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Speaker 1: I want to start today with a bit of a

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visualization exercise. Oh okay, I know, I know. Usually we

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just jump right in, but trust me on this one.

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I want you to close your eyes unless you are driving,

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in which case, please, for the love of physics, keep

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them open. I want you to picture.

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Speaker 2: The universe, all right, I'm picturing it the void.

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Speaker 1: What do you see? What's in that void? Uh?

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Speaker 2: The usual, you know, a vast infinite blackness. Maybe some

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scattered diamond dust, which you know that represents the stars. Sure,

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maybe a spiral galaxy or two floating in the distance

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like frisbees. It's mostly empty, right, that's the main takeaway.

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Speaker 1: Right, that's the classic view, kind of random speckled darkness.

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But I want you to wipe that image away, just deleted.

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I want you to replace that majestic, silent void with something, well, something.

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Speaker 2: Uglier, uglier. I mean, how can the universe be ugly?

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Speaker 1: Oh? It can?

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Speaker 2: Yeah.

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Speaker 1: I want you to picture an orc.

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Speaker 2: An orc, an orc like from a fantasy novel, green skin,

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protruding tusks, holding a crude club, ready to rate a village.

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Speaker 1: That kind of work, exactly, that kind of ork. Because,

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according to a stunning new paper we are breaking down today.

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If you look at the structure of our specific corner

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of the universe, I mean the distribution of matter and

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the void surrounding us, and you visualize it just right,

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the universe is making a face at us, and that

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face looks like an orc.

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Speaker 2: It sounds absolutely ridiculous when you say it out loud,

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It really does. It sounds like we've completely lost our minds,

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I know. But the physics behind that image, the density

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maps that actually create that face, are incredibly serious.

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Speaker 1: And here's the kicker and the real reason we are

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doing this show today. That orc face implies that we

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are living in a cosmic sandwich.

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Speaker 2: A sandwich.

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Speaker 1: Specifically, we are living in a thin, compressed pancake of

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dark matter that is being squeezed between two massive empty voids.

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Speaker 2: It is a striking, almost claustrophobic image when you really

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think about it, and honestly, it changes the way you

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look at the right. It turns out our neighborhood, our

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entire galaxy cluster, isn't just a random suburb in space.

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It's a structural anomaly. It's a special place.

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Speaker 1: Welcome to Thrilling Threads. I'm your host, and today I

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am ready to have my perception of reality completely flattened

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like a crape.

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Speaker 2: And I'm here to help pick up the pieces and

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hopefully explain why living in a pancake might solve one

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of the biggest crises in modern physics.

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Speaker 1: We are unpacking a really fascinating and honestly kind of

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kind of troubling new paper today. It suggests that our

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place in the universe isn't just random, it's statistically weird,

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and it might force us to completely rewrite what we

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think we know about the invisible stuff that makes up

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well most of the cosmos, that.

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Speaker 2: Is the core of it. This isn't just about mapping

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where we are. It's about understanding the invisible scaffolding, the

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dark matter, the dark matter, the stuff that holds the

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universe together, or, as this paper suggests, the invisible scaffolding

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that might be oh, it might be crumbling under the

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weight of new observation.

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Speaker 1: So we have an orc, we have a pancake, and

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we have a potential crisis in the standard model of cosmology.

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Let's get into the set. Before we get to the sandwich,

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we need to talk about the ingredients, or maybe more accurately,

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the missing ingredients.

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Speaker 2: Right. To understand why this new paper is such a bombshell,

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we have to establish the baseline. For decades now, the

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dominant theory and cosmology, the gold standard has been the

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Lambda CDM model Lambda CDM.

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Speaker 1: It sounds like a fraternity for physicists. Can we break

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that acronym down quickly for everyone, just so we're all

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on the same page.

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Speaker 2: Sure, it's essentially the standard model of the Big Bang.

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Lambda represents dark energy.

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Speaker 1: The mysterious force that is accelerating the expansion of the.

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Speaker 2: Universe exactly, that's the pushing out force. And then CDM

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stands for cold.

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Speaker 1: Dark matter, cold dark matter.

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Speaker 2: Yes, the theory posits that the vast majority of matter

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in the universe is this slow moving stuff. That's the

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cold part, and it's invisible, that's the dark part. We

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call it dark matter, and that's.

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Speaker 1: The famous eighty percent figure, right or something like that.

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Speaker 2: Roughly, Yeah, The idea is that about eighty percent to

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eighty five percent of all the matter in the universe

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is this invisible substance. It has mass, so it exerts gravity,

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and it basically acts as the glue holding galaxies together.

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Speaker 1: So without it, galaxies would just fly apart.

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Speaker 2: They would if you just look at the visible matter stars,

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gas planets, you me this microphone. There isn't enough gravity

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to keep a galaxy like the Milky Way from flinging

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itself apart as it spins.

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Speaker 1: So dark matter is the safety belt at the galaxy.

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Speaker 2: It's even more fundamental than that. It's the scaffolding. Okay,

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imagine a building where you can only see the dry wall,

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but you can't see any of the steel beams. The

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dark matter is the steel beams. We assume it's there

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because well, because the building is standing up, and we

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all know drywall doesn't stand up on its own.

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Speaker 1: That is a great analogy. But and here is the

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butt that keeps me up at nine, and I know

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it bothers a lot of people in your field. We

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have never actually seen this deal beams.

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Speaker 2: We haven't, not directly, and that is the source of

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all the tension. We haven't found decisive evidence that it

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is a particle. I mean, we have built these massive detectors,

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buried them deep underground, and abandoned minds to shield them

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from cosmic radiation, like.

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Speaker 1: The lux z Plen experiment, a giant tank of xenon.

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Speaker 2: Exactly huge tanks of liquid xenon, just waiting, waiting for

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a dark matter particle to bump into one of its nuclei.

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We've smashed atoms together at the Large Hadron Collider, hoping

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to produce one and nothing. We haven't found a single

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particle that fits the description.

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Speaker 1: So it's a ghost in the machine. But I mean,

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we haven't proven it doesn't exist either.

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Speaker 2: Have we No, And that's the problem. We have no

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decisive evidence against it being a particle either. The math

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just works so well on large scales that we can't

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let it go. We are stuck in this scientific limbo,

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as the source material for Today puts it. And I

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love this quote. It's really infuriating.

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Speaker 1: I love that too. It's infuriating. You can feel the

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visceral frustration of the physicists in that line, can't you. Absolutely,

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it's not just a puzzle anymore. It's an annoyance. It's

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like looking for your keys when you know they are

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in the house, but you've torn the catch up part

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three times and they're just not there.

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Speaker 2: And you're starting to wonder if the keys ever existed

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in the first place, or if you just you know, hallucinated.

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Speaker 1: Them exactly and this is where the drama really starts

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to build, because the standard theory of dark matter, the

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one we've all been taught in school, the one on

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all the posters at the science Museum, is starting to

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feel a little bit shaky.

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Speaker 2: Shaky is a very polite way to put it.

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Speaker 1: The source goes even further. They imply that the standard

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theory is starting to feel less like hard science and

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more like a creative writing exercise.

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Speaker 2: That is a stinging critique, but it captures the mood

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in the community perfectly. We are seeing a trend where

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to keep the dark matter theory alive in the face

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of new data, we have to keep adding new rules.

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We have to keep tweaking the story.

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Speaker 1: It's like a plot hole in a movie that the

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writers try to fix with a really convoluted backstory, and

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then that creates another plot hole, so they have to

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write a prequel to explain that one precisely.

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Speaker 2: And that brings us right back to this new paper,

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because if this paper is right, we are sitting in

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a very very peculiar structural anomaly that the standard simple

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models struggle to explain naturally, not without even more creative writing.

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Speaker 1: Okay, let's get into segment one, the shape of our reality.

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I want to go back to this pancake because when

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I hear pantake, I think breakfast. But we're talking about

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a galactic scale here. What exactly is the local sheet?

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Speaker 2: So to understand this you have to know about way

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way out, way past the Milky Way. Okay, we are

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part of a group of galaxies called the local group.

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You've got Us, Andromeda a few others, and the local

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group is part of a larger structure.

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Speaker 1: A supercluster. Is that the right term?

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Speaker 2: Essentially, yes, and the paper describes our local environment. The

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technical term is the local sheet as a flat, thin

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concentration of mass. Imagine a vast, flattened region where all

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the galaxies, including the Milky Way, Andromeda, and our neighbors

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in the Virgo cluster, are all clustered together.

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Speaker 1: Why is flat weird? I mean, the Solar system is flat, right,

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the planet's orbit in a disc. Galaxies themselves are flat discs.

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Why shouldn't the cluster be flat?

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Speaker 2: That's a great question, and it's an important distinction. Solar

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systems and galaxies are flat because of angular momentum.

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Speaker 1: They're spinning.

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Speaker 2: They spin, and that spinning flattens them out like pizza do.

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But on the scale of galaxy clusters we are talking

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tens of millions of light years across. Gravity usually just

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pulls things into filaments or big spherical blob like a spun.

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Speaker 1: I've heard it called the cosmic web.

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Speaker 2: Exactly. The cosmic web usually looks like a three D

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spund or aus spider web. Finding a distinct razor thin

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sheet that extends for this enormous distance is well, it's unique.

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It implies a very specific type of compression happened.

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Speaker 1: Okay, so instead of a big round ball of galaxies

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or a scattered cloud, we are living in a cosmic

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shaitt a pancake.

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Speaker 2: Precisely, and this pancake of dark matter is sandwiched on

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either side of this flat sheet. There are two huge,

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almost void regions, bubbles of nothingness, almost empty bubbles, is

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how the source describes them. One of them is called

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the local void.

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Speaker 1: The local void that sounds like a dive bar in

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a sci fi movie.

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Speaker 2: It does, doesn't it. It's a massive region of space

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with very very few galaxies. And on the other side

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you have another underdense region, often associated with something called

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the North Polar spur.

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Speaker 1: So let me see if I have this right, you

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have this high density wall or sheet in the mirror

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axis and then just deep emptiness on both sides.

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Speaker 2: That's the picture that is.

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Speaker 1: Such a weird mental image. It's like we are living

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on a partition wall between two gigantic empty rooms, or

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like the cream filling in an oreo if the cookies

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were made of nothingness.

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Speaker 2: That is a great analogy. And the paper suggests that

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dark matter, if it exists in the way Lambda CDM

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says it does, must be strongly concentrated along this mirror axis.

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It squeezed into the pancake, leaving the bubbles empty, and this.

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Speaker 1: Is where the orc comes in. The source mentioned that

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if you look at the visualization of this structure, the

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pancake and the voids, it looks like an orc. I'm

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still trying to picture it. Are the voids the eyes.

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Speaker 2: It's a bit of a roar shot test for cosmologists,

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you know. But yes, if you look at the density

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maps from the simulation, the voids act as these large

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hollowed out eye sockets. They are dark and empty.

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Speaker 1: Okay, I can see that, and the local.

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Speaker 2: Sheet, the dense region where we live forms the bridge

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of the nose, the heavy brow ridge, and maybe the mouth.

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Speaker 1: It's funny, but it's also kind of haunting. The universe

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has a face, and it's not a friendly face. It's

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an orc.

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Speaker 2: It definitely has character. But the point the author was

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making is playful but serious. The universe isn't just a

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uniform fog. It has structure, it has distinct features, and

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we happen to live in one of the most distinct

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features of all.

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Speaker 1: And when we say we are in the pancake, we

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need to clarify we. I'm assuming we don't just mean

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Earth or the Solar System.

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Speaker 2: No, no, not just Earth, not just the Solar System, not

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even just the Milky Way galaxy. When the paper says we,

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it refers to the entire cluster of galaxies. We are

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surrounded by our whole cosmic neighborhood.

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Speaker 1: That is a massive neighborhood.

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Speaker 2: It is the scale is tens of millions of light years,

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and yet on that enormous scale, it's flat. It's a sheet.

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Speaker 1: It makes you feel kind of special, doesn't it. I mean,

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we aren't just floating in some random soup. We are

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in the pancake of destiny.

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Speaker 2: We'll hold that thought on destiny because usually in cosmology,

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if you find yourself in a special place, that is

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a massive red flag.

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Speaker 1: Why everyone wants to be special. My mom told me

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I was special.

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Speaker 2: Your mom is definitely right. But in physics, special is

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a problem. We rely on something called Copernican.

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Speaker 1: Principle, the idea that we are not the center of

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the universe.

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Speaker 2: Right, we are not in a privileged position. The universe

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should look roughly the same no matter where you are standing.

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That's a core assumption called homogeneity.

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Speaker 1: So if the universe is supposed to be the same everywhere,

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finding ourselves in this highly specific odd structure that looks

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like an orc, well, it raises some mybrows.

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Speaker 2: Exactly. It suggests that maybe our local patch of the

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universe is violating the standard rules, or perhaps more disturbingly,

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that the standard rules don't actually predict what we see around.

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Speaker 1: Us, which is a perfect segue. Okay, so we are

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in an orc shaped dark matter sandwich. That's the one.

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Now I want to get into the why this is

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a problem. This brings us to segment two, the trouble

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with dark matter. You mentioned earlier that the theory is

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becoming a creative writing exercise, let's uttack that what exactly

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is going wrong with the theory.

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Speaker 2: This is where we have to look at the track

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record of the dark matter theory over the last decade

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or so. The issue is that the observations what we

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actually see through a telescopes keep contradicting what the dark

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matter computer models predict.

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Speaker 1: And every time that happens, the theorists have to go

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back and fix the model.

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Speaker 2: Right, and in science, you want a theory that predicts things,

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not a theory that you have to constant patch up

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after the fact. If you have to keep adding what

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we call epicycles, extra little distinct rules to make it work.

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Eventually you have to ask if the core theory is flawed.

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Speaker 1: Okay, give me a concrete example. What's the first big anomaly.

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Speaker 2: Let's talk about galactic cores. This is often called the

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cusp core problem.

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Speaker 1: The cusp core problem sounds pointy. Lay it on me

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in plain English.

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Speaker 2: Standard cold dark matter theory is very very clear on

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how gravity works. It predicts that dark matter should clump

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effectively in the center of galaxies. It should get very

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very dense in the middle. We call this a cusp.

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A cusp think of it like a sharp mountain peak

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of density.

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Speaker 1: So if we could see dark matter, there should be

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a big, bright, well invitible ball of heavy stuff right

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in the middle of the Milky Way, a sharp.

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Speaker 2: Spike, correct a very sharp spike in density. But when

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we observe the way stars and gas move near the

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centers of galaxies, we don't see evidence for that sharp spike.

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Speaker 1: What do we see instead?

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Speaker 2: The observation suggest the core is much smoother. It's flat.

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It's a core, not a cusp. Imagine a flat plateau

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instead of a mountain peak. The dark matter seems to

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be spread out evenly, not clumped up in the middle.

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Speaker 1: So the map doesn't match the territory. Yeah, the theory

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says mountain, and the telescope says plateau exactly.

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Speaker 2: So what do the theorists do. They don't throw out

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the theory, of course not. They tweak the model. They

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introduce what they call baryonic feedback.

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Speaker 1: Buryonic feedback. That sounds suspiciously technical.

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Speaker 2: It's a fancy way of saying supernova's. They say, well,

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maybe supernova explosions in the center of the galaxy push

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the dark matter out, or maybe there's some complex feedback

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mechanism between gas and dark matter that smoothed out the bump.

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Speaker 1: Is that plausible? I mean, could that actually.

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Speaker 2: Happen physically possible? Supernovas are incredibly powerful, but you have

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to fine tune the math just right to make it

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happen in every galaxy we see. As the source says,

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one can make that work, but it feels forced.

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Speaker 1: One can make that work. Yeah, it sounds like when

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I'm trying to to fix a waterly table and I

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just keep shoving folded paper under the leg until it

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stops moving. It works, but it's not exactly elegant engineering.

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Speaker 2: That is a distressingly accurate analogy. You're patching the theory

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and it happens again with satellite galaxies. Okay, this is

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the missing satellites problem.

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Speaker 1: I've heard of this. This is about the little, tiny

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galaxies that orbit big ones like ours.

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Speaker 2: Yes, the dark matter simulations predict that large galaxies like

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our Milky Way should be surrounded by hundreds, potentially thousands,

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of smaller clumps of dark matter, each one hosting a

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tiny dwarf galaxy like.

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Speaker 1: A swarm of bees around a hive.

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Speaker 2: Exactly because the dark matter is messy, right, it should

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break off into little chunks. Gravity is fractal in these simulations.

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It makes big clumps and little clumps. The simulation says, look.

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Speaker 1: For the swarm, and whether we see a swarm.

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Speaker 2: We see a few. We have the Magellanic clouds, which

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are beautiful, and we've found a handful of other ultra

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faint dwarfs. But we don't see hundreds. We see vastly,

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vastly fewer. And the theory.

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Speaker 1: Predicts so the swarm is missing. Where did they go?

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Speaker 2: That's the multi billion dollar question? So how do they

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make that work?

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Speaker 1: Let me guess they adjust the model again.

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Speaker 2: They adjust the model. They say, well, maybe the small

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clumps of dark matter exist, but they just didn't manage

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to attract enough gas to form stars. So the clumps

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are there, but they are invisible. They are dark galaxies.

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Speaker 1: That feels incredibly convenient. The invisible stuff is there, it's

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just doubly invisible now because it didn't light up.

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Speaker 2: It protects the theory from being falsified. If you can

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always claim the missing evidence is just too faint to see,

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you can never really be proven wrong.

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Speaker 1: You see the pattern, one can make that work.

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Speaker 2: And then there's the big one. The new kid on

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the block, A not only number three courtesy of the

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James Webb Space Telescope.

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Speaker 1: The Early Universe. I remember the headlines when JWST started

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sending back those first pictures. People were freaking out.

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Speaker 2: They were right to freak out, because under the standard

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dark matter model, galaxies build up slowly. It's a bottom

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up process, right. Gravity takes time to pull things together.

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You start small and messy, and over billions of years

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you get big, structured galaxies, slow and.

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Speaker 1: Stead He wins the race. You don't get a skyscraper

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five minutes after you break around.

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Speaker 2: That was the prediction. But JWST looked back at the

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very early universe. We're talking red shifts of ten or eleven,

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almost right after the Big Bang cosmologically speaking, and what

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did it find?

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Speaker 1: Big galaxies, huge fully.

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Speaker 2: Formed, bright galaxies, some of them massive enough to rival

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our own Milky Way, but existing at a time when

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the universe was just in its infancy.

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Speaker 1: It's like walking into a nursery and finding a newborn

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baby who was already six feet tall, wearing a suit

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and trading stocks.

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Speaker 2: A perfect analogy. It completely defies the developmental timeline we

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expected the universe shouldn't have been able to organize itself

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that quickly if it was relying on the slow, steady

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trickle of cold dark matter gravity.

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Speaker 1: And what was the response? Did they scrap the theory?

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Speaker 2: Oh? They said, well, maybe star formation was just more

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efficient back then, or maybe our calibration was off, maybe

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the dust obscures the real mass. They find a way

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to keep the dark matter framework, but they have to

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bend it into a pretzel to make it fit, and.

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Speaker 1: That's why the source calls it a creative writing exercise.

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Speaker 2: Yes, the critique is this, at what point does a

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theory stop being predictive and start being merely reactive? If

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you have to modify the story after every single new discovery,

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are you actually explaining the universe or are you just

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describing it after the fact.

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Speaker 1: That is a savage burn on the physics community. But

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I mean, given the list you just gave, it feels

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kind of justified.

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Speaker 2: It is a valid scientific concern. Science is supposed to

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be about falsifiability. You have to be able to be

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proven wrong. If your theory acts like a chameleon and

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changes color to match whatever background you put it against,

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it's not a very useful theory anymore.

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Speaker 1: Which brings us back to the pancake, because this new

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paper is essentially saying, Okay, if you want to keep

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the standard model, if you want to keep LAMB to CDM,

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here is the extremely weird shape you have to accept

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we live in.

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Speaker 2: Right. They are testing the limits of the model by

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looking at our local address in the cosmos.

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Speaker 1: Okay, let's move to segment three. How did they find it?

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Because we've established pretty clearly that dark matter is invisible,

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So how do these researchers know we're in a pancake

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between two voids? Did they just look at the stars

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and guess?

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Speaker 2: No guessing involved. They used a very sophisticated tool called

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structure simulation models. Specifically, they used a technique called constrained realizations.

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Speaker 1: Okay, break that down for me. Constrained realizations. That sounds

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like a therapy technique. I had a constrained realization about

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my childhood.

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Speaker 2: Today, Doc, It does, doesn't it? But in physics it

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means running a simulation that isn't random. Oka. Usually when

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cosmologists simulate the universe, they just throw in some random

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initial conditions, press play and see what kind of universe

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pops out. They get a generic universe.

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Speaker 1: A generic universe like buying a universe starter pack from

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a store exactly.

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Speaker 2: But that doesn't help us understand our specific neighborhood. So

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these researchers did something different. They started with the standard

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cosmological model Lambda CDM, but they added.

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Speaker 1: Constraints, constraints, what kind of constraints.

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Speaker 2: They forced the simulation to match the actual position of

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the galaxies we see in the sky today. They basically said, okay, computer,

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simulate a universe from the Big Bang forward. But at

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the end of the simulation, the Milky Way must be here,

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Andromeda must be over there, and the Virgo cluster must

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be in that exact spot.

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Speaker 1: So they rigged the game. They started with the answer.

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Speaker 2: In a way, Yes, they rigged it to match reality.

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They reverse engineered the Big Bang. They asked the question,

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what must the initial conditions have been, and more importantly,

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where must the unseen dark matter be today to produce

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this specific arrangement of visible galaxies that we observe.

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Speaker 1: Ah, I see so because the galaxies are just the

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tip of the iceberg. They're like the lights on the

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Christmas tree. If you know exactly where all the lights are,

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you can figure out the shape of the invisible branches

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holding them up exactly.

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Speaker 2: That is the perfect metaphoras. Galaxies are the tracers. They

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follow the gravitational pull of the dark matter. So if

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you see a sheet of galaxies, the computer deduces that

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there must be a sheet of dark matter holding them there.

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Speaker 1: And they didn't just run this once.

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Speaker 2: Oh no, they ran it thousands of times. They created

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thousands of potential universes that all ended up looking exactly

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like our local neighborhood in terms of the visible matter.

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Speaker 1: And what was the common denominator? What did they all

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have in common?

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Speaker 2: In every single simulation that matched our visible reality, the

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underlying dark matter structure was the same. It was that

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specific pancake shape with the two massive voids on either side.

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Speaker 1: WHOA. So they didn't just see the pancake. They deduced

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that the pancake must be there for our reality to

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make sense under the current rules.

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Speaker 2: Exactly. There was no other way to get the visible

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result without that specific invisible structure To explain why our

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galaxies are arranged the way they are. The dark matter

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has to be squeezed into this thin sheet between empty bubbles.

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Speaker 1: So it's not just a pretty pick or a funny

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orc face. It's a mathematical necessity of the LAMB to

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CDM model when you apply it to our specific location.

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Speaker 2: Correct. If the standard model is true, then the orc

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is real.

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Speaker 1: That's incredibly cool and also incredibly weird, which leads us

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00:22:15,920 --> 00:22:20,440
to segment four, the odds and the significance. Is this normal?

471
00:22:20,880 --> 00:22:24,480
Are their cosmic pancakes everywhere? Or are we the odd

472
00:22:24,480 --> 00:22:25,000
ones out?

473
00:22:25,200 --> 00:22:28,039
Speaker 2: That is the big question. How rare is a cosmic work?

474
00:22:28,240 --> 00:22:31,279
Speaker 1: I'm guessing pretty rare. I mean orcs in fantasy usually

475
00:22:31,319 --> 00:22:35,279
travel in hordes, but maybe cosmic orcs are solitary creatures.

476
00:22:35,359 --> 00:22:37,559
Speaker 2: The paper tries to quantify this. They looked at how

477
00:22:37,599 --> 00:22:41,559
often structures like our local sheet and these specific voids

478
00:22:41,640 --> 00:22:45,799
appear in those generic random universe simulations we talked about earlier.

479
00:22:45,920 --> 00:22:48,119
Speaker 1: Okay, lay the stance on me. How special are we?

480
00:22:48,319 --> 00:22:50,839
Speaker 2: Earlier estimates and these are from studies looking at similar

481
00:22:50,880 --> 00:22:53,759
structures put the probability of finding ourselves in such a

482
00:22:53,759 --> 00:22:56,559
spot at somewhere between two point five and three point

483
00:22:56,559 --> 00:22:57,400
three sigma.

484
00:22:57,799 --> 00:23:00,680
Speaker 1: Okay, speak English, professor, what is this sigma? I know

485
00:23:00,680 --> 00:23:02,359
it's a Greek letter, but what does it mean in

486
00:23:02,400 --> 00:23:03,279
this context?

487
00:23:03,680 --> 00:23:07,039
Speaker 2: Sigma is a measure of statistical significance. It tells you

488
00:23:07,119 --> 00:23:09,960
how far away a result is from the average from

489
00:23:10,000 --> 00:23:13,799
what's normal. In this context, one sigma is like flipping

490
00:23:13,839 --> 00:23:15,160
a coin and getting heads.

491
00:23:15,160 --> 00:23:16,519
Speaker 1: Totally normal happens all the.

492
00:23:16,440 --> 00:23:20,640
Speaker 2: Time, exactly. Five sigma is the gold standard in particle physics.

493
00:23:20,680 --> 00:23:24,039
For a discovery that's winning the lottery, it's basically considered proof.

494
00:23:24,319 --> 00:23:27,000
Speaker 1: And two point five to three point three sigma where

495
00:23:27,039 --> 00:23:27,640
does that land?

496
00:23:28,039 --> 00:23:30,599
Speaker 2: That translates roughly to a one in one hundred to

497
00:23:30,640 --> 00:23:32,119
a one in one thousand chance.

498
00:23:32,319 --> 00:23:34,440
Speaker 1: So if I have a bag of a thousand universes,

499
00:23:34,640 --> 00:23:37,160
only one of them has us living in this specific

500
00:23:37,319 --> 00:23:38,079
orc sandwich.

501
00:23:38,359 --> 00:23:40,400
Speaker 2: Roughly, Yes, that's the idea.

502
00:23:40,519 --> 00:23:43,519
Speaker 1: That feels rare, but it's not impossible. It's not one in.

503
00:23:43,480 --> 00:23:47,119
Speaker 2: A billion exactly. It's what we call statistically significant but

504
00:23:47,200 --> 00:23:51,359
not impossible. It's in that uncomfortable middle ground. It's just

505
00:23:51,559 --> 00:23:53,519
rare enough to make you wonder if something else is

506
00:23:53,559 --> 00:23:56,279
going on, but not rare enough to completely disprove the

507
00:23:56,279 --> 00:23:57,119
theory on its own.

508
00:23:57,200 --> 00:23:58,920
Speaker 1: It's like winning a raffle at a school for that

509
00:23:58,920 --> 00:24:02,160
you didn't even know you entered. It happens, but you're

510
00:24:02,200 --> 00:24:03,000
pretty surprised.

511
00:24:03,119 --> 00:24:06,200
Speaker 2: Yes, and this brings us to the bullshit meter.

512
00:24:06,680 --> 00:24:09,160
Speaker 1: I love that the source used a bullshit meter. We

513
00:24:09,240 --> 00:24:11,680
need more of those in science. So what was the

514
00:24:11,720 --> 00:24:12,759
score for this paper?

515
00:24:13,440 --> 00:24:14,599
Speaker 2: She gave it a one out of ten?

516
00:24:14,920 --> 00:24:16,599
Speaker 1: Wait, one is low rate or is one high?

517
00:24:16,759 --> 00:24:20,079
Speaker 2: One is very low bullshit? A ten would be total nonsense.

518
00:24:20,119 --> 00:24:22,359
A one means this is solid science.

519
00:24:23,000 --> 00:24:26,119
Speaker 1: Okay. So despite the weird ORC imagery and the strange result,

520
00:24:26,480 --> 00:24:28,440
the methodology behind it is sound.

521
00:24:29,079 --> 00:24:31,880
Speaker 2: It is, but she noted a limitation, which is why

522
00:24:31,920 --> 00:24:34,079
she gave it a one and not a perfect zero.

523
00:24:34,680 --> 00:24:38,720
She can't personally judge the computer simulations. These codes are

524
00:24:38,759 --> 00:24:42,119
incredibly complex, written by teams over years. You have to

525
00:24:42,160 --> 00:24:44,920
trust that the researcher set up the simulation correctly.

526
00:24:45,039 --> 00:24:47,880
Speaker 1: Trust but verify the old motto exactly.

527
00:24:48,160 --> 00:24:51,160
Speaker 2: And she had one other minor annoyance. Oh, the paper

528
00:24:51,279 --> 00:24:55,240
didn't calculate the exact probability for their specific new model.

529
00:24:55,599 --> 00:24:58,440
They relied on those earlier two point five to three

530
00:24:58,519 --> 00:25:01,640
point three sigma estimates from previous studies. She wanted them

531
00:25:01,680 --> 00:25:04,279
to run the numbers fresh for this particular.

532
00:25:03,880 --> 00:25:05,839
Speaker 1: ORC, so we know it's rare, but we don't know

533
00:25:05,880 --> 00:25:09,920
exactly how rare this specific pancake orc situation is correct.

534
00:25:10,160 --> 00:25:12,720
Speaker 2: Hopefully another team will run the numbers soon and give

535
00:25:12,799 --> 00:25:17,279
us a precise figure. But the qualitative result stands we

536
00:25:17,359 --> 00:25:19,839
live in a rare squeezed environment.

537
00:25:20,079 --> 00:25:23,079
Speaker 1: So let's get to segment five, the bigger picture, the

538
00:25:23,119 --> 00:25:26,279
so what question? Why does it matter that I live

539
00:25:26,319 --> 00:25:29,200
in a pancake? I mean, my rent is still the same,

540
00:25:29,279 --> 00:25:32,160
my coffee still tastes the same this morning. Why should

541
00:25:32,200 --> 00:25:34,240
the average listener care about the local sheet?

542
00:25:34,480 --> 00:25:37,039
Speaker 2: It matters because it connects right back to that creative

543
00:25:37,079 --> 00:25:40,440
writing problem we discussed. The more we try to fit

544
00:25:40,480 --> 00:25:44,440
our observations to the standard dark matter model, the weirder

545
00:25:44,480 --> 00:25:46,759
and more special our local environment appears to be.

546
00:25:47,000 --> 00:25:50,240
Speaker 1: It's imagine you have a suit that doesn't fit. You

547
00:25:50,279 --> 00:25:52,000
can tailor it, you can tuck it, you can pin

548
00:25:52,079 --> 00:25:53,960
it here and there, but eventually you look in the

549
00:25:54,000 --> 00:25:57,079
mirror and you just look ridiculous. The proportions are all wrong, And.

550
00:25:57,079 --> 00:25:59,480
Speaker 2: At that point you have to ask yourself a fundamental question,

551
00:25:59,720 --> 00:26:02,160
is my body weird? Or is the suit just the

552
00:26:02,160 --> 00:26:02,799
wrong size?

553
00:26:02,920 --> 00:26:04,599
Speaker 1: Or maybe it's the wrong suit entirely.

554
00:26:04,759 --> 00:26:07,000
Speaker 2: That is the philosophical point at the heart of this

555
00:26:07,319 --> 00:26:10,319
is the universe naturally weird and we just happen to

556
00:26:10,400 --> 00:26:13,200
land in a one in one thousand spot by sheer luck.

557
00:26:13,839 --> 00:26:17,440
Or is our theory of dark matter wrong? The source

558
00:26:17,480 --> 00:26:19,640
suggests that we might be missing something.

559
00:26:19,400 --> 00:26:22,920
Speaker 1: Big, something big, like maybe dark matter isn't a particle

560
00:26:22,920 --> 00:26:23,319
at all.

561
00:26:23,559 --> 00:26:27,839
Speaker 2: That is the leading alternative. There are theories like MOND,

562
00:26:28,079 --> 00:26:31,720
which stands for modified Newtonian dynamics, that suggest we don't

563
00:26:31,759 --> 00:26:34,920
need invisible matter, we just need to tweak our understanding

564
00:26:34,920 --> 00:26:36,200
of gravity itself.

565
00:26:36,440 --> 00:26:39,480
Speaker 1: So maybe gravity just works differently on really big scales,

566
00:26:39,559 --> 00:26:42,720
like how boiling water behaves differently than a single water

567
00:26:42,799 --> 00:26:44,039
molecule exactly.

568
00:26:44,079 --> 00:26:45,880
Speaker 2: And if you change the laws of gravity, maybe this

569
00:26:46,000 --> 00:26:49,319
pancake structure isn't an anomaly anymore. Maybe it's exactly what

570
00:26:49,359 --> 00:26:50,400
you'd expect to see.

571
00:26:50,599 --> 00:26:53,319
Speaker 1: Well, that would certainly solve the creative writing problem. You

572
00:26:53,359 --> 00:26:57,440
wouldn't need to invent invisible galaxies or use supernovas to

573
00:26:57,519 --> 00:26:59,559
push matter around to explain things.

574
00:27:00,519 --> 00:27:03,039
Speaker 2: But mon D has its own set of problems. It's

575
00:27:03,039 --> 00:27:05,960
not a perfect fix either. It really struggles to explain

576
00:27:06,000 --> 00:27:10,160
the cosmic microwave background radiation, for instance, But the tension

577
00:27:10,200 --> 00:27:13,920
between these ideas is leading us somewhere new. And you

578
00:27:13,960 --> 00:27:16,359
mentioned quantum gravity before. How does that fit in?

579
00:27:16,559 --> 00:27:18,519
Speaker 1: Yes, the holy grail of physics.

580
00:27:18,599 --> 00:27:21,279
Speaker 2: That is the ultimate prize. Right now, we have two

581
00:27:21,319 --> 00:27:24,799
different rule books for the universe. We have general relativity,

582
00:27:24,839 --> 00:27:28,720
which handles big stuff like gravity, pancakes, and galaxies, and

583
00:27:28,759 --> 00:27:31,440
we have quantum mechanics, which handles the tiny stuff like

584
00:27:31,559 --> 00:27:33,640
atoms and subatomic particle And.

585
00:27:33,599 --> 00:27:35,440
Speaker 1: They don't get along at all.

586
00:27:35,559 --> 00:27:38,640
Speaker 2: They hate each other, they don't mathematically work together. We

587
00:27:38,720 --> 00:27:42,279
are desperately searching for a theory of quantum gravity, the

588
00:27:42,319 --> 00:27:43,880
one single theory that.

589
00:27:43,960 --> 00:27:46,839
Speaker 1: Unifies them, and solving the dark matter mystery can help

590
00:27:46,920 --> 00:27:47,400
us find it.

591
00:27:48,000 --> 00:27:51,799
Speaker 2: The source argues that, yes, absolutely, if we finally solve

592
00:27:51,839 --> 00:27:54,200
the riddle of dark matter, why the universe looks like

593
00:27:54,200 --> 00:27:56,960
an orc, why the galaxy is spin too fast, it

594
00:27:57,000 --> 00:27:59,440
won't just tell us what the invisible stuff is. It

595
00:27:59,519 --> 00:28:01,440
might give us it's the crucial clue we need to

596
00:28:01,519 --> 00:28:04,119
understand the fundamental nature of quantum gravity.

597
00:28:04,160 --> 00:28:05,759
Speaker 1: It's a two for one deal, two.

598
00:28:05,759 --> 00:28:09,039
Speaker 2: Unsolved mysteries for the price of one. If dark matter

599
00:28:09,119 --> 00:28:11,799
turns out to be a misunderstanding of how gravity works

600
00:28:11,839 --> 00:28:15,000
on a quantum level, it might reveal the bridge between

601
00:28:15,039 --> 00:28:17,519
the quantum world and the cosmic world.

602
00:28:17,680 --> 00:28:21,720
Speaker 1: I love that it turns this frustration, this infuriating creative

603
00:28:21,720 --> 00:28:25,680
writing exercise, into a massive opportunity. The fact that the

604
00:28:25,720 --> 00:28:29,039
model is breaking isn't a failure. It's actually good news.

605
00:28:29,759 --> 00:28:32,680
It means we are about to learn something profound.

606
00:28:32,920 --> 00:28:34,519
Speaker 2: That is the best way to look at it. The

607
00:28:34,559 --> 00:28:38,240
anomalies aren't failures, they are clues. The orc is a clue.

608
00:28:38,400 --> 00:28:40,559
Speaker 1: All right, let's wrap this up. This has been a

609
00:28:40,599 --> 00:28:43,599
wild ride. We started with an orc, moved to a pancake,

610
00:28:43,839 --> 00:28:46,599
realized our scientific model is held together by tape and

611
00:28:46,680 --> 00:28:49,279
creative writing, and we ended up at the holy grail

612
00:28:49,319 --> 00:28:49,799
of physics.

613
00:28:49,839 --> 00:28:51,759
Speaker 2: Just a typical Tuesday and cosmology.

614
00:28:52,160 --> 00:28:54,480
Speaker 1: But there's something really beautiful about it, isn't there. The

615
00:28:54,519 --> 00:28:57,359
source had this lovely reflection at the end of her analysis.

616
00:28:57,720 --> 00:29:00,680
Speaker 2: Yes, it's so easy to get lost and the math

617
00:29:00,799 --> 00:29:03,279
and the sigmas and all the jargon. But if you

618
00:29:03,279 --> 00:29:06,440
step back for a moment, everything we talked about today,

619
00:29:06,519 --> 00:29:10,640
the voids, the pancake, the galaxies, the orc, it all

620
00:29:10,759 --> 00:29:15,480
formed from minuscule quantum fluctuations over billions and billions of.

621
00:29:15,519 --> 00:29:19,160
Speaker 1: Years, Tiny little jitters in the energy of the early universe.

622
00:29:19,319 --> 00:29:24,519
Speaker 2: Tiny jitters, literally random quantum noise that gravity amplified into

623
00:29:24,559 --> 00:29:28,039
the massive cosmic structures we see today. As the host said,

624
00:29:28,079 --> 00:29:29,839
if you ever feel let down by the world, just

625
00:29:29,920 --> 00:29:33,880
remember it's all just quantum fluctuations that evolved into little

626
00:29:33,960 --> 00:29:36,000
human beings crawling around on planets.

627
00:29:36,160 --> 00:29:39,200
Speaker 1: That is weirdly comforting. I'm just a highly organized quantum

628
00:29:39,240 --> 00:29:41,160
fluctuation with a podcast.

629
00:29:40,720 --> 00:29:42,799
Speaker 2: And really the only thing to blame for all of this,

630
00:29:43,000 --> 00:29:45,559
the mess, the mystery, the ork is physics.

631
00:29:45,680 --> 00:29:47,480
Speaker 1: Blame physics. I'm going to use that next time I

632
00:29:47,559 --> 00:29:49,839
relate for a meeting. Sorry, physics made the universe weird

633
00:29:49,839 --> 00:29:51,279
and I got got in the local sheet.

634
00:29:51,440 --> 00:29:53,519
Speaker 2: It might not hold up in court, but it is

635
00:29:53,720 --> 00:29:55,880
on a fundamental level, technically true.

636
00:29:56,000 --> 00:30:00,359
Speaker 1: So here is the summary of today's thrilling thread. We

637
00:30:00,400 --> 00:30:03,799
are very likely living in a dark matter pancake sandwich

638
00:30:03,839 --> 00:30:08,039
between two giant voids. The theory we use to explain

639
00:30:08,160 --> 00:30:12,200
this is struggling to keep up with reality, requiring more

640
00:30:12,240 --> 00:30:15,559
and more creative writing to make sense. And the universe

641
00:30:15,640 --> 00:30:18,720
is wonderfully, stubbornly beautifully strange.

642
00:30:18,880 --> 00:30:19,960
Speaker 2: A perfect summary.

643
00:30:20,119 --> 00:30:21,839
Speaker 1: Now I want to turn this over to you, the listener.

644
00:30:22,200 --> 00:30:25,200
We've presented the evidence, we've shown you the fixes and

645
00:30:25,279 --> 00:30:28,519
the patches the scientists are making to the theory. So

646
00:30:28,640 --> 00:30:29,279
what do you think?

647
00:30:29,440 --> 00:30:31,920
Speaker 2: Yes, that is the real question. Do you think the

648
00:30:32,039 --> 00:30:34,799
dark matter model is just going through some growing pains

649
00:30:34,880 --> 00:30:37,079
and we'll eventually find that particle in a lab and

650
00:30:37,119 --> 00:30:38,920
it will all make sense. Or is it time to

651
00:30:39,000 --> 00:30:40,039
scrap it?

652
00:30:40,079 --> 00:30:42,599
Speaker 1: Is it time to burn the creative writing, the manuscript

653
00:30:42,599 --> 00:30:44,480
and start a new book. Are we missing something big?

654
00:30:44,640 --> 00:30:47,920
Speaker 2: It is the biggest question in modern science, and honestly,

655
00:30:48,079 --> 00:30:50,279
right now your guess is as good as ours.

656
00:30:50,440 --> 00:30:51,880
Speaker 1: Leave a comment let us know where you stand. Are

657
00:30:51,960 --> 00:30:54,599
you team dark matter or are you on team something new.

658
00:30:55,000 --> 00:30:57,400
Speaker 2: I'm very curious to see what people think about this one.

659
00:30:57,599 --> 00:31:00,839
Speaker 1: Me too. As always, thank you for joining us on

660
00:31:00,880 --> 00:31:04,880
this journey through the cosmos. Keep looking up and watch out.

661
00:31:04,720 --> 00:31:06,480
Speaker 2: For the orcs and mind the voids.

662
00:31:06,599 --> 00:31:08,640
Speaker 1: This has been thrilling threads. See you next time.

