>Large Hadron Collider smashed protons together to see if they

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<v Speaker 4>could prove that the Higgs boson exists, and guess what,

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<v Speaker 4>bitches it does. You're not bitches. Some people call this

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<v Speaker 4>the god particle because it's so fundamental to all matter

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<v Speaker 4>in the universe. Does Doctor Higgs like this name? No,

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<v Speaker 4>he's an atheist. He thinks it sucks. And the guy

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<v Speaker 4>who coined did the God particle actually wanted to call

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<v Speaker 4>it the goddamn particle, but his publisher made him change

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<v Speaker 4>it in a book. So the Large Hadron Collider. One

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<v Speaker 4>of the things it does smashes these protons together into

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<v Speaker 4>smaller things to figure out why matter has mass. There

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<v Speaker 4>you go. Also, the Large Hadron Collider accidentally has its

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<v Speaker 4>name spelled wrong on its own website as Large hard

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<v Speaker 4>On Collider once would be mortifying. But what if they

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<v Speaker 4>did it more than once, like twice or five times?

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<v Speaker 4>That's impossible, is it? Because a search on their site

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<v Speaker 4>revealed they'd spelled it large hard On Collider one hundred

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<v Speaker 4>and sixty five times. Thank God particle for that. That's

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<v Speaker 4>just precious. So whenever you're like, I don't understand this stuff.

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<v Speaker 4>Maybe I'm not smart enough. Just think someone typed in

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<v Speaker 4>large hard on collider over one hundred and fifty times

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<v Speaker 4>and they built the thing. So how else do people

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<v Speaker 4>figure this shit out? About very important things that we

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<v Speaker 4>can't see.

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<v Speaker 5>But there are other ways to do particle physics measuring

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<v Speaker 5>how particles interact with each other, throwing particles at other things,

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<v Speaker 5>accelerating stuff, and seeing what happens, all of that kind

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<v Speaker 5>of stuff. On the experimental side and on the theory side,

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<v Speaker 5>it's a lot about trying to understand like the fundamental

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<v Speaker 5>forces of nature, so like how how atoms hold together,

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<v Speaker 5>how you know particles can change into other particles in

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<v Speaker 5>certain conditions, how gravity fits into all that, which it

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<v Speaker 5>doesn't at the moment theoretically, Okay, okay, it's very hard

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<v Speaker 5>to get gravity and particle physics to work together. This

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<v Speaker 5>is kind of yeah, it's it's sort of This may

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<v Speaker 5>be another topic, but like, this is the reason string

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<v Speaker 5>theory was invented.

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<v Speaker 4>Real quick, What is string theory? Well, in a very

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<v Speaker 4>quark sized, tiny nutshell, the premise of strength theory is

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<v Speaker 4>that basic objects are not point like, but they're string like.

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<v Speaker 4>So a quark might be made of a loop that

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<v Speaker 4>kind of vibrates and moves around. Every kind of particle

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<v Speaker 4>is like a different wiggly string. So why does anyone care?

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<v Speaker 4>Why are people so horny for string theory? Well, number one,

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<v Speaker 4>it's from the eighties, and maybe this is like the

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<v Speaker 4>scrunchy of particle physics. I don't know. More importantly, string

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<v Speaker 4>theory is a theory that works with both Einstein's general

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<v Speaker 4>relativity and that mister Einstein pose that what we perceive

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<v Speaker 4>as the force of gravity is the curvature of space

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<v Speaker 4>and time. More on that in a minute, and quantum mechanics,

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<v Speaker 4>which is the physics of the tiniest building blocks that exist.

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<v Speaker 4>So remember those quirks that made up protons and neutrons?

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<v Speaker 4>What are those made of? Maybe these stringlike loops of matter.

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<v Speaker 4>Every time I hear string theory mentioned, I think of

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<v Speaker 4>string cheese. I cannot And I was writing and researching

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<v Speaker 4>this episode, and I found myself on a website like

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<v Speaker 4>two thirty in the morning learning that string cheese, as

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<v Speaker 4>we know what, was invented in Wisconsin in nineteen seventy six,

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<v Speaker 4>and the way they get it to string is to

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<v Speaker 4>heat it to one hundred and forty degrees fahrenheit, and

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<v Speaker 4>that aligns all the milk proteins. Also, the first iterations

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<v Speaker 4>of string cheese were bigger and chunkier and served to

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<v Speaker 4>drunks in bars. Should we get back to physics, Okay, I'm.

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<v Speaker 5>Sorry, And this is like the big question in physics

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<v Speaker 5>is that, like, so, there there are a few sort

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<v Speaker 5>of fundamental forces of nature. Right, there's electromagnetism, and that's

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<v Speaker 5>like light and you know, like static cling and all

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<v Speaker 5>of those kinds of things, right, and magnetism. And then

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<v Speaker 5>there's the weak nuclear force, which has to do with

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<v Speaker 5>like how particles decay in radioactivity that kind of thing,

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<v Speaker 5>and how particles can change into other particles under certain conditions.

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<v Speaker 5>There's the strong nuclear force, and that holds particles together

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<v Speaker 5>in the centers of at Okay, and those all kind

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<v Speaker 5>of make sense together theoretically, like you can write down

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<v Speaker 5>equations that make those all fit in some way more

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<v Speaker 5>or less.

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<v Speaker 4>When Katie says you can write down equations that make

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<v Speaker 4>those all fit, I appreciate her being inclusive with the

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<v Speaker 4>second person, But I cannot write down equations to make

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<v Speaker 4>those all fit in some way. I cannot do that.

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<v Speaker 5>But then there's gravity, and gravity just doesn't follow any

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<v Speaker 5>of the same rules. It's like it's very hard to

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<v Speaker 5>put together a theory that includes those the fundamental forces

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<v Speaker 5>of particle physics and gravity.

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<v Speaker 4>So so it's gravity like the bad boy in a

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<v Speaker 4>teen drama. It's just like it's just not following any rules.

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<v Speaker 5>It's weird. It's like like gravity is all about space time,

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<v Speaker 5>you know, so gravity like, So the theory of gravity

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<v Speaker 5>that we have is Einstein's theory of relativity, so general relativity.

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<v Speaker 5>This is the theory of gravity.

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<v Speaker 4>Where okay, yeah, heres Einstein. Here's how the universe of

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<v Speaker 4>which you are a part works.

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<v Speaker 5>The basic picture is that you can think of space

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<v Speaker 5>as this malleable thing, and if you have something that

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<v Speaker 5>has mass, it creates like a dent in space. It

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<v Speaker 5>sort of bends space around it, okay, and so other

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<v Speaker 5>things moving past will respond to that and like fall

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<v Speaker 5>into that dent. And that's like how gravitational attraction works.

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<v Speaker 5>You can think of it in this geometric way, okay,

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<v Speaker 5>and it works really well like geometrically to think of

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<v Speaker 5>it like that. But then there are fundamental principles that

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<v Speaker 5>happen in that like the speed of light, as a

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<v Speaker 5>limiting factor and all sorts of things like that, so

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<v Speaker 5>only certain paths things can follow and everything. But then

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<v Speaker 5>the particle physics stuff, like all the equations of particle

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<v Speaker 5>physics are done without thinking about gravity because on those scales,

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<v Speaker 5>like gravity isn't important. It's a really really weak force, okay.

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<v Speaker 5>But also like there are the way that the particle

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<v Speaker 5>physics is is formulated in the standard model of particle physics,

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<v Speaker 5>which is what we use to talk about all these interactions.

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<v Speaker 5>It doesn't have the same like, it doesn't follow the

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<v Speaker 5>same rules as gravity, Like there are ways in which

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<v Speaker 5>the whole like speed of light thing is violated in

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<v Speaker 5>one way that you can formulate how particles move around,

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<v Speaker 5>which is kind of like there's kind of like there's

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<v Speaker 5>this way of formulating it where a particle going from

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<v Speaker 5>point A to point B passes through every possible path

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<v Speaker 5>on the way between point A and point B, and

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<v Speaker 5>it's only by by using that idea that you get

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<v Speaker 5>the right answer for how that particle is moving in

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<v Speaker 5>the particle physics point of view, And that doesn't work

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<v Speaker 5>with relativity. So there are a couple of things like that,

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<v Speaker 5>where like quantum mechanics and relativity just do not like

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<v Speaker 5>each other really, And it gets especially problematic when you

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<v Speaker 5>get to black hole because a black hole is this

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<v Speaker 5>very like intense gravitational system mm hmm. It's basically a

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<v Speaker 5>dent in space time that's so deep that like everything

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<v Speaker 5>falls into it if it gets close enough. But at

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<v Speaker 5>the edge of a black hole, the event horizon, you

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<v Speaker 5>have this weird quantum mechanical thing happening where you can

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<v Speaker 5>have like particles evaporating off of it, and that sets

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<v Speaker 5>like a sort of scale of the black hole, and

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<v Speaker 5>that means there's quantum mechanics happening in a strong gravitational system,

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<v Speaker 5>and then just everything breaks. It just goes totally haywire,

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<v Speaker 5>because if you look at it from a gravitational point

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<v Speaker 5>of view, like a relativity point of view, you should

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<v Speaker 5>see nothing at all interesting happening when you when you

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<v Speaker 5>fall into the black hole, like aside from like you're

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<v Speaker 5>you're killed by the gravity, right, Like you don't see

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<v Speaker 5>like nothing weird happens when you pass the horizon. But

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<v Speaker 5>from a particle physics point of view, like there there

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<v Speaker 5>might be like this like firewall, like there might be

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<v Speaker 5>like a sort of like boundary of intense radiation there

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<v Speaker 5>because of the way you have to think about how

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<v Speaker 5>the particle physics works. This is a complicated story, but.

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<v Speaker 6>Basically the astrophysics typically is yeah, I'm not explaining it

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<v Speaker 6>very well, but but basically, like like, basically, when you

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<v Speaker 6>get to that point when you have a black hole

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<v Speaker 6>has an evaporation happening where particles are coming off the

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<v Speaker 6>edge of the event horizon, one way of looking at

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<v Speaker 6>it says that that that means that whatever you.

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<v Speaker 5>Fought through into the black hole, you can't ever find

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<v Speaker 5>out what it was. That information is destroid. But quantum mechanics,

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<v Speaker 5>like the particle point of view, says you can't do that,

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<v Speaker 5>and so there has to be some kind of loophole

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<v Speaker 5>and then gravity doesn't like that and you just you

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<v Speaker 5>just end up with chaos. And so there's this there's

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<v Speaker 5>this big problem called the black hole information paradox, which

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<v Speaker 5>has been around forever, and every once in a while

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<v Speaker 5>somebody's like, oh, I solved it, and then it's really

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<v Speaker 5>complicated and people don't really understand how that works.

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<v Speaker 4>Has anyone actually solved that?

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<v Speaker 5>I mean, I so technically I'm just not qualified to

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<v Speaker 5>know that for sure, because it requires understanding quantum gravity

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<v Speaker 5>in a way that I do not. But there have

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<v Speaker 5>been some solutions suggested, but in general there's still a

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<v Speaker 5>lot of discussion, so I don't know.

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<v Speaker 4>Okay, wait, so what does a cosmologist do.

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<v Speaker 5>A cosmologist just means you study the universe as a whole, right,

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<v Speaker 5>so you study maybe the beginning of the universe, the

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<v Speaker 5>end of the universe, how it changes over time. But

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<v Speaker 5>you can be a physicist cosmologist or an astronomer cosmologist,

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<v Speaker 5>and those are different, and it's culturally different. Like, but

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<v Speaker 5>the so if you're a physicist, if you hang out

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<v Speaker 5>with particle physics people and you say you're a cosmologist,

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<v Speaker 5>then then the implication is that you work on like

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<v Speaker 5>the beginning of the universe and the forces of nature

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<v Speaker 5>and maybe the end of the universe something like that.

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<v Speaker 5>If you hang out with astrophysicists and you say you're

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<v Speaker 5>a cosmologist, then you just study things that are really

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<v Speaker 5>far away, or you study you know, some something you

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<v Speaker 5>know more fundamental. But like, you can be a cosmologist

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<v Speaker 5>in astrophysics and you're a cosmologist because you study very

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<v Speaker 5>very distant galaxies. The reason that counts as cosmology is

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<v Speaker 5>because that means you're studying the very distant past of

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<v Speaker 5>the universe.

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<v Speaker 4>So there are different flavors of cosmology, but they're all

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<v Speaker 4>kind of linked, at least in my opinion, by like, oh,

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<v Speaker 4>where are we? What are we? What are we made of? AKA,

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<v Speaker 4>it's a branch of astronomy that involves the origin and

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<v Speaker 4>evolution of the universe. That's a less panicky way to

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<v Speaker 4>put it.

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<v Speaker 5>And so so then you're studying like how the universe

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<v Speaker 5>has changed over time. So there are kind of different

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<v Speaker 5>ways of doing it. And I've done all of those

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<v Speaker 5>different kinds of cosmology, I guess because I've spent my

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<v Speaker 5>time kind of bouncing back and forth between the particle

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<v Speaker 5>physics and the astrophysics communities. So I've worked on you know,

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<v Speaker 5>the Big Bang and like theories of the early universe,

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<v Speaker 5>and I've worked on distant galaxies and how galaxies form.

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<v Speaker 5>And I've worked on black holes and weird stuff like

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<v Speaker 5>cosmic strings and just all sorts of things.

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<v Speaker 4>What is a cosmic string?

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<v Speaker 5>A cosmic string is kind of like a sort of

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<v Speaker 5>line or wiggly line of energy that stretches across the cosmos.

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<v Speaker 5>Might not exist, probably doesn't exist, but there could be

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<v Speaker 5>this like whole network of strings. Of like it's kind

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<v Speaker 5>of like if you think of like a black hole,

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<v Speaker 5>but you like stretch it out across the whole universe.

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<v Speaker 5>You get it's kind of like that, what does it do?

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<v Speaker 7>What?

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<v Speaker 4>It?

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<v Speaker 5>So really interesting things. So if you have two cosmic

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<v Speaker 5>strings and they cross each other they collide, they can

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<v Speaker 5>like reconnect in a different way. So you can have

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<v Speaker 5>two cosmic strings that are about to collide and then

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<v Speaker 5>they like change so that now you have two sort

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<v Speaker 5>of loops of cosmic strings. They're going into deficite directions,

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<v Speaker 5>like so they sort of passed through each other by

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<v Speaker 5>branching off in this weird way.

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<v Speaker 4>So cosmic strings may or may not exist. Now, if

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<v Speaker 4>they do exist, some theorists have used them to maybe

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<v Speaker 4>sketch out some stuff about time travel. Please figure that out,

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<v Speaker 4>please fix some stuff, thank you.

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<v Speaker 5>And you can make a loop of cosmic string, and

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<v Speaker 5>then that loop of cosmic string will like wiggle around

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<v Speaker 5>and make gravitational radiation and disappear into nothingness. And if

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<v Speaker 5>you have a cosmic string, like if you have a

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<v Speaker 5>cosmic string between you and some distant galaxy, then you

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<v Speaker 5>might see two pictures of that galaxy because it like

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<v Speaker 5>splits the space kind of. It's really cool.

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<v Speaker 4>Now, how much do you think about all of this

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<v Speaker 4>in your day to day life? And like when you're

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<v Speaker 4>deciding if you should upgrade your rental car and like

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<v Speaker 4>if you should cut bangs and what happens to your

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<v Speaker 4>molecules after you die? Like how much do you let

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<v Speaker 4>this kind of get to your own existence? Ah?

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<v Speaker 5>Yeah, somebody asked me that the other day, Like how

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<v Speaker 5>much do I like get sort of just overwhelmed by

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<v Speaker 5>these ideas or whatever? It's not very often, Like most

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<v Speaker 5>of the time this is like this is fun stuff

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<v Speaker 5>to work on, but like most of this time it

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<v Speaker 5>feels more like some kind of combination of science fiction

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<v Speaker 5>and a fun puzzle, you know. So like I'm trying

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<v Speaker 5>to solve a problem. I'm trying to calculate something and

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<v Speaker 5>trying to come up with a new idea for how

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<v Speaker 5>to do something, and so it's like a puzzle. It's

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<v Speaker 5>like some kind of neat thing to work out, And

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<v Speaker 5>I don't think of it as connecting to my own

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<v Speaker 5>life or existence because it's way far away or way

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<v Speaker 5>in the past, or you know, probably doesn't exist. Or whatever. Right,

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<v Speaker 5>But then every once in a while, like I'll be

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<v Speaker 5>I'll be thinking about this stuff and I'll be like,

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<v Speaker 5>oh my God, like there's this stuff is out there.

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<v Speaker 5>Like I'll be thinking about black holes or gravitational waves

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<v Speaker 5>or like the inflation period in the early universe or

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<v Speaker 5>something like that, and I'll be like I'll have to

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<v Speaker 5>like hold on to something and be like, oh God,

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<v Speaker 5>because these are huge, like mind bendingly intense forces and

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<v Speaker 5>massive things and like the kinds of energies and the

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<v Speaker 5>kinds of like force and just I don't know the

401
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<v Speaker 5>explosions and everything. It's just we cannot comprehend this stuff.

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<v Speaker 5>I mean, the Earth is really tiny and really unimportant,

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<v Speaker 5>like in a big way. So, okay, you know there's

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<v Speaker 5>this there's this famous photograph, the Pale Blue Dot. Yes,

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<v Speaker 5>huh yeah, So this is a picture that was taken

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<v Speaker 5>by the Voyager spacecraft.

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<v Speaker 4>So the Pale Blue Dot photo was taken on Valentine's

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<v Speaker 4>Day in nineteen ninety as Voyager one was leaving the

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<v Speaker 4>Solar System. It was like by by I'm out, and

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<v Speaker 4>astronomer Carl Sagan said, Oh, let's turn that lens around.

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<v Speaker 4>Let's take a pick of all of us far away.

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<v Speaker 4>What do you say, might as well? And it was

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<v Speaker 4>three point seven billion miles away. It's little galaxy's longest range.

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<v Speaker 4>Selfie this photo itself. It looks like you accidentally took

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<v Speaker 4>like a blurry image of a few Christmas lights and

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<v Speaker 4>there was like a speck of dust on your lens.

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<v Speaker 4>Those lights are just a few scattered rays of sun.

418
00:24:25.559 --> 00:24:28.200
<v Speaker 4>And someone would have to point out that that dust

419
00:24:28.720 --> 00:24:32.960
<v Speaker 4>is our planet is such a tiny speck. And I'll

420
00:24:33.039 --> 00:24:36.759
<v Speaker 4>let Carl Sagan put this in context. He's the pro here,

421
00:24:37.720 --> 00:24:38.559
<v Speaker 4>that's here.

422
00:24:39.240 --> 00:24:42.799
<v Speaker 7>That's home, that's us on it.

423
00:24:43.680 --> 00:24:48.559
<v Speaker 8>Everyone you love, everyone you know, everyone you ever heard of,

424
00:24:49.000 --> 00:24:54.440
<v Speaker 8>Every human being whoever was, lived out their lives the

425
00:24:54.599 --> 00:25:00.880
<v Speaker 8>argregate our joy and suffering, thousands of confident religion, ideologies

426
00:25:00.880 --> 00:25:06.720
<v Speaker 8>and economic doctrines. Every hunter and forager, every hero and coward,

427
00:25:06.799 --> 00:25:08.240
<v Speaker 8>every creator.

428
00:25:07.759 --> 00:25:13.039
<v Speaker 2>And destroyer of civilization, every king and peasant, every young

429
00:25:13.119 --> 00:25:18.319
<v Speaker 2>couple in love, every mother and father, hopeful child, inventor

430
00:25:18.440 --> 00:25:25.200
<v Speaker 2>and explorer, every teacher of morals, every corrupt politician, every superstar,

431
00:25:25.680 --> 00:25:30.319
<v Speaker 2>every supreme leader, every saint and sinner in the history

432
00:25:30.319 --> 00:25:30.680
<v Speaker 2>of our.

433
00:25:30.599 --> 00:25:38.519
<v Speaker 7>Species lived there on a motive. Dust suspended in a sunbeam.

434
00:25:38.799 --> 00:25:43.720
<v Speaker 7>The Earth is a very small stage in a vast

435
00:25:44.440 --> 00:25:45.880
<v Speaker 7>cosmic arena.

436
00:25:46.680 --> 00:25:49.319
<v Speaker 5>Sometimes when I give talks about cosmology, I'll end with

437
00:25:49.400 --> 00:25:52.240
<v Speaker 5>this picture, and I'll be like, you know, she's thinking

438
00:25:52.240 --> 00:25:56.640
<v Speaker 5>about how vast the universe is and how really insignificant

439
00:25:56.680 --> 00:26:01.079
<v Speaker 5>we are. And the insignificant is even deeper than just

440
00:26:01.160 --> 00:26:03.000
<v Speaker 5>what you see from that picture, because in that picture

441
00:26:03.039 --> 00:26:04.839
<v Speaker 5>you see like there's a whole lot empty space and

442
00:26:04.880 --> 00:26:07.359
<v Speaker 5>then there's a little tiny rock. Yeah, and we're on

443
00:26:07.400 --> 00:26:10.039
<v Speaker 5>that little tiny rock, right, oh, and there's a lot

444
00:26:10.039 --> 00:26:14.720
<v Speaker 5>of space. But it's even worse than that because because like,

445
00:26:14.960 --> 00:26:17.559
<v Speaker 5>not only are we not the center of like the

446
00:26:17.680 --> 00:26:20.279
<v Speaker 5>universe or a galaxy or a solicism or anything like that,

447
00:26:20.359 --> 00:26:24.319
<v Speaker 5>the matter that we're made of is also really unimportant

448
00:26:24.559 --> 00:26:28.240
<v Speaker 5>because because like like just the kind of stuff that

449
00:26:28.279 --> 00:26:30.400
<v Speaker 5>we are and that we can understand and interact with,

450
00:26:30.920 --> 00:26:34.440
<v Speaker 5>regular matter is like five percent of the universe. So

451
00:26:34.759 --> 00:26:38.279
<v Speaker 5>most of the universe is something called dark energy that

452
00:26:38.319 --> 00:26:41.240
<v Speaker 5>we really don't understand, but it's some sort of mysterious

453
00:26:41.240 --> 00:26:43.920
<v Speaker 5>stuff that's making the universe expand faster and faster and

454
00:26:43.920 --> 00:26:46.799
<v Speaker 5>it's going to take over eventually. And then there's dark matter,

455
00:26:46.839 --> 00:26:50.160
<v Speaker 5>which is some kind of invisible matter that is most

456
00:26:50.160 --> 00:26:52.079
<v Speaker 5>of what the galaxy is made of, and most of

457
00:26:52.119 --> 00:26:54.400
<v Speaker 5>what all galaxies are made of. So like our galaxy,

458
00:26:54.920 --> 00:26:56.559
<v Speaker 5>you know, we think of it as like this pretty

459
00:26:56.599 --> 00:26:59.880
<v Speaker 5>disc of stars, but it's actually embedded in this invisible

460
00:27:00.039 --> 00:27:03.119
<v Speaker 5>blob of extra stuff that we can't see. And that

461
00:27:03.119 --> 00:27:05.599
<v Speaker 5>blob is way bigger than the stuff that we can

462
00:27:05.640 --> 00:27:08.160
<v Speaker 5>actually see. So dark matter is like eighty five percent

463
00:27:08.160 --> 00:27:09.880
<v Speaker 5>of the matter in the universe or something like that,

464
00:27:09.960 --> 00:27:12.079
<v Speaker 5>Oh my god. And then dark energy is like seventy

465
00:27:12.119 --> 00:27:15.079
<v Speaker 5>percent of all of the stuff in the universe. Like

466
00:27:15.200 --> 00:27:19.200
<v Speaker 5>so so then we're this like tiny five percent slice

467
00:27:19.240 --> 00:27:22.559
<v Speaker 5>and that's just the kind of matter that we can understand,

468
00:27:22.680 --> 00:27:24.839
<v Speaker 5>that we can do experiments on, that we can see

469
00:27:24.920 --> 00:27:29.480
<v Speaker 5>or touch or interact with in any reasonable way. And

470
00:27:30.000 --> 00:27:34.759
<v Speaker 5>then it's like not only not only are we like

471
00:27:34.799 --> 00:27:37.160
<v Speaker 5>a tiny speck of dust on a tiny speck of dust,

472
00:27:37.240 --> 00:27:40.799
<v Speaker 5>like who's you know, Like we are so insignificant, Like

473
00:27:40.839 --> 00:27:44.000
<v Speaker 5>the universe doesn't even it doesn't even matter that we're

474
00:27:44.279 --> 00:27:46.680
<v Speaker 5>like that our kind of stuff is there.

475
00:27:46.519 --> 00:27:49.039
<v Speaker 4>You know, the best thing about this conversation is, yeah,

476
00:27:49.319 --> 00:27:52.720
<v Speaker 4>I'm having it with a cosmologist, and like an astrophysicist,

477
00:27:52.960 --> 00:27:55.119
<v Speaker 4>but I could also be having the same conversation with

478
00:27:55.240 --> 00:27:57.559
<v Speaker 4>any of my college roommates who had like a seven

479
00:27:57.599 --> 00:28:02.319
<v Speaker 4>foot bong in their garage. Astro Physicists and cosmologists get together, yeah,

480
00:28:02.640 --> 00:28:04.599
<v Speaker 4>is it just kind of like a round robin of

481
00:28:04.640 --> 00:28:08.200
<v Speaker 4>like stoner existentialism, Like because they feel like there's such

482
00:28:08.240 --> 00:28:13.599
<v Speaker 4>a fine line, like and then you're either incredibly incredibly

483
00:28:13.640 --> 00:28:16.440
<v Speaker 4>smart and thoughtful and knowledgeable about this stuff, or you're

484
00:28:16.519 --> 00:28:19.160
<v Speaker 4>just like you've just numbed yourself enough or you allow

485
00:28:19.200 --> 00:28:20.599
<v Speaker 4>yourself to think about it, and then and it's like

486
00:28:20.680 --> 00:28:23.200
<v Speaker 4>the Bell curve. There's this big white swath of people

487
00:28:23.200 --> 00:28:25.119
<v Speaker 4>who are like I can't even think about it. It's

488
00:28:25.160 --> 00:28:26.680
<v Speaker 4>too much, you know.

489
00:28:27.160 --> 00:28:30.720
<v Speaker 5>I mean, so when I do get together with other

490
00:28:30.720 --> 00:28:34.480
<v Speaker 5>cosmologists and we talk shop, it's usually very very technical,

491
00:28:35.039 --> 00:28:38.119
<v Speaker 5>and so we don't get into this stuff at all,

492
00:28:38.200 --> 00:28:41.000
<v Speaker 5>like we're it's it's usually you know, we're just talking

493
00:28:41.079 --> 00:28:44.279
<v Speaker 5>about we're talking in a lot of jargon about like

494
00:28:44.359 --> 00:28:47.079
<v Speaker 5>some measurement or something, and we're throwing out numbers and

495
00:28:47.119 --> 00:28:49.480
<v Speaker 5>we're trying to like figure out like is this a

496
00:28:49.519 --> 00:28:52.400
<v Speaker 5>reasonable measurement to make or whatever, Like what kind of

497
00:28:52.400 --> 00:28:55.839
<v Speaker 5>plot can we make to to, you know, to illustrate

498
00:28:55.880 --> 00:28:57.960
<v Speaker 5>this point, or what kind of calculation should we do,

499
00:28:58.319 --> 00:29:01.960
<v Speaker 5>or like what's the important variable? It would not be

500
00:29:02.000 --> 00:29:05.839
<v Speaker 5>interesting to somebody who is not in the field. So

501
00:29:05.880 --> 00:29:07.559
<v Speaker 5>it's really only when I'm talking about people who are

502
00:29:07.599 --> 00:29:12.559
<v Speaker 5>not in cosmology, where like I have these moments of like,

503
00:29:12.599 --> 00:29:16.079
<v Speaker 5>oh god, you know, but the thing I mean, but

504
00:29:16.119 --> 00:29:18.640
<v Speaker 5>it's it's a little bit dangerous to talk about this

505
00:29:18.640 --> 00:29:22.559
<v Speaker 5>stuff though, because then sometimes people get the idea that

506
00:29:22.599 --> 00:29:25.000
<v Speaker 5>we really are just kind of sitting around making stuff up,

507
00:29:25.039 --> 00:29:29.160
<v Speaker 5>you know, like and so then people think like, oh,

508
00:29:29.200 --> 00:29:31.640
<v Speaker 5>I can be a cosmologist, Like what if the universe

509
00:29:31.720 --> 00:29:32.640
<v Speaker 5>is shaped like a football?

510
00:29:32.759 --> 00:29:32.920
<v Speaker 3>You know?

511
00:29:33.200 --> 00:29:36.759
<v Speaker 5>And I think that that the sort of disconnect there

512
00:29:36.839 --> 00:29:40.440
<v Speaker 5>is that like the ideas themselves, if they're not backed

513
00:29:40.480 --> 00:29:43.480
<v Speaker 5>up by the data or by like a very rigorous model,

514
00:29:43.559 --> 00:29:48.599
<v Speaker 5>are really not that important. Like once we have data

515
00:29:48.680 --> 00:29:52.000
<v Speaker 5>and we have some kind of unifying theory that says

516
00:29:52.000 --> 00:29:54.440
<v Speaker 5>that this is probably the way things are, then it's

517
00:29:54.480 --> 00:29:59.960
<v Speaker 5>like super cool, right, But if somebody had said, like, oh,

518
00:30:00.039 --> 00:30:02.119
<v Speaker 5>you know, maybe the universe is like this, like we

519
00:30:02.160 --> 00:30:03.960
<v Speaker 5>don't really know what to do with that, and it does,

520
00:30:04.119 --> 00:30:06.000
<v Speaker 5>it's not really helpful and you.

521
00:30:05.960 --> 00:30:07.000
<v Speaker 4>Can just spitball.

522
00:30:07.680 --> 00:30:11.400
<v Speaker 5>Yeah, yeah, exactly, like like you have to. It has

523
00:30:11.440 --> 00:30:13.680
<v Speaker 5>to be connected to something we can test or or

524
00:30:14.559 --> 00:30:18.680
<v Speaker 5>write down mathematically or else. It just it's kind of

525
00:30:18.720 --> 00:30:21.160
<v Speaker 5>not helpful, which which is, you know, it's a bummer.

526
00:30:21.200 --> 00:30:24.079
<v Speaker 5>But but once you do have the sort of mathematical

527
00:30:24.119 --> 00:30:27.359
<v Speaker 5>tools and stuff and you can speak that language, you know,

528
00:30:28.319 --> 00:30:30.359
<v Speaker 5>then you can get really creative and then you can

529
00:30:30.839 --> 00:30:34.000
<v Speaker 5>just do really fun things. So like I have I

530
00:30:34.039 --> 00:30:36.359
<v Speaker 5>have a project I'm working on that has to do

531
00:30:36.440 --> 00:30:40.640
<v Speaker 5>with I have a few interesting projects actually, so I

532
00:30:40.640 --> 00:30:44.039
<v Speaker 5>have one. So here's one that it could be fun.

533
00:30:44.079 --> 00:30:47.400
<v Speaker 5>So it has to do with black holes and galaxies

534
00:30:47.440 --> 00:30:52.079
<v Speaker 5>and the bending of space. Okay, So so every time

535
00:30:52.119 --> 00:30:55.079
<v Speaker 5>there's a massive object, it bends space around it, and

536
00:30:55.119 --> 00:30:58.359
<v Speaker 5>so that means that light when it goes past bends

537
00:30:58.400 --> 00:31:01.359
<v Speaker 5>around so like a lens. Like the massive object acts

538
00:31:01.400 --> 00:31:03.720
<v Speaker 5>like a lens for light, and so light gets bent around.

539
00:31:04.079 --> 00:31:07.640
<v Speaker 5>So there's this way to study like what galaxies are

540
00:31:07.680 --> 00:31:11.759
<v Speaker 5>made of by having a very bright light behind the galaxy,

541
00:31:11.839 --> 00:31:14.960
<v Speaker 5>like really far away and looking at how that light

542
00:31:15.200 --> 00:31:18.920
<v Speaker 5>like bends around inside that galaxy and like how the

543
00:31:19.000 --> 00:31:22.319
<v Speaker 5>light fluctuates as things move and stuff like that, and

544
00:31:22.680 --> 00:31:25.640
<v Speaker 5>that's called gravitational micro lensing in this case the kind

545
00:31:25.680 --> 00:31:28.160
<v Speaker 5>of thing I'm working on, but the details aren't important,

546
00:31:28.200 --> 00:31:32.440
<v Speaker 5>but it's this thing where like the thing that's making

547
00:31:32.440 --> 00:31:35.359
<v Speaker 5>the bright light is also a black hole. Because it

548
00:31:35.359 --> 00:31:37.599
<v Speaker 5>turns out when you have a super massive black hole,

549
00:31:37.680 --> 00:31:41.079
<v Speaker 5>like billions of times as massive as the sun, those

550
00:31:41.119 --> 00:31:45.000
<v Speaker 5>things can be pulling matter into themselves and that matter

551
00:31:45.119 --> 00:31:49.359
<v Speaker 5>lights up like a whirlpool of stuff, and it can

552
00:31:49.400 --> 00:31:51.880
<v Speaker 5>make this incredibly bright light that you can see like

553
00:31:51.920 --> 00:31:56.559
<v Speaker 5>across the universe. And so we use that as like

554
00:31:56.599 --> 00:32:00.400
<v Speaker 5>a back light to study this stuff in a more

555
00:32:00.519 --> 00:32:03.640
<v Speaker 5>nearby galaxy to find out how many black holes there

556
00:32:03.640 --> 00:32:04.680
<v Speaker 5>are in that galaxy.

557
00:32:04.960 --> 00:32:07.960
<v Speaker 4>So black holes make lights sometimes, Yeah, it's supposed to

558
00:32:07.960 --> 00:32:08.599
<v Speaker 4>be confusing.

559
00:32:09.000 --> 00:32:11.079
<v Speaker 5>Yeah, it's like I think, I mean, I think it's

560
00:32:11.119 --> 00:32:13.279
<v Speaker 5>like it's one of these things that's like the biggest

561
00:32:13.279 --> 00:32:16.160
<v Speaker 5>misconception about black holes is that they're dark. Usually they're not,

562
00:32:16.440 --> 00:32:18.640
<v Speaker 5>like the ones we know about are usually not dark,

563
00:32:18.799 --> 00:32:21.720
<v Speaker 5>and it's it's yeah, it's because they're not. It's it's

564
00:32:21.759 --> 00:32:25.720
<v Speaker 5>because like technically the black hole itself can't be seen,

565
00:32:26.240 --> 00:32:29.519
<v Speaker 5>but it's doing so much that it like affects everything

566
00:32:29.559 --> 00:32:33.000
<v Speaker 5>around it, and so usually you can see black holes

567
00:32:33.039 --> 00:32:37.000
<v Speaker 5>because they're like really destructive and like the stuff is

568
00:32:37.039 --> 00:32:40.480
<v Speaker 5>falling into them, kind of like if you if you

569
00:32:40.599 --> 00:32:43.440
<v Speaker 5>had a drain at the bottom of a bathtub, uh huh,

570
00:32:44.400 --> 00:32:46.880
<v Speaker 5>Like you might not be able to see the drain

571
00:32:47.039 --> 00:32:49.319
<v Speaker 5>through like the you know, bubbles or something, but you

572
00:32:49.359 --> 00:32:52.599
<v Speaker 5>can see that there's like a whirlpool of stuff falling

573
00:32:52.680 --> 00:32:55.000
<v Speaker 5>in at that point, oh man. And that's how we

574
00:32:55.039 --> 00:32:59.160
<v Speaker 5>see black holes in space usually is we see that

575
00:32:59.200 --> 00:33:01.279
<v Speaker 5>they're they're pulling in a lot of matter and so

576
00:33:01.359 --> 00:33:04.200
<v Speaker 5>they like that matter lights up and so once it

577
00:33:04.240 --> 00:33:06.200
<v Speaker 5>goes into the black hole, we can't see it, but

578
00:33:06.400 --> 00:33:08.880
<v Speaker 5>it spends a lot of time whirling around really fast.

579
00:33:09.119 --> 00:33:11.880
<v Speaker 4>It's like an intergalactic garbage disposal.

580
00:33:12.160 --> 00:33:14.359
<v Speaker 5>Yeah, yeah, and it can be. It's some of the

581
00:33:14.359 --> 00:33:16.880
<v Speaker 5>brightest things in the universe are black holes. We call

582
00:33:16.920 --> 00:33:19.240
<v Speaker 5>them quasars when they're when they're the super massive ones

583
00:33:19.279 --> 00:33:24.160
<v Speaker 5>and they're pulling matter in like that and and we

584
00:33:24.279 --> 00:33:27.400
<v Speaker 5>have so so that's like those are for black holes

585
00:33:27.440 --> 00:33:29.680
<v Speaker 5>that are like millions or billions of times as massive

586
00:33:29.720 --> 00:33:30.240
<v Speaker 5>as the sun.

587
00:33:30.559 --> 00:33:32.240
<v Speaker 4>And how far away are those pep beats?

588
00:33:32.359 --> 00:33:37.359
<v Speaker 5>All right? Well, Okay, super massive black holes, the ones

589
00:33:37.359 --> 00:33:39.319
<v Speaker 5>I was just talking about millions or billions of times

590
00:33:39.319 --> 00:33:43.480
<v Speaker 5>the mass of the Sun. Those seem to exist at

591
00:33:43.480 --> 00:33:46.880
<v Speaker 5>the centers of pretty much every reasonably sized galaxy we

592
00:33:46.960 --> 00:33:48.640
<v Speaker 5>know about at the centers.

593
00:33:48.839 --> 00:33:50.759
<v Speaker 4>Yes, so including ours?

594
00:33:51.240 --> 00:33:54.920
<v Speaker 5>Yes, really, yes, so our galaxy.

595
00:33:55.000 --> 00:33:58.839
<v Speaker 4>Okay, quick note, let's do a few cosmological basics. Our

596
00:33:58.920 --> 00:34:02.359
<v Speaker 4>galaxy is Smoky Way, right, And this next analogy I

597
00:34:02.400 --> 00:34:05.759
<v Speaker 4>got right off of NASA's Night Sky website, which I

598
00:34:05.799 --> 00:34:08.800
<v Speaker 4>think is for children, but it's so helpful. So okay,

599
00:34:08.880 --> 00:34:13.599
<v Speaker 4>imagine our Sun. It's one star among hundreds of billions

600
00:34:13.639 --> 00:34:16.239
<v Speaker 4>of stars in our Milky Way. Right. So if we

601
00:34:16.320 --> 00:34:18.920
<v Speaker 4>shrink the Sun down to smaller than a grain of sand,

602
00:34:19.400 --> 00:34:24.840
<v Speaker 4>our little solar system Venus Mercury Earth, all of those

603
00:34:25.159 --> 00:34:27.679
<v Speaker 4>would be small enough to fit the whole solar system

604
00:34:27.679 --> 00:34:30.119
<v Speaker 4>in the palm of your hand. Now, on that scale,

605
00:34:30.159 --> 00:34:32.960
<v Speaker 4>with our solar system in your hand, the Milky Way

606
00:34:33.000 --> 00:34:36.519
<v Speaker 4>galaxy would be the size of North America. And the

607
00:34:36.559 --> 00:34:40.840
<v Speaker 4>Milky Way's big. But our next, our neighbor and Drameda galaxy,

608
00:34:41.000 --> 00:34:43.559
<v Speaker 4>it's about twice as big as the Milky Way. Scale

609
00:34:43.960 --> 00:34:46.519
<v Speaker 4>is important here, I suppose, But at the center of

610
00:34:46.559 --> 00:34:50.159
<v Speaker 4>our galaxy there's a black hole. So the Milky Way.

611
00:34:50.360 --> 00:34:52.559
<v Speaker 5>Is like a disc of stars and gas and dusts

612
00:34:52.559 --> 00:34:55.239
<v Speaker 5>and stuff, and we're sort of out toward an edge

613
00:34:55.800 --> 00:34:58.559
<v Speaker 5>and at the center there's a bulge of stars and

614
00:34:58.599 --> 00:35:00.719
<v Speaker 5>gas and nusts, and then in the middle of there's

615
00:35:00.760 --> 00:35:03.400
<v Speaker 5>a black hole. It's four million times as massive as

616
00:35:03.440 --> 00:35:03.760
<v Speaker 5>the Sun.

617
00:35:04.000 --> 00:35:04.840
<v Speaker 4>I didn't know that.

618
00:35:04.880 --> 00:35:07.039
<v Speaker 5>Do we have a name for it, Yeah, yeah, we

619
00:35:07.079 --> 00:35:10.079
<v Speaker 5>have a name for it. We call it Sagittarius a star, okay,

620
00:35:10.199 --> 00:35:13.159
<v Speaker 5>which is a silly name. It's because it's the kind

621
00:35:13.159 --> 00:35:16.480
<v Speaker 5>of I think it was like I think a radio source,

622
00:35:16.840 --> 00:35:20.440
<v Speaker 5>and because it was pulling in some matter and so

623
00:35:20.480 --> 00:35:22.079
<v Speaker 5>it was lighting up in the radio a little bit,

624
00:35:22.159 --> 00:35:24.360
<v Speaker 5>and so ours is not pulling in very much matter

625
00:35:24.400 --> 00:35:26.840
<v Speaker 5>at all, Like very occasionally it'll lead a little blobb

626
00:35:26.840 --> 00:35:30.159
<v Speaker 5>of gas and the astronomers get super excited, but like

627
00:35:30.199 --> 00:35:33.400
<v Speaker 5>there's very little happening with it, but it does. It

628
00:35:33.440 --> 00:35:37.840
<v Speaker 5>is really big, and it's got a bunch of stars

629
00:35:37.920 --> 00:35:40.519
<v Speaker 5>orbiting really closely around it, and so you can actually

630
00:35:40.519 --> 00:35:45.159
<v Speaker 5>go online and see like data follow like tracing out

631
00:35:45.280 --> 00:35:47.719
<v Speaker 5>the paths of some of these stars, and you can

632
00:35:47.760 --> 00:35:50.679
<v Speaker 5>see them like whip around as they go really close

633
00:35:50.719 --> 00:35:52.280
<v Speaker 5>to the black hole in their orbits. So some of

634
00:35:52.280 --> 00:35:54.159
<v Speaker 5>them have these orbits that they're really far away and

635
00:35:54.199 --> 00:35:56.079
<v Speaker 5>they come in really close and they go boom like

636
00:35:56.119 --> 00:35:58.480
<v Speaker 5>that right around the black hole. And so you can

637
00:35:58.519 --> 00:36:00.679
<v Speaker 5>figure out exactly like how big it is and where

638
00:36:00.719 --> 00:36:03.400
<v Speaker 5>it is by watching these stars go around it really quickly.

639
00:36:03.519 --> 00:36:06.000
<v Speaker 4>So I did a little looking and if you google

640
00:36:06.440 --> 00:36:11.360
<v Speaker 4>European Southern Observatory and s AS in SAM too, you'll

641
00:36:11.360 --> 00:36:13.119
<v Speaker 4>find this, oh my god, like a rim shot in

642
00:36:13.159 --> 00:36:15.199
<v Speaker 4>a basketball game, like yeah, yeah.

643
00:36:14.920 --> 00:36:17.119
<v Speaker 5>Yeah, like that, except it comes back around. You know,

644
00:36:17.159 --> 00:36:20.840
<v Speaker 5>it's on an orbit. So yeah, so there's stuff orbiting

645
00:36:20.840 --> 00:36:24.119
<v Speaker 5>really close. So that black hole, that one is like, well,

646
00:36:24.760 --> 00:36:28.679
<v Speaker 5>let's see, it's eight thousand parsecs away. I don't know

647
00:36:28.960 --> 00:36:32.559
<v Speaker 5>how much that is. A parsec is about three something

648
00:36:32.679 --> 00:36:35.480
<v Speaker 5>light years. So a light year is how far how

649
00:36:35.519 --> 00:36:38.800
<v Speaker 5>far to how far light travels in a year? Right,

650
00:36:39.599 --> 00:36:41.920
<v Speaker 5>So light moves very quickly, so that's a very long way.

651
00:36:43.320 --> 00:36:47.519
<v Speaker 5>So for example, light travels it takes light eight minutes

652
00:36:47.559 --> 00:36:51.280
<v Speaker 5>to get between the Sun and us. There's a rule

653
00:36:51.320 --> 00:36:53.480
<v Speaker 5>of thumb. Actually, if you want to know how far

654
00:36:53.599 --> 00:36:56.960
<v Speaker 5>how fast light speed is, it goes about a foot

655
00:36:57.039 --> 00:36:58.679
<v Speaker 5>per nanosecond.

656
00:36:58.320 --> 00:37:02.159
<v Speaker 4>A foot per nanosecond. Yes, oh, that's easy to calculate. Yeah,

657
00:37:02.320 --> 00:37:04.480
<v Speaker 4>just a punch of zeros, right, yea, just put a

658
00:37:04.559 --> 00:37:05.280
<v Speaker 4>zero on it.

659
00:37:05.400 --> 00:37:07.440
<v Speaker 5>Yeah, yeah, it's easy and now, but it's kind of

660
00:37:07.440 --> 00:37:09.280
<v Speaker 5>cool because then you can like you can say, like,

661
00:37:09.360 --> 00:37:11.199
<v Speaker 5>if somebody is like ten feet away from you, they

662
00:37:11.199 --> 00:37:12.559
<v Speaker 5>are ten nanoseconds in the past.

663
00:37:13.920 --> 00:37:17.480
<v Speaker 4>They're ten nanoseconds in the past. Oh man, I'm going

664
00:37:17.559 --> 00:37:18.440
<v Speaker 4>to trip out.

665
00:37:19.719 --> 00:37:22.760
<v Speaker 5>So like we're like three nanoseconds apart, right, So.

666
00:37:22.920 --> 00:37:29.280
<v Speaker 4>Weird, it's so weird. It's great though, And I learned

667
00:37:29.320 --> 00:37:31.320
<v Speaker 4>this recently and I've already forgotten it, which is embarrassing.

668
00:37:31.559 --> 00:37:37.599
<v Speaker 4>The distance between us and the Sun is a certain

669
00:37:38.119 --> 00:37:38.760
<v Speaker 4>what is the U?

670
00:37:39.400 --> 00:37:41.400
<v Speaker 5>Oh that's an astronomical unit.

671
00:37:41.559 --> 00:37:42.519
<v Speaker 4>Astronomical unit.

672
00:37:42.639 --> 00:37:44.360
<v Speaker 5>Yeah, that was the distance between us and the Sun.

673
00:37:44.559 --> 00:37:46.639
<v Speaker 4>I just learned that and then completely forgot it all

674
00:37:46.679 --> 00:37:48.000
<v Speaker 4>in the span of a couple of weeks.

675
00:37:48.519 --> 00:37:50.679
<v Speaker 5>It's okay, there's no reason to know that stuff.

676
00:37:51.119 --> 00:37:52.840
<v Speaker 4>I want to know a little bit more about when

677
00:37:52.840 --> 00:37:54.719
<v Speaker 4>you were a kid. By the time Katie was about

678
00:37:54.719 --> 00:37:58.519
<v Speaker 4>ten years old, she was inspired to pursue some form

679
00:37:58.519 --> 00:38:02.280
<v Speaker 4>of cosmology, and she was already a fan of British

680
00:38:02.280 --> 00:38:07.360
<v Speaker 4>cosmologist and theoretical physicist Stephen Hawking, she was already hip

681
00:38:07.360 --> 00:38:09.920
<v Speaker 4>to him. She's like, I know this dude. Now. If

682
00:38:09.920 --> 00:38:11.760
<v Speaker 4>you need a quick brush up on him as a

683
00:38:11.800 --> 00:38:17.320
<v Speaker 4>person after this podcast, watch the twenty fourteen Eddy Redmain

684
00:38:17.440 --> 00:38:20.840
<v Speaker 4>film The Theory of Everything. I'm a cosmologist, what's that?

685
00:38:21.880 --> 00:38:24.239
<v Speaker 4>I study the marriage of space and.

686
00:38:24.159 --> 00:38:27.880
<v Speaker 6>Time, the perfect couple.

687
00:38:28.039 --> 00:38:30.000
<v Speaker 4>Or you can just watch the trailer and start crying

688
00:38:30.760 --> 00:38:33.760
<v Speaker 4>like somebody you know. Now, if thinking about living on

689
00:38:33.760 --> 00:38:37.239
<v Speaker 4>a dust moat floating in a sunbeam was an inspiration

690
00:38:37.360 --> 00:38:39.199
<v Speaker 4>to do what you want to do in life, consider

691
00:38:39.320 --> 00:38:42.199
<v Speaker 4>a human who's figuring out the mysteries of the cosmos,

692
00:38:42.480 --> 00:38:47.400
<v Speaker 4>doing computations and cracking theories about which I can't even comprehend.

693
00:38:47.840 --> 00:38:51.599
<v Speaker 4>The first paragraph of the Wikipedia page Also while living

694
00:38:51.639 --> 00:38:55.400
<v Speaker 4>with als, Katie is one of several billion people inspired

695
00:38:55.440 --> 00:38:58.719
<v Speaker 4>by Stephen Hawking. What was it that Stephen Hawking did

696
00:38:58.960 --> 00:39:01.199
<v Speaker 4>or what did you How did you become aware of

697
00:39:01.280 --> 00:39:03.360
<v Speaker 4>him and how did you kind of absorb what he did? Well?

698
00:39:03.519 --> 00:39:05.559
<v Speaker 5>I'm not sure how I became aware of him. I

699
00:39:05.639 --> 00:39:07.679
<v Speaker 5>think that you know, he was on TV every once

700
00:39:07.719 --> 00:39:10.079
<v Speaker 5>in a while, and I had A Brief History of

701
00:39:10.119 --> 00:39:14.679
<v Speaker 5>Time the book, and I read that and I just like,

702
00:39:15.440 --> 00:39:17.519
<v Speaker 5>I don't know, Like I was interested in black holes,

703
00:39:17.639 --> 00:39:20.119
<v Speaker 5>and I was interested in like the Big Bang.

704
00:39:20.000 --> 00:39:23.360
<v Speaker 4>The Big Bang theory being that the universe began those

705
00:39:23.400 --> 00:39:27.079
<v Speaker 4>thirteen billion years ago with high temperatures and high density

706
00:39:27.159 --> 00:39:32.719
<v Speaker 4>it's continued to expand Also note if you google Big

707
00:39:32.760 --> 00:39:37.400
<v Speaker 4>Bang theory, all roads lead to Sheldon, so just be

708
00:39:37.559 --> 00:39:41.440
<v Speaker 4>cash call it big Bang as far as Wikipedia is concerned.

709
00:39:41.519 --> 00:39:43.599
<v Speaker 5>And so I would read about that stuff. And Stephen

710
00:39:43.639 --> 00:39:46.840
<v Speaker 5>Hawking was a big figure in those those areas, and

711
00:39:47.320 --> 00:39:52.480
<v Speaker 5>he was doing a lot of science communication and he

712
00:39:52.480 --> 00:39:55.440
<v Speaker 5>would visit cal Tech every once in a while. And

713
00:39:55.480 --> 00:39:57.719
<v Speaker 5>I was growing up in LA and St. Long Beach,

714
00:39:57.800 --> 00:40:00.639
<v Speaker 5>and so I would sometimes, like my mom would take

715
00:40:00.639 --> 00:40:03.920
<v Speaker 5>me to see talks by by physicists because I was

716
00:40:03.920 --> 00:40:07.039
<v Speaker 5>super excited about these things. And so I remember seeing

717
00:40:07.480 --> 00:40:10.480
<v Speaker 5>talked by him. I remember seeing a talk by Paul Davies,

718
00:40:10.559 --> 00:40:15.599
<v Speaker 5>and like, you know, just prominent theorists would give talks sometimes,

719
00:40:15.639 --> 00:40:17.320
<v Speaker 5>and somehow my mom would find out about them and

720
00:40:17.360 --> 00:40:20.079
<v Speaker 5>take me along because she's she's really into science and

721
00:40:20.119 --> 00:40:22.280
<v Speaker 5>science fiction and physics and everything.

722
00:40:22.679 --> 00:40:24.760
<v Speaker 4>Have you gotten to meet have you gotten to meet

723
00:40:24.800 --> 00:40:25.440
<v Speaker 4>stupid Hawking.

724
00:40:25.679 --> 00:40:30.760
<v Speaker 5>Yeah. Yeah, So when I was at Cambridge. So I

725
00:40:30.800 --> 00:40:33.920
<v Speaker 5>spent a year at Cambridge during grad school, just kind

726
00:40:33.920 --> 00:40:35.960
<v Speaker 5>of visiting and working with people on some research. And

727
00:40:36.000 --> 00:40:39.079
<v Speaker 5>I was mostly based in his department and my office

728
00:40:39.199 --> 00:40:43.079
<v Speaker 5>was like directly below his. Yeah, and we were in

729
00:40:43.119 --> 00:40:46.519
<v Speaker 5>the same like research group basically, I mean like like

730
00:40:46.599 --> 00:40:49.039
<v Speaker 5>we didn't talk, like we weren't. I wasn't in his

731
00:40:49.079 --> 00:40:51.039
<v Speaker 5>research group, but we were in the same as the

732
00:40:51.039 --> 00:40:53.440
<v Speaker 5>center for the article cosmology, and like we were both

733
00:40:53.519 --> 00:40:55.679
<v Speaker 5>based there. So there were you know, half a dozen

734
00:40:56.039 --> 00:40:58.000
<v Speaker 5>professors who were told to that he was one of them.

735
00:40:58.000 --> 00:41:01.920
<v Speaker 5>And I was a grad student visiting and so I

736
00:41:01.960 --> 00:41:04.159
<v Speaker 5>would go to all these like you know meetings and

737
00:41:04.199 --> 00:41:09.239
<v Speaker 5>the coffee and stuff. And shortly after I was shortly

738
00:41:09.280 --> 00:41:13.239
<v Speaker 5>after I started being a visitor there, somebody asked me

739
00:41:13.320 --> 00:41:17.159
<v Speaker 5>to do one of the like lunch seminars.

740
00:41:17.360 --> 00:41:20.559
<v Speaker 4>So basically, if you're a physicist and you're visiting another department,

741
00:41:20.960 --> 00:41:23.079
<v Speaker 4>you're kind of obligated to give a talk. That's kind

742
00:41:23.079 --> 00:41:26.119
<v Speaker 4>of how it works. So they say, hey, can you

743
00:41:26.119 --> 00:41:28.199
<v Speaker 4>give a talk. She's like, yeah, I'll give a talk

744
00:41:28.280 --> 00:41:29.960
<v Speaker 4>for the Thursday lunch seminar.

745
00:41:30.719 --> 00:41:33.159
<v Speaker 5>So she does it, and it turns out that it

746
00:41:33.199 --> 00:41:37.960
<v Speaker 5>was the lunch seminar that like Hawking goes to. I'm

747
00:41:38.039 --> 00:41:41.239
<v Speaker 5>getting ready to give the talk, and I see like

748
00:41:41.320 --> 00:41:44.519
<v Speaker 5>several of my professors in the audience like looking expectantly

749
00:41:44.559 --> 00:41:48.239
<v Speaker 5>at me, and this is when I'm like freaking out.

750
00:41:48.239 --> 00:41:51.920
<v Speaker 5>But he wasn't there. Hawking wasn't there. So I was like,

751
00:41:51.920 --> 00:41:54.840
<v Speaker 5>it's fine, it's fine, and I'm getting ready to give

752
00:41:54.880 --> 00:41:58.519
<v Speaker 5>the talk. And then I hear this like beee pee pee.

753
00:41:58.800 --> 00:42:01.760
<v Speaker 4>Oh my god, my stomach is cramping just hearing this.

754
00:42:02.239 --> 00:42:03.000
<v Speaker 5>And he shows up.

755
00:42:03.000 --> 00:42:04.039
<v Speaker 4>Oh gets so much worse.

756
00:42:04.880 --> 00:42:07.719
<v Speaker 5>Oh god. So I told this story before, but it's

757
00:42:08.320 --> 00:42:12.039
<v Speaker 5>it's still it's still like is it makes me like sweat?

758
00:42:12.079 --> 00:42:15.119
<v Speaker 5>So so I was I was getting ready to give

759
00:42:15.159 --> 00:42:17.559
<v Speaker 5>the talk, and so I start the talk, like I

760
00:42:17.679 --> 00:42:20.079
<v Speaker 5>put up the title side, and I was the The

761
00:42:20.159 --> 00:42:23.599
<v Speaker 5>topic was primordial black holes, which is a concept that

762
00:42:23.760 --> 00:42:26.039
<v Speaker 5>Hawking came up with along with some other people.

763
00:42:27.360 --> 00:42:27.800
<v Speaker 4>Pressure.

764
00:42:28.159 --> 00:42:32.199
<v Speaker 5>Yeah, And as I'm starting, like as I after I

765
00:42:32.199 --> 00:42:35.639
<v Speaker 5>introduced the title and stuff, I hear this this voice

766
00:42:35.679 --> 00:42:39.679
<v Speaker 5>say and it was his voice, and I was like,

767
00:42:40.639 --> 00:42:43.280
<v Speaker 5>and everybody kind of laughed, you know, and I thought

768
00:42:43.280 --> 00:42:46.599
<v Speaker 5>maybe he was like thanking me for talking about the

769
00:42:46.599 --> 00:42:48.519
<v Speaker 5>thing that he invented, you know, but I don't know,

770
00:42:48.559 --> 00:42:51.480
<v Speaker 5>and you can't ask him to elaborate because he's his

771
00:42:51.559 --> 00:42:54.920
<v Speaker 5>speech is very like slow. So he uses this machine

772
00:42:54.960 --> 00:42:56.920
<v Speaker 5>thing and it just it's very slow.

773
00:42:57.360 --> 00:42:58.559
<v Speaker 4>Attracks his eye movements.

774
00:42:59.320 --> 00:43:02.199
<v Speaker 5>Yeah, well no, not exactly. It tracks there's a little

775
00:43:02.239 --> 00:43:04.840
<v Speaker 5>sensor that looks at his cheek and so he kind

776
00:43:04.840 --> 00:43:08.559
<v Speaker 5>of winks and that like selects words on this like

777
00:43:08.639 --> 00:43:11.840
<v Speaker 5>list and it takes a couple of minutes per words sometimes, right,

778
00:43:11.880 --> 00:43:14.599
<v Speaker 5>So you weren't like I couldn't elaborate, Yeah, yeah, so

779
00:43:14.639 --> 00:43:17.880
<v Speaker 5>I had, so so I just kept going and then

780
00:43:17.920 --> 00:43:21.119
<v Speaker 5>eventually like I heard it again, yes, or later on

781
00:43:21.880 --> 00:43:25.440
<v Speaker 5>or I don't know, or just random things as I'm going,

782
00:43:25.480 --> 00:43:27.039
<v Speaker 5>And every time, like I'd look at him and I'd

783
00:43:27.039 --> 00:43:29.199
<v Speaker 5>be like, you know, but he would just kind of

784
00:43:29.239 --> 00:43:31.360
<v Speaker 5>look blankly at me. And the person who was like

785
00:43:31.400 --> 00:43:33.000
<v Speaker 5>taking care of him is the lunch seminar, So the

786
00:43:33.039 --> 00:43:34.719
<v Speaker 5>person who was taking care of him like feedium, and

787
00:43:34.760 --> 00:43:36.519
<v Speaker 5>she just kind of looked blankly at me, and like

788
00:43:36.800 --> 00:43:38.679
<v Speaker 5>I had no idea what was going on, and so

789
00:43:38.719 --> 00:43:42.679
<v Speaker 5>I would just kind of pause and then continue because

790
00:43:43.000 --> 00:43:44.199
<v Speaker 5>like what am I gonna do?

791
00:43:45.360 --> 00:43:46.440
<v Speaker 4>What was happening here?

792
00:43:46.559 --> 00:43:49.079
<v Speaker 5>Had no idea, and I was so nervous, and like

793
00:43:49.159 --> 00:43:51.920
<v Speaker 5>all the professors were there and already one of the

794
00:43:51.920 --> 00:43:54.159
<v Speaker 5>other professors had been like asking a whole bunch of

795
00:43:54.199 --> 00:43:56.800
<v Speaker 5>really tough questions on like the second slide. So I

796
00:43:56.880 --> 00:43:58.199
<v Speaker 5>was already like freaked out.

797
00:43:58.519 --> 00:44:03.480
<v Speaker 4>Just imagine being in this situation. It's a nightmare. It's

798
00:44:03.519 --> 00:44:06.079
<v Speaker 4>like the best nightmare ever.

799
00:44:06.480 --> 00:44:08.719
<v Speaker 5>But like I answered the questions and that he seemed

800
00:44:08.760 --> 00:44:11.480
<v Speaker 5>to be okay with it. So I finished the talk

801
00:44:11.679 --> 00:44:15.000
<v Speaker 5>and Hawking left and he hadn't asked any questions. And

802
00:44:15.800 --> 00:44:18.800
<v Speaker 5>I asked one of the seminar organizers, like what what

803
00:44:18.880 --> 00:44:22.280
<v Speaker 5>was that? And he was like, oh, well, when he eats,

804
00:44:22.760 --> 00:44:27.199
<v Speaker 5>the machine is chewing and it just picks random stuff

805
00:44:27.239 --> 00:44:32.639
<v Speaker 5>from like the quick select menu, So nothing to do

806
00:44:32.760 --> 00:44:35.039
<v Speaker 5>with you at all. It was just like it was

807
00:44:35.119 --> 00:44:38.079
<v Speaker 5>just like here's the you know, here's the most common phrases. Yes, no,

808
00:44:38.239 --> 00:44:39.519
<v Speaker 5>maybe I don't know. I don't think so.

809
00:44:40.920 --> 00:44:43.599
<v Speaker 4>Oh my god, this is like the worst deodorant ad ever.

810
00:44:43.840 --> 00:44:47.239
<v Speaker 4>Like this is the most stressful situation you could possibly

811
00:44:47.320 --> 00:44:47.719
<v Speaker 4>ever be.

812
00:44:48.320 --> 00:44:50.920
<v Speaker 5>Oh my god, And like they could have told.

813
00:44:50.800 --> 00:44:53.719
<v Speaker 4>Me, yeah, they could have given you every time.

814
00:44:54.039 --> 00:44:58.360
<v Speaker 5>Oh my god, they just like they just didn't mention.

815
00:44:58.239 --> 00:45:00.519
<v Speaker 4>It any word on whether or not he like you talk.

816
00:45:00.880 --> 00:45:01.599
<v Speaker 5>I have no idea.

817
00:45:01.840 --> 00:45:05.199
<v Speaker 4>Oh my god, could you ever tell him that you

818
00:45:05.719 --> 00:45:08.239
<v Speaker 4>went into cosmology because of him?

819
00:45:08.519 --> 00:45:12.480
<v Speaker 5>I don't well. So the first time I met him

820
00:45:12.719 --> 00:45:18.599
<v Speaker 5>when I was sixteen, oh just by fourteen fourteen, baby baby,

821
00:45:18.719 --> 00:45:21.000
<v Speaker 5>I did tell him then that I was a big fan.

822
00:45:21.280 --> 00:45:25.400
<v Speaker 4>So Hawking was at cal Tech and Katie got her

823
00:45:25.400 --> 00:45:28.159
<v Speaker 4>mom to drive her and a friend there to hear

824
00:45:28.239 --> 00:45:30.800
<v Speaker 4>him speak. And afterward they were walking the same way

825
00:45:30.800 --> 00:45:33.119
<v Speaker 4>that he was going. When they were leaving, and she

826
00:45:33.199 --> 00:45:34.840
<v Speaker 4>was too nervous to say hi.

827
00:45:34.840 --> 00:45:37.599
<v Speaker 5>I my friend went up to him and said, my

828
00:45:37.679 --> 00:45:39.000
<v Speaker 5>friend would like to speak to you.

829
00:45:39.800 --> 00:45:40.719
<v Speaker 4>She had a wingman.

830
00:45:42.400 --> 00:45:44.360
<v Speaker 5>So I went up and said that I was a

831
00:45:44.400 --> 00:45:47.400
<v Speaker 5>big fan and I enjoyed his work, and I thanked him,

832
00:45:47.400 --> 00:45:48.320
<v Speaker 5>and he said.

833
00:45:48.199 --> 00:45:49.320
<v Speaker 2>Thank you very much.

834
00:45:49.639 --> 00:45:52.760
<v Speaker 4>Oh Now, what happens to you when you get that?

835
00:45:52.880 --> 00:45:55.880
<v Speaker 4>Because you're really I mean, I'm not going to fangirl

836
00:45:56.039 --> 00:45:57.639
<v Speaker 4>right here, I'll do it in the intro. But you're

837
00:45:57.719 --> 00:46:01.119
<v Speaker 4>like a very big voice in science communication, Like you're

838
00:46:01.320 --> 00:46:05.440
<v Speaker 4>a very well known astrophysicists, cosmologist. How do you feel

839
00:46:05.440 --> 00:46:06.800
<v Speaker 4>when people come up to you and say I was

840
00:46:06.840 --> 00:46:09.320
<v Speaker 4>inspired to study this or you've changed my course, Like,

841
00:46:09.880 --> 00:46:11.239
<v Speaker 4>what kind of reactions do you get?

842
00:46:11.480 --> 00:46:14.960
<v Speaker 5>It's I mean, it doesn't so it's not I'm not

843
00:46:15.599 --> 00:46:18.079
<v Speaker 5>like Stephen Hawking, Like I'm not that level of famous,

844
00:46:18.079 --> 00:46:20.719
<v Speaker 5>and I'm not that level of like important in physics

845
00:46:20.800 --> 00:46:23.320
<v Speaker 5>and stuff and and you know, so it's it's kind

846
00:46:23.320 --> 00:46:25.760
<v Speaker 5>of a different thing, but I do. You know, sometimes

847
00:46:25.800 --> 00:46:31.320
<v Speaker 5>people do like tell me that they like So one

848
00:46:31.320 --> 00:46:33.400
<v Speaker 5>of the messages I've gotten a couple of times is

849
00:46:33.639 --> 00:46:38.800
<v Speaker 5>a like a teenage girl will say that she didn't

850
00:46:38.840 --> 00:46:42.199
<v Speaker 5>think she could do astrophysics, but she really loved it

851
00:46:42.239 --> 00:46:44.559
<v Speaker 5>and then she saw what I was saying on Twitter

852
00:46:44.639 --> 00:46:47.320
<v Speaker 5>or something, or she saw me speak and then she

853
00:46:47.400 --> 00:46:48.760
<v Speaker 5>decided she was going to go for it.

854
00:46:48.880 --> 00:46:49.119
<v Speaker 4>Wow.

855
00:46:49.719 --> 00:46:54.519
<v Speaker 5>So I do get that sometimes, and I like my feelings,

856
00:46:54.519 --> 00:46:57.719
<v Speaker 5>don't know what to do with that, but it's really

857
00:46:58.000 --> 00:46:59.679
<v Speaker 5>it's really sweet.

858
00:46:59.440 --> 00:47:02.480
<v Speaker 4>And roam in a black hole no feeling here.

859
00:47:03.800 --> 00:47:07.480
<v Speaker 5>I mean, it is really sweet. It's really like rewarding

860
00:47:07.519 --> 00:47:10.480
<v Speaker 5>when that happens, and it makes me feel like maybe

861
00:47:10.519 --> 00:47:14.199
<v Speaker 5>like this stuff is maybe the stuff I'm doing is worthwhile.

862
00:47:14.280 --> 00:47:16.159
<v Speaker 5>When people say stuff like that or like a little

863
00:47:16.239 --> 00:47:18.480
<v Speaker 5>kid will sometimes say that they want to be an

864
00:47:18.480 --> 00:47:21.360
<v Speaker 5>astrophysicist or something, and they'll be really excited to meet me,

865
00:47:21.519 --> 00:47:25.199
<v Speaker 5>like I was. I was in Raleigh a couple of

866
00:47:25.239 --> 00:47:27.800
<v Speaker 5>weeks ago, and I was I was sitting in a

867
00:47:27.800 --> 00:47:29.840
<v Speaker 5>cafe and I was wearing my NASA jacket with a

868
00:47:29.880 --> 00:47:32.880
<v Speaker 5>little NASA badge on it that I got it JPL.

869
00:47:33.320 --> 00:47:36.840
<v Speaker 4>JPL, by the way, is NASA's Jet Propulsion Laboratory and

870
00:47:36.880 --> 00:47:41.159
<v Speaker 4>it's nestled in the Golden Hills of Pasadena, California, and

871
00:47:41.199 --> 00:47:45.119
<v Speaker 4>it's responsible for things like rovers on Mars. And according

872
00:47:45.159 --> 00:47:48.760
<v Speaker 4>to press materials, JPL's function is to engineer and fabricate

873
00:47:48.880 --> 00:47:52.519
<v Speaker 4>cool ass shit. That's like so dope, that's very bold.

874
00:47:52.599 --> 00:47:55.519
<v Speaker 4>NASA also do not fact check that part and is

875
00:47:55.599 --> 00:47:56.920
<v Speaker 4>not true.

876
00:47:57.320 --> 00:47:59.480
<v Speaker 5>And this little girl came up to me and she

877
00:47:59.559 --> 00:48:03.800
<v Speaker 5>was probably like eight or something, and she asked me

878
00:48:03.880 --> 00:48:05.760
<v Speaker 5>if I work for NASA, and I said, I don't

879
00:48:05.760 --> 00:48:09.719
<v Speaker 5>work for NASA, but I am an astrophysicist and and

880
00:48:10.079 --> 00:48:12.480
<v Speaker 5>so we'd like talk a little bit. And she said

881
00:48:12.480 --> 00:48:14.880
<v Speaker 5>that she really is into space and stuff, and I

882
00:48:14.920 --> 00:48:17.079
<v Speaker 5>was like, well, I'm giving a talk at the museum

883
00:48:17.159 --> 00:48:18.679
<v Speaker 5>in a couple of days you can come and hear

884
00:48:18.719 --> 00:48:21.480
<v Speaker 5>my talk. And so she and her mom came to

885
00:48:21.559 --> 00:48:24.840
<v Speaker 5>my talk and she asked a question and it was

886
00:48:24.880 --> 00:48:27.199
<v Speaker 5>just really sweet, and I was like, oh, what was

887
00:48:27.199 --> 00:48:31.280
<v Speaker 5>her question? I think her I think her question was

888
00:48:31.320 --> 00:48:33.280
<v Speaker 5>about like what's inside a black hole?

889
00:48:33.400 --> 00:48:35.639
<v Speaker 4>M h, which is a good question, like a bunch

890
00:48:35.679 --> 00:48:36.639
<v Speaker 4>of space garbage.

891
00:48:36.880 --> 00:48:39.159
<v Speaker 5>Well, yeah, so it's I mean, that's it's not as

892
00:48:39.199 --> 00:48:42.400
<v Speaker 5>straightforward answer really because once stuff goes inside the black hole,

893
00:48:42.440 --> 00:48:44.320
<v Speaker 5>it has to go straight to the singularity, and I

894
00:48:44.360 --> 00:48:46.960
<v Speaker 5>can't do anything else, and so then does it really

895
00:48:47.000 --> 00:48:50.239
<v Speaker 5>exist at that point? Like that's kind of subtle, But anyways,

896
00:48:50.239 --> 00:48:52.519
<v Speaker 5>a good question. And apparently, like she was talking about

897
00:48:52.559 --> 00:48:54.800
<v Speaker 5>the talk later on and I was like, hey, you know,

898
00:48:54.880 --> 00:48:56.000
<v Speaker 5>I inspired somebody.

899
00:48:56.159 --> 00:48:57.960
<v Speaker 4>She's going to be in your department later and give

900
00:48:58.480 --> 00:49:03.719
<v Speaker 4>your lunch Shami dumb questions. Explain the singularity?

901
00:49:03.920 --> 00:49:07.559
<v Speaker 5>Oh yeah, yeah, So a singularity is so it comes

902
00:49:07.639 --> 00:49:09.559
<v Speaker 5>up in the context of the Big Bang and in

903
00:49:09.599 --> 00:49:13.320
<v Speaker 5>the context of a black hole. A singularity is like

904
00:49:13.519 --> 00:49:20.320
<v Speaker 5>a point of infinite density. Okay, Usually in physics, when

905
00:49:20.360 --> 00:49:23.000
<v Speaker 5>you have a singularity, I mean, a singularity basically means

906
00:49:23.079 --> 00:49:26.400
<v Speaker 5>it's a point where something infinite happens like where things

907
00:49:26.480 --> 00:49:29.960
<v Speaker 5>diverge in some way, and usually when that happens in physics,

908
00:49:29.960 --> 00:49:32.480
<v Speaker 5>it means you've done something wrong, okay, and it's a

909
00:49:32.480 --> 00:49:35.199
<v Speaker 5>sign that the theory is broken and you just can't

910
00:49:35.239 --> 00:49:37.519
<v Speaker 5>deal with that because it is none of the none

911
00:49:37.559 --> 00:49:42.199
<v Speaker 5>of the theory like really works at a point of infinite anything, Okay.

912
00:49:43.400 --> 00:49:45.719
<v Speaker 5>In the black hole, like the way that black holes

913
00:49:45.719 --> 00:49:47.559
<v Speaker 5>are defined and the way that we understand how the

914
00:49:47.599 --> 00:49:50.079
<v Speaker 5>gravity works, there really should be a singularity at the

915
00:49:50.119 --> 00:49:53.639
<v Speaker 5>center of the black hole and everything has to move

916
00:49:53.679 --> 00:49:56.519
<v Speaker 5>toward it. So so the you know, the black hole

917
00:49:56.519 --> 00:49:58.840
<v Speaker 5>has this is this thing that like the way you

918
00:49:58.880 --> 00:50:00.599
<v Speaker 5>make a black hole go back up.

919
00:50:00.559 --> 00:50:02.079
<v Speaker 4>One, yeah, no, backup, because they're like, where do they

920
00:50:02.079 --> 00:50:02.800
<v Speaker 4>come from? What's the deal?

921
00:50:02.960 --> 00:50:04.679
<v Speaker 5>Yeah, So the way you make black holes you take

922
00:50:04.719 --> 00:50:08.559
<v Speaker 5>a really massive star and you wait a while millions

923
00:50:08.559 --> 00:50:13.039
<v Speaker 5>of years, and the star will explode and the core

924
00:50:13.119 --> 00:50:15.199
<v Speaker 5>of the star will collapse on itself. And if it's

925
00:50:15.239 --> 00:50:19.239
<v Speaker 5>massive enough, then I mean the reason that the star

926
00:50:19.320 --> 00:50:22.039
<v Speaker 5>didn't collapse before is because it had nuclear burning happening.

927
00:50:22.159 --> 00:50:24.360
<v Speaker 5>It was kind of keeping it puffed up, okay, right,

928
00:50:24.960 --> 00:50:26.960
<v Speaker 5>and so you had this energy source that's sort of

929
00:50:27.000 --> 00:50:29.119
<v Speaker 5>pushing against it, kind of like if you have like

930
00:50:29.159 --> 00:50:32.840
<v Speaker 5>a balloon in the air inside is pushing the plastic

931
00:50:33.079 --> 00:50:37.280
<v Speaker 5>the rubber out right. When the star explodes, there's nothing

932
00:50:37.320 --> 00:50:41.800
<v Speaker 5>to keep it from collapsing under its own gravity. You know,

933
00:50:41.880 --> 00:50:44.320
<v Speaker 5>you get to a point where there's you can't do

934
00:50:44.440 --> 00:50:46.079
<v Speaker 5>any more nuclear fusion.

935
00:50:46.159 --> 00:50:49.440
<v Speaker 4>So nuclear fusion is when atoms join to become a

936
00:50:49.440 --> 00:50:52.639
<v Speaker 4>different kind of atom and they give off energy in

937
00:50:52.679 --> 00:50:56.840
<v Speaker 4>the process, like two hydrogens becoming a helium and giving

938
00:50:56.880 --> 00:51:00.280
<v Speaker 4>off energy. Now, this happens with atoms up to the

939
00:51:00.320 --> 00:51:03.880
<v Speaker 4>size of iron, at which point that fusion starts to

940
00:51:04.079 --> 00:51:04.840
<v Speaker 4>take energy.

941
00:51:04.960 --> 00:51:07.400
<v Speaker 5>You can't get any more energy out of those processes

942
00:51:07.440 --> 00:51:09.400
<v Speaker 5>because you've gotten to a point where you've just the

943
00:51:09.400 --> 00:51:13.079
<v Speaker 5>whole center of the star is iron basically, and it

944
00:51:13.519 --> 00:51:15.960
<v Speaker 5>can't go farther than that. And so then you have

945
00:51:16.039 --> 00:51:18.760
<v Speaker 5>this like huge chunk of iron that's not being held

946
00:51:18.800 --> 00:51:20.920
<v Speaker 5>up by anything, and so it starts to clapse under

947
00:51:20.920 --> 00:51:23.679
<v Speaker 5>its own gravity. Like that stuff just falls in and

948
00:51:23.760 --> 00:51:25.960
<v Speaker 5>it has to go toward the center, and it has

949
00:51:26.000 --> 00:51:28.719
<v Speaker 5>to keep going toward the center, and it can't go

950
00:51:28.719 --> 00:51:32.000
<v Speaker 5>any other direction, and so you end up with this singularity,

951
00:51:32.280 --> 00:51:36.079
<v Speaker 5>this point of infinite density. Technically, what is this shape?

952
00:51:36.159 --> 00:51:36.280
<v Speaker 7>Like?

953
00:51:36.360 --> 00:51:39.320
<v Speaker 4>Is it like an ice cream cone that has an

954
00:51:39.440 --> 00:51:40.559
<v Speaker 4>infinite tail?

955
00:51:40.719 --> 00:51:43.119
<v Speaker 5>Or what I mean? You can visualize it that way

956
00:51:43.159 --> 00:51:46.480
<v Speaker 5>if you think about it in terms of like a

957
00:51:46.519 --> 00:51:49.559
<v Speaker 5>two D analog. Like usually when we think of space time,

958
00:51:49.760 --> 00:51:52.320
<v Speaker 5>like the pictures are always like a big rub rubber sheet.

959
00:51:52.519 --> 00:51:57.719
<v Speaker 4>The rubber sheet visual is so helpful for comprehending space time.

960
00:51:59.480 --> 00:52:03.000
<v Speaker 4>But also when I think of rubber sheets, usually the

961
00:52:03.079 --> 00:52:07.719
<v Speaker 4>situation is not comfortable. It's either like an awkward grad

962
00:52:07.960 --> 00:52:13.400
<v Speaker 4>school slumber party explanation or some suburban dungeon kink that

963
00:52:13.519 --> 00:52:20.039
<v Speaker 4>sounds exasperating at best. But for space rubber sheets, thumbs up.

964
00:52:20.320 --> 00:52:21.840
<v Speaker 5>And you have this big rubber sheet, and you put

965
00:52:21.840 --> 00:52:25.159
<v Speaker 5>a bowling ball in one spot and that bends around,

966
00:52:25.360 --> 00:52:27.159
<v Speaker 5>and so then when you take your tennis ball and

967
00:52:27.159 --> 00:52:28.559
<v Speaker 5>you try and roll it past the bowling ball, it

968
00:52:28.599 --> 00:52:30.760
<v Speaker 5>makes a little orbit and falls in rightow. This is

969
00:52:30.840 --> 00:52:34.519
<v Speaker 5>the usual visualization for space time. But that doesn't have

970
00:52:34.519 --> 00:52:37.440
<v Speaker 5>the right number of dimensions because space is space is

971
00:52:37.480 --> 00:52:40.119
<v Speaker 5>three dimensional, and then you can think of time as

972
00:52:40.159 --> 00:52:42.440
<v Speaker 5>another dimension, but that's kind of separate.

973
00:52:42.679 --> 00:52:45.400
<v Speaker 3>Mum, why did they call it Scottish cheese?

974
00:52:45.559 --> 00:52:48.920
<v Speaker 4>It's cottage cheese, honey. And I'm not sure the dogs

975
00:52:48.920 --> 00:52:52.760
<v Speaker 4>in other countries speak different languages. Yeah, I think so.

976
00:52:53.119 --> 00:52:54.480
<v Speaker 3>Well when we get there.

977
00:52:54.400 --> 00:52:56.360
<v Speaker 4>Well, we've got to fix the car first, but there's

978
00:52:56.360 --> 00:53:00.440
<v Speaker 4>someone coming to help us. Is it the man from Geneva.

979
00:53:00.639 --> 00:53:03.159
<v Speaker 4>He's from a Viva Oh there's the van.

980
00:53:03.280 --> 00:53:03.440
<v Speaker 5>Now.

981
00:53:03.760 --> 00:53:06.920
<v Speaker 4>For car insurance with breakdown rescue, it takes a Viva

982
00:53:07.039 --> 00:53:09.679
<v Speaker 4>visit a Viva Data eat to say fifteen percent.

983
00:53:09.519 --> 00:53:12.559
<v Speaker 3>Acceptance criteria, terms and conditions apply minimum premium of three

984
00:53:12.599 --> 00:53:14.719
<v Speaker 3>hundred and ten year old fifteen percent discan't applies to

985
00:53:14.800 --> 00:53:17.599
<v Speaker 3>new policies bought online. See a Viva Dota E for details.

986
00:53:17.679 --> 00:53:20.119
<v Speaker 3>Car insurance is underwritten by a Viva Insurance Ireland DOC

987
00:53:20.159 --> 00:53:22.639
<v Speaker 3>A Viva Direct Arland Limited is regulated by the Central

988
00:53:22.639 --> 00:53:23.320
<v Speaker 3>Bank of Ireland.

989
00:53:23.840 --> 00:53:25.760
<v Speaker 4>I am curious about time is a fourth dimension?

990
00:53:25.840 --> 00:53:26.960
<v Speaker 5>Okay, well we can talk about that.

991
00:53:27.000 --> 00:53:29.679
<v Speaker 4>Okay, I'm sorry I have so many questions.

992
00:53:29.920 --> 00:53:32.639
<v Speaker 5>But anyways, So if you if space is three dimensional,

993
00:53:32.760 --> 00:53:36.400
<v Speaker 5>then the way gravity like works on it is that

994
00:53:36.480 --> 00:53:39.920
<v Speaker 5>it kind of like pulls space inward toward itself. So

995
00:53:40.000 --> 00:53:42.679
<v Speaker 5>like a massive thing kind of pulls space inward toward itself.

996
00:53:42.920 --> 00:53:46.400
<v Speaker 5>So in the context of a black hole, it would

997
00:53:46.400 --> 00:53:49.400
<v Speaker 5>be like a place where space gets really scrunched up, right,

998
00:53:49.800 --> 00:53:51.800
<v Speaker 5>But it's easier to think about it in the two

999
00:53:51.800 --> 00:53:53.639
<v Speaker 5>dimensional case. So it would be like you have your

1000
00:53:53.719 --> 00:53:56.800
<v Speaker 5>rubber sheet and you pinch a piece of the rubber

1001
00:53:56.840 --> 00:53:58.039
<v Speaker 5>sheet and you just pull it down and you just

1002
00:53:58.079 --> 00:54:01.119
<v Speaker 5>keep pulling it down, and it just goes to a

1003
00:54:01.159 --> 00:54:03.280
<v Speaker 5>point and it's like, you know, forever, and it gets

1004
00:54:03.280 --> 00:54:07.360
<v Speaker 5>deeper and narrower whatever. Right, So you can think about

1005
00:54:07.360 --> 00:54:08.920
<v Speaker 5>it like that, But then you think about like a

1006
00:54:08.960 --> 00:54:10.920
<v Speaker 5>three dimensional analog, and your brain kind of breaks and

1007
00:54:10.960 --> 00:54:14.719
<v Speaker 5>it's fader. But yeah, so it's basically a place where

1008
00:54:14.800 --> 00:54:19.679
<v Speaker 5>space is really supercurved, okay, really super bent inward. And

1009
00:54:19.960 --> 00:54:23.920
<v Speaker 5>so there's a point. So if you think again about

1010
00:54:23.920 --> 00:54:27.519
<v Speaker 5>the two D kind of thing the rubber sheet, you

1011
00:54:27.639 --> 00:54:30.840
<v Speaker 5>can you can still move past, Like if you have

1012
00:54:30.960 --> 00:54:33.519
<v Speaker 5>your your like little hole that you pulled down on

1013
00:54:33.719 --> 00:54:35.559
<v Speaker 5>rubber sheet, you can still take your tennis ball and

1014
00:54:35.639 --> 00:54:37.760
<v Speaker 5>roll it past that and it'll keep going. But if

1015
00:54:37.760 --> 00:54:40.039
<v Speaker 5>it gets too close, it'll fall in and there's nothing

1016
00:54:40.039 --> 00:54:42.159
<v Speaker 5>you can do about it, and it'll always go toward

1017
00:54:42.280 --> 00:54:46.079
<v Speaker 5>the deepest point. And so that's like there's this horizon

1018
00:54:46.199 --> 00:54:49.519
<v Speaker 5>this this distance from this from that singularity where if

1019
00:54:49.519 --> 00:54:51.519
<v Speaker 5>you get closer than that, you will fall in no

1020
00:54:51.519 --> 00:54:53.679
<v Speaker 5>matter what, and you will just keep going and you

1021
00:54:53.719 --> 00:54:56.880
<v Speaker 5>can't ever escape. And light itself will fall in too,

1022
00:54:57.079 --> 00:55:01.320
<v Speaker 5>because light follows the curve of space, and so if

1023
00:55:01.320 --> 00:55:03.519
<v Speaker 5>space is curved enough, then light will just follow that

1024
00:55:03.559 --> 00:55:07.400
<v Speaker 5>curve all the way down. Oh man, So once you know,

1025
00:55:07.480 --> 00:55:09.840
<v Speaker 5>so you throw flow a flashlight into a black hole

1026
00:55:09.920 --> 00:55:12.159
<v Speaker 5>like that light never comes out again, It just goes

1027
00:55:12.280 --> 00:55:15.320
<v Speaker 5>that that light beam. No matter which direction the flashlight

1028
00:55:15.360 --> 00:55:17.320
<v Speaker 5>is facing, the light beam will bend toward the center.

1029
00:55:17.840 --> 00:55:21.280
<v Speaker 4>And what is that danger zone called the event horizon. Okay,

1030
00:55:21.280 --> 00:55:21.920
<v Speaker 4>that is the event.

1031
00:55:22.199 --> 00:55:24.800
<v Speaker 5>Yeah, that's the event horizon. I mean you should probably

1032
00:55:24.800 --> 00:55:30.039
<v Speaker 5>stay farther than the event event in general, because other

1033
00:55:30.079 --> 00:55:31.599
<v Speaker 5>bad things can happen to you if you get close

1034
00:55:31.639 --> 00:55:32.199
<v Speaker 5>to the black hole.

1035
00:55:32.239 --> 00:55:35.840
<v Speaker 4>If you listen to Ology's episode one Volcanology and thought

1036
00:55:36.159 --> 00:55:39.440
<v Speaker 4>jumping into a volcano was intense, like hang on to

1037
00:55:39.480 --> 00:55:40.360
<v Speaker 4>your butts right now.

1038
00:55:40.519 --> 00:55:43.880
<v Speaker 5>I mean, so, for one thing, the most of the

1039
00:55:44.119 --> 00:55:46.239
<v Speaker 5>most of the ones that we've seen directly with light

1040
00:55:46.400 --> 00:55:50.280
<v Speaker 5>are pulling in matter, right, and so that means that

1041
00:55:50.320 --> 00:55:52.920
<v Speaker 5>there's a lot of hot stuff falling into the black

1042
00:55:52.920 --> 00:55:56.480
<v Speaker 5>hole in the form of a disk, and so that'll

1043
00:55:56.559 --> 00:55:58.880
<v Speaker 5>radiate you to death if you get too close. And

1044
00:55:58.920 --> 00:56:01.239
<v Speaker 5>then if you if you get close, if it's a

1045
00:56:01.239 --> 00:56:03.880
<v Speaker 5>small enough black hole, then when you get close, the

1046
00:56:03.920 --> 00:56:07.039
<v Speaker 5>tidal forces will kill you. So tidal force is where

1047
00:56:07.079 --> 00:56:10.559
<v Speaker 5>you have like, it's where you have more more gravity.

1048
00:56:10.800 --> 00:56:12.840
<v Speaker 5>The gravity is pulling stronger on part of you than

1049
00:56:12.880 --> 00:56:15.960
<v Speaker 5>another part. Oh, so like if like if you imagine,

1050
00:56:16.000 --> 00:56:18.960
<v Speaker 5>you know, you're falling feet first toward a black hole,

1051
00:56:19.960 --> 00:56:23.079
<v Speaker 5>the gravity goes the strength of the gravity goes up

1052
00:56:23.119 --> 00:56:26.960
<v Speaker 5>so steeply because it's such a compact, steep thing. Then

1053
00:56:27.280 --> 00:56:29.440
<v Speaker 5>your feet will be pulled on much more tightly than

1054
00:56:29.440 --> 00:56:32.239
<v Speaker 5>your head and you'll be stretched out. And it's it's

1055
00:56:32.280 --> 00:56:36.719
<v Speaker 5>there's a word for it. It's called spaghettification. It's actually

1056
00:56:36.760 --> 00:56:38.079
<v Speaker 5>called that.

1057
00:56:38.079 --> 00:56:40.239
<v Speaker 4>That's honest thing I've ever heard of my life.

1058
00:56:40.320 --> 00:56:44.199
<v Speaker 5>Yeah. Yeah, So you have to watch out for spaghetification

1059
00:56:44.599 --> 00:56:46.320
<v Speaker 5>if you get too close to a black hole. Who

1060
00:56:46.400 --> 00:56:49.519
<v Speaker 5>the hell, maybe I don't know, I don't know. I

1061
00:56:49.519 --> 00:56:51.480
<v Speaker 5>mean Hawking uses it, I don't And maybe he came

1062
00:56:51.559 --> 00:56:52.639
<v Speaker 5>up with it. I'm not really sure.

1063
00:56:52.800 --> 00:56:55.119
<v Speaker 4>Oh my god, But of all of the things to

1064
00:56:55.199 --> 00:56:55.639
<v Speaker 4>call it.

1065
00:56:55.920 --> 00:57:00.199
<v Speaker 5>Yeah, it turns you to spaghetti. I don't know, Like

1066
00:57:00.239 --> 00:57:02.360
<v Speaker 5>that's just what else are you gonna call it? Like

1067
00:57:03.280 --> 00:57:07.320
<v Speaker 5>it's title disruption, But I love it the most.

1068
00:57:07.760 --> 00:57:11.800
<v Speaker 4>Yeah, Spaghnification was indeed coined by Hawking in his book

1069
00:57:12.239 --> 00:57:15.639
<v Speaker 4>A Brief History of Time, And if you happen to

1070
00:57:15.880 --> 00:57:19.280
<v Speaker 4>Google image search this you will find a bounty of

1071
00:57:20.000 --> 00:57:24.239
<v Speaker 4>photoshopped images of astronauts being tapered into space noodles by

1072
00:57:24.280 --> 00:57:29.360
<v Speaker 4>cosmic forces. I'm so impressed by this astrophysical whimsy.

1073
00:57:29.559 --> 00:57:30.719
<v Speaker 5>Yeah, there are a lot of There are a lot

1074
00:57:30.760 --> 00:57:33.320
<v Speaker 5>of really silly names in astronomy.

1075
00:57:33.480 --> 00:57:34.800
<v Speaker 4>Who gets to name this stuff?

1076
00:57:35.719 --> 00:57:38.079
<v Speaker 5>Whoever comes up with it? I mean people come up

1077
00:57:38.119 --> 00:57:40.360
<v Speaker 5>with a name it, but like sometimes the community names it,

1078
00:57:40.400 --> 00:57:44.159
<v Speaker 5>like the Big Bang. That that was a joke, Like

1079
00:57:44.360 --> 00:57:46.320
<v Speaker 5>that was the word was a joke, the term the

1080
00:57:46.320 --> 00:57:48.519
<v Speaker 5>Big Bang. Like somebody came up with the idea that,

1081
00:57:48.639 --> 00:57:51.519
<v Speaker 5>you know, the universe started small and has been expanding,

1082
00:57:52.599 --> 00:57:56.199
<v Speaker 5>and somebody was like, oh, the Big Bang, and that

1083
00:57:56.920 --> 00:57:57.400
<v Speaker 5>it stuck.

1084
00:57:57.800 --> 00:57:59.480
<v Speaker 4>No, it was a throwaway.

1085
00:57:59.679 --> 00:58:01.000
<v Speaker 5>Yeah, it was like it was mocking.

1086
00:58:01.400 --> 00:58:03.079
<v Speaker 4>Did that person get pissed and it stuck?

1087
00:58:04.079 --> 00:58:04.679
<v Speaker 5>I'm not sure.

1088
00:58:04.760 --> 00:58:09.519
<v Speaker 4>Okay, So English astronomer Fred Hoyle coined the term big bang.

1089
00:58:09.760 --> 00:58:12.960
<v Speaker 4>It was during a radio broadcast in the late nineteen

1090
00:58:13.039 --> 00:58:16.079
<v Speaker 4>forties and it was kind of an accident. Now the

1091
00:58:16.159 --> 00:58:20.159
<v Speaker 4>story is he's so bent that it's stuck, but apparently

1092
00:58:20.159 --> 00:58:24.880
<v Speaker 4>he denies that. So drama in ms. What in terms

1093
00:58:24.960 --> 00:58:27.840
<v Speaker 4>of what your output is? You're you're a professor, you

1094
00:58:27.880 --> 00:58:30.400
<v Speaker 4>give talks, you travel all over the world, Like what

1095
00:58:30.599 --> 00:58:34.239
<v Speaker 4>is your big goal as a cosmologist? Like do you

1096
00:58:34.280 --> 00:58:38.360
<v Speaker 4>want to write an encyclopedia about cosmology? Like what's your endgame?

1097
00:58:38.519 --> 00:58:42.039
<v Speaker 5>So I'm almost a professor, you are, I'm going to

1098
00:58:42.079 --> 00:58:44.039
<v Speaker 5>be a professor. Well, I'm going to be an assistant

1099
00:58:44.039 --> 00:58:47.519
<v Speaker 5>professor starting January first, yay. Yeah, so I'm not quite

1100
00:58:47.559 --> 00:58:48.360
<v Speaker 5>a professor yet.

1101
00:58:48.400 --> 00:58:51.159
<v Speaker 4>So in a matter of days pretty much, Katie will

1102
00:58:51.199 --> 00:58:55.400
<v Speaker 4>be assistant professor of physics at North Carolina State University.

1103
00:58:55.760 --> 00:58:58.480
<v Speaker 4>So tweeted her and say, congrats.

1104
00:58:58.800 --> 00:59:01.960
<v Speaker 5>So what my goal? I mean? I want to figure

1105
00:59:01.960 --> 00:59:04.639
<v Speaker 5>stuff out, but I don't have like there's not like

1106
00:59:04.760 --> 00:59:07.159
<v Speaker 5>one thing where it's like I must solve this problem.

1107
00:59:07.320 --> 00:59:11.480
<v Speaker 5>I kind of like, uh, just working on whatever fun

1108
00:59:11.480 --> 00:59:14.719
<v Speaker 5>stuff comes up, which is not what you're supposed to do.

1109
00:59:15.599 --> 00:59:16.599
<v Speaker 4>But it's what you like.

1110
00:59:16.840 --> 00:59:18.559
<v Speaker 5>It's always what I like. I mean. So the big

1111
00:59:18.559 --> 00:59:20.000
<v Speaker 5>thing I'm working on right now has to do with

1112
00:59:20.079 --> 00:59:23.800
<v Speaker 5>dark matter. So dark matter is this invisible stuff, you know,

1113
00:59:25.119 --> 00:59:28.199
<v Speaker 5>And it's possible that dark matter has this weird property

1114
00:59:28.239 --> 00:59:30.559
<v Speaker 5>where if you take a dark matter particle and another

1115
00:59:30.639 --> 00:59:34.159
<v Speaker 5>dark matter particle and you you like, collide them into

1116
00:59:34.239 --> 00:59:36.559
<v Speaker 5>each other in just the right way, they'll annihilate and

1117
00:59:36.599 --> 00:59:40.760
<v Speaker 5>create other kinds of particles. So that's a possibility. And

1118
00:59:40.800 --> 00:59:43.440
<v Speaker 5>if that's the case, if that's a thing that happens,

1119
00:59:43.519 --> 00:59:45.760
<v Speaker 5>then it can mess with how the first stars and

1120
00:59:45.800 --> 00:59:49.280
<v Speaker 5>galaxies form, because those form and like blobs of dark matter,

1121
00:59:49.880 --> 00:59:53.800
<v Speaker 5>and the formation of those is kind of delicate because

1122
00:59:53.800 --> 00:59:55.599
<v Speaker 5>you have to get the right balance of the gravity

1123
00:59:55.599 --> 00:59:57.840
<v Speaker 5>and the gas and all this stuff. So if dark

1124
00:59:57.880 --> 01:00:00.880
<v Speaker 5>matter is going and like annihilating all the time, then

1125
01:00:00.960 --> 01:00:03.920
<v Speaker 5>that sort of messes with that balance, and so it

1126
01:00:03.960 --> 01:00:06.280
<v Speaker 5>can change the way the first stars and galaxies form,

1127
01:00:06.320 --> 01:00:08.760
<v Speaker 5>and then we can look for the evidence of that

1128
01:00:08.840 --> 01:00:11.320
<v Speaker 5>with telescopes. So this is the kind of problem that

1129
01:00:11.360 --> 01:00:13.639
<v Speaker 5>I like, where you have like a sort of fundamental

1130
01:00:13.639 --> 01:00:15.719
<v Speaker 5>particle physics problem and then you try and figure out

1131
01:00:15.719 --> 01:00:16.880
<v Speaker 5>how to look for it. With telescopes.

1132
01:00:17.239 --> 01:00:19.119
<v Speaker 4>So what is your work involved. Do you have like

1133
01:00:19.159 --> 01:00:23.519
<v Speaker 4>a moleskin that's just filled with like gobbledygook equations, or

1134
01:00:23.599 --> 01:00:25.840
<v Speaker 4>are you working on a computer with data sets like

1135
01:00:25.880 --> 01:00:28.519
<v Speaker 4>when you're like when you get down to work, what

1136
01:00:28.559 --> 01:00:29.280
<v Speaker 4>does that look like?

1137
01:00:29.760 --> 01:00:32.559
<v Speaker 5>So I do have my muleskin with full of equations

1138
01:00:32.599 --> 01:00:36.280
<v Speaker 5>over there. I brought it with me, so I have that.

1139
01:00:38.360 --> 01:00:40.960
<v Speaker 5>I also have a whole bunch of code that I've

1140
01:00:40.960 --> 01:00:43.960
<v Speaker 5>written to try to solve some of these equations that

1141
01:00:44.000 --> 01:00:46.840
<v Speaker 5>are in the moleskin. I mean, so the usual thing

1142
01:00:46.960 --> 01:00:51.719
<v Speaker 5>is like, Okay, you talk to people who work on

1143
01:00:51.880 --> 01:00:55.239
<v Speaker 5>similar things, and you try and come up with like

1144
01:00:55.360 --> 01:00:57.960
<v Speaker 5>what is it how can we answer this question? Or

1145
01:00:57.960 --> 01:00:59.920
<v Speaker 5>what is a question we can answer with this obser

1146
01:01:00.559 --> 01:01:02.800
<v Speaker 5>or like what would be a cool thing that might

1147
01:01:02.880 --> 01:01:04.760
<v Speaker 5>happen that we could find out if it does happen.

1148
01:01:04.920 --> 01:01:07.800
<v Speaker 4>So then physicists talk to each other and writes it

1149
01:01:07.960 --> 01:01:11.599
<v Speaker 4>down and look at papers and write down more equations.

1150
01:01:11.880 --> 01:01:14.400
<v Speaker 4>And I was kind of surprised to realize how collaborative

1151
01:01:14.440 --> 01:01:16.679
<v Speaker 4>this could be. I always imagine physicists needed to be

1152
01:01:16.679 --> 01:01:21.000
<v Speaker 4>like sequestered in a well appointed lab or a classy

1153
01:01:21.119 --> 01:01:23.840
<v Speaker 4>den to just think clearly, but now there's like a

1154
01:01:23.880 --> 01:01:24.920
<v Speaker 4>lot of chatting happening.

1155
01:01:25.159 --> 01:01:28.159
<v Speaker 5>And then once you figure out like what equations you

1156
01:01:28.199 --> 01:01:31.119
<v Speaker 5>need to solve and what things you need to calculate,

1157
01:01:31.199 --> 01:01:33.280
<v Speaker 5>then you then you go to the computer and you

1158
01:01:33.320 --> 01:01:37.960
<v Speaker 5>write code to calculate those things and to put out

1159
01:01:38.039 --> 01:01:41.840
<v Speaker 5>numbers and draw graphs, and then you see if you

1160
01:01:41.920 --> 01:01:43.159
<v Speaker 5>have something interesting or not.

1161
01:01:43.840 --> 01:01:45.920
<v Speaker 4>If it all kind of clicks yeah, yeah, and.

1162
01:01:45.840 --> 01:01:48.679
<v Speaker 5>You see if like, you know, does this tell us

1163
01:01:48.679 --> 01:01:50.840
<v Speaker 5>that this is going to be an interesting technique to

1164
01:01:50.880 --> 01:01:54.519
<v Speaker 5>test the theory or not? And then depending on you know,

1165
01:01:54.719 --> 01:01:58.519
<v Speaker 5>because this is all theoretical work. Sometimes sometimes you find well,

1166
01:01:58.519 --> 01:02:00.559
<v Speaker 5>this is just really uninteresting and is going to care,

1167
01:02:00.559 --> 01:02:03.599
<v Speaker 5>so I'm not going to write it up. Sometimes you're like, well,

1168
01:02:03.800 --> 01:02:05.800
<v Speaker 5>you know, it turns out you can't measure this thing

1169
01:02:05.840 --> 01:02:07.880
<v Speaker 5>with this technique, but we should write that down anyway,

1170
01:02:07.920 --> 01:02:12.079
<v Speaker 5>because people might have tried otherwise. And then sometimes it's like, oh,

1171
01:02:12.079 --> 01:02:14.679
<v Speaker 5>we can measure this thing with this thing and that'll

1172
01:02:14.719 --> 01:02:16.599
<v Speaker 5>be a really interesting result and we'll get a better

1173
01:02:16.639 --> 01:02:19.239
<v Speaker 5>answer than anybody's gotten before, So we're gonna write it

1174
01:02:19.280 --> 01:02:20.440
<v Speaker 5>up and be really happy about it.

1175
01:02:20.639 --> 01:02:23.199
<v Speaker 4>And then you go toward writing it up and publishing it.

1176
01:02:23.360 --> 01:02:25.679
<v Speaker 5>Yeah, yeah, and then and then you write the paper,

1177
01:02:25.719 --> 01:02:27.800
<v Speaker 5>and then you publish the paper, and then you know,

1178
01:02:27.960 --> 01:02:29.920
<v Speaker 5>or you send it to the journal, and the journals

1179
01:02:30.079 --> 01:02:32.679
<v Speaker 5>the editors or the referees are like, yeah, you should

1180
01:02:32.719 --> 01:02:34.480
<v Speaker 5>do this differently, and so you do that differently, and

1181
01:02:34.519 --> 01:02:36.039
<v Speaker 5>then eventually it gets published.

1182
01:02:36.480 --> 01:02:39.199
<v Speaker 4>What is the craziest paper that you've ever had published?

1183
01:02:39.199 --> 01:02:41.800
<v Speaker 4>When the title of the craziest paper, because just looking

1184
01:02:41.840 --> 01:02:44.760
<v Speaker 4>at paper titles is, yeah, so funny to me because

1185
01:02:44.760 --> 01:02:46.639
<v Speaker 4>they're so specific and wonderful.

1186
01:02:47.000 --> 01:02:48.599
<v Speaker 5>I mean, I guess it depends on what you mean.

1187
01:02:48.719 --> 01:02:53.719
<v Speaker 5>I wrote a paper called known Unknowns of dark Matter

1188
01:02:53.800 --> 01:02:57.239
<v Speaker 5>Annihilation over Cosmic Time that.

1189
01:02:57.320 --> 01:03:00.480
<v Speaker 4>Sounds like the best like Norwegian metal album them Ever,

1190
01:03:01.079 --> 01:03:04.000
<v Speaker 4>it was like, well, yeah, so that was all about

1191
01:03:04.079 --> 01:03:06.480
<v Speaker 4>like what we know we don't know about this problem?

1192
01:03:06.599 --> 01:03:11.480
<v Speaker 5>Mm hmm. I've calculated a bunch of stuff. I've I

1193
01:03:11.639 --> 01:03:18.480
<v Speaker 5>had some papers about, uh like axions and and those

1194
01:03:18.519 --> 01:03:21.079
<v Speaker 5>are theoretical particles that are super cool.

1195
01:03:21.719 --> 01:03:23.840
<v Speaker 4>Is there an upper limit to how many words your

1196
01:03:23.840 --> 01:03:24.920
<v Speaker 4>paper title can be?

1197
01:03:25.480 --> 01:03:27.000
<v Speaker 5>Yeah, you don't want to. I mean you kind of

1198
01:03:27.039 --> 01:03:29.360
<v Speaker 5>wanted to be punchy, right, like like the whole non

1199
01:03:29.400 --> 01:03:32.360
<v Speaker 5>unknowns thing is I wanted it to be like eye catching.

1200
01:03:32.199 --> 01:03:34.000
<v Speaker 4>Right, it's good marketing.

1201
01:03:34.280 --> 01:03:36.920
<v Speaker 5>Yeah, yeah, so you got to think about marketing to

1202
01:03:36.960 --> 01:03:39.679
<v Speaker 5>some degree, and you don't want it to be a

1203
01:03:39.679 --> 01:03:41.480
<v Speaker 5>long title because people are going to be skimming out.

1204
01:03:41.519 --> 01:03:44.920
<v Speaker 4>This part is crazy. It's like trying to buy Beyonce tickets.

1205
01:03:45.320 --> 01:03:47.880
<v Speaker 4>So the way that people find papers to read is

1206
01:03:47.920 --> 01:03:52.559
<v Speaker 4>every day, every weekday. The website, it's a r xiv

1207
01:03:53.199 --> 01:03:56.400
<v Speaker 4>dot org. There's like a hundred new papers about astronomy

1208
01:03:56.440 --> 01:03:57.599
<v Speaker 4>and physics and math and stuff.

1209
01:03:57.679 --> 01:04:01.440
<v Speaker 5>So the way that people find papers to read is

1210
01:04:01.719 --> 01:04:09.079
<v Speaker 5>every day, every single day, every weekday. The archive website,

1211
01:04:09.360 --> 01:04:12.079
<v Speaker 5>it's a r xiv is how it's spelled, but we

1212
01:04:12.119 --> 01:04:16.280
<v Speaker 5>call it the archive. The archive website displays like one

1213
01:04:16.400 --> 01:04:21.239
<v Speaker 5>hundred papers, new papers about astronomy, and there's just a

1214
01:04:21.320 --> 01:04:23.840
<v Speaker 5>list and the titles. So there's the titles and the

1215
01:04:23.880 --> 01:04:26.079
<v Speaker 5>authors and maybe like the abstract depending on how you

1216
01:04:26.119 --> 01:04:31.719
<v Speaker 5>read the archive. And if you're a responsible astronomer, then

1217
01:04:31.760 --> 01:04:35.000
<v Speaker 5>every morning you wake up and you read the archive

1218
01:04:35.039 --> 01:04:37.760
<v Speaker 5>and you skim the papers and the and the abstracts

1219
01:04:37.760 --> 01:04:39.639
<v Speaker 5>and you see which ones are relevant to your work,

1220
01:04:39.840 --> 01:04:42.239
<v Speaker 5>and then you you know open those and read, you know,

1221
01:04:42.280 --> 01:04:44.840
<v Speaker 5>skim those papers and find out if like they tell

1222
01:04:44.840 --> 01:04:47.400
<v Speaker 5>you something interesting, you get information. This is how you

1223
01:04:47.480 --> 01:04:51.880
<v Speaker 5>keep up with the field. It's so much work. It's

1224
01:04:51.920 --> 01:04:53.320
<v Speaker 5>like of a lot of work. And if you're somebody

1225
01:04:53.360 --> 01:04:56.559
<v Speaker 5>who maybe does you know particle theory stuff as well,

1226
01:04:56.840 --> 01:04:59.480
<v Speaker 5>then there's a whole other archive for like particle theory,

1227
01:04:59.519 --> 01:05:02.519
<v Speaker 5>and then part of phenomenology, which is more like the

1228
01:05:02.559 --> 01:05:05.159
<v Speaker 5>phenomenology is like where you try and figure out what

1229
01:05:05.199 --> 01:05:07.880
<v Speaker 5>you would see in this in the universe that's closer

1230
01:05:07.880 --> 01:05:10.199
<v Speaker 5>to what I do. So then if you're trying to

1231
01:05:10.239 --> 01:05:14.760
<v Speaker 5>read particle theory and phenomenology and astronomy, you can get

1232
01:05:14.800 --> 01:05:17.239
<v Speaker 5>like one hundred and fifty papers or something every day.

1233
01:05:17.400 --> 01:05:18.199
<v Speaker 4>It's a black hole.

1234
01:05:18.559 --> 01:05:20.159
<v Speaker 5>It's just it's impossible to keep up.

1235
01:05:20.159 --> 01:05:20.760
<v Speaker 4>Oh my god.

1236
01:05:20.920 --> 01:05:24.440
<v Speaker 5>But anyway, so because of that, you want your paper

1237
01:05:24.480 --> 01:05:28.639
<v Speaker 5>title to be punchy and eye catching. But the other thing,

1238
01:05:28.760 --> 01:05:32.159
<v Speaker 5>so there's a this is like so totally inside baseball,

1239
01:05:32.199 --> 01:05:36.239
<v Speaker 5>but there's there's this ridiculous thing that happens.

1240
01:05:36.280 --> 01:05:39.000
<v Speaker 4>So the order of the papers as they appear on

1241
01:05:39.039 --> 01:05:42.719
<v Speaker 4>the website is determined just by what time they were

1242
01:05:42.760 --> 01:05:47.599
<v Speaker 4>sent in and after not too long. These are literal geniuses.

1243
01:05:47.679 --> 01:05:49.079
<v Speaker 4>They were like duck.

1244
01:05:49.360 --> 01:05:53.480
<v Speaker 5>There's a cutoff time of like four pm and sometimes

1245
01:05:53.480 --> 01:05:56.320
<v Speaker 5>on I don't remember which one, where if you get

1246
01:05:56.360 --> 01:05:59.559
<v Speaker 5>your paper in as close as possible after that time,

1247
01:05:59.679 --> 01:06:02.679
<v Speaker 5>it will appear at the top of the god. And

1248
01:06:02.719 --> 01:06:05.480
<v Speaker 5>so there's this you can people have written papers about

1249
01:06:05.519 --> 01:06:09.719
<v Speaker 5>like the spike insubmission times, where like everybody's trying to

1250
01:06:09.719 --> 01:06:13.480
<v Speaker 5>get like, for you know, a clock zero zero one second,

1251
01:06:13.599 --> 01:06:16.119
<v Speaker 5>Like they all want to get it like exactly at

1252
01:06:16.159 --> 01:06:18.119
<v Speaker 5>that moment so that their paper will be on the

1253
01:06:18.119 --> 01:06:19.639
<v Speaker 5>top of the list. Because a lot of people, you know,

1254
01:06:19.800 --> 01:06:21.639
<v Speaker 5>like they open the archive and then they just get

1255
01:06:21.679 --> 01:06:23.960
<v Speaker 5>like exhausted by the time they've gone through five papers,

1256
01:06:24.000 --> 01:06:25.559
<v Speaker 5>and so they don't get to the end of the list.

1257
01:06:25.599 --> 01:06:31.320
<v Speaker 5>And so there's this ridiculous, like this ridiculous ritual of

1258
01:06:31.440 --> 01:06:33.639
<v Speaker 5>when you're when you submit your paper to the archive,

1259
01:06:33.719 --> 01:06:36.079
<v Speaker 5>you're trying like you watch the clock and you try

1260
01:06:36.079 --> 01:06:38.400
<v Speaker 5>and hit the submit button exactly the right moment.

1261
01:06:38.480 --> 01:06:41.440
<v Speaker 4>That makes me so anxious. It's like when someone people

1262
01:06:41.480 --> 01:06:44.159
<v Speaker 4>comment first on YouTube vation it should.

1263
01:06:43.960 --> 01:06:47.320
<v Speaker 5>Be randomized because like it's also been shown that it

1264
01:06:47.360 --> 01:06:49.480
<v Speaker 5>does matter in terms of like citations.

1265
01:06:49.639 --> 01:06:53.719
<v Speaker 4>That's not right, it's not right. Oh my god. Yeah,

1266
01:06:53.800 --> 01:06:55.599
<v Speaker 4>Oh wait, what was the question that I had right

1267
01:06:55.639 --> 01:06:58.360
<v Speaker 4>on top of that? It was definitely a dem one.

1268
01:06:58.760 --> 01:07:00.000
<v Speaker 4>It was definitely a stupid question.

1269
01:07:01.280 --> 01:07:03.559
<v Speaker 5>I don't think any questions are stupid, Are you sure?

1270
01:07:03.760 --> 01:07:06.360
<v Speaker 5>I think these are good questions. These are important questions

1271
01:07:06.360 --> 01:07:09.760
<v Speaker 5>because like what it doesn't like you know, these are

1272
01:07:10.000 --> 01:07:12.639
<v Speaker 5>like if you're asking questions about something because you're not

1273
01:07:12.679 --> 01:07:14.400
<v Speaker 5>an expert in that field, Like you can't be an

1274
01:07:14.400 --> 01:07:16.920
<v Speaker 5>expert in every field. If I ask questions about entomology,

1275
01:07:16.960 --> 01:07:20.239
<v Speaker 5>I'm gonna have no idea what's going on? Okay, But

1276
01:07:20.280 --> 01:07:22.440
<v Speaker 5>I'm like, I'm still trying to remember what the difference

1277
01:07:22.440 --> 01:07:24.639
<v Speaker 5>beviews between a bug and not a bug, right, Like,

1278
01:07:24.719 --> 01:07:25.239
<v Speaker 5>I don't know.

1279
01:07:25.920 --> 01:07:27.719
<v Speaker 4>I'll give you some clearance on that, okay. But the

1280
01:07:27.719 --> 01:07:33.159
<v Speaker 4>problem is is you study the universe? Yes, so could

1281
01:07:33.199 --> 01:07:37.159
<v Speaker 4>your field be any broader? Like no, no, it could not

1282
01:07:37.480 --> 01:07:38.639
<v Speaker 4>literally everything.

1283
01:07:39.079 --> 01:07:41.320
<v Speaker 5>Yeah, And this can be a problem too, Like when

1284
01:07:41.320 --> 01:07:46.360
<v Speaker 5>I give talks, I have to be prepared for anything

1285
01:07:46.639 --> 01:07:48.840
<v Speaker 5>the questions and that used to just freak me out

1286
01:07:48.840 --> 01:07:50.440
<v Speaker 5>a lot, and now I just feel like like I

1287
01:07:50.519 --> 01:07:53.800
<v Speaker 5>just have to I have to read as widely as possible,

1288
01:07:53.960 --> 01:07:57.519
<v Speaker 5>and sometimes I'll be like, I have no idea but like, like,

1289
01:07:57.559 --> 01:08:00.960
<v Speaker 5>I gave the talk about gravitational waves in Raleigh the

1290
01:08:01.039 --> 01:08:04.880
<v Speaker 5>other week and one of the questions was, tell me

1291
01:08:04.920 --> 01:08:07.239
<v Speaker 5>about the Great Red Spot on Jupiter, And I was like,

1292
01:08:09.039 --> 01:08:16.720
<v Speaker 5>it's a storm, it's been shrinking. There's a spacecraft looking

1293
01:08:16.720 --> 01:08:20.600
<v Speaker 5>at it. You should maybe talk to somebody who studies

1294
01:08:20.640 --> 01:08:20.960
<v Speaker 5>about that.

1295
01:08:21.239 --> 01:08:24.520
<v Speaker 4>The Great Red Spot, by the way, that's its actual name.

1296
01:08:24.600 --> 01:08:27.199
<v Speaker 4>It's a little on the nose. Also, people mix it

1297
01:08:27.279 --> 01:08:31.000
<v Speaker 4>up sometimes with the Great Dark Spot, which was near

1298
01:08:31.119 --> 01:08:35.000
<v Speaker 4>Jupiter's northern poul. So y'all call me, let me name

1299
01:08:35.039 --> 01:08:38.399
<v Speaker 4>some of these things. Also, how did Katie feel about

1300
01:08:38.399 --> 01:08:42.399
<v Speaker 4>the detection of gravitational waves? This was the Lago project

1301
01:08:42.439 --> 01:08:44.199
<v Speaker 4>you may have heard about in twenty sixteen.

1302
01:08:44.319 --> 01:08:49.760
<v Speaker 5>The detection of gravitational waves by the Lego instrument was

1303
01:08:49.840 --> 01:08:53.239
<v Speaker 5>probably the biggest discovery in physics in my lifetime.

1304
01:08:53.920 --> 01:08:54.319
<v Speaker 4>Damn.

1305
01:08:54.800 --> 01:08:57.479
<v Speaker 5>Yeah, that's a big deal. It's a super big deal.

1306
01:08:58.199 --> 01:09:02.600
<v Speaker 5>I when so the first the first detection was last

1307
01:09:02.640 --> 01:09:05.479
<v Speaker 5>year sometime. Well, the detection was the end of twenty

1308
01:09:05.479 --> 01:09:08.560
<v Speaker 5>fifteen and it was announced I guess during twenty sixteen.

1309
01:09:10.399 --> 01:09:14.159
<v Speaker 5>The announcement was in I don't remember what times when

1310
01:09:14.199 --> 01:09:15.920
<v Speaker 5>it was or whatever, but it was such that it

1311
01:09:15.960 --> 01:09:18.479
<v Speaker 5>was going to be two am local time in Melbourne,

1312
01:09:19.479 --> 01:09:23.680
<v Speaker 5>and so a bunch of us got together and like

1313
01:09:23.800 --> 01:09:28.079
<v Speaker 5>had a party in a university department. Like we brought

1314
01:09:28.119 --> 01:09:31.119
<v Speaker 5>food and booze and like we watched videos and like

1315
01:09:31.199 --> 01:09:34.279
<v Speaker 5>we took like we took selfies. It was really late,

1316
01:09:35.600 --> 01:09:37.920
<v Speaker 5>but we were just like we got to see this live,

1317
01:09:38.239 --> 01:09:40.520
<v Speaker 5>you know. And and there were there were two people

1318
01:09:40.520 --> 01:09:43.960
<v Speaker 5>in the room who were part of the collaboration, so

1319
01:09:44.000 --> 01:09:46.520
<v Speaker 5>they they already knew what was going to be done.

1320
01:09:46.560 --> 01:09:48.640
<v Speaker 5>But the rest of us, like we'd heard rumors, but

1321
01:09:48.640 --> 01:09:50.199
<v Speaker 5>we didn't know for sure what was what that was

1322
01:09:50.199 --> 01:09:53.039
<v Speaker 5>going to be announced. And yeah, it was. It was

1323
01:09:53.119 --> 01:09:55.359
<v Speaker 5>just a huge party and it was a we were

1324
01:09:55.399 --> 01:09:59.920
<v Speaker 5>really excited and like we just everybody was like clap

1325
01:10:00.279 --> 01:10:02.680
<v Speaker 5>and stuff when it happened, and I mean it was

1326
01:10:02.760 --> 01:10:03.520
<v Speaker 5>it was a huge deal.

1327
01:10:03.520 --> 01:10:07.359
<v Speaker 4>Of the way that it was announced was like a

1328
01:10:07.600 --> 01:10:10.199
<v Speaker 4>press conference from like an awesome eighties movie.

1329
01:10:10.359 --> 01:10:17.880
<v Speaker 8>Yeah, ladies and gentlemen, we have detected gravitational waves.

1330
01:10:18.079 --> 01:10:18.800
<v Speaker 3>We did it.

1331
01:10:22.199 --> 01:10:24.720
<v Speaker 4>I mean, how cute is that? So that was Dave Ritzi.

1332
01:10:24.880 --> 01:10:27.640
<v Speaker 4>He's a laser physicist and he's director of the Lego Lab,

1333
01:10:27.880 --> 01:10:31.960
<v Speaker 4>And I love that audio so much. It's just like

1334
01:10:32.199 --> 01:10:38.279
<v Speaker 4>pure triumph, like the last scene of a Schwarzenegger movie

1335
01:10:38.359 --> 01:10:44.760
<v Speaker 4>or something. We have detected gravitational waves. It was like

1336
01:10:45.159 --> 01:10:45.640
<v Speaker 4>the best.

1337
01:10:45.800 --> 01:10:47.600
<v Speaker 5>Yeah, yeah, no, I remember that very clearly.

1338
01:10:48.000 --> 01:10:50.920
<v Speaker 4>So explain to me why the detection of gravitational waves

1339
01:10:50.960 --> 01:10:51.920
<v Speaker 4>is such a big deal.

1340
01:10:52.239 --> 01:10:56.600
<v Speaker 5>Okay, So, first, gravitational waves are are ripples in this

1341
01:10:56.760 --> 01:10:59.199
<v Speaker 5>fabric of space time. So you know, the space space

1342
01:10:59.239 --> 01:11:02.359
<v Speaker 5>can be bent around massive objects. And when massive objects

1343
01:11:02.399 --> 01:11:05.680
<v Speaker 5>are moving through space, if they're moving in an accelerated way,

1344
01:11:05.680 --> 01:11:07.760
<v Speaker 5>which could be in an orbit in orbit as a

1345
01:11:07.840 --> 01:11:13.520
<v Speaker 5>kind of accelerated motion, that creates ripples in this sort

1346
01:11:13.560 --> 01:11:15.920
<v Speaker 5>of space time fabric, which is kind of hard to

1347
01:11:16.000 --> 01:11:19.760
<v Speaker 5>visualize and explain, but it ripples through space. And so

1348
01:11:20.359 --> 01:11:23.840
<v Speaker 5>like when you have really massive objects moving really quickly,

1349
01:11:24.920 --> 01:11:28.479
<v Speaker 5>that can make large disturbances relative to other things. I mean,

1350
01:11:28.520 --> 01:11:30.920
<v Speaker 5>if I wave my hands, I'm making gravitational waves, but

1351
01:11:31.159 --> 01:11:36.399
<v Speaker 5>like that's not detectable. So so two black holes orbiting

1352
01:11:36.439 --> 01:11:40.640
<v Speaker 5>each other make really big detectable gravitational waves, especially when

1353
01:11:40.680 --> 01:11:43.319
<v Speaker 5>they get so close that they're about to merge into

1354
01:11:43.359 --> 01:11:46.479
<v Speaker 5>one thing. So you can have two black holes in

1355
01:11:46.520 --> 01:11:48.800
<v Speaker 5>a binary orbit orbiting each other, and then as they

1356
01:11:48.800 --> 01:11:51.760
<v Speaker 5>get closer and closer, the signal gets stronger and stronger,

1357
01:11:52.399 --> 01:11:54.319
<v Speaker 5>you know, the waves get stronger and stronger, and then

1358
01:11:54.359 --> 01:11:56.680
<v Speaker 5>they merge and that makes this big sort of burst

1359
01:11:57.239 --> 01:12:03.760
<v Speaker 5>of gravitational waves. And the way that gravitational waves work,

1360
01:12:04.119 --> 01:12:06.399
<v Speaker 5>they're not like ripples on a pond. Usually when you

1361
01:12:06.479 --> 01:12:10.720
<v Speaker 5>see a visualization, it's like ripples on a pond, but

1362
01:12:10.800 --> 01:12:15.920
<v Speaker 5>that's that two dimensional analog, you know again, And they're

1363
01:12:15.960 --> 01:12:20.800
<v Speaker 5>not like if you're standing there, the gravitational wave like

1364
01:12:21.119 --> 01:12:24.399
<v Speaker 5>moves your space that you're in, but it doesn't just

1365
01:12:24.479 --> 01:12:27.000
<v Speaker 5>like move you up and down. What it does is

1366
01:12:27.279 --> 01:12:31.039
<v Speaker 5>it stretches and squeezes the space that you're in. So

1367
01:12:31.159 --> 01:12:33.680
<v Speaker 5>let's say that you're standing there and a gravitational wave comes,

1368
01:12:33.680 --> 01:12:36.319
<v Speaker 5>it hits you in the face. What that does to

1369
01:12:36.359 --> 01:12:39.000
<v Speaker 5>you is it stretches your space a little bit, so

1370
01:12:39.000 --> 01:12:41.199
<v Speaker 5>you get a little bit taller and at the same

1371
01:12:41.199 --> 01:12:42.960
<v Speaker 5>time a little skinnier, and then a little bit shorter

1372
01:12:43.000 --> 01:12:46.079
<v Speaker 5>and a little wider, and like it oscillates back and forth.

1373
01:12:46.119 --> 01:12:49.039
<v Speaker 5>So as the waves are coming at you, each wave

1374
01:12:49.119 --> 01:12:53.119
<v Speaker 5>is giving you that that stretch and squeeze, stretch and squeeze,

1375
01:12:53.920 --> 01:12:56.840
<v Speaker 5>and so it's actually distorting your shape. Oh my god,

1376
01:12:56.840 --> 01:12:57.720
<v Speaker 5>what is happening.

1377
01:12:57.800 --> 01:13:00.960
<v Speaker 4>This is like a big boy and it it keeps

1378
01:13:01.079 --> 01:13:05.840
<v Speaker 4>like for everything that creates gravitational waves. Is this doing

1379
01:13:06.119 --> 01:13:08.920
<v Speaker 4>this to us all the time? Micro micro basis?

1380
01:13:09.000 --> 01:13:13.880
<v Speaker 5>Yeah, yeah, So the Lego experiment is built to detect

1381
01:13:14.039 --> 01:13:16.520
<v Speaker 5>these things. So they have two detectors, and each detector

1382
01:13:16.600 --> 01:13:21.039
<v Speaker 5>is like it's an L shaped thing. Each arm is

1383
01:13:21.119 --> 01:13:22.239
<v Speaker 5>four kilometers long.

1384
01:13:22.359 --> 01:13:24.880
<v Speaker 4>Now, if you've seen photos of this, you might think

1385
01:13:25.159 --> 01:13:27.439
<v Speaker 4>from a distance, is some shit that we build like

1386
01:13:27.479 --> 01:13:32.439
<v Speaker 4>on Mars, because there's just this treeless, ocre landscape in

1387
01:13:32.479 --> 01:13:35.600
<v Speaker 4>the desert. It seems to look lonely in every direction.

1388
01:13:35.920 --> 01:13:37.720
<v Speaker 4>But no, it's just Washington State.

1389
01:13:37.840 --> 01:13:41.079
<v Speaker 5>And they shoot lasers back and forth along these two

1390
01:13:41.159 --> 01:13:44.159
<v Speaker 5>arms there. They meet at the center and they're measuring.

1391
01:13:44.239 --> 01:13:46.359
<v Speaker 5>The lasers are just there to measure the length of

1392
01:13:46.399 --> 01:13:50.880
<v Speaker 5>those arms, basically, and when a gravitational wave comes and

1393
01:13:51.000 --> 01:13:54.479
<v Speaker 5>hits that detector, it makes one of the arms a

1394
01:13:54.520 --> 01:13:56.479
<v Speaker 5>little longer while the other one gets a little shorter,

1395
01:13:56.560 --> 01:13:59.600
<v Speaker 5>and vice versa, depending on the direction and the you

1396
01:13:59.600 --> 01:14:03.680
<v Speaker 5>know and everything. So if it does that, then the

1397
01:14:03.720 --> 01:14:06.319
<v Speaker 5>detector can detect that the length of the arms has

1398
01:14:06.439 --> 01:14:11.359
<v Speaker 5>changed and then that's the signal, is the changing of

1399
01:14:11.399 --> 01:14:14.720
<v Speaker 5>the length of the arms and the level on which

1400
01:14:14.760 --> 01:14:17.479
<v Speaker 5>that happened. So this is four kilometers right, Yeah.

1401
01:14:17.279 --> 01:14:20.199
<v Speaker 4>That's about two and a half miles America.

1402
01:14:20.279 --> 01:14:24.600
<v Speaker 5>The first detection, when it was detected, the length of

1403
01:14:24.640 --> 01:14:28.520
<v Speaker 5>that four kilometer arm changed in length by a thousandth

1404
01:14:28.680 --> 01:14:29.760
<v Speaker 5>the width of a proton.

1405
01:14:30.000 --> 01:14:31.239
<v Speaker 4>Oh my god.

1406
01:14:31.560 --> 01:14:34.560
<v Speaker 5>Yeah that's a teensy tiny that's really small.

1407
01:14:34.760 --> 01:14:37.920
<v Speaker 4>And this was a huge collision.

1408
01:14:38.079 --> 01:14:40.520
<v Speaker 5>Yeah, yeah, this was like it was one point three

1409
01:14:40.560 --> 01:14:43.399
<v Speaker 5>billion light years away, so it's very far. But it

1410
01:14:43.479 --> 01:14:45.880
<v Speaker 5>was like the black holes were around thirty times as

1411
01:14:45.960 --> 01:14:49.840
<v Speaker 5>massive as the Sun and they collided, and so it

1412
01:14:49.920 --> 01:14:53.079
<v Speaker 5>was a pretty strong signal, Like it was a surprisingly

1413
01:14:53.119 --> 01:14:55.479
<v Speaker 5>strong signal, Like if you actually looked at the data,

1414
01:14:55.880 --> 01:14:57.760
<v Speaker 5>raw data, like you could see it, which is not

1415
01:14:57.960 --> 01:15:01.000
<v Speaker 5>usually the case in this kind of field. Usually, like

1416
01:15:01.039 --> 01:15:03.079
<v Speaker 5>you have to do lots of processing, but like you

1417
01:15:03.119 --> 01:15:07.359
<v Speaker 5>can see the signal is very strong. So but yeah,

1418
01:15:07.560 --> 01:15:10.520
<v Speaker 5>thousands the width of a proton, so that you know,

1419
01:15:10.600 --> 01:15:13.079
<v Speaker 5>your own height is changing much less than that, right,

1420
01:15:13.119 --> 01:15:15.520
<v Speaker 5>because you're not four kilometers long, sure.

1421
01:15:15.680 --> 01:15:18.159
<v Speaker 4>So I'm getting a little bit not quite as tall

1422
01:15:18.199 --> 01:15:19.840
<v Speaker 4>and not quite as skinny, and not kind of quite

1423
01:15:19.840 --> 01:15:23.239
<v Speaker 4>as short as fat as it's not noticeable in a photograph.

1424
01:15:23.319 --> 01:15:26.600
<v Speaker 5>Say, yes, yeah, yeah, it's really it's a really subtle effect.

1425
01:15:27.279 --> 01:15:31.239
<v Speaker 5>But but yeah, so that's the gravitational wave. It's the

1426
01:15:31.279 --> 01:15:35.880
<v Speaker 5>detection of that change in length, that sort of stretching

1427
01:15:35.920 --> 01:15:38.920
<v Speaker 5>and squeezing of space time. And each time the black holes,

1428
01:15:39.479 --> 01:15:43.119
<v Speaker 5>you know, black holes or something collide, you get this

1429
01:15:43.279 --> 01:15:46.640
<v Speaker 5>kind of like the the wiggles will come faster and

1430
01:15:46.640 --> 01:15:49.800
<v Speaker 5>closer together. And so the frequency of this changing of

1431
01:15:50.039 --> 01:15:52.640
<v Speaker 5>shape is going up, and the amplitude is going up,

1432
01:15:52.640 --> 01:15:54.760
<v Speaker 5>and so it makes this kind of rising sound if

1433
01:15:54.800 --> 01:15:57.239
<v Speaker 5>you transmit it, if you change it into sound, it's

1434
01:15:57.279 --> 01:16:01.079
<v Speaker 5>like a sort of like the like end part is

1435
01:16:01.079 --> 01:16:04.560
<v Speaker 5>when they collide. And the reason people change it to

1436
01:16:04.600 --> 01:16:08.279
<v Speaker 5>sound a lot is because the frequency of these waves coming,

1437
01:16:08.399 --> 01:16:11.680
<v Speaker 5>like how how quickly the stretching and squeezing happens, is

1438
01:16:11.720 --> 01:16:15.119
<v Speaker 5>about the same frequency as like sound waves. Okay, so

1439
01:16:15.399 --> 01:16:17.399
<v Speaker 5>it is kind of audible, Like if you change it

1440
01:16:17.399 --> 01:16:18.560
<v Speaker 5>to sound, it's kind of audible.

1441
01:16:19.000 --> 01:16:22.279
<v Speaker 4>And that was like the the boop heard around the world, right.

1442
01:16:22.239 --> 01:16:25.239
<v Speaker 5>Yeah, yeah, it's called a chirp, A chirp, yes, just.

1443
01:16:27.600 --> 01:16:31.039
<v Speaker 4>Okay, you ready for this? This is the sound of history.

1444
01:16:32.880 --> 01:16:37.800
<v Speaker 4>So what does that mean going forward for astrophysicists, And like,

1445
01:16:38.000 --> 01:16:39.840
<v Speaker 4>how many more have we heard since then?

1446
01:16:40.640 --> 01:16:42.920
<v Speaker 5>So there have been oh gosh, I didn't even know

1447
01:16:42.960 --> 01:16:47.960
<v Speaker 5>the number, like something like five scene now and the

1448
01:16:48.000 --> 01:16:50.960
<v Speaker 5>most recent, most recent one was was two black holes.

1449
01:16:50.960 --> 01:16:53.000
<v Speaker 5>But the one before that was the neutrons. There was

1450
01:16:53.000 --> 01:16:55.760
<v Speaker 5>two neutrons stars and those were a big deal because

1451
01:16:56.319 --> 01:16:59.600
<v Speaker 5>those when they collided, also created a gamma ray.

1452
01:16:59.439 --> 01:17:04.479
<v Speaker 4>Burst gamma ray burst super energetic explosion, so we can't

1453
01:17:04.520 --> 01:17:07.600
<v Speaker 4>see gamma rays but the pack of punch and a burst.

1454
01:17:07.479 --> 01:17:10.159
<v Speaker 5>And so we were able to see the collision from

1455
01:17:10.239 --> 01:17:13.840
<v Speaker 5>the gravitational waves but also from light and that was

1456
01:17:13.880 --> 01:17:16.399
<v Speaker 5>a huge deal. And I can talk about that for hours,

1457
01:17:17.600 --> 01:17:20.640
<v Speaker 5>but it's it's a big deal. The whole thing is

1458
01:17:20.680 --> 01:17:22.439
<v Speaker 5>a big deal for a bunch of reasons. One is

1459
01:17:22.479 --> 01:17:27.079
<v Speaker 5>that this, like the existence of gravitational waves was kind

1460
01:17:27.119 --> 01:17:31.279
<v Speaker 5>of known indirectly because we'd seen systems where like you

1461
01:17:31.319 --> 01:17:34.640
<v Speaker 5>had two pulsars orbiting each other, So pulsar is a

1462
01:17:34.680 --> 01:17:36.880
<v Speaker 5>kind of neutron star. A neutron star is like the

1463
01:17:36.880 --> 01:17:42.159
<v Speaker 5>core of a dead star. It's so we'd seen things

1464
01:17:42.239 --> 01:17:45.800
<v Speaker 5>orbiting each other where the changing of the orbit could

1465
01:17:45.800 --> 01:17:49.319
<v Speaker 5>only really be easily explained by gravitational waves kind of

1466
01:17:49.479 --> 01:17:52.079
<v Speaker 5>radiating energy away from the orbit, and so the orbit

1467
01:17:52.119 --> 01:17:55.159
<v Speaker 5>got smaller because gravitational waves were pulling energy away, oh

1468
01:17:55.880 --> 01:18:00.319
<v Speaker 5>and sort of shrinking that orbit. So so we had

1469
01:18:00.680 --> 01:18:03.560
<v Speaker 5>indirect evidence the gravitational waves existed, but we'd never seen

1470
01:18:03.560 --> 01:18:08.760
<v Speaker 5>them directly. And seeing like directly, like detecting, like feeling

1471
01:18:08.840 --> 01:18:12.159
<v Speaker 5>the gravitational wave is a huge deal, right, And the

1472
01:18:12.520 --> 01:18:16.079
<v Speaker 5>gravitational waves were like the last, the last prediction of

1473
01:18:16.079 --> 01:18:18.039
<v Speaker 5>Einstein's relativity to be confirmed.

1474
01:18:18.079 --> 01:18:21.880
<v Speaker 4>Einstein's theory of relativity. Remember, our perception of the force

1475
01:18:21.920 --> 01:18:26.800
<v Speaker 4>of gravity is a bendy spacetime thing. I'm very paraphrasing

1476
01:18:27.119 --> 01:18:27.520
<v Speaker 4>a lot.

1477
01:18:28.079 --> 01:18:31.880
<v Speaker 5>So he predicted them one hundred years about one hundred

1478
01:18:31.960 --> 01:18:35.520
<v Speaker 5>years before the first detection was made, So it was

1479
01:18:35.560 --> 01:18:38.439
<v Speaker 5>it took a long time to see these things, but

1480
01:18:38.680 --> 01:18:42.239
<v Speaker 5>so it was confirmed that And it's just this incredible

1481
01:18:42.319 --> 01:18:48.680
<v Speaker 5>laboratory for relativity for physics because by detecting the gravitational

1482
01:18:48.720 --> 01:18:51.239
<v Speaker 5>waves and looking at the signal, we were able to

1483
01:18:51.279 --> 01:18:53.840
<v Speaker 5>determine that gravitational waves travel at the speed of light.

1484
01:18:54.399 --> 01:18:56.520
<v Speaker 5>We didn't know for sure before. That was part of

1485
01:18:56.560 --> 01:18:58.520
<v Speaker 5>the theory, but we didn't know for sure, so we

1486
01:18:58.880 --> 01:19:02.760
<v Speaker 5>figured that out. It told us stuff about how black

1487
01:19:02.760 --> 01:19:05.079
<v Speaker 5>holes are made, like what black holes are made of,

1488
01:19:05.119 --> 01:19:08.239
<v Speaker 5>sort of like the properties of black holes, by examining

1489
01:19:08.319 --> 01:19:12.199
<v Speaker 5>very closely how they come together and merge, how much

1490
01:19:12.319 --> 01:19:17.520
<v Speaker 5>energy the gravitational wave burst creates, you know, a lot

1491
01:19:17.560 --> 01:19:20.399
<v Speaker 5>of stuff about about that. And then because now we

1492
01:19:20.479 --> 01:19:26.000
<v Speaker 5>can we can watch black holes colliding in the distant universe,

1493
01:19:26.079 --> 01:19:28.920
<v Speaker 5>we can learn about how black holes grow, you know,

1494
01:19:29.119 --> 01:19:31.279
<v Speaker 5>by when they collide with each other, and that tells

1495
01:19:31.359 --> 01:19:33.960
<v Speaker 5>us something about how black holes grow. It tells us

1496
01:19:34.000 --> 01:19:36.840
<v Speaker 5>something about how galaxies grow. It tells us something about

1497
01:19:36.880 --> 01:19:40.119
<v Speaker 5>how stars form, because black holes are the end results

1498
01:19:40.119 --> 01:19:40.520
<v Speaker 5>of stars.

1499
01:19:40.600 --> 01:19:42.319
<v Speaker 4>When you were a kid, were you ever hoping that

1500
01:19:42.359 --> 01:19:45.199
<v Speaker 4>this that we would be able to detect gravitational waves

1501
01:19:46.000 --> 01:19:47.880
<v Speaker 4>where you like, I've been waiting since I was a

1502
01:19:47.920 --> 01:19:48.720
<v Speaker 4>little girl.

1503
01:19:50.239 --> 01:19:53.319
<v Speaker 5>So so I didn't know a whole lot about gravitational

1504
01:19:53.359 --> 01:19:54.840
<v Speaker 5>waves when I was a little kid. But there was

1505
01:19:54.920 --> 01:19:59.560
<v Speaker 5>there was a really beautiful moment during one of the

1506
01:20:00.039 --> 01:20:02.760
<v Speaker 5>detection of the neutron star collisions when one of the

1507
01:20:02.800 --> 01:20:07.159
<v Speaker 5>scientists was he was he was talking about the neutron

1508
01:20:07.199 --> 01:20:09.560
<v Speaker 5>star collision and the neutron stars when they collide, they

1509
01:20:09.560 --> 01:20:11.840
<v Speaker 5>make a slightly different kind of like chirp sound.

1510
01:20:11.960 --> 01:20:15.880
<v Speaker 4>Okay, here's the sound of the neutron stars booping themselves together.

1511
01:20:22.039 --> 01:20:24.039
<v Speaker 5>So the black hole one is actually a lot quicker

1512
01:20:24.119 --> 01:20:26.039
<v Speaker 5>than what I said, But the neutron star one goes

1513
01:20:26.079 --> 01:20:28.880
<v Speaker 5>like it takes it. It takes a while and it

1514
01:20:28.920 --> 01:20:33.399
<v Speaker 5>does it. So and there'd been simulations of this for years.

1515
01:20:33.439 --> 01:20:35.720
<v Speaker 5>I mean, the scientists who was talking about the discovery

1516
01:20:35.800 --> 01:20:38.920
<v Speaker 5>said that he'd been waiting to hear that sound from

1517
01:20:39.039 --> 01:20:43.319
<v Speaker 5>nature for twenty years and he just did and it

1518
01:20:43.399 --> 01:20:44.199
<v Speaker 5>was really touching.

1519
01:20:44.239 --> 01:20:44.479
<v Speaker 4>I mean.

1520
01:20:44.520 --> 01:20:47.560
<v Speaker 5>So for me, I knew about LEGO because it was

1521
01:20:49.079 --> 01:20:51.680
<v Speaker 5>it was partly headed by people at cal Tech, and

1522
01:20:51.680 --> 01:20:53.880
<v Speaker 5>I was an undergrad at Caltech, And so when I

1523
01:20:53.920 --> 01:20:56.800
<v Speaker 5>was an undergrad there people were talking about a lot

1524
01:20:56.840 --> 01:21:00.920
<v Speaker 5>and there was there was a famous bet between like

1525
01:21:01.119 --> 01:21:03.199
<v Speaker 5>Kip Thorn and Stephen Hawking or something.

1526
01:21:03.319 --> 01:21:06.680
<v Speaker 4>Kip Thorn, by the way, is a theoretical physicist, the

1527
01:21:06.920 --> 01:21:08.920
<v Speaker 4>twenty seventeen Nobel.

1528
01:21:08.680 --> 01:21:11.960
<v Speaker 5>Laureate about whether or not gravitational waves would be detected

1529
01:21:11.960 --> 01:21:15.039
<v Speaker 5>by the year two thousand. I started cal Tech in

1530
01:21:15.159 --> 01:21:19.399
<v Speaker 5>ninety nine, so they were not detected by year two thousand,

1531
01:21:19.439 --> 01:21:22.800
<v Speaker 5>so that bet was lost. But it was a funny

1532
01:21:22.880 --> 01:21:24.920
<v Speaker 5>thing because when I first got to cal Tech, they

1533
01:21:24.920 --> 01:21:27.359
<v Speaker 5>were building LAGO and it was this big deal and

1534
01:21:27.399 --> 01:21:29.640
<v Speaker 5>everybody's like, we're going to detect gravitational waves. It's gonna

1535
01:21:29.640 --> 01:21:33.199
<v Speaker 5>be amazing. And then you know, and LEGO is being built,

1536
01:21:33.239 --> 01:21:35.159
<v Speaker 5>and I was like, oh, it's any minute now. And

1537
01:21:35.199 --> 01:21:37.760
<v Speaker 5>then I left cal Tech and I went to grad

1538
01:21:37.800 --> 01:21:40.399
<v Speaker 5>school and then after a while, I was like, I

1539
01:21:40.439 --> 01:21:42.239
<v Speaker 5>haven't heard anything about this for a while, you know,

1540
01:21:42.239 --> 01:21:45.199
<v Speaker 5>And I realized that like they kind they'd kind of

1541
01:21:45.279 --> 01:21:47.359
<v Speaker 5>like they'd been like, yeah, we're going to detect gravitational waves,

1542
01:21:47.399 --> 01:21:49.119
<v Speaker 5>and then they kind of got quiet for a while,

1543
01:21:49.119 --> 01:21:51.119
<v Speaker 5>and I found out later on asked about it, and

1544
01:21:51.159 --> 01:21:53.199
<v Speaker 5>they were like, oh no, it's advanced.

1545
01:21:52.760 --> 01:21:55.199
<v Speaker 4>LIGO was so there were some upgrades over the years

1546
01:21:55.359 --> 01:22:01.279
<v Speaker 4>from initial LAGO to Enhanced LAGO to advances LAGO. It's

1547
01:22:01.359 --> 01:22:05.920
<v Speaker 4>kind of like the tall Grande and Venti gravitational wave

1548
01:22:06.039 --> 01:22:09.119
<v Speaker 4>detectors just then maybe need a little more to get

1549
01:22:09.119 --> 01:22:09.960
<v Speaker 4>the job done.

1550
01:22:09.880 --> 01:22:12.439
<v Speaker 5>Really going to do the detection. The initial LEGO was

1551
01:22:12.439 --> 01:22:14.399
<v Speaker 5>like maybe it would get lucky, but advanced LAGO will

1552
01:22:14.399 --> 01:22:18.720
<v Speaker 5>really see something. I'm like really, So, like for a while,

1553
01:22:18.760 --> 01:22:20.560
<v Speaker 5>I was like, I don't know what I feel like,

1554
01:22:20.760 --> 01:22:22.319
<v Speaker 5>I don't know if I believe that this is really

1555
01:22:22.319 --> 01:22:24.560
<v Speaker 5>going to happen. But then you know, as soon as

1556
01:22:24.600 --> 01:22:28.560
<v Speaker 5>they turned advanced lago on, like within like a week

1557
01:22:28.720 --> 01:22:32.199
<v Speaker 5>or something, they saw this thing. So that's like they

1558
01:22:32.279 --> 01:22:34.359
<v Speaker 5>really they really did it. And it's the most like

1559
01:22:34.600 --> 01:22:38.359
<v Speaker 5>it's the most precise instrument ever built by humans. I

1560
01:22:38.359 --> 01:22:42.159
<v Speaker 5>think I read that somewhere. It's like the I mean,

1561
01:22:42.239 --> 01:22:44.760
<v Speaker 5>you're measuring something so tiny.

1562
01:22:45.000 --> 01:22:45.720
<v Speaker 4>It's crazy.

1563
01:22:45.960 --> 01:22:51.119
<v Speaker 5>It's it's impossible. I use, it's incredible. How like what

1564
01:22:51.159 --> 01:22:54.680
<v Speaker 5>went into it in terms of the engineering and you know,

1565
01:22:54.880 --> 01:22:57.279
<v Speaker 5>just the physics and like they had to they had

1566
01:22:57.279 --> 01:23:00.359
<v Speaker 5>to correct for things like the like how how much

1567
01:23:00.479 --> 01:23:03.119
<v Speaker 5>the photon's hitting the mirrors would move them.

1568
01:23:03.439 --> 01:23:05.399
<v Speaker 4>Oh my god, Oh my god.

1569
01:23:05.880 --> 01:23:08.840
<v Speaker 5>That's a big part of the noise in the signal

1570
01:23:09.640 --> 01:23:12.119
<v Speaker 5>that's called the photon shot noise. They have to deal

1571
01:23:12.159 --> 01:23:14.960
<v Speaker 5>with that. Yeah, so stuff like that. I mean, it's

1572
01:23:15.000 --> 01:23:16.800
<v Speaker 5>it's incredible that they were able to do this.

1573
01:23:16.960 --> 01:23:19.439
<v Speaker 4>So can you get the chirp as a ring tone?

1574
01:23:19.600 --> 01:23:21.800
<v Speaker 5>I believe you can. You can, I believe so, Yeah,

1575
01:23:21.880 --> 01:23:24.439
<v Speaker 5>would you get the the neutron whoop? Or would you

1576
01:23:24.479 --> 01:23:27.159
<v Speaker 5>get the the black hole one? The black hole one,

1577
01:23:27.399 --> 01:23:29.439
<v Speaker 5>you have to speed it up to make it sound cool,

1578
01:23:30.079 --> 01:23:31.720
<v Speaker 5>so you can still hear it, but it's more like

1579
01:23:31.720 --> 01:23:36.319
<v Speaker 5>a like so so in the actual data, it's like that,

1580
01:23:36.319 --> 01:23:38.399
<v Speaker 5>that's kind of what it sounds like. But then when

1581
01:23:38.479 --> 01:23:40.760
<v Speaker 5>you when you speed it up, it goes whoop whoop,

1582
01:23:40.880 --> 01:23:42.960
<v Speaker 5>but it's very quick, whereas the neutron star one, it's

1583
01:23:43.000 --> 01:23:44.319
<v Speaker 5>like ooop.

1584
01:23:45.119 --> 01:23:47.000
<v Speaker 4>I feel like, yeah, I feel like that's the way

1585
01:23:47.039 --> 01:23:47.239
<v Speaker 4>to go.

1586
01:23:47.640 --> 01:23:48.000
<v Speaker 5>Yeah.

1587
01:23:48.159 --> 01:23:51.640
<v Speaker 4>Let's say someone is interesting cosmology but doesn't know a

1588
01:23:51.680 --> 01:23:53.720
<v Speaker 4>lot about it and is intimidated by it. What is

1589
01:23:53.720 --> 01:23:56.680
<v Speaker 4>the best book to pick up? I actually, and this

1590
01:23:56.720 --> 01:23:57.880
<v Speaker 4>is that. I don't know if you've ever read this,

1591
01:23:57.920 --> 01:24:00.319
<v Speaker 4>but I was. I was in Thailand and I was

1592
01:24:00.319 --> 01:24:02.159
<v Speaker 4>staying in a hut and there was some there was

1593
01:24:02.159 --> 01:24:04.640
<v Speaker 4>a free book pile, and I picked up a book

1594
01:24:04.640 --> 01:24:07.399
<v Speaker 4>called Quantum Mechanics Can't Hurt You. This book was actually

1595
01:24:07.439 --> 01:24:11.520
<v Speaker 4>called Quantum Theory Cannot Hurt You. It's by Marcus Choone

1596
01:24:11.880 --> 01:24:15.319
<v Speaker 4>and it's delightful. I found my copy. It's still moldy

1597
01:24:15.399 --> 01:24:17.800
<v Speaker 4>from a monsoon. It was good, it was very it

1598
01:24:17.800 --> 01:24:22.119
<v Speaker 4>was very layperson's terms, but I clearly don't didn't retain

1599
01:24:22.159 --> 01:24:25.359
<v Speaker 4>any of it. But is there a book or a

1600
01:24:25.399 --> 01:24:27.920
<v Speaker 4>documentary or something that's just a good primer, because like

1601
01:24:28.039 --> 01:24:32.159
<v Speaker 4>in this episode, there's no way to describe everything, but like,

1602
01:24:32.359 --> 01:24:36.680
<v Speaker 4>what's a good go to, like astrophysics for dummies? What

1603
01:24:36.760 --> 01:24:40.199
<v Speaker 4>are we talking here? Is there a pamphlet? Uh?

1604
01:24:40.600 --> 01:24:43.239
<v Speaker 5>So I wish I had a really good answer for

1605
01:24:43.319 --> 01:24:44.399
<v Speaker 5>this that.

1606
01:24:44.359 --> 01:24:48.279
<v Speaker 4>It makes me feel like you don't you're winter.

1607
01:24:49.039 --> 01:24:52.239
<v Speaker 5>So the thing is like, I don't. I don't read

1608
01:24:52.600 --> 01:24:57.359
<v Speaker 5>a lot of popular level stuff. And there's a couple

1609
01:24:57.399 --> 01:24:58.079
<v Speaker 5>of reasons for that.

1610
01:24:58.479 --> 01:25:01.079
<v Speaker 4>So number one, she doesn't have much time to read

1611
01:25:01.399 --> 01:25:04.079
<v Speaker 4>non papers because there's like a billion papers, and when

1612
01:25:04.079 --> 01:25:07.560
<v Speaker 4>she does, she likes to read about spaceships. Okay too,

1613
01:25:07.760 --> 01:25:11.600
<v Speaker 4>when something is written for the general public, astro physicists

1614
01:25:12.079 --> 01:25:15.319
<v Speaker 4>have to take that lay information and kind of back

1615
01:25:15.439 --> 01:25:18.920
<v Speaker 4>translate it to a more technical version in their head.

1616
01:25:19.119 --> 01:25:22.000
<v Speaker 4>So it's like if you're a bartender and someone writes

1617
01:25:22.159 --> 01:25:26.199
<v Speaker 4>she drank a whiskey, but you're distracted wondering a whiskey,

1618
01:25:26.359 --> 01:25:29.640
<v Speaker 4>Well it like a bourbon? Is this a single malt scotch?

1619
01:25:29.760 --> 01:25:32.319
<v Speaker 4>Was it a rye Tennessee whiskey is this on the

1620
01:25:32.399 --> 01:25:35.159
<v Speaker 4>rocks was in a cocktail? There's so much detail a minute.

1621
01:25:35.319 --> 01:25:38.479
<v Speaker 5>I mean, Sean Carroll's written several books that are really good,

1622
01:25:39.439 --> 01:25:44.039
<v Speaker 5>so take a look at those. There's a physicist Katie Freeze,

1623
01:25:44.279 --> 01:25:48.439
<v Speaker 5>Catherine Freeze, who's a dark matter theorist like me. Oh,

1624
01:25:48.960 --> 01:25:51.319
<v Speaker 5>she's a dark menical corismologist, and she's written a book

1625
01:25:51.399 --> 01:25:56.439
<v Speaker 5>called Cosmic Cocktail and it's all about about dark matter

1626
01:25:56.680 --> 01:25:59.399
<v Speaker 5>and also like some audibiographical stuff. It's really cool.

1627
01:26:02.159 --> 01:26:05.479
<v Speaker 4>What about What about movies? Do you have a favorite

1628
01:26:05.560 --> 01:26:08.560
<v Speaker 4>or a least favorite movie about space or cosmology?

1629
01:26:08.680 --> 01:26:10.640
<v Speaker 5>You're like, could I not answer some of these?

1630
01:26:10.880 --> 01:26:11.159
<v Speaker 4>Yes?

1631
01:26:11.279 --> 01:26:17.800
<v Speaker 5>Yes, yes, okay, so so favorite yes. So there aren't

1632
01:26:17.840 --> 01:26:20.720
<v Speaker 5>a lot of movies where I feel like the cosmology,

1633
01:26:20.800 --> 01:26:23.840
<v Speaker 5>Like cosmology is hard to have as a topic of

1634
01:26:23.880 --> 01:26:26.079
<v Speaker 5>a movie because it's just too big a topic, and

1635
01:26:26.159 --> 01:26:29.279
<v Speaker 5>like stuff happens on cosmological time scales, which is like

1636
01:26:30.039 --> 01:26:35.399
<v Speaker 5>incredibly long times, and so having something happen within a

1637
01:26:35.439 --> 01:26:40.720
<v Speaker 5>movie timeframe is really hard. But there's a movie that

1638
01:26:40.840 --> 01:26:44.000
<v Speaker 5>I really liked for how it portrayed the scientists and

1639
01:26:44.039 --> 01:26:49.840
<v Speaker 5>it had some cosmology ish stuff in it, So that

1640
01:26:49.920 --> 01:26:54.239
<v Speaker 5>was sunshine okay, which the science is wrong, just putting

1641
01:26:54.239 --> 01:26:57.399
<v Speaker 5>that out there. It's about the sun has like burned

1642
01:26:57.439 --> 01:26:59.720
<v Speaker 5>out or is burning out and they have to fix it,

1643
01:26:59.760 --> 01:27:02.199
<v Speaker 5>and none of that can happen. All of that's false,

1644
01:27:02.319 --> 01:27:04.880
<v Speaker 5>All that's fake. But it's done really well in terms

1645
01:27:04.920 --> 01:27:07.920
<v Speaker 5>of like they have physicists who who acts like a physicist,

1646
01:27:08.000 --> 01:27:10.600
<v Speaker 5>and like they have people who talk like scientists. And

1647
01:27:10.640 --> 01:27:13.359
<v Speaker 5>I kind of just enjoyed it. Okay, so I thought that,

1648
01:27:13.479 --> 01:27:15.800
<v Speaker 5>and then there's like a monster thing, so anyway, but

1649
01:27:15.920 --> 01:27:20.119
<v Speaker 5>I thought that was done really well. I really enjoyed gravity.

1650
01:27:20.560 --> 01:27:23.520
<v Speaker 5>There's also bad physics in gravity in some places, but

1651
01:27:23.680 --> 01:27:27.359
<v Speaker 5>I thought it was a beautiful movie and it portrayed

1652
01:27:27.399 --> 01:27:28.199
<v Speaker 5>space very well.

1653
01:27:28.239 --> 01:27:29.520
<v Speaker 4>How do you feel about space balls?

1654
01:27:29.560 --> 01:27:32.000
<v Speaker 5>I think it was funny. It's been a long time.

1655
01:27:32.680 --> 01:27:33.880
<v Speaker 4>Oh hell yes, that was good.

1656
01:27:34.079 --> 01:27:37.640
<v Speaker 5>Yeah. Other space movies like The Martian was fun. Interstellar

1657
01:27:37.680 --> 01:27:39.199
<v Speaker 5>had a very pretty black hole in it.

1658
01:27:39.399 --> 01:27:44.359
<v Speaker 4>Okay, that's that you are being very complimentary, and that

1659
01:27:44.520 --> 01:27:48.239
<v Speaker 4>is duly noted. You are being a very nice person.

1660
01:27:49.960 --> 01:27:52.399
<v Speaker 5>The black hole and the wormhole and Interstellar were very

1661
01:27:52.439 --> 01:27:58.000
<v Speaker 5>beautifully done and done with with proper relativistic equations. It

1662
01:27:58.039 --> 01:28:00.399
<v Speaker 5>was very clever because what they did is they they

1663
01:28:00.800 --> 01:28:03.439
<v Speaker 5>had these simulations that are very very difficult and take

1664
01:28:03.479 --> 01:28:06.960
<v Speaker 5>a very long time on supercomputers, and they gave them

1665
01:28:07.000 --> 01:28:10.439
<v Speaker 5>to the the the people who do movie graphics, who

1666
01:28:10.479 --> 01:28:14.199
<v Speaker 5>have really powerful supercomputers, and they're like, no, we need

1667
01:28:14.239 --> 01:28:17.279
<v Speaker 5>to do this black hole properly. So they calculated it,

1668
01:28:17.319 --> 01:28:19.199
<v Speaker 5>and now they got some like papers out of it

1669
01:28:19.239 --> 01:28:23.640
<v Speaker 5>because the result was such such a good calculation that

1670
01:28:23.680 --> 01:28:26.079
<v Speaker 5>they were able to get actual science out of the

1671
01:28:26.880 --> 01:28:29.520
<v Speaker 5>calculation done for the graphics in the movie.

1672
01:28:29.720 --> 01:28:31.199
<v Speaker 4>Because movies are better funded.

1673
01:28:31.239 --> 01:28:35.119
<v Speaker 5>Then yeah, yeah, yea, so it was a very good move.

1674
01:28:35.680 --> 01:28:37.960
<v Speaker 5>But but you should you should know that that the

1675
01:28:38.079 --> 01:28:41.560
<v Speaker 5>black hole in Interstellar, although there are some aspects that

1676
01:28:41.600 --> 01:28:44.359
<v Speaker 5>are done very faithfully, they did have they did tweak

1677
01:28:44.399 --> 01:28:48.600
<v Speaker 5>some things, so it actually would look pretty different if

1678
01:28:48.600 --> 01:28:50.680
<v Speaker 5>we saw an actual black hole in real life. So

1679
01:28:50.720 --> 01:28:52.239
<v Speaker 5>there are a couple of things that were tweaked that

1680
01:28:52.279 --> 01:28:53.119
<v Speaker 5>were a bit different.

1681
01:28:53.199 --> 01:28:55.880
<v Speaker 4>So, speaking of movies, Katie and I were supposed to

1682
01:28:56.000 --> 01:28:58.600
<v Speaker 4>go to one after this interview, and we did, but

1683
01:28:58.640 --> 01:29:02.119
<v Speaker 4>we barely made it. Because this is all really great information.

1684
01:29:02.600 --> 01:29:05.079
<v Speaker 4>We hadn't even gotten to the rapid fire around of

1685
01:29:05.119 --> 01:29:08.640
<v Speaker 4>all of your questions, so I asked your questions. We

1686
01:29:08.920 --> 01:29:11.520
<v Speaker 4>race to the showing and this poor woman had to

1687
01:29:11.560 --> 01:29:14.680
<v Speaker 4>smuggle a burrito and eat it in the theater. I'm

1688
01:29:14.720 --> 01:29:16.720
<v Speaker 4>so sorry. By the way, we saw murder on the

1689
01:29:16.800 --> 01:29:21.159
<v Speaker 4>Oran Express. It features a very bizarre mustache. I will

1690
01:29:21.159 --> 01:29:24.439
<v Speaker 4>give it that, So stay tuned the first two parter

1691
01:29:24.479 --> 01:29:28.479
<v Speaker 4>Anology's history when we resume with your questions, so you

1692
01:29:28.560 --> 01:29:31.239
<v Speaker 4>now have a solid base, Tune in next week to

1693
01:29:31.279 --> 01:29:36.279
<v Speaker 4>hear Astro Katie address your questions, including is there a

1694
01:29:36.319 --> 01:29:39.720
<v Speaker 4>name for the disorientation and panic one feels when considering

1695
01:29:39.760 --> 01:29:42.960
<v Speaker 4>the vastness of the universe there is Are any of

1696
01:29:43.000 --> 01:29:45.720
<v Speaker 4>the sci fi movie methods to save the planet plausible?

1697
01:29:46.199 --> 01:29:49.439
<v Speaker 4>Or are we basically doomed if an asteroid uses us

1698
01:29:49.439 --> 01:29:53.479
<v Speaker 4>as a target? Will the universe expand forever? What's the

1699
01:29:53.520 --> 01:29:58.840
<v Speaker 4>deal with multiverses? Are there aliens? And speaking of your submissions,

1700
01:29:58.880 --> 01:30:01.039
<v Speaker 4>I wanted to let you know I totally see the

1701
01:30:01.079 --> 01:30:04.840
<v Speaker 4>reviews you write on iTunes and it's so appreciated. Rating

1702
01:30:04.920 --> 01:30:09.000
<v Speaker 4>and reviewing and subscribing is free, It takes very little time,

1703
01:30:09.279 --> 01:30:12.439
<v Speaker 4>and it helps ologies stay up there in the science charts,

1704
01:30:12.479 --> 01:30:15.359
<v Speaker 4>so more folks know about it. So thank you so much.

1705
01:30:16.319 --> 01:30:19.039
<v Speaker 4>Katie is at astro Katie on Twitter, where she has

1706
01:30:19.119 --> 01:30:24.479
<v Speaker 4>approximately one billion trillion followers, and she is academic Nomad

1707
01:30:24.600 --> 01:30:27.479
<v Speaker 4>on Instagram. So thank you to all you ologites for

1708
01:30:27.560 --> 01:30:30.680
<v Speaker 4>tweeting and gramming and meming at us, and to all

1709
01:30:30.680 --> 01:30:33.359
<v Speaker 4>the folks on Patreon who make the show possible. It

1710
01:30:33.439 --> 01:30:37.399
<v Speaker 4>is currently four am on a Friday night and I'm

1711
01:30:37.439 --> 01:30:39.840
<v Speaker 4>recording this to send it off to Steven ray Morris.

1712
01:30:40.159 --> 01:30:42.960
<v Speaker 4>He's going to help edit it, and your funding is

1713
01:30:43.000 --> 01:30:46.439
<v Speaker 4>making this dream project possible and putting a lot of

1714
01:30:46.479 --> 01:30:50.159
<v Speaker 4>facts in a lot of human minds. You can also

1715
01:30:50.239 --> 01:30:53.079
<v Speaker 4>keep the show going by stopping at ologiesmerch dot com.

1716
01:30:53.399 --> 01:30:58.520
<v Speaker 4>We have new pins in stock Horology clockpins and amazing

1717
01:30:58.680 --> 01:31:02.279
<v Speaker 4>shimmery bird pins for eight bucks each, designed by Shannon

1718
01:31:02.319 --> 01:31:06.199
<v Speaker 4>Feltis with merch help from Bonnie Dutch. I also want

1719
01:31:06.239 --> 01:31:08.359
<v Speaker 4>you to know that, yes, it's super late at night,

1720
01:31:08.720 --> 01:31:13.840
<v Speaker 4>and I'm recording this partly because the mass of porridge

1721
01:31:14.319 --> 01:31:17.399
<v Speaker 4>that occupies the space where a brain would be. I

1722
01:31:17.520 --> 01:31:19.920
<v Speaker 4>had to spend a little longer trying to understand and

1723
01:31:19.960 --> 01:31:23.680
<v Speaker 4>explain these concepts that I thought. And right now, as

1724
01:31:23.720 --> 01:31:26.680
<v Speaker 4>I record this middle of the night, my neighbors had

1725
01:31:26.720 --> 01:31:31.520
<v Speaker 4>been blasting techno Christmas pop songs for four hours while

1726
01:31:31.520 --> 01:31:36.239
<v Speaker 4>I was learning about wormholes. The world feels very surreal. Also,

1727
01:31:36.720 --> 01:31:39.079
<v Speaker 4>congratulations to anyone who made it to the end of

1728
01:31:39.159 --> 01:31:42.600
<v Speaker 4>this episode. Man, you stuck it out. I appreciate that.

1729
01:31:43.600 --> 01:31:45.119
<v Speaker 4>As a special thanks, I'm going to tell you a

1730
01:31:45.159 --> 01:31:48.000
<v Speaker 4>secret that no one in the world knows. Earlier tonight,

1731
01:31:48.039 --> 01:31:50.560
<v Speaker 4>I ate cereal. I bought from a gas station and

1732
01:31:50.640 --> 01:31:53.119
<v Speaker 4>I loved it. So if you listen to the end

1733
01:31:53.279 --> 01:31:55.760
<v Speaker 4>of this episode, feel free to holler at ologies or

1734
01:31:55.800 --> 01:31:58.279
<v Speaker 4>Ali Ward. I'm sure I'll have a new secret for

1735
01:31:58.319 --> 01:32:00.560
<v Speaker 4>you next week at the very end, when we are

1736
01:32:00.640 --> 01:32:04.239
<v Speaker 4>back with Katie, Max Q and A. So until then,

1737
01:32:04.439 --> 01:32:06.640
<v Speaker 4>ask smart people dumb questions because they love it and

1738
01:32:06.720 --> 01:32:10.680
<v Speaker 4>we're just tiny meat blobs on a dust spec So

1739
01:32:10.800 --> 01:32:16.880
<v Speaker 4>let's just live. Can we live? Okay? Byebye? Pacadermatology, hobbiology

1740
01:32:17.159 --> 01:32:32.800
<v Speaker 4>or do zoology, lithology, technology, meteorology and pedatology, ethology, zeriology, elenology,
