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 Astronomy 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>Welcome everyone. Today, we are strapping in for a ride

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<v Speaker 2>that might just completely upend our sense of cosmic orientation.

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<v Speaker 2>We're asking a question that sounds incredibly fundamental, almost simple.

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<v Speaker 2>How fast and in what direction is our solar system

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<v Speaker 2>actually moving through the universe.

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<v Speaker 3>It really does seem like a simple question, doesn't it.

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<v Speaker 3>But the answer is, well, it's anything but. And trying

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<v Speaker 3>to determine our absolute velocity relative to the most distant

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<v Speaker 3>things we can see. That's not just some mapping exercise.

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<v Speaker 3>It's a foundational taesk for how well we actually understand

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<v Speaker 3>dan the very fabric of space, time and everything that's happened.

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<v Speaker 2>Since the Big Bang exactly. We've been looking at some

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<v Speaker 2>truly fascinating research that zeros in on measuring this specific velocity.

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<v Speaker 2>The sources we're analyzing center around a huge study, a

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<v Speaker 2>landmark study really published recently in Physical Review letters. It

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<v Speaker 2>was led by an astrophysicist named Lucas Booma and his

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<v Speaker 2>team at Beilafeld University.

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<v Speaker 3>And our goal here is pretty straightforward. We need to

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<v Speaker 3>unpack these findings because they deliver a serious, maybe even

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<v Speaker 3>a fatal blow to one of the bedrock assumptions of

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<v Speaker 3>the standard model of cosmology. And for you listening, we

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<v Speaker 3>have to start with the really staggering conclusion based on

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<v Speaker 3>their analysis of distant galaxies, the Solar system is moving

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<v Speaker 3>get this, more than three times faster than every single

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<v Speaker 3>existing cosmological model predicts.

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<v Speaker 2>Three times faster. That sounds less like a scientific measurement

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<v Speaker 2>and more like a cosmic speeding ticket. And this isn't

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<v Speaker 2>some minor calibration error, right, This is a statistical deviation

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<v Speaker 2>so vast that I'm quoting Brom here. It forces the

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<v Speaker 2>entire scientific community to reconsider our previous assumptions, assumptions about

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<v Speaker 2>how the universe is built on the largest scales.

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<v Speaker 3>It's a genuine shockwave, and it's a shockwave precisely because

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<v Speaker 3>it forces this confrontation with the most successful framework we

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<v Speaker 3>have for understanding the universe. I mean, the standard model

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<v Speaker 3>of cosmology, you know, land to CDM, has explained pretty

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<v Speaker 3>much everything from the proportions of elements in the early

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<v Speaker 3>universe all the way to the rate of cosmic expansion.

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<v Speaker 2>It's the reigning champion of theories.

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<v Speaker 3>It is so when a measurement comes along that contradicts

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<v Speaker 3>this model, and does so with such incredible statistical certainty,

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<v Speaker 3>scientists can't just ignore it. They can't just sweep it

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<v Speaker 3>under the rug. They have to fundamentally test the foundations

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<v Speaker 3>of reality itself.

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<v Speaker 2>Okay, let's unpack the groundwork here before we get into

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<v Speaker 2>this new, frankly shocking speed. We need to establish the baseline.

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<v Speaker 2>Why is pinning down the speed of our solar system

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<v Speaker 2>so crucial to our cosmological under standing. What's the fundamental

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<v Speaker 2>principle it's testing.

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<v Speaker 3>It's testing something we call the cosmological principle. And this

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<v Speaker 3>principle is I mean, it is the unshakable foundation of

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<v Speaker 3>all of modern cosmology. Essentially, it posits two things about

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<v Speaker 3>the universe. When you look at it on the grandest

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<v Speaker 3>scales past a few hundred million light years or so,

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<v Speaker 3>it says the universe is both homogeneous and isotropic.

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<v Speaker 2>Okay, So homogenating means it's mostly smooth and uniform, like

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<v Speaker 2>a giant perfectly mixed soup.

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<v Speaker 3>No big lumps exactly, no big lumps, and isotropy means

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<v Speaker 3>it looks the same in every direction you look. There's

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<v Speaker 3>no special direction, no preferred access, no up or down

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<v Speaker 3>in the cosmos, no cosmic north star precisely. And if

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<v Speaker 3>the universe really is homogeneous and isotropic, it has no center.

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<v Speaker 3>That means gravity should be pulling more or less equally

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<v Speaker 3>in all directions. On a large enough scale, our motion

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<v Speaker 3>therefore should be relatively constrained. It should align with the

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<v Speaker 3>overall flow of cosmic expansion and the small local gravitational

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<v Speaker 3>tugs from our immediate cosmic neighborhood, things like the Virgo supercluster.

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<v Speaker 2>I see. So the standard model doesn't just pull a

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<v Speaker 2>speed out of thin air. It uses this assumption of

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<v Speaker 2>large scale uniformity the cosmological principle to establish what you

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<v Speaker 2>could call a cosmic rest frame.

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<v Speaker 3>That's the perfect way to put it. The ultimate cosmic

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<v Speaker 3>rest frame is defined by the cosmic microwave background, or

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<v Speaker 3>the CNB. This is the faint afterglow radiation left over

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<v Speaker 3>from the big bank. It fills the entire universe, and

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<v Speaker 3>if you are truly at rest cosmologically, the CMB should

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<v Speaker 3>look perfectly uniform, the same temperature no matter where you look.

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<v Speaker 2>But we know we are moving relative to the CMB.

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<v Speaker 2>That's something we've measured for decades.

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<v Speaker 3>Right, we have, yes, and it's one of the great

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<v Speaker 3>discoveries of modern cosmology. When we look at the CMB

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<v Speaker 3>with sensitive instruments, we see a tiny but very distinct

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<v Speaker 3>temperature asymmetry. One side of the sky is ever so

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<v Speaker 3>slightly hotter, which means it's blue shifted, and the other

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<v Speaker 3>side is slightly cooler or red shifted.

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<v Speaker 2>This is the famous CMB dipole.

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<v Speaker 3>That's the one, and it's a direct measurement. It tells

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<v Speaker 3>us how fast we the Solar System are moving relative

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<v Speaker 3>to the universe's background radiation. And that speed is about

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<v Speaker 3>three hundred and seventy kilometers per second.

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<v Speaker 2>So that's our expected baseline motion. That's the speed we

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<v Speaker 2>should be going at because of all the known local

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<v Speaker 2>gravitational influences and the overall expansion of the universe, the

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<v Speaker 2>standard cosmological model is perfectly happy with that speed.

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<v Speaker 3>Correct It all fits together very neatly. But and this

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<v Speaker 3>is the crucial point, this new research wasn't measuring our

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<v Speaker 3>motion relative to the CMB. It was measuring our motion

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<v Speaker 3>relative to matter, specifically the distribution of incredibly distant galaxies.

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<v Speaker 2>So two different rulers to measure the same thing exactly.

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<v Speaker 3>The CMB gives us a benchmark for the very early universe,

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<v Speaker 3>just a few hundred thousand years after the Big Bang,

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<v Speaker 3>but the distribution of distant galaxies that provides a benchmark

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<v Speaker 3>for the current large scale structure of the universe if

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<v Speaker 3>the cosmological principle holds, if the universe is truly uniform,

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<v Speaker 3>these two measurements are speedid relative to the CMB and

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<v Speaker 3>our speed relative to all that distant matter. They should align.

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<v Speaker 3>They should give us a very similar velocity.

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<v Speaker 2>And this is where the contradiction just slams into you.

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<v Speaker 2>Lead author Booma explicitly states his words that this new

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<v Speaker 2>velocity measurement clearly contradicts expectations based on standard cosmology.

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<v Speaker 3>It's so much more than just a deviation. The velocity

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<v Speaker 3>they measured based on the actual material distribution of the

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<v Speaker 3>universe is statistically forcing us to conclude that we're moving

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<v Speaker 3>three times faster than we should be, and that translates

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<v Speaker 3>directly into a much much stronger directional tug. It means

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<v Speaker 3>that the universe as defined by where the galaxies are

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<v Speaker 3>appears significantly less uniform than the universe as defined by

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<v Speaker 3>that ancient microwave background light.

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<v Speaker 2>Wow. Okay, so this presents a massive problem for the

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<v Speaker 2>standard model. It suggests that either there is some truly monumental,

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<v Speaker 2>previously unseen gravitational engine in our local universe that is

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<v Speaker 2>accelerating us.

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<v Speaker 3>Or the fundamental assumption that matter is spread out smoothly

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<v Speaker 3>and uniformly across the cosmos is.

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<v Speaker 2>Wrong, and that choice between a local gravitational anomaly and

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<v Speaker 2>a fundamental structural flaw in the universe itself. That's really

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<v Speaker 2>the entire pivot point of this whole discovery, isn't it is?

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<v Speaker 3>And we can only really address that choice once we

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<v Speaker 3>understand how on Earth it even made this detection, because

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<v Speaker 3>you can't just use a regular telescope when you're looking

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<v Speaker 3>that far back in time.

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<v Speaker 2>That sets the stage perfectly for the technical side, how

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<v Speaker 2>did they do it? How did they detect the speed?

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<v Speaker 2>They needed an extremely distant, effectively fixed reference point, and.

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<v Speaker 3>For that they chose radio galaxies as their cosmic markers. Now,

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<v Speaker 3>these are not your average spiral or elliptical galaxies. These

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<v Speaker 3>are very distant galaxies that are distinguished by these massive

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<v Speaker 3>jets of particles. They're powered by supermassive black holes at

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<v Speaker 3>their centers, and these jets emit incredibly powerful radio waves.

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<v Speaker 3>That's a form of electromagnetic radiation with very very long wavelengths.

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<v Speaker 2>And what is it about radio galaxies that makes them

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<v Speaker 2>the ideal targets for this kind of measurement as opposed to, say,

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<v Speaker 2>using standard optical telescopes like Hubble.

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<v Speaker 3>The key advantage is observational depth and penetration. In space,

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<v Speaker 3>visible light the kind our icee is easily scattered and blocked.

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<v Speaker 3>It gets absorbed by cosmic dust, by gas clouds, by

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<v Speaker 3>all sorts of intervening matter. So optical instruments can only

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<v Speaker 3>see so far with perfect clarity.

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<v Speaker 2>It's like trying to see through cosmic fog.

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<v Speaker 3>A perfect analogy. But radio waves, because of their very

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<v Speaker 3>long wavelengths, can essentially bypass that cosmic fog. They penetrate

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<v Speaker 3>the interstellar and intergalactic medium far more effectively. They just

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<v Speaker 3>sail right on through.

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<v Speaker 2>So by using radio telescopes. These researchers can see much,

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<v Speaker 2>much deeper into the cosmic structure. It gives them a

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<v Speaker 2>vastly larger sample size of objects to establish that universal

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<v Speaker 2>background reference frame.

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<v Speaker 3>Exactly, you're counting objects that are so incredibly far away

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<v Speaker 3>that their spatial distribution should perfectly reflect that large scale

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<v Speaker 3>uniformity that the cosmological principle assumes. You really need billions

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<v Speaker 3>of these faint sources to achieve the kind of statistical

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<v Speaker 3>precision required for this measurement.

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<v Speaker 2>Okay, so they have their targets billions of radio galaxies.

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<v Speaker 2>Now let's get into the physical mechanism of detection. They

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<v Speaker 2>aren't tracking a single galaxy over time like a police

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<v Speaker 2>radar gun. They're looking at the distribution of all of them.

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<v Speaker 3>So how does our solar system's motion translate into a

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<v Speaker 3>discernible pattern in these light sources. Let's talk about this

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<v Speaker 3>headwind principle.

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<v Speaker 2>Okay. The headwind principle relies on a couple of relativistic

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<v Speaker 2>effects that are tied to motion. The first is the

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<v Speaker 2>Doppler effect, which most people are familiar with. The second

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<v Speaker 2>is something called light aberration.

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<v Speaker 3>Let's start with the familiar one, then the Doppler effect. Right,

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<v Speaker 3>So if you're moving rapidly toward a stationary source of waves,

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<v Speaker 3>sound or light, doesn't matter. The waves appear compressed to you,

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<v Speaker 3>they get shifted to higher frequencies, and if you move away,

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<v Speaker 3>they appear stretched out shifted to lower frequencies. Think of

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<v Speaker 3>an ambulance.

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<v Speaker 2>Siren, right, It gets higher pitched as it comes towards you,

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<v Speaker 2>lower as it goes away.

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<v Speaker 3>Exactly. Now, when you apply that to light, means objects

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<v Speaker 3>were moving toward appear slightly brighter and bluer. That's the

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<v Speaker 3>higher frequency part, and objects we're moving away from appear

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<v Speaker 3>slightly dimmer and redder the lower frequency part. So this

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<v Speaker 3>introduces a fundamental asymmetry in the intensity of the light

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<v Speaker 3>we receive from different directions.

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<v Speaker 2>That makes sense, But the researchers weren't just measuring the

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<v Speaker 2>intensity of the light. They were counting the actual number

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<v Speaker 2>of galaxies. So how does that work.

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<v Speaker 3>That's where the second effect, light aberration, comes in. And

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<v Speaker 3>this is really what the headwind metaphor is all about.

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<v Speaker 3>Think of it like this. If you're running forward in

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<v Speaker 3>the rain, even if the rain is coming straight down,

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<v Speaker 3>more rain trops hit you in the face than on

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<v Speaker 3>your back.

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<v Speaker 2>Okay, I can picture that.

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<v Speaker 3>It's a similar idea with light. Our motion through space

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<v Speaker 3>causes a slight directional bending of the incoming light rays

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<v Speaker 3>from these distant galaxies. So objects that are actually distributed

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<v Speaker 3>perfectly uniformly across the sky will appear statistically to be

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<v Speaker 3>slightly more concentrated in the direction of our velocity. We

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<v Speaker 3>sort of sweep up more of them in our forward view.

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<v Speaker 2>So to put it all together, if the Solar system

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<v Speaker 2>is speeding toward the constellation Leo, we will perceive slightly

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<v Speaker 2>more radio galaxies in that specific direction, a kind of

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<v Speaker 2>subtle cosmic pile up, and this perceived asymmetry more galaxies

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<v Speaker 2>counted in one direction than the opposite. That is the

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<v Speaker 2>technical signature they're looking for. It's called a dipole anisocropy.

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<v Speaker 3>Percisely, it's an anisotropy, a lack of uniformity that should

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<v Speaker 3>be caused entirely by our own motion relative to that

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<v Speaker 3>distant static background. But I really have to stress this again,

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<v Speaker 3>this difference is absolutely minuscule. It's tiny. If the universe

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<v Speaker 3>truly adheres to the standard model, this dipole should be

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<v Speaker 3>incredibly faint. Detecting it requires counting sources in the billions

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<v Speaker 3>and using instruments of just immense sensitivity.

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<v Speaker 2>And to make those extremely sensitive measurements, the team relied

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<v Speaker 2>on what might be the world's most impressive listening device,

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<v Speaker 2>the Low Far telescope. The Low Frequency Array.

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<v Speaker 3>Lo FAR is absolutely critical to this discovery. It's important

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<v Speaker 3>to understand it's not a single massive dish like you

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<v Speaker 3>might picture. It's a network of thousands of small antenna

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<v Speaker 3>stations that are spread out across several countries in Europe,

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<v Speaker 3>and they're all linked together electronically to act as one

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<v Speaker 3>giant telescope.

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<v Speaker 2>So that distributed nature, having antennas so far apart, that

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<v Speaker 2>gives them an unparalleled baseline right the distance between its

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<v Speaker 2>farthest components, and that translates to incredible angular.

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<v Speaker 3>Resolution, incredible resolution and immense sensitivity, especially for detecting these

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<v Speaker 3>very faint low frequency radio waves from the early universe.

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<v Speaker 3>They could map the distribution of these radio galaxies with

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<v Speaker 3>a precision that previous single dish telescopes simply couldn't dream

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<v Speaker 3>of achieving.

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<v Speaker 2>So they took the primary data from lo FAR, and

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<v Speaker 2>the sources say they combine it with information from two

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<v Speaker 2>additional radio observatories. I assume that's to cross check their data.

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<v Speaker 3>Yes, to ensure their galaxy count was as comprehensive and

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<v Speaker 3>accurate as possible, to make sure they weren't missing anything.

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<v Speaker 3>But their challenge wasn't just collecting all this data, it

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<v Speaker 3>was analyzing it accurately, and that led to a really

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<v Speaker 3>key part of their work.

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<v Speaker 2>The statistical innovation. The sources note that the team needed

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<v Speaker 2>a new statistical method, specifically because many radio galaxies consist

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<v Speaker 2>of multiple components. Why was that such a big hurdle?

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<v Speaker 3>Well, imagine you're trying to count distant street lights from

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<v Speaker 3>a satellite. But sometimes a single street light isn't just

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<v Speaker 3>one bulb. Maybe it's a big sign with two or

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<v Speaker 3>three separate light bulbs very close together. If your telescope

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<v Speaker 3>doesn't have the resolution to distinguish them as part of

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<v Speaker 3>a single sign, you might count three lights when you

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<v Speaker 3>should really only be counting one originating source.

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<v Speaker 2>Ah. I see, And if you don't account for those

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<v Speaker 2>multi component sources correctly, you could artificially inflate or skew

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<v Speaker 2>your galaxy counts in certain areas of the sky, which

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<v Speaker 2>would ruin the whole measurement exactly right.

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<v Speaker 3>Radio galaxies are often these incredibly complex structures. You've got

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<v Speaker 3>the central core where the black hole is, and then

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<v Speaker 3>you have these two massive radio lobes, these jets extending

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<v Speaker 3>far out into space on either side. The oldest statistical

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<v Speaker 3>methods often struggled with this. They would sometimes treat these

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<v Speaker 3>lobes as separate sources from the core.

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<v Speaker 2>So the new statistical method developed by Boomis team was

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<v Speaker 2>designed to be smarter about that, to recognize that a

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<v Speaker 2>core and its two lobes are all part of one

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<v Speaker 2>single galaxy.

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<v Speaker 3>Yes, it counts for this multi component nature, ensuring that

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<v Speaker 3>the team was counting distinct originating galaxies rather than just

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<v Speaker 3>counting the individual bright parts of a single galaxy.

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<v Speaker 2>And this methodological rigor is so important because the source

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<v Speaker 2>material points out something that I found really interesting. This

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<v Speaker 2>improved analysis yielded measurement uncertainties that were larger but also

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<v Speaker 2>more realistic.

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<v Speaker 3>And that is a huge sign of robust, honest science.

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<v Speaker 3>When scientists report larger, more realistic uncertainties, it means they've

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<v Speaker 3>been conservative. It means they have fully acknowledged the inherent

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<v Speaker 3>imperfections and complexities of measuring this kind of data across

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<v Speaker 3>vast cosmic distances. They weren't trying to make their data

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<v Speaker 3>look tidier or more certain than it actually was.

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<v Speaker 2>And despite introducing these larger uncertainties, which should make it

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<v Speaker 2>harder to claim a.

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<v Speaker 3>Discovery, the measured signal was so powerful, so strong that

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<v Speaker 3>it still completely defied the standard model's expectations.

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<v Speaker 2>And that leads us directly to the statistical weight of

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<v Speaker 2>this finding. This is where the conversation turns from just

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<v Speaker 2>methodology to a genuine discovery. We have to talk about

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<v Speaker 2>five sigma. Even with the larger, more realistic uncertainties applied

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<v Speaker 2>by their new statistical method, the deviation from expectation exceeded

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<v Speaker 2>five sigma.

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<v Speaker 3>Five sigma is the gold standard of scientific discovery, especially

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<v Speaker 3>in particle physics and cosmology. To put that into context

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<v Speaker 3>for you, in many fields, a three sigma result is

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<v Speaker 3>considered pretty interesting. It's evidence of a signal, it makes

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<v Speaker 3>people pay attention. But five sigma. Five sigma means that

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<v Speaker 3>the probability that this result is just a statistical fluke,

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<v Speaker 3>some random error in the data that will vanish if

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<v Speaker 3>you measured again, is less than one in three point

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<v Speaker 3>five million.

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<v Speaker 2>One in three point five five million. It is the

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<v Speaker 2>threshold for popping the champagne and shouting we found something

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<v Speaker 2>new in physics. Why is such a stringent threshold necessary,

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<v Speaker 2>particularly in a field like cosmology.

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<v Speaker 3>It's because the theories you're testing, like the standard model,

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<v Speaker 3>are so incredibly successful and so fundamental. If you're going

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<v Speaker 3>to stand up and claim you found something that fundamentally

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<v Speaker 3>breaks decades of established physics, you had better be virtually

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<v Speaker 3>certain that your instrument or your analysis hasn't somehow misled you.

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<v Speaker 3>Five signal provides a statistical certainty. It's the community's way

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<v Speaker 3>of saying, Okay, this isn't noise. This discrepancy is physically real.

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<v Speaker 2>And what exactly is this robust physical discrepancy they found?

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<v Speaker 2>It's the specific anisotropy that dipole that we are just

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<v Speaker 2>discussing right.

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<v Speaker 3>Their measurement shows that the directional asymmetry and the distribution

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<v Speaker 3>of all those radio galaxies, that dipole is quantified as

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<v Speaker 3>being three point seven times stronger than what the standard

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<v Speaker 3>model predicts it should be.

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<v Speaker 2>So the measured headwind is three point seven times stronger

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<v Speaker 2>than the model allows. And if the strength of that

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<v Speaker 2>dipole directly correlates with our velocity relative to those distant sources.

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<v Speaker 2>Then our solar system must be traveling three point seven

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<v Speaker 2>times faster than the expected cosmological speed. That is the

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<v Speaker 2>core finding.

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<v Speaker 3>That is the core finding. It's not just a small deviation.

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<v Speaker 3>It's a profound conflict. If the distribution of matter in

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<v Speaker 3>the universe were truly uniform, and if we were moving

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<v Speaker 3>at the expected CMB derived velocity, the dipole that low

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<v Speaker 3>Far measured would be much much weaker. This excessive strength

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<v Speaker 3>indicates a velocity that is wholly incompatible with a smooth,

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<v Speaker 3>uniform universe.

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<v Speaker 2>What's so fascinating here, and what makes this so compelling,

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<v Speaker 2>is that the scientists didn't just stop at their own

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<v Speaker 2>lofar data. They proactively sought independent validation. And that's the

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<v Speaker 2>critical step that elevates this from just an interesting result

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<v Speaker 2>to a potential paradigm shift. The paper says, the new

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<v Speaker 2>results confirm earlier observations based on studying quasars.

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<v Speaker 3>This step is absolutely non negotiable for a claim this large.

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<v Speaker 3>You have to do this. Let's define quasars clearly for everyone.

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<v Speaker 3>They are the super mass of black holes at the

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<v Speaker 3>very heart of distant active galaxies. They're in the process

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<v Speaker 3>of consuming enormous amounts of matter, and as they do,

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<v Speaker 3>they heat up and emit so much energy that they

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<v Speaker 3>can outshine their entire host galaxy. They are the brightest

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<v Speaker 3>beacons in the universe.

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<v Speaker 2>So why is the quasar confirmation so important here? What

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<v Speaker 2>makes it such a powerful piece of evidence.

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<v Speaker 3>It's because the earlier studies that found a similar effect

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<v Speaker 3>were looking at quasars using infrared data. Now, think about

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<v Speaker 3>the difference there. The Boom study used radio waves, very

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<v Speaker 3>low frequency, very long wavelength, and focused on radio galaxies,

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<v Speaker 3>which are defined by their extended jets. The earlier confirming

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<v Speaker 3>studies used infrared light, a much higher frequency, shorter wavelength,

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<v Speaker 3>and focused on the extremely bright, compact central cores of quasars.

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<v Speaker 2>So the detection method was entirely different. They were using

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<v Speaker 2>a different part of the electromagnetic spectrum, and they were

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<v Speaker 2>measuring completely different types of distant objects, and yet they

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<v Speaker 2>yielded the same unusual effect.

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<v Speaker 3>This is the scientific clincher. It's what makes the result

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<v Speaker 3>so hard to dismiss. If two entirely independent observational techniques,

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<v Speaker 3>using two different cosmic marker populations, two different spectral bands

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<v Speaker 3>and two completely different instruments setups. If they both point

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<v Speaker 3>to the exact same massive, statistically significant directional asymmetry, then

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<v Speaker 3>the signal is almost certainly genuine.

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<v Speaker 2>It's not a fluke in the Lofar and Tennis exactly.

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<v Speaker 3>Yes, strongly suggests that this massive velocity they detected is

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<v Speaker 3>a real feature of our motion through the cosmic matter distribution,

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<v Speaker 3>and not some weird systematic error in the lo far

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<v Speaker 3>instruments with some peculiar property of how radio galaxies emit light.

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<v Speaker 2>And this just moves the conversation entirely away from questioning

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<v Speaker 2>the instruments and directly to questioning the fundamental laws of cosmology,

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<v Speaker 2>which leaves us with the inevitable and frankly enormous question,

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<v Speaker 2>if the measurement is correct, what has to be wrong

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<v Speaker 2>about our understanding of the universe.

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<v Speaker 3>Well, if we connect this to the bigger picture, the

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<v Speaker 3>entire framework of cosmology is now under a huge amount

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<v Speaker 3>of stress. A co author on the paper, a Professor

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<v Speaker 3>Dominic J. Schwartz, he frames the situation perfectly. He says,

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<v Speaker 3>if the Solar system is truly moving this fast, we

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<v Speaker 3>are forced to question fundamental assumptions about the large scale structure.

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<v Speaker 2>Of the universe, and the research has laid out two

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<v Speaker 2>major alternatives, two really distinct ways to interpret this excess speed,

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<v Speaker 2>and these two hypotheses force cosmologists down two radically different

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<v Speaker 2>theoretical roads. Let's break down the first one. We can

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<v Speaker 2>call it the kinematic hypothesis or hypothesis A.

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<v Speaker 3>Okay, so, hypothesis A basically says the universe's uniform on

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<v Speaker 3>large scales. It says the cosmological principle still holds. Therefore,

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<v Speaker 3>the conclusion must be that our solar system's motion is

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<v Speaker 3>genuinely physically far faster than we expected. The measurement is

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<v Speaker 3>a measurement of our actual speed, and.

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<v Speaker 2>If that's true, it means there has to be some enormous,

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<v Speaker 2>previously undetected gravitational force that's responsible for accelerating us at

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<v Speaker 2>this unexpected rate.

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<v Speaker 3>Precisely, we know about the gravitational pull of the Virgo

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<v Speaker 3>supercluster and the local group of galaxies, and our general

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<v Speaker 3>flow toward the Shapley supercluster what's sometimes called the Great attractor.

399
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<v Speaker 3>But all of those known forces are already factored into

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<v Speaker 3>the expected velocity of three hundred and seventy kilometers per second.

401
00:21:16.519 --> 00:21:18.960
<v Speaker 3>To account for a speed three point seven times greater,

402
00:21:19.319 --> 00:21:22.160
<v Speaker 3>you need to invoke either a colossal structure far larger

403
00:21:22.160 --> 00:21:24.680
<v Speaker 3>and more distant than anything we have currently mapped, or

404
00:21:24.680 --> 00:21:27.359
<v Speaker 3>some kind of unusual cosmological flow we don't understand.

405
00:21:27.839 --> 00:21:30.200
<v Speaker 2>This really reminds me of the debate from years ago

406
00:21:30.279 --> 00:21:32.119
<v Speaker 2>surrounding a concept called dark flow.

407
00:21:32.279 --> 00:21:37.000
<v Speaker 3>It's a fantastic parallel. Darkflow is this hypothesized non random

408
00:21:37.039 --> 00:21:41.119
<v Speaker 3>motion of entire galaxy clusters that couldn't be explained by

409
00:21:41.160 --> 00:21:45.960
<v Speaker 3>any known gravitational attractors within the observable universe. The suggestion

410
00:21:46.119 --> 00:21:48.119
<v Speaker 3>was that our whole local patch of the universe was

411
00:21:48.160 --> 00:21:51.359
<v Speaker 3>being pulled towards something absolutely massive that was lurking just

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<v Speaker 3>beyond the edge of what we can see. This new finding,

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<v Speaker 3>if you interpret it through this kinematic lens, implies a

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<v Speaker 3>velocity component for our solar system that is equal mysterious

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<v Speaker 3>and non standard.

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<v Speaker 2>So under hypothesis a the standard model of the universe

417
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<v Speaker 2>itself holds, But our local cosmic environment is vastly more

418
00:22:09.039 --> 00:22:12.519
<v Speaker 2>complex than we thought. We're either missing an enormous concentration

419
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<v Speaker 2>of mass, maybe a huge filament of dark matter that

420
00:22:15.319 --> 00:22:18.200
<v Speaker 2>is currently pulling on us, or maybe the fundamental laws

421
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<v Speaker 2>that govern gravity on these massive intergalactic scales needs some

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00:22:21.960 --> 00:22:22.680
<v Speaker 2>kind of adjustment.

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00:22:22.799 --> 00:22:25.519
<v Speaker 3>The big problem with hypothesis A, though, is that given

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00:22:25.599 --> 00:22:28.839
<v Speaker 3>how deep the low far data looks, it should be

425
00:22:28.880 --> 00:22:32.839
<v Speaker 3>measuring our velocity relative to objects so incredibly distant that

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00:22:33.000 --> 00:22:36.359
<v Speaker 3>any local gravitational tugs should be negligible. They should just

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00:22:36.440 --> 00:22:38.880
<v Speaker 3>average out. I mean, we're looking back to the relatively

428
00:22:38.960 --> 00:22:42.720
<v Speaker 3>early universe. For a local structure to create such a

429
00:22:42.799 --> 00:22:46.799
<v Speaker 3>massive dipole in the distant matter distribution, that structure would

430
00:22:46.799 --> 00:22:50.240
<v Speaker 3>need to be astronomically large, potentially spanning billions of light

431
00:22:50.319 --> 00:22:51.480
<v Speaker 3>years itself.

432
00:22:51.240 --> 00:22:53.920
<v Speaker 2>Which naturally leads us to this second and I would

433
00:22:54.000 --> 00:22:58.880
<v Speaker 2>argue far more radical alternative hypothesis B, the structural hypothesis.

434
00:22:59.000 --> 00:23:01.680
<v Speaker 3>Hypothesis B is the one that really keeps cosmologists up

435
00:23:01.680 --> 00:23:04.119
<v Speaker 3>at night. It suggests that our model of the universe

436
00:23:04.119 --> 00:23:07.519
<v Speaker 3>itself is fundamentally flawed. It implies that the distribution of

437
00:23:07.519 --> 00:23:10.880
<v Speaker 3>those radio galaxies the cosmic background of matter itself, is

438
00:23:11.279 --> 00:23:12.960
<v Speaker 3>less uniform than we have believed.

439
00:23:13.039 --> 00:23:15.519
<v Speaker 2>So in this scenario, the headwind isn't just because we're

440
00:23:15.559 --> 00:23:18.920
<v Speaker 2>moving fast, it's because the air itself is thicker. In

441
00:23:18.960 --> 00:23:19.559
<v Speaker 2>one direction.

442
00:23:19.720 --> 00:23:21.799
<v Speaker 3>That's a perfect way to put it. If the background

443
00:23:21.880 --> 00:23:26.000
<v Speaker 3>itself is not uniform, then the cosmological principle is violated.

444
00:23:26.240 --> 00:23:29.480
<v Speaker 3>The universe would be fundamentally anisotropic. It would genuinely look

445
00:23:29.519 --> 00:23:32.559
<v Speaker 3>different in different directions at these vast scales.

446
00:23:32.279 --> 00:23:35.119
<v Speaker 2>And that is a deep, deep challenge to the core

447
00:23:35.240 --> 00:23:39.920
<v Speaker 2>of modern physics. Why is the cosmological principle so crucial.

448
00:23:39.880 --> 00:23:44.000
<v Speaker 3>Because it underpins the mathematics we use. It dramatically simplifies

449
00:23:44.039 --> 00:23:48.319
<v Speaker 3>the solutions to Einstein's equations of general relativity on cosmic scales.

450
00:23:48.599 --> 00:23:51.880
<v Speaker 3>If the universe is not homogeneous and isotropic, our current

451
00:23:51.960 --> 00:23:55.440
<v Speaker 3>standard solutions to those field equations either break down or

452
00:23:55.559 --> 00:23:58.240
<v Speaker 3>the very least, they become vastly more complicated to solve.

453
00:23:58.519 --> 00:24:02.319
<v Speaker 2>And this kind of structural non uniformity would have profound

454
00:24:02.400 --> 00:24:05.519
<v Speaker 2>implications for our theories of the very early universe, wouldn't it,

455
00:24:05.680 --> 00:24:07.680
<v Speaker 2>Particularly the theory of cosmic inflation.

456
00:24:08.119 --> 00:24:12.279
<v Speaker 3>Absolutely. The theory of inflation states that just a fraction

457
00:24:12.319 --> 00:24:15.240
<v Speaker 3>of a second after the Big Bang, the universe underwent

458
00:24:15.279 --> 00:24:19.519
<v Speaker 3>this period of incredible exponential expansion, and the primary purpose

459
00:24:19.519 --> 00:24:24.119
<v Speaker 3>of inflation, cosmologically speaking, was to smooth out any initial

460
00:24:24.200 --> 00:24:28.240
<v Speaker 3>structural irregularities. It's the mechanism that's supposed to guarantee that

461
00:24:28.240 --> 00:24:31.920
<v Speaker 3>the universe looks the same everywhere. Is why the cosmological

462
00:24:31.960 --> 00:24:34.039
<v Speaker 3>principle is such a good fit for the standard model.

463
00:24:34.200 --> 00:24:37.799
<v Speaker 2>But if hypothesis B is true and the distant matter

464
00:24:37.880 --> 00:24:42.200
<v Speaker 2>distribution is inherently clumpy or textured or has a preferred direction,

465
00:24:42.839 --> 00:24:46.240
<v Speaker 2>it implies that inflation either didn't happen exactly as we thought,

466
00:24:46.920 --> 00:24:49.319
<v Speaker 2>or that it wasn't nearly as effective at smoothing out

467
00:24:49.319 --> 00:24:51.359
<v Speaker 2>the cosmos as our current models demand.

468
00:24:51.480 --> 00:24:54.240
<v Speaker 3>It raises the terrifying possibility that the cosmos has a

469
00:24:54.279 --> 00:24:57.440
<v Speaker 3>preferred direction or an axis on the largest scales, and

470
00:24:57.480 --> 00:24:59.720
<v Speaker 3>that's a concept that just fundamentally defies the idea of

471
00:24:59.720 --> 00:25:03.599
<v Speaker 3>an eyeotropic universe. If the dipole we're measuring isn't entirely

472
00:25:03.720 --> 00:25:06.039
<v Speaker 3>due to our motion, but is partly due to the

473
00:25:06.039 --> 00:25:08.839
<v Speaker 3>background density of galaxies being higher in one direction and

474
00:25:08.880 --> 00:25:12.039
<v Speaker 3>lower in another, then higher map of the cosmic web

475
00:25:12.079 --> 00:25:12.440
<v Speaker 3>is wrong.

476
00:25:12.880 --> 00:25:16.480
<v Speaker 2>So this one detection of a high velocity dipole forces

477
00:25:16.599 --> 00:25:20.160
<v Speaker 2>us into this incredible binary choice. Either we redefine our

478
00:25:20.200 --> 00:25:23.640
<v Speaker 2>local kinematics with hypothesis A, which requires us to find

479
00:25:23.640 --> 00:25:28.519
<v Speaker 2>some unseen colossal attractors, or we redefine the foundational structure

480
00:25:28.640 --> 00:25:32.480
<v Speaker 2>of the entire universe with hypothesis B, which challenges general

481
00:25:32.519 --> 00:25:36.279
<v Speaker 2>relativity and inflation theory itself. Neither of those options is

482
00:25:36.319 --> 00:25:38.799
<v Speaker 2>exactly palatable for established science.

483
00:25:38.839 --> 00:25:41.359
<v Speaker 3>And that is the absolute beauty of this work. The

484
00:25:41.400 --> 00:25:44.480
<v Speaker 3>study doesn't definitively choose between A and B, but it

485
00:25:44.559 --> 00:25:48.319
<v Speaker 3>powerfully concludes that these new observational methods, using the dep

486
00:25:48.319 --> 00:25:51.839
<v Speaker 3>breach of radio waves, advanced statistical tools, and independent cross checks,

487
00:25:52.039 --> 00:25:54.799
<v Speaker 3>can fundamentally reshape the questions we're even allowed to ask.

488
00:25:55.319 --> 00:25:58.799
<v Speaker 3>They have generated definitive evidence that something is profoundly unexpected

489
00:25:58.799 --> 00:26:00.519
<v Speaker 3>in our cosmic inventory.

490
00:26:00.240 --> 00:26:02.480
<v Speaker 2>And the research suggests that the next few years will

491
00:26:02.480 --> 00:26:05.519
<v Speaker 2>be focused on increasing the precision of these background measurements,

492
00:26:05.880 --> 00:26:09.400
<v Speaker 2>maybe using even more powerful telescopes pushing even further out

493
00:26:09.400 --> 00:26:13.319
<v Speaker 2>into the universe to see if this excessive dipole eventually dissipates.

494
00:26:13.960 --> 00:26:16.160
<v Speaker 2>If it remains strong even when looking back to the

495
00:26:16.200 --> 00:26:20.119
<v Speaker 2>earliest possible radio galaxies, that would heavily favor the structural

496
00:26:20.160 --> 00:26:21.680
<v Speaker 2>hypothesis hypothesis B.

497
00:26:21.960 --> 00:26:25.000
<v Speaker 3>But if the dipole signal gets weaker and disappears, the

498
00:26:25.079 --> 00:26:28.759
<v Speaker 3>farther out you look. That might favor the kinematic hypothesis.

499
00:26:28.880 --> 00:26:32.319
<v Speaker 3>Hypothesis A it would suggest the pole is more local.

500
00:26:33.160 --> 00:26:35.960
<v Speaker 3>This journey from a simple speed measurement to questioning the

501
00:26:36.039 --> 00:26:39.880
<v Speaker 3>very structure of reality is exactly why cosmology remains such

502
00:26:39.920 --> 00:26:43.480
<v Speaker 3>a fascinating and rapidly evolving field. We started with what

503
00:26:43.519 --> 00:26:46.640
<v Speaker 3>seemed like a technical detail, the Sun's speed, and we've

504
00:26:46.680 --> 00:26:49.640
<v Speaker 3>ended up asking whether the entirely universe's uniform, or if

505
00:26:49.680 --> 00:26:51.920
<v Speaker 3>it's structured in a way that completely defies our most

506
00:26:51.960 --> 00:26:53.279
<v Speaker 3>successful predictive model.

507
00:26:53.519 --> 00:26:56.319
<v Speaker 2>Let's just try to summarize this incredible journey for you,

508
00:26:56.400 --> 00:27:00.200
<v Speaker 2>our listener. We establish the baseline the universe suppose to

509
00:27:00.200 --> 00:27:03.559
<v Speaker 2>be smooth, and that assumption limits our expected velocity to

510
00:27:03.640 --> 00:27:06.960
<v Speaker 2>about three hundred and seventy kilometers per second. We then

511
00:27:07.119 --> 00:27:10.400
<v Speaker 2>use the unparalleled sensitivity of the Lofar radio array to

512
00:27:10.440 --> 00:27:14.599
<v Speaker 2>count billions of distant radio galaxies, measuring a faint asymmetry

513
00:27:14.759 --> 00:27:17.079
<v Speaker 2>a cosmic headwind caused by our motion.

514
00:27:17.079 --> 00:27:20.640
<v Speaker 3>And that headwind or dipole anisotropy, was found to be

515
00:27:20.680 --> 00:27:24.279
<v Speaker 3>a staggering three point seven times stronger than predicted. This

516
00:27:24.440 --> 00:27:27.440
<v Speaker 3>result was then confirmed at the rigorous five sigma level

517
00:27:27.440 --> 00:27:30.200
<v Speaker 3>of certainty, which essentially rules out the possibility of it

518
00:27:30.240 --> 00:27:33.279
<v Speaker 3>being a statistical fluke. And critically, this finding was independently

519
00:27:33.359 --> 00:27:36.319
<v Speaker 3>verified by earlier studies that were looking at infrared quasars,

520
00:27:36.400 --> 00:27:39.799
<v Speaker 3>guaranteeing that the signal is real and not an instrumental error, and.

521
00:27:39.720 --> 00:27:43.359
<v Speaker 2>That forces the entire scientific community to consider two major

522
00:27:43.519 --> 00:27:47.440
<v Speaker 2>radical paths forward. Either our solar system is being dramatically

523
00:27:47.440 --> 00:27:51.759
<v Speaker 2>pulled much faster than expected by some colossal, unseen mass concentrations.

524
00:27:51.759 --> 00:27:56.359
<v Speaker 2>That's hypothesis a the kinematic one, or the universe itself

525
00:27:56.400 --> 00:27:59.559
<v Speaker 2>at its very largest scales is not the smooth, uniform

526
00:27:59.599 --> 00:28:01.920
<v Speaker 2>back drip we have always assumed it to be, which

527
00:28:01.960 --> 00:28:06.839
<v Speaker 2>would violate the cosmological principle. That's hypothesis be the structural one, and.

528
00:28:06.799 --> 00:28:10.160
<v Speaker 3>The implications of hypothesis be the idea that the underlying

529
00:28:10.279 --> 00:28:13.640
<v Speaker 3>assumption of a uniform distribution of matter and the cosmos

530
00:28:13.799 --> 00:28:18.119
<v Speaker 3>which underpins decades of modern cosmological thinking, is just wrong.

531
00:28:18.240 --> 00:28:20.160
<v Speaker 3>They're absolutely staggering to consider.

532
00:28:20.279 --> 00:28:22.759
<v Speaker 2>So let's leave you with this. If the matter distribution

533
00:28:22.920 --> 00:28:26.319
<v Speaker 2>really is anisotropic, if the cosmos is clumpier or has

534
00:28:26.319 --> 00:28:29.160
<v Speaker 2>a preferred grain, or a bias in certain directions. What

535
00:28:29.319 --> 00:28:33.359
<v Speaker 2>unexpected textures, patterns, or voids might this newly revealed anisotropy

536
00:28:33.400 --> 00:28:34.200
<v Speaker 2>be pointing toward?

537
00:28:34.480 --> 00:28:38.440
<v Speaker 3>And if the universe really does have a large scale directionality,

538
00:28:38.880 --> 00:28:42.680
<v Speaker 3>how drastically might this non uniformity change our maps of

539
00:28:42.720 --> 00:28:45.279
<v Speaker 3>the cosmic web? I mean, think about it. We rely

540
00:28:45.359 --> 00:28:47.960
<v Speaker 3>on a smooth universe to calculate how old it is,

541
00:28:48.319 --> 00:28:51.799
<v Speaker 3>how dark energy is accelerating it, and how matter originally

542
00:28:51.839 --> 00:28:54.839
<v Speaker 3>clumped together to form the first stars and galaxies. If

543
00:28:54.880 --> 00:28:58.079
<v Speaker 3>the background isn't smooth, every single one of those fundamental

544
00:28:58.079 --> 00:29:01.920
<v Speaker 3>calculations is based on a false res This discovery might

545
00:29:01.960 --> 00:29:05.079
<v Speaker 3>not just tweak our cosmic history. It might require a

546
00:29:05.119 --> 00:29:07.839
<v Speaker 3>complete rewrite of the first second of the Big Bang itself.

547
00:29:08.039 --> 00:29:10.440
<v Speaker 2>It's a potent reminder, isn't it, that even when we

548
00:29:10.480 --> 00:29:13.480
<v Speaker 2>think we have the biggest answers locked down, the universe

549
00:29:13.559 --> 00:29:16.640
<v Speaker 2>always always finds a way to surprise us, pushing us

550
00:29:16.640 --> 00:29:20.200
<v Speaker 2>toward deeper and much more challenging truths. We really encourage

551
00:29:20.240 --> 00:30:00.799
<v Speaker 2>you to keep exploring these profound questions right alongside us,

552
00:30:01.119 --> 00:30:54.359
<v Speaker 2>most past the US school sto
