WEBVTT

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<v Speaker 1>Welcome to Bedtime Astronomy. Explore the wonders of the cosmos

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<v Speaker 1>with our soothing Bedtime Astronomie podcast. Each episode offers a

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<v Speaker 1>gentle journey through the stars, planets, and beyond, perfect for

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<v Speaker 1>unwinding after a long day. Let's travel through the mysteries

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<v Speaker 1>of the universe as you drift off into a peaceful

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<v Speaker 1>slumber under the night sky.

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<v Speaker 2>Imagine for a second you're driving down this long, flat

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<v Speaker 2>stretch of highway, you know, the kind where you can

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<v Speaker 2>just see for miles totally clear day. You're cruising along

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<v Speaker 2>and you pass a police car parked on the shoulder.

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<v Speaker 2>The officer points a radar gun at you clocks your speed.

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<v Speaker 3>I think most of us have felt that specific spike

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<v Speaker 3>of adrenalist.

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<v Speaker 2>Absolutely. But then a mile down the road there's another

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<v Speaker 2>police officer, also an expert, also holding a state of

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<v Speaker 2>the art, perfectly calibrated radar gun, and he clocks you too. Okay, Now,

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<v Speaker 2>imagine both of these officers are the best in the business.

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<v Speaker 2>Their equipment is flawless, They technically never make mistakes. But

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<v Speaker 2>a week later you get the ticket. The first officer

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<v Speaker 2>says you were going seventy three miles per hour. Right,

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<v Speaker 2>the second officer says you were going sixty seven miles

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<v Speaker 2>per hour.

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<v Speaker 3>That is a very confusing court date.

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<v Speaker 2>Right, who do you believe? They're both experts. They're using

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<v Speaker 2>top gear technology to measure the exact same event, your

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<v Speaker 2>car moving, but the numbers don't match.

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<v Speaker 3>In our world, you'd probably blame it on a faulty battery.

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<v Speaker 2>Or something exactly. But in astrophysics, this isn't about a

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<v Speaker 2>speeding ticket. It's about the speed of the universe itself,

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<v Speaker 2>and this discrepancy it is, and this is not an exaggeration,

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<v Speaker 2>the single biggest headache in modern cosmology.

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<v Speaker 3>You were referring to the hubble tension. Yeah, and you're

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<v Speaker 3>right to frame it as a headache. It's it's really

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<v Speaker 3>more of a crisis. We aren't talking about a car.

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<v Speaker 3>We're talking about the fabric of space.

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<v Speaker 2>Expanding, the universe getting bigger, and.

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<v Speaker 3>We have two very different, very precise ways of measuring

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<v Speaker 3>that exp ancient and for the last decade they have

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<v Speaker 3>just refused to agree.

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<v Speaker 2>It's the cosmic speed trap. And usually when we talk

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<v Speaker 2>about this, the solutions people propose are I mean, they're

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<v Speaker 2>incredibly wild.

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<v Speaker 3>Oh yeah, you get into some really high concept stuff.

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<v Speaker 2>People start talking about dark energy changing over time or

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<v Speaker 2>gravity leaking into other dimensions. But today we're looking at

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<v Speaker 2>a new contender. A new paper just dropped literally today

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<v Speaker 2>February fifteenth, twenty twenty six, that suggests the answer isn't

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<v Speaker 2>some new phantom force. It might be something, well, something

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<v Speaker 2>surprisingly domestic.

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<v Speaker 3>Domestic is an interesting word for it, considering the scale.

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<v Speaker 3>But yes, the fundamental force is certainly something you encounter

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<v Speaker 3>in your kitchen every day.

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<v Speaker 2>We were talking about magnetism. The same force that holds your

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<v Speaker 2>grocery list to the fridge might just be the key

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<v Speaker 2>to fixing the biggest broken number in physics.

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<v Speaker 3>Although to be fair, the magnets we're discussing today are

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<v Speaker 3>a little different than a fridge magnet. We're talking about

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<v Speaker 3>primordial magnetic fields.

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<v Speaker 2>Primordial, so ancient.

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<v Speaker 3>Incredibly ancient. These are invisible fields that were generated mere

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<v Speaker 3>milliseconds after the Big Bang, and we think stretch across

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<v Speaker 3>the entire cosmos.

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<v Speaker 2>So on today's deep dive, we are going to look

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<v Speaker 2>at why the universe's speedometers seems broken. We're going to

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<v Speaker 2>unpack this new paper by researchers Pagosian, Jadamziic and Abel

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<v Speaker 2>we'll find out what a peicogus.

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<v Speaker 3>Is, and why clumping is the technical.

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<v Speaker 2>Term you need to know, and how these invisible magnetic

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<v Speaker 2>webs might be the bridge between two numbers that just

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<v Speaker 2>won't play nice.

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<v Speaker 3>And I think this is the most exciting part. We're

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<v Speaker 3>going to explore how this research doesn't just fix a

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<v Speaker 3>math problem. It potentially opens a window into high energy

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<v Speaker 3>physics that we could never ever hope to replicate in

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<v Speaker 3>a lab on.

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<v Speaker 2>Earth, using the universe as its own particle collider precisely. Okay,

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<v Speaker 2>let's unpack this. We have to start with the problem itself,

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<v Speaker 2>the Hubble tension. I feel like we hear this term

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<v Speaker 2>a lot, but let's really drill down. It all starts

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<v Speaker 2>with Edwin Hubble, doesn't.

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<v Speaker 3>It does. You have to go back to thenineteen twenties,

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<v Speaker 3>before Hubble, the scientific consensus was that the universe was static.

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<v Speaker 3>It was just there, eternal, unchanging.

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<v Speaker 2>The way it is now is the way it's always

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<v Speaker 2>been exactly.

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<v Speaker 3>But Hubble pointed his telescope at the night sky and

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<v Speaker 3>just fundamentally shattered that view of reality. He showed that

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<v Speaker 3>the universe is actually getting bigger. Galaxies are moving away

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<v Speaker 3>from us.

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<v Speaker 2>And it wasn't just random movement, right. There was a

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<v Speaker 2>distinct pattern to it.

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<v Speaker 3>Very clear pattern. He found that the farther away a

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<v Speaker 3>galaxy is the faster it's receding from us. It's the

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<v Speaker 3>classic analogy of dots on.

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<v Speaker 2>A balloon, right as you inflate it.

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<v Speaker 3>As you inflate the balloon, every dot moves away from

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<v Speaker 3>every other dot. But the dots that start further apart

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<v Speaker 3>seem to move away from each other much faster because

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<v Speaker 3>there's just more balloon expanding between them.

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<v Speaker 2>And that rate of recession, that specific relationship between speed

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<v Speaker 2>and distance, that's the Hubble constant.

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<v Speaker 3>Correct, it's the fundamental expansion rate of the cosmos. Now,

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<v Speaker 3>the units we used to measure it are a bit

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<v Speaker 3>of a mouthful kilometers per second per megaparsec.

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<v Speaker 2>Okay, hold on, let's break that down per second. That's easy,

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<v Speaker 2>that's just speed. But per megaparsec. What on Earth is

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<v Speaker 2>a megaparsec?

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<v Speaker 3>Right, Let's build up to it. So, a parsek is

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<v Speaker 3>a unit of distance we use in astronomy. One parsek

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<v Speaker 3>is about three point twenty six light years.

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<v Speaker 2>Which is already an incomprehensibly huge distance.

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<v Speaker 3>Massive, but a megaparsek is one million parsecs.

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<v Speaker 2>So we are talking about a distance of roughly three

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<v Speaker 2>point twenty six million light years.

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<v Speaker 3>That's the one. So we say the Hubble constant is,

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<v Speaker 3>for example, seventy kilometers mpc. It means that for every

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<v Speaker 3>megaparsek you go further out into space.

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<v Speaker 2>A galaxy appears to be moving away from US seventy

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<v Speaker 2>kilometers per second faster.

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<v Speaker 3>Precisely, it's a rate of stretching. If a galaxy is

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<v Speaker 3>one megaparsec away, it's moving its seventy kilometers. If it's

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<v Speaker 3>two away, it's one hundred and forty kilometers. It just

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<v Speaker 3>scales up.

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<v Speaker 2>Okay, got it. So we have the speed limit we're

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<v Speaker 2>trying to measure now. As we said in the intro,

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<v Speaker 2>there are two police officers, two ways to measure this number.

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<v Speaker 2>And this is where the fight starts. Let's call the

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<v Speaker 2>METHODA and method B. Method A is the approach, the

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<v Speaker 2>look out the window method.

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<v Speaker 3>That's a good way to put it. Method A looks

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<v Speaker 3>at the late universe, the universe as it exists now

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<v Speaker 3>or in the relatively recent cosmic past. This is the

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<v Speaker 3>method that follows directly in Edwin Hubble's footsteps. We look

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<v Speaker 3>at galaxies and we measure how fast they're moving away.

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<v Speaker 2>Okay, speed seems easy enough to measure, right, You just

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<v Speaker 2>use red shift.

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<v Speaker 3>Speed is very straightforward. Yeah, we look at the light spectrum.

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<v Speaker 3>If it's shifted toward the red that's moving away, we

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<v Speaker 3>can measure that to an incredibly high precision. The tricky part,

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<v Speaker 3>the absolute nightmare of observational astronomy, is knowing exactly how

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<v Speaker 3>far away the object is. You can't just use a

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<v Speaker 3>tape measure.

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<v Speaker 2>Because in space you completely lose depth perception. A really

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<v Speaker 2>bright thing far away can look exactly the same as

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<v Speaker 2>a dim thing that's close up exactly.

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<v Speaker 3>To solve this, astronomers use something called standard candles.

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<v Speaker 2>I love this analogy. Break it down for us.

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<v Speaker 3>Okay, so imagine you are standing in a long dark

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<v Speaker 3>field at night. You see a light in the distance.

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<v Speaker 3>Is it a dim, little flashlight ten feet away or

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<v Speaker 3>is it a massive search light ten miles away? You

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<v Speaker 3>can't really tell just by looking. But what if you

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<v Speaker 3>knew for a fact that the light was a specific

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<v Speaker 3>brand of sixty watt light.

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<v Speaker 2>Bulb, then you'd know exactly how bright it should be at.

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<v Speaker 3>The source, exactly if you know, it's intrinsic brightness. The wattage,

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<v Speaker 3>you can measure how dim it appears to your eye,

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<v Speaker 3>and then some simple physics tells you exactly how far

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<v Speaker 3>away it must be to look that dimp.

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<v Speaker 2>So we need to find the universe's sixty watt light bulbs.

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<v Speaker 3>And we have them. Our primary standard candles are what

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<v Speaker 3>we call Type EA supernovae exploding stars.

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<v Speaker 2>But why are they all the same brightness? Explosions seem

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<v Speaker 2>like they'd be messy and you know, kind of random.

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<v Speaker 3>They're incredibly messy, but the physics that triggers them is

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<v Speaker 3>remarkably consistent. A type as supernova happens in a binary

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<v Speaker 3>star system. You have a white dwarf, which is a dead,

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<v Speaker 3>super dense star core orbiting a companion star. Okay, the

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<v Speaker 3>white dwarf's gravity is so strong it starts to steal

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<v Speaker 3>matter from its companion. It just siphons it off, getting

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<v Speaker 3>heavier and heavier. But there is a strict fundamental limit

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<v Speaker 3>to how heavy a white.

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<v Speaker 2>Dwarf can get, the Chundra Sicar limit.

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<v Speaker 3>That's the one. It's about one point four times the

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<v Speaker 3>mass of our Sun. Once the white dwarf hits that

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<v Speaker 3>exact limit, it can no longer support its own weight

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<v Speaker 3>against gravity. It collapses and detonates in a thermonuclear explosion.

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<v Speaker 2>And because the mass at the moment of detonation is always.

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<v Speaker 3>The same, the brightness of the explosion is always the same.

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<v Speaker 3>It's nature's standard bomb.

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<v Speaker 2>Wow.

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<v Speaker 3>We also use another kind of star, cephade variables, which

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<v Speaker 3>pulse and the speed of their pulse is directly related

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<v Speaker 3>to their intrinsic brightness. So by combining these measurements using

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<v Speaker 3>the Whole Space telescope, and now that James webistronomers have

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<v Speaker 3>built this very precise cosmic distance ladder.

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<v Speaker 2>They climb that ladder, they check the speedometer, and what

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<v Speaker 2>number do they get?

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<v Speaker 3>Consistently, when looking at the late universe with supernovae and cephades,

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<v Speaker 3>we get a hubble constant of roughly seventy three kilometers

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<v Speaker 3>per second per mega parsek.

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<v Speaker 2>Okay, seventy three. Lock that number in. That's officer number one.

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<v Speaker 2>Now let's look at method B, the indirect approach. This

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<v Speaker 2>is the look at the baby pictures method.

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<v Speaker 3>Yes, this method is completely different. It has nothing to

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<v Speaker 3>do with stars or galaxies. It looks at the cosmic

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<v Speaker 3>microwave background the CMB.

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<v Speaker 2>The after glow of the Big Bang.

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<v Speaker 3>Itself the oldest light in the universe. It was released

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<v Speaker 3>when the cosmos was only about three hundred and eighty

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<v Speaker 3>thousand years old. Before that moment, the universe was this hot, dense,

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<v Speaker 3>opaque fog like a plasma exactly. And when it cooled

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<v Speaker 3>enough that fog cleared and light could finally travel freely.

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<v Speaker 3>That light has been streaming through space for thirteen point

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<v Speaker 3>eight billion years, stretching as the universe expands, until today

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<v Speaker 3>it falls into the microwave part of the spectrum.

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<v Speaker 2>So we have this picture, the snapshot of the baby universe,

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<v Speaker 2>and when we look at it, it's not perfectly smooth,

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<v Speaker 2>is it.

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<v Speaker 3>No, not at all. It has tiny fluctuations, hot spots

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<v Speaker 3>and cold spots that correspond to tiny, tiny ripples in density.

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<v Speaker 2>So we have a map, a map of the infant cosmos.

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<v Speaker 2>What on Earth do you get a speed limit out

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<v Speaker 2>of a static map?

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<v Speaker 3>Ah? Well, we use our best understanding of physics. It's

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<v Speaker 3>called the Standard Model of cosmology. It's this incredible mathematical

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<v Speaker 3>framework for gravity, matter, dark energy, everything. We take the

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<v Speaker 3>data from that baby picture, which was measured with incredible

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<v Speaker 3>precision by the Plank Space telescope and we plug it

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<v Speaker 3>into the model. We basically hit fast forward on a

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<v Speaker 3>giant cosmic simulation.

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<v Speaker 2>You're simulating the entire thirteen point eight billion year history

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<v Speaker 2>of the universe.

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<v Speaker 3>In a sense, yes, we say, okay, if the universe

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<v Speaker 3>started with these specific ingredients and these specific density patterns,

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<v Speaker 3>and if the laws of physics are what we think

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<v Speaker 3>they are, how fast should the universe be expanding today?

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<v Speaker 2>So it's a prediction. It's like looking at a Toddler's

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<v Speaker 2>growth chart and predicting how tall I'll be when they

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<v Speaker 2>turn twenty.

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<v Speaker 3>It's a very very precise prediction based on what we

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<v Speaker 3>believe to be fundamental physics. And when we do that calculation,

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<v Speaker 3>the number we get is not seventy three.

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<v Speaker 2>What is it?

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<v Speaker 3>It is roughly sixty seven kilometers per second per megaparsec.

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<v Speaker 2>Sixty seven versus seventy three. Now I have to play

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<v Speaker 2>Devil's advocate here for a second. To someone on the street,

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<v Speaker 2>that sounds I mean, that sounds pretty close. If I

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<v Speaker 2>guessed a jar had sixty seven jelly beans and it

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<v Speaker 2>turned out to have seventy three, I'd be thrilled with myself.

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<v Speaker 2>Are we sure this matters.

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<v Speaker 3>In many many fields, that would be a celebratory agreement,

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<v Speaker 3>but in precision cosmology it is a disaster. Or a disaster, yes,

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<v Speaker 3>because over the last decade both sides have refined their

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<v Speaker 3>measurements again and again. The air bars, you know, the

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<v Speaker 3>margins of uncertainty, have shrunk to be incredibly small, and

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<v Speaker 3>they do not overlap anymore.

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<v Speaker 2>So it's definitely not just a rounding error.

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<v Speaker 3>The statistical significance is over what we call five sigma

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<v Speaker 3>in science. That means the odds of this being a

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<v Speaker 3>random fluke are less than one in three point five million.

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<v Speaker 3>It is a genuine, undeniable conflict.

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<v Speaker 2>So either the police officer looking at the supernovae is wrong,

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<v Speaker 2>maybe our understanding of cosmic dust is off, or our

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<v Speaker 2>light bulbs aren't as standard as we.

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<v Speaker 3>Think, or the officer looking at the baby picture is.

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<v Speaker 2>Wrong, or the law of the road itself is wrong.

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<v Speaker 2>The physics we're using to connect to the two is broken.

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<v Speaker 3>Exactly. If the measurements are as good as we think

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<v Speaker 3>they are, then our standard model, our entire understanding of

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<v Speaker 3>how the universe evolved, is missing a piece. We get

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<v Speaker 3>a tiebreaker, or a whole new rule of physics.

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<v Speaker 2>And this brings us to the new research this paper

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<v Speaker 2>published today, authored by Pagosian, Jadamziic and Abel. They are

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<v Speaker 2>suggesting the missing piece is magnetism.

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<v Speaker 3>Yes, primordial magnetic fields. And to understand why this is

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<v Speaker 3>such a compelling idea, we actually have to talk about

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<v Speaker 3>another mystery, a totally different problem in astrophysics that seems

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<v Speaker 3>unrelated but might just be the key to the whole thing.

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<v Speaker 2>I love a good subplot. What's the second mystery.

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<v Speaker 3>It's the mystery of where cosmic magnetic fields come from.

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<v Speaker 2>In the first place, I feel like we take magnetism

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<v Speaker 2>for granted. I mean, Earth has a magnetic field. It

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<v Speaker 2>protects us from solar radiation. The Sun has one, We

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<v Speaker 2>have magnets on our fridge. It just seems like it's everywhere.

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<v Speaker 3>It is everywhere, And we understand planetary instellar fee fields

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<v Speaker 3>pretty well. They're generated by dynamos basically churning conducting fluids

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<v Speaker 3>inside the planet or star. The spinning molten iron in

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<v Speaker 3>Earth's core is what creates our field.

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<v Speaker 2>It's like a generator, a natural.

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<v Speaker 3>Generator, yes, But when we look out at the cosmos

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<v Speaker 3>on a grander scale, we see something puzzling. We see

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<v Speaker 3>massive magnetic fields threading through entire galaxies.

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<v Speaker 2>You mean the Milky Way itself is magnetic, very much so, and.

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<v Speaker 3>Not just galaxies. We see magnetic fields in the gas

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<v Speaker 3>between galaxies and clusters, and we think they might even

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<v Speaker 3>exist in the great cosmic voids, the emptiest parts of space.

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<v Speaker 3>The question is where did those come from?

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<v Speaker 2>It's the classic chicken and egg problem, isn't it. Did

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<v Speaker 2>the galaxy form first and then spin up a magnetic field,

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<v Speaker 2>or was a magnetic field there first, maybe helping the

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<v Speaker 2>galaxy to form.

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<v Speaker 3>And here's the problem with the galaxy first idea. It

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<v Speaker 3>is very, very difficult to explain the strength of the

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<v Speaker 3>galactic fields we see today just by spinning them up

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<v Speaker 3>from nothing. You need a seed You need some tiny

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<v Speaker 3>initial bit of magnetism to get the dynamo process started.

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<v Speaker 2>A starter used for the sourdough, if you will.

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<v Speaker 3>That's a perfect analogy. Without a seed field, the math

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<v Speaker 3>just doesn't work to grow the strong fields we observe.

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<v Speaker 3>And this is what leads to the theory of primordial

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<v Speaker 3>magnetic fields. The idea is that magnetism wasn't made by

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<v Speaker 3>stars and galaxies. It arose in the chaos of the

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<v Speaker 3>Big Bang itself.

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<v Speaker 2>So the universe was born with magnetism warven right into

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<v Speaker 2>the fabric of space time.

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<v Speaker 3>That's the theory. It could have been generated during cosmic

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<v Speaker 3>inflation or during one of the big phase transitions in

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<v Speaker 3>the first fraction of a second. But for a long

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<v Speaker 3>time this was just a hypothesis to solve that one problem,

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<v Speaker 3>the seed problem.

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<v Speaker 2>But now these authors Pagosian, Jadamziic, and Abel are asking

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<v Speaker 2>a much bigger question. They're asking, if these primordial fields exist,

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<v Speaker 2>could they do more than just seed galaxies? Could they

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<v Speaker 2>actually fix the Hubble tension exactly?

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<v Speaker 3>They wondered if this one invisible force could solve two

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<v Speaker 3>of the biggest problems in cosmology at the same time,

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<v Speaker 3>the seed problem and the broken speedometer problem.

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<v Speaker 2>Okay, so let's get into the mechanics of this. How

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<v Speaker 2>does a magnetic field, primordial or not, actually change the

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<v Speaker 2>expansion rate of the universe. It feels like those two

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<v Speaker 2>things shouldn't be related at all.

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<v Speaker 3>To understand the mechanism, we have to go back to

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<v Speaker 3>that moment I mentioned earlier, the formation of the cosmic

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<v Speaker 3>microwave background. It's an era of the universe called recombination.

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<v Speaker 2>Right, let's set the scene. The universe is about three

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<v Speaker 2>hundred thousand years old. It's hot, it's dense, it's a soup.

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<v Speaker 3>It's a plasma, and that means it's just too hot

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<v Speaker 3>for atoms to hold together. The electrons, which have a

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<v Speaker 3>negative charge have been ripped away from the protons, which

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<v Speaker 3>have a positive charge. They're just flying around independently.

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<v Speaker 2>And because those electrons are free, they scatter light like crazy,

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<v Speaker 2>like a.

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<v Speaker 3>Thick, impenetrable fog. A photon, a particle of light, can't

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<v Speaker 3>travel more than a tiny distance before it smacks into

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<v Speaker 3>a free electron and gets bounced in a random direction,

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<v Speaker 3>and the universe is opaque.

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<v Speaker 2>But all this time, the universe is expanding, and it's cooling.

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<v Speaker 3>Down right, And eventually it gets cool enough down to

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<v Speaker 3>about three thousand kelvin that the protons can finally capture

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<v Speaker 3>the electrons, they can finally bond. They form the first

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<v Speaker 3>neutral hydrogen atoms.

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<v Speaker 2>They hold hands.

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<v Speaker 3>And this is the crucial part. Neutral hydrogen does not

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<v Speaker 3>scatter light the same way the fog lifts. The universe

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<v Speaker 3>in an instant goes from opaque to transparent. That moment

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<v Speaker 3>is called recombination.

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<v Speaker 2>Okay, so that's the standard story. Now let's throw a

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<v Speaker 2>primordial magnetic field into that hot, foggy soup. What changes.

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<v Speaker 3>Well, magnetic fields interact with charged particles. They push and

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<v Speaker 3>pall on them. It's called the Lorentz force. So now

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<v Speaker 3>imagine you have this plasma. Gravity is trying to pull

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<v Speaker 3>the matter together into little clumps, but the intense pressure

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<v Speaker 3>of all that radiation is trying to push it apart.

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<v Speaker 3>It's a constant tug of war.

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00:16:52.080 --> 00:16:54.360
<v Speaker 2>And the magnetic field jumps in as a third player.

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<v Speaker 3>Yes, And what it does is it creates what we

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00:16:57.039 --> 00:17:00.799
<v Speaker 3>call baryon clumping. The magnetic fields create these lowize spots

359
00:17:00.799 --> 00:17:03.559
<v Speaker 3>of pressure and tension in the plasma. They force the

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00:17:03.679 --> 00:17:06.960
<v Speaker 3>charged particles, the protons and electrons, to clump together just

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00:17:07.039 --> 00:17:09.400
<v Speaker 3>a little bit more than gravity would do on its own.

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00:17:09.720 --> 00:17:12.400
<v Speaker 2>So the soup gets lumpy, a little bit lumpier than

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00:17:12.400 --> 00:17:12.960
<v Speaker 2>it would have been.

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00:17:13.119 --> 00:17:15.880
<v Speaker 3>The soup gets lumpy. And here is the key bit

365
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<v Speaker 3>of chemistry. Recombination. The process of protons and electrons forming

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<v Speaker 3>those hydrogen atoms happens faster in denser regions.

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<v Speaker 2>Why is that?

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00:17:26.640 --> 00:17:29.119
<v Speaker 3>Think of it like a crowded party or a singles mixer.

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00:17:29.759 --> 00:17:32.000
<v Speaker 3>If you have one hundred people spread out across a

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00:17:32.079 --> 00:17:35.119
<v Speaker 3>huge football field, it might take a long time for

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<v Speaker 3>people to find each other and.

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00:17:36.319 --> 00:17:37.880
<v Speaker 2>Pair up right the too far apart.

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00:17:38.039 --> 00:17:40.319
<v Speaker 3>But if you crowd all one hundred people into one

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<v Speaker 3>corner of the room, they're constantly bumping into each other,

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<v Speaker 3>They're going to pair up much much faster.

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00:17:45.640 --> 00:17:49.920
<v Speaker 2>That is a surprisingly perfect analogy. So by clumping the

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00:17:49.960 --> 00:17:53.400
<v Speaker 2>matter together, the magnetic fields make it easier for protons

378
00:17:53.440 --> 00:17:55.839
<v Speaker 2>to find their electron dance partners exactly.

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00:17:56.160 --> 00:17:58.880
<v Speaker 3>And the consequence of that is that recombination as a

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<v Speaker 3>whole finishes sooner, sooner.

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00:18:00.720 --> 00:18:03.680
<v Speaker 2>That's the key word, isn't it. The fog lifts earlier

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00:18:03.720 --> 00:18:05.519
<v Speaker 2>than our standard model assumes it does.

383
00:18:05.839 --> 00:18:09.799
<v Speaker 3>The universe becomes transparent earlier. The baby picture is taken

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00:18:09.839 --> 00:18:11.319
<v Speaker 3>earlier in cosmic history.

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00:18:11.519 --> 00:18:13.960
<v Speaker 2>Okay, I'm following the physics, I think, but I'm still

386
00:18:13.960 --> 00:18:16.960
<v Speaker 2>missing the final connection to the sixty seven versus seventy

387
00:18:17.000 --> 00:18:20.440
<v Speaker 2>three number. Why does the fog lifting a bit early

388
00:18:20.599 --> 00:18:22.240
<v Speaker 2>change the speed reading we get today?

389
00:18:22.400 --> 00:18:24.200
<v Speaker 3>This is the most technical part, but it's also the

390
00:18:24.200 --> 00:18:27.720
<v Speaker 3>most elegant. Nora method B the indirect method, the one

391
00:18:27.799 --> 00:18:28.920
<v Speaker 3>using the baby picture.

392
00:18:28.720 --> 00:18:29.839
<v Speaker 2>The one that gives us sixty seven.

393
00:18:29.920 --> 00:18:33.039
<v Speaker 3>Yes, it relies on measuring the size of the patterns

394
00:18:33.039 --> 00:18:36.279
<v Speaker 3>in the CMB. Those patterns, those hot and cold spots,

395
00:18:36.519 --> 00:18:39.519
<v Speaker 3>are essentially sound waves that were traveling through the plasma.

396
00:18:39.640 --> 00:18:42.839
<v Speaker 2>Sound waves in the early universe. That's just wild to

397
00:18:42.880 --> 00:18:43.319
<v Speaker 2>think about.

398
00:18:43.440 --> 00:18:47.079
<v Speaker 3>We call them veryan acoustic oscillations. Imagine dropping a stone

399
00:18:47.079 --> 00:18:50.640
<v Speaker 3>in a pond. Ripples spread out. In the early universe.

400
00:18:50.680 --> 00:18:53.839
<v Speaker 3>These ripples of pressure traveled through the plasma until the

401
00:18:53.880 --> 00:18:57.319
<v Speaker 3>moment of recombination. As soon as the universe became transparent,

402
00:18:57.359 --> 00:19:00.079
<v Speaker 3>the plasma turned into neutral gas, and the sound way

403
00:19:00.119 --> 00:19:01.400
<v Speaker 3>is basically froze in place.

404
00:19:01.720 --> 00:19:03.559
<v Speaker 2>So the size of those frozen ripples we see in

405
00:19:03.599 --> 00:19:05.759
<v Speaker 2>the CMB is determined by how long they had to

406
00:19:05.759 --> 00:19:07.319
<v Speaker 2>travel before everything froze.

407
00:19:07.599 --> 00:19:10.119
<v Speaker 3>Exactly the distance they were able to travel is called

408
00:19:10.160 --> 00:19:14.119
<v Speaker 3>the sound horizon, and for decades it has been our

409
00:19:14.200 --> 00:19:18.440
<v Speaker 3>standard ruler for the early universe. We know, or at

410
00:19:18.519 --> 00:19:21.799
<v Speaker 3>least we thought we knew exactly how long that ruler is.

411
00:19:22.079 --> 00:19:27.880
<v Speaker 2>Ah. But if the magnetic fields made recombination happen sooner, then.

412
00:19:27.799 --> 00:19:29.720
<v Speaker 3>The sound waves didn't have as much time to travel.

413
00:19:29.759 --> 00:19:30.799
<v Speaker 2>The ripples are smaller.

414
00:19:31.000 --> 00:19:32.000
<v Speaker 3>The ruler is shorter.

415
00:19:32.240 --> 00:19:34.000
<v Speaker 2>Oh wow, okay, let me just restate this and make

416
00:19:34.039 --> 00:19:36.880
<v Speaker 2>sure I've got it straight. We have been looking at

417
00:19:36.920 --> 00:19:39.920
<v Speaker 2>these patterns in the sky, these ripples, assuming they were

418
00:19:39.920 --> 00:19:43.279
<v Speaker 2>made with a ruler that is say twelve inches long, right,

419
00:19:43.759 --> 00:19:46.440
<v Speaker 2>But because of the magnetic field speeding everything up, the

420
00:19:46.519 --> 00:19:49.079
<v Speaker 2>ruler was actually only say eleven inches long.

421
00:19:49.160 --> 00:19:50.519
<v Speaker 3>That's the perfect way to describe it.

422
00:19:50.599 --> 00:19:53.039
<v Speaker 2>And if you measure a giant room with a ruler

423
00:19:53.079 --> 00:19:55.039
<v Speaker 2>that you think is the full length, but it's actually

424
00:19:55.079 --> 00:19:57.079
<v Speaker 2>too short, you're going to get the dimensions of the

425
00:19:57.160 --> 00:19:57.640
<v Speaker 2>room wrong.

426
00:19:57.920 --> 00:20:01.079
<v Speaker 3>You will miscalculate the distance to the CNA, and as

427
00:20:01.160 --> 00:20:04.720
<v Speaker 3>a result, you will miscalculate the expansion rate required to

428
00:20:04.759 --> 00:20:07.839
<v Speaker 3>get from there to hear. If you correct for the

429
00:20:07.880 --> 00:20:11.640
<v Speaker 3>magnetic fields, if you shrink the ruler in your calculations

430
00:20:11.680 --> 00:20:15.680
<v Speaker 3>to its true shorter size, then the inferred hubble constant

431
00:20:15.720 --> 00:20:16.440
<v Speaker 3>has to shift.

432
00:20:16.519 --> 00:20:17.079
<v Speaker 2>It goes up.

433
00:20:17.160 --> 00:20:21.200
<v Speaker 3>It goes up, It moves from sixty seven toward seventy.

434
00:20:20.759 --> 00:20:24.119
<v Speaker 2>Three boom the magnetic bridge magnetic bridge.

435
00:20:24.279 --> 00:20:28.000
<v Speaker 3>By accounting for these fields, the baby picture prediction can

436
00:20:28.000 --> 00:20:30.759
<v Speaker 3>be brought into alignment with the supernova measurement. The two

437
00:20:30.839 --> 00:20:33.920
<v Speaker 3>police officers are actually agreeing, we just interpreted the second

438
00:20:34.000 --> 00:20:36.799
<v Speaker 3>officer's data wrong because we didn't know about the magnetic

439
00:20:36.799 --> 00:20:37.759
<v Speaker 3>interference on the road.

440
00:20:38.000 --> 00:20:41.160
<v Speaker 2>That is just incredibly elegant. It doesn't require inventing some new,

441
00:20:41.519 --> 00:20:44.759
<v Speaker 2>weird kind of dark energy. It's just saying, hey, everyone,

442
00:20:44.799 --> 00:20:46.599
<v Speaker 2>we forgot to account for the magnetism.

443
00:20:46.720 --> 00:20:50.759
<v Speaker 3>It is elegant. But elegance doesn't automatically mean it's true.

444
00:20:50.799 --> 00:20:52.960
<v Speaker 3>For that, you need proof, or at the very least,

445
00:20:52.960 --> 00:20:55.559
<v Speaker 3>you need rigorous simulation. And that is what this new

446
00:20:55.559 --> 00:20:57.240
<v Speaker 3>paper finally provides.

447
00:20:57.000 --> 00:20:59.319
<v Speaker 2>Right because up until now this was mostly a back

448
00:20:59.319 --> 00:21:01.920
<v Speaker 2>of the napkin, wasn't it, or at least the simplified

449
00:21:01.920 --> 00:21:03.640
<v Speaker 2>one dimensional calculation.

450
00:21:03.440 --> 00:21:07.119
<v Speaker 3>Correct Back in twenty twenty two of the authors, Karston,

451
00:21:07.160 --> 00:21:11.279
<v Speaker 3>Jadamzic and Levon Pegosian, first demonstrated this effect was possible

452
00:21:11.279 --> 00:21:14.920
<v Speaker 3>with a simplified model. But real plasma physics is messy,

453
00:21:15.200 --> 00:21:18.200
<v Speaker 3>it's turbulent. You can't just approximate three dimensional chaos on

454
00:21:18.240 --> 00:21:18.880
<v Speaker 3>a piece of paper.

455
00:21:18.960 --> 00:21:20.599
<v Speaker 2>So what did they do differently? This time?

456
00:21:20.920 --> 00:21:26.319
<v Speaker 3>They ran the first full three dimensional magnetohydrodynamic MHD simulations

457
00:21:26.359 --> 00:21:29.480
<v Speaker 3>of the primordial plasma with magnetic fields embedded in it.

458
00:21:29.519 --> 00:21:33.039
<v Speaker 2>They built a virtual baby universe in a supercomputer.

459
00:21:32.519 --> 00:21:35.319
<v Speaker 3>A virtual size of one. Yes, they tracked the history

460
00:21:35.319 --> 00:21:38.160
<v Speaker 3>of hydrogen formation in three D. They didn't just guess

461
00:21:38.160 --> 00:21:41.200
<v Speaker 3>at the clumping effect. They simulated the fluid dynamics, the

462
00:21:41.240 --> 00:21:44.119
<v Speaker 3>magnetic stresses, the photon interactions.

463
00:21:43.519 --> 00:21:45.200
<v Speaker 2>Everything, and what did the computer say?

464
00:21:45.640 --> 00:21:49.559
<v Speaker 3>The results were compelling. They compared their simulation data against

465
00:21:49.559 --> 00:21:52.680
<v Speaker 3>the actual observations from the Plank satellite and other cosmological

466
00:21:52.759 --> 00:21:55.200
<v Speaker 3>data sets, and they found that the real world data

467
00:21:55.279 --> 00:21:59.119
<v Speaker 3>shows a consistent mild preference for the existence of these

468
00:21:59.160 --> 00:21:59.880
<v Speaker 3>magnetic fields.

469
00:22:00.079 --> 00:22:02.279
<v Speaker 2>Mild preference. That sounds a little cautious.

470
00:22:02.559 --> 00:22:07.039
<v Speaker 3>Scientists are professionally cautious. It's in our DNA. We rely

471
00:22:07.160 --> 00:22:10.839
<v Speaker 3>on sigma values to quantify this stuff. In statistical terms,

472
00:22:11.000 --> 00:22:14.400
<v Speaker 3>the preference they found ranges from about one point five

473
00:22:14.480 --> 00:22:16.799
<v Speaker 3>to three standard deviations or sigma.

474
00:22:17.200 --> 00:22:19.680
<v Speaker 2>Okay, translate that for us. What does that mean?

475
00:22:19.880 --> 00:22:22.480
<v Speaker 3>Well, five sigma is the gold standard for a discovery.

476
00:22:22.880 --> 00:22:24.920
<v Speaker 3>That's when you pop the champagne and start booking your

477
00:22:24.960 --> 00:22:28.839
<v Speaker 3>flight to Stockholm for the Nobel Prize. Three sigmas generally

478
00:22:28.839 --> 00:22:32.119
<v Speaker 3>considered strong evidence. So one point five to three is

479
00:22:32.119 --> 00:22:34.920
<v Speaker 3>a meaningful hint. It's like finding a clear fingerprint at

480
00:22:34.920 --> 00:22:37.640
<v Speaker 3>the crime scene. It doesn't prove who did it yet,

481
00:22:37.720 --> 00:22:40.799
<v Speaker 3>maybe there's another explanation for the fingerprint, but it matches

482
00:22:40.839 --> 00:22:43.400
<v Speaker 3>your main suspect. It tells you that you are definitely

483
00:22:43.400 --> 00:22:44.119
<v Speaker 3>on the right track.

484
00:22:44.240 --> 00:22:46.519
<v Speaker 2>So it's not a done deal, but it's a very

485
00:22:46.839 --> 00:22:48.720
<v Speaker 2>very strong lead exactly.

486
00:22:49.359 --> 00:22:51.960
<v Speaker 3>But there's a second piece of evidence in the paper that,

487
00:22:52.119 --> 00:22:55.119
<v Speaker 3>in my opinion, makes it even stronger. It's the specific

488
00:22:55.119 --> 00:22:56.880
<v Speaker 3>strength of the magnetic fields required.

489
00:22:57.000 --> 00:22:59.200
<v Speaker 2>This is the peico Gauss thing we mentioned in the intro.

490
00:22:59.480 --> 00:23:02.519
<v Speaker 3>It is the simulation tells us not just if there

491
00:23:02.519 --> 00:23:04.920
<v Speaker 3>were fields, but how strong they would need to be

492
00:23:05.079 --> 00:23:07.759
<v Speaker 3>to solve the hubble tension. The number of the data

493
00:23:07.799 --> 00:23:10.960
<v Speaker 3>seems to favor is between five and ten piico gause.

494
00:23:11.279 --> 00:23:13.559
<v Speaker 2>Okay, let's contextualize that a pika gaus. I have a

495
00:23:13.559 --> 00:23:14.400
<v Speaker 2>magnet on my fridge.

496
00:23:14.400 --> 00:23:17.240
<v Speaker 3>How many gass is that a typical fridge magnet is

497
00:23:17.319 --> 00:23:21.480
<v Speaker 3>about fifty to one hundred gaus. The Earth's magnetic field,

498
00:23:21.480 --> 00:23:23.519
<v Speaker 3>the one that moves your compass needle is about.

499
00:23:23.319 --> 00:23:25.319
<v Speaker 2>Half a gas, and this is a peico gous.

500
00:23:25.400 --> 00:23:27.319
<v Speaker 3>Piker gous is one trillionth of a gaus.

501
00:23:27.400 --> 00:23:32.559
<v Speaker 2>So these are I mean they're unbelievably weak fields, vanishingly weak,

502
00:23:32.720 --> 00:23:34.200
<v Speaker 2>you would never ever feel them.

503
00:23:34.480 --> 00:23:38.480
<v Speaker 3>But remember they are pervasive. They span the entire cosmos,

504
00:23:38.640 --> 00:23:42.039
<v Speaker 3>so the total energy involved across that scale is actually significant.

505
00:23:42.359 --> 00:23:44.960
<v Speaker 3>But here's the real aha moment. I'm ready remember the

506
00:23:45.000 --> 00:23:48.160
<v Speaker 3>seed problem, the other great mystery of where galactic magnetic

507
00:23:48.200 --> 00:23:48.960
<v Speaker 3>fields came from.

508
00:23:49.039 --> 00:23:51.279
<v Speaker 2>Yes, the sourdok starter for galaxies.

509
00:23:51.599 --> 00:23:56.359
<v Speaker 3>Right. Well, astrophysicists have calculated, independently, in a totally separate

510
00:23:56.400 --> 00:24:00.119
<v Speaker 3>line of research, completely unrelated to the Hubble tension, how

511
00:24:00.160 --> 00:24:02.079
<v Speaker 3>strong a seed field would need to be in the

512
00:24:02.119 --> 00:24:06.759
<v Speaker 3>early universe to eventually grow through dynamo effects into the

513
00:24:06.759 --> 00:24:09.359
<v Speaker 3>galactic fields we see today. And let me guess the

514
00:24:09.359 --> 00:24:13.599
<v Speaker 3>required strength they calculated is roughly five to ten picogaus.

515
00:24:14.319 --> 00:24:16.680
<v Speaker 2>No way, yes, way, it's the same number.

516
00:24:16.839 --> 00:24:19.720
<v Speaker 3>The Goldilocks strength needed to fix the Hubble tension. Is

517
00:24:19.759 --> 00:24:23.039
<v Speaker 3>the exact same strength needed to explain why galaxies are

518
00:24:23.079 --> 00:24:24.279
<v Speaker 3>magnetic in the first place.

519
00:24:24.680 --> 00:24:27.119
<v Speaker 2>That feels like more than a coincidence. That feels like

520
00:24:27.160 --> 00:24:30.400
<v Speaker 2>a major puzzle piece just clicking perfectly into place.

521
00:24:30.559 --> 00:24:33.720
<v Speaker 3>It fits both locks with a single key. That is

522
00:24:33.759 --> 00:24:37.039
<v Speaker 3>what makes this paper so exciting to the community. Nature

523
00:24:37.079 --> 00:24:39.839
<v Speaker 3>tends to be efficient. It seems highly unlikely that the

524
00:24:39.920 --> 00:24:42.279
<v Speaker 3>universe would have one field to solve the Hubble tension

525
00:24:42.640 --> 00:24:46.039
<v Speaker 3>and a totally different, unrelated field to seed galaxies when

526
00:24:46.079 --> 00:24:48.119
<v Speaker 3>one field can do both jobs perfectly.

527
00:24:48.279 --> 00:24:50.359
<v Speaker 2>So if this turns out to be true, it really

528
00:24:50.400 --> 00:24:52.599
<v Speaker 2>does rewrite the history of the early universe.

529
00:24:52.960 --> 00:24:57.039
<v Speaker 3>It absolutely does. It means that magnetism was a fundamental

530
00:24:57.079 --> 00:25:00.279
<v Speaker 3>player from the very very beginning. We usually think of

531
00:25:00.319 --> 00:25:03.079
<v Speaker 3>gravity as the main sculptor of the universe, but this

532
00:25:03.119 --> 00:25:05.400
<v Speaker 3>suggests magnetism was holding the chisel too.

533
00:25:05.440 --> 00:25:08.759
<v Speaker 2>And that leads to some pretty profound implications. You mentioned

534
00:25:08.759 --> 00:25:10.759
<v Speaker 2>at the start that this could be a window into

535
00:25:10.799 --> 00:25:12.240
<v Speaker 2>physics we can't do on Earth.

536
00:25:12.319 --> 00:25:14.799
<v Speaker 3>Well, think about where these fields would have to come from.

537
00:25:14.839 --> 00:25:18.119
<v Speaker 3>We said primordial. That means they were generated in the

538
00:25:18.160 --> 00:25:20.519
<v Speaker 3>first fraction of a second after the Big Bang.

539
00:25:20.519 --> 00:25:23.640
<v Speaker 2>During the era of inflation, or maybe the electro weak

540
00:25:23.680 --> 00:25:24.559
<v Speaker 2>phase transition.

541
00:25:24.839 --> 00:25:28.319
<v Speaker 3>Precisely, these are moments when the universe was incredibly hot

542
00:25:28.359 --> 00:25:32.079
<v Speaker 3>and dense, energy levels that are billions or even trillions

543
00:25:32.079 --> 00:25:34.240
<v Speaker 3>of times higher than anything we could generate in the

544
00:25:34.319 --> 00:25:35.440
<v Speaker 3>large Hadron collider.

545
00:25:35.839 --> 00:25:38.680
<v Speaker 2>We just can't build a machine that big or that powerful.

546
00:25:38.960 --> 00:25:43.480
<v Speaker 3>No but the universe was that machine. And if we

547
00:25:43.559 --> 00:25:47.440
<v Speaker 3>can confirm these magnetic fields exist, and if we can

548
00:25:47.480 --> 00:25:51.799
<v Speaker 3>measure their properties precisely, their strength, their shape, they act

549
00:25:51.839 --> 00:25:54.400
<v Speaker 3>as fossils from that era. They are like a diary

550
00:25:54.559 --> 00:25:55.960
<v Speaker 3>entry from the moment of creation.

551
00:25:56.400 --> 00:25:58.880
<v Speaker 2>That is just mind blowing. We're analyzing a glitch and

552
00:25:58.920 --> 00:26:01.839
<v Speaker 2>a cosmic spitamen to try and read a diary from

553
00:26:01.880 --> 00:26:04.119
<v Speaker 2>the first Peko second of the Big Bang.

554
00:26:04.279 --> 00:26:07.480
<v Speaker 3>That is the beauty and the madness of cosmology. Everything

555
00:26:07.519 --> 00:26:10.759
<v Speaker 3>is connected. You pull on one tiny thread here, a

556
00:26:10.799 --> 00:26:14.279
<v Speaker 3>small discrepancy and expansion rates, and you find yourself unraveling

557
00:26:14.319 --> 00:26:16.559
<v Speaker 3>the fundamental physics of the first second of time.

558
00:26:16.759 --> 00:26:18.839
<v Speaker 2>So what's the next step. How do we go from

559
00:26:18.920 --> 00:26:23.160
<v Speaker 2>a meaningful hint to a confirmed discovery. How do we

560
00:26:23.200 --> 00:26:26.359
<v Speaker 2>get from three sigma to that five sigma gold standard?

561
00:26:26.440 --> 00:26:29.559
<v Speaker 3>We need better maps. The paper notes that this theory

562
00:26:29.680 --> 00:26:34.200
<v Speaker 3>survives the most detailed test available today, but available today

563
00:26:34.279 --> 00:26:35.240
<v Speaker 3>is the key phrase there.

564
00:26:35.279 --> 00:26:36.599
<v Speaker 2>We need better eyes on the sky.

565
00:26:36.799 --> 00:26:39.079
<v Speaker 3>We need to look at the cosmic microwave background with

566
00:26:39.119 --> 00:26:42.119
<v Speaker 3>even higher precision, and specifically, we need to look for

567
00:26:42.240 --> 00:26:45.680
<v Speaker 3>very particular patterns in the polarization of that ancient.

568
00:26:45.440 --> 00:26:48.000
<v Speaker 2>Light polarization is the direction the light waves are sort

569
00:26:48.039 --> 00:26:49.480
<v Speaker 2>of wiggling correct.

570
00:26:49.680 --> 00:26:52.599
<v Speaker 3>And magnetic field should leave a specific twisting signature, a

571
00:26:52.680 --> 00:26:56.079
<v Speaker 3>kind of fingerprint on the polarization of the CMB. If

572
00:26:56.079 --> 00:26:58.359
<v Speaker 3>the fields are there, they should have twisted the light

573
00:26:58.519 --> 00:27:00.720
<v Speaker 3>in a very predictable way we could look for.

574
00:27:01.079 --> 00:27:02.759
<v Speaker 2>Are there missions planned to do that?

575
00:27:03.039 --> 00:27:06.279
<v Speaker 3>There are. There's the Simon's Observatory being built right now

576
00:27:06.279 --> 00:27:09.559
<v Speaker 3>in the Atacama Desert in Chile. There's a satellite mission

577
00:27:09.559 --> 00:27:14.200
<v Speaker 3>from Japan called light Bird, and the huge CMBs four project.

578
00:27:14.960 --> 00:27:18.559
<v Speaker 3>These are all upcoming experiments designed specifically to map the

579
00:27:18.599 --> 00:27:22.359
<v Speaker 3>CMB polarization with unprecedented sensitivity.

580
00:27:22.400 --> 00:27:24.559
<v Speaker 2>And if they see that specific twist.

581
00:27:24.319 --> 00:27:26.559
<v Speaker 3>If they see that signature, then the Hubble tension is

582
00:27:26.720 --> 00:27:30.400
<v Speaker 3>likely resolved. We can say with confidence the universe is

583
00:27:30.440 --> 00:27:33.720
<v Speaker 3>expanding at seventy three kilometers mpc. And the reason we

584
00:27:33.759 --> 00:27:36.559
<v Speaker 3>thought otherwise is because we forgot to include the magnetism

585
00:27:36.559 --> 00:27:37.960
<v Speaker 3>in our baby pictures.

586
00:27:37.599 --> 00:27:39.359
<v Speaker 2>And the standard model of cosmology.

587
00:27:39.480 --> 00:27:42.960
<v Speaker 3>It survives, but it gets an important update. It's not broken,

588
00:27:43.160 --> 00:27:46.680
<v Speaker 3>it was just incomplete. We add primordial magnetism to the

589
00:27:46.680 --> 00:27:48.400
<v Speaker 3>official Recipe Book of the Universe.

590
00:27:48.519 --> 00:27:50.680
<v Speaker 2>It's amazing how science works like that. We hate it

591
00:27:50.680 --> 00:27:53.720
<v Speaker 2>when the numbers don't add up. It's frustrating, But that frustration,

592
00:27:53.799 --> 00:27:56.400
<v Speaker 2>that tension is actually where the discovery lives.

593
00:27:56.720 --> 00:28:00.160
<v Speaker 3>Precisely, if the numbers had matched perfectly ten years ago go,

594
00:28:00.920 --> 00:28:04.279
<v Speaker 3>if both methods gave us a clean seven eight, we

595
00:28:04.440 --> 00:28:07.000
<v Speaker 3>never would have looked this hard for these magnetic fields.

596
00:28:07.519 --> 00:28:10.079
<v Speaker 3>We might have missed this entire layer of reality. The

597
00:28:10.240 --> 00:28:11.839
<v Speaker 3>tension is what forced the innovation.

598
00:28:12.039 --> 00:28:14.319
<v Speaker 2>The grit in the oyster makes the pearl a.

599
00:28:14.279 --> 00:28:17.079
<v Speaker 3>Poetic way to put it, but yes, completely accurate.

600
00:28:17.480 --> 00:28:20.119
<v Speaker 2>So to recap our journey today, we started with a

601
00:28:20.119 --> 00:28:23.759
<v Speaker 2>broken speedometer, two trusted methods giving us different answers for

602
00:28:23.799 --> 00:28:26.599
<v Speaker 2>the expansion of the universe, A sixty seven versus a

603
00:28:26.680 --> 00:28:27.359
<v Speaker 2>seventy three.

604
00:28:27.519 --> 00:28:32.640
<v Speaker 3>We introduced a suspect, Yeah, these weak, invisible, ancient primordial

605
00:28:32.680 --> 00:28:33.640
<v Speaker 3>magnetic fields.

606
00:28:33.720 --> 00:28:36.480
<v Speaker 2>We then looked at the mechanism. These fields made the

607
00:28:36.519 --> 00:28:39.400
<v Speaker 2>plasma in the early universe a little bit clumpy, which

608
00:28:39.440 --> 00:28:41.480
<v Speaker 2>caused neutral hydrogen to form sooner than.

609
00:28:41.400 --> 00:28:44.720
<v Speaker 3>We thought, which in turn shrinks the sound horizon our

610
00:28:44.759 --> 00:28:48.119
<v Speaker 3>cosmic ruler, and when we use the correct shorter ruler,

611
00:28:48.400 --> 00:28:50.920
<v Speaker 3>our measurement of the expansion rate shifts up, moving from

612
00:28:51.039 --> 00:28:54.079
<v Speaker 3>sixty seven to match the seventy three from the local observations.

613
00:28:54.400 --> 00:28:57.400
<v Speaker 2>And finally we saw that the new three D simulations

614
00:28:57.440 --> 00:29:00.440
<v Speaker 2>back this all up, showing that the specifics strength of

615
00:29:00.480 --> 00:29:04.079
<v Speaker 2>magnetism needed to fix the tension those five to ten

616
00:29:04.160 --> 00:29:07.559
<v Speaker 2>picogaus is the exact same strength needed to solve a

617
00:29:07.599 --> 00:29:11.559
<v Speaker 2>totally different problem, why galaxies are magnetic at all.

618
00:29:11.680 --> 00:29:15.200
<v Speaker 3>A single unifying solution to two major cosmic puzzles.

619
00:29:15.279 --> 00:29:17.880
<v Speaker 2>It really makes you think about the invisible scaffolding of

620
00:29:17.920 --> 00:29:19.720
<v Speaker 2>the universe, doesn't it. We look up at the stars

621
00:29:19.759 --> 00:29:22.599
<v Speaker 2>and we think that's it, that's the universe. But there

622
00:29:22.640 --> 00:29:27.160
<v Speaker 2>are these vast, invisible webs of force, magnetism, gravity, dark

623
00:29:27.240 --> 00:29:29.039
<v Speaker 2>matter that are really running the show.

624
00:29:29.160 --> 00:29:31.400
<v Speaker 3>We are just seeing the foam on top of the ocean.

625
00:29:31.920 --> 00:29:34.960
<v Speaker 3>The deep currents underneath are what dictate where all that

626
00:29:35.000 --> 00:29:38.519
<v Speaker 3>foam goes. This paper suggests that magnetism is one of

627
00:29:38.519 --> 00:29:41.559
<v Speaker 3>those deep, powerful currents that has been pushing and pulling

628
00:29:41.599 --> 00:29:43.720
<v Speaker 3>on the cosmos since the very beginning.

629
00:29:43.799 --> 00:29:47.160
<v Speaker 2>It's a powerful reminder that the universe is a connected system.

630
00:29:47.640 --> 00:29:51.119
<v Speaker 2>You can't tweak the beginning without fundamentally changing the end.

631
00:29:51.200 --> 00:29:54.240
<v Speaker 3>And you can't fully understand the end without knowing exactly

632
00:29:54.279 --> 00:29:55.359
<v Speaker 3>what happened at the beginning.

633
00:29:55.519 --> 00:29:57.640
<v Speaker 2>I want to leave our listeners with a final thought. Then,

634
00:29:57.880 --> 00:30:01.079
<v Speaker 2>we've been talking about magnetic fields today, something we usually

635
00:30:01.160 --> 00:30:05.039
<v Speaker 2>associate with you fridge magnets, and compasses. But if these

636
00:30:05.160 --> 00:30:08.240
<v Speaker 2>fields really did shape the early universe, if they really

637
00:30:08.279 --> 00:30:13.079
<v Speaker 2>did alter the timeline of creation, what other invisible forces

638
00:30:13.160 --> 00:30:15.640
<v Speaker 2>might be out there pushing and pulling on the cosmos

639
00:30:16.000 --> 00:30:19.039
<v Speaker 2>that we haven't even thought to put into our equations yet.

640
00:30:19.160 --> 00:30:22.000
<v Speaker 3>That is the ultimate question, isn't it. If we could

641
00:30:22.000 --> 00:30:25.240
<v Speaker 3>miss something as fundamental as magnetism for this long, what

642
00:30:25.279 --> 00:30:28.599
<v Speaker 3>else are we missing? Is our standard model incomplete? In

643
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<v Speaker 3>other ways? Are there other fossils from the Big Bang

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<v Speaker 3>hiding in plain sight, in the data, just waiting for

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<v Speaker 3>someone to ask the right question.

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<v Speaker 2>Something to wonder about next time you look up at

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<v Speaker 2>the night sky, or I suppose next time you look

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<v Speaker 2>at your refrigerator. Indeed, thanks for joining us on this

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<v Speaker 2>deep dive into the magnetic universe. Keep looking up and

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<v Speaker 2>keep wondering.

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<v Speaker 3>MS
