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>Have you ever just stopped and really considered what shaped

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<v Speaker 2>the universes?

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<v Speaker 3>Yeah?

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<v Speaker 2>Not its size, right, No, not the size, but it's

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<v Speaker 2>actual fundamental geometry for what the last century, the answer

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<v Speaker 2>that has really been the bedrock of modern cosmology has

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<v Speaker 2>been astonishingly simple. That it's perfect, perfectly uniform, consistent, and

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<v Speaker 2>this is the most important part, symmetrical.

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<v Speaker 3>And you know that assumption of universal symmetry. It's more

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<v Speaker 3>than just some elegant philosophical idea. Oh absolutely, it's what

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<v Speaker 3>allows physics to work on the grandest cosmic scales. I mean,

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<v Speaker 3>without it, the mathematical description of the universe, which is

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<v Speaker 3>all rooted in Einstein's general relativity, it just becomes impossible, unmanageable.

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<v Speaker 3>It simplifies the equations to a point where we can

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<v Speaker 3>actually build a working predictive model of the entire cosmos.

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<v Speaker 2>And that's the model we all learn about, right, the

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<v Speaker 2>one everyone references from undergraduate physics to the latest research papers,

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<v Speaker 2>the Standard Cosmological Model LAMB to CDM. It's beautiful in

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<v Speaker 2>its success. It explains everything from the slight temperature ripples

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<v Speaker 2>in the early universe all the way to the mechanism's

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<v Speaker 2>driving cosmic expansion.

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<v Speaker 3>He really does.

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<v Speaker 2>But what happens if we find out that this foundational assumption,

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<v Speaker 2>this idea of perfect symmetry is actually wrong. What if

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<v Speaker 2>the universe is well inherently lopsided.

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<v Speaker 3>That is precisely the core tension we are looking at today.

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<v Speaker 3>This discussion focuses on a major review, one that synthesizes

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<v Speaker 3>years and years of observational data that this elegant uniform

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<v Speaker 3>cosmos might actually be fundamentally asymmetric.

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<v Speaker 2>And it's not just a small problem.

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<v Speaker 3>No, it's a challenge to the standard model so profound

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<v Speaker 3>that some researchers are suggesting it forces us to reconsider

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<v Speaker 3>the most basic mathematical premises of space and time.

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<v Speaker 2>We're looking into what is I think maybe the most

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<v Speaker 2>significant structural challenge to the standard model yet the cosmic

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<v Speaker 2>Diepool anomaly. This is a scientific discord so measurable, so

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<v Speaker 2>robust across all these different observational techniques that it may

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<v Speaker 2>force physicists to what potentially scrap the current framework entirely

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<v Speaker 2>and truly go back to square one.

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<v Speaker 3>That's the question on the table. So our mission today

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<v Speaker 3>is to really understand the fundamental assumptions that birth this

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<v Speaker 3>symmetric universe model. Why one of the most precise consistency

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<v Speaker 3>tests in cosmology has failed so spectacularly in recent years,

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<v Speaker 3>and you know what a lopsided universe truly implies for

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<v Speaker 3>the future of physics.

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<v Speaker 2>Okay, let's unpack this, starting with that very first idea,

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<v Speaker 2>the idea of a perfectly symmetric universe.

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<v Speaker 3>So when we talk about the bedrock of modern cosmology,

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<v Speaker 3>we are really talking about two fundamental linked principles that

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<v Speaker 3>govern the cosmos on the largest scales, uniformity and isotropy,

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<v Speaker 3>and together they form the cosmological principle.

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<v Speaker 2>Okay, let's nail down those two terms, because I think

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<v Speaker 2>they're often used interchangeably, but they mean very distinct things

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<v Speaker 2>in this context, right they do.

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<v Speaker 3>So Uniformity or what we call homogeneity, means that if

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<v Speaker 3>you zoom out far enough, and we're talking scales exceeding

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<v Speaker 3>say one point two billion light years. The universe looks

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<v Speaker 3>the same.

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<v Speaker 2>Everywhere, so location doesn't matter, right.

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<v Speaker 3>Think of it this way. If you take a cubic

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<v Speaker 3>mile of water in the middle of the ocean, it

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<v Speaker 3>looks exactly the same as any other cubic mile of water.

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<v Speaker 2>You couldn't tell where you were just based on the

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<v Speaker 2>water itself.

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<v Speaker 3>Exactly, the average density, the chemical composition, it's all the same.

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<v Speaker 3>So similarly, in the universe, if you pick a random

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<v Speaker 3>billion light year cube of space in one location, it

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<v Speaker 3>will have the same average density of matter and the

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<v Speaker 3>same average distribution of galaxies as a cube taken from

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<v Speaker 3>the complete opposite side of the observable universe.

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<v Speaker 2>But hang on a second. We know the universe is clumpy.

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<v Speaker 2>I mean, we see galaxies, we see clusters of galaxies,

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<v Speaker 2>we see these huge voids. Isn't that already a violation

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<v Speaker 2>of homogeneity.

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<v Speaker 3>That is a critical point, and it's why we always

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<v Speaker 3>have to add that caveat on large scales. Okay, Yes, Locally,

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<v Speaker 3>the universe is extremely in homogeneous. I mean, if you

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<v Speaker 3>compared a cubic meter containing Earth to a cubic meter

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<v Speaker 3>of vacuum in deep space, they are vastly different. But

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<v Speaker 3>the cosmological principle argues that these local differences they just

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<v Speaker 3>smooth out completely once you average over truly immense volumes.

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<v Speaker 3>The structures what we call the cosmic web, they're just

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<v Speaker 3>you know, ripples on it, otherwise uniform fluid.

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<v Speaker 2>So homogeneity is about location independence, it doesn't matter where

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<v Speaker 2>you are. And the second principle isotropy. That's about direction independence.

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<v Speaker 3>Correct isotropy means the universe looks the same in all

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<v Speaker 3>directions from our vantage point. If you were floating in

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<v Speaker 3>deep space and looked left, right, up or down. The

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<v Speaker 3>overall statistical picture of the cosmos, the distribution of distant

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<v Speaker 3>light sources, the density of gas, it would all appear identical.

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<v Speaker 2>And the standard cosmological model LAMB to CDM it rests

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<v Speaker 2>squarely on both of these ideas being true.

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<v Speaker 3>Exactly on the conjunction of both isotropy and homogeneity. Once

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<v Speaker 3>you average things out on these massive scales. That's the

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<v Speaker 3>cosmological principle.

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<v Speaker 2>And this symmetric vision. It wasn't just like a pretty

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<v Speaker 2>philosophical choice. Historically, it was a practical necessity it was

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<v Speaker 2>shortcut for handling the monster that is general relativity.

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<v Speaker 3>Absolutely, the equations of general relativity describe how matter and

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<v Speaker 3>energy curve space time, and then how that curve space

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<v Speaker 3>time dictates where matter and energy move. They are incredibly

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<v Speaker 3>complex tensor equations.

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<v Speaker 2>So you couldn't possibly account for every single star.

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<v Speaker 3>Not even close. If you had to account for every star,

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<v Speaker 3>every galaxy in their unique gravityational interaction across the entire cosmos,

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<v Speaker 3>the equations would be impossible to solve analytically. You'd have

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<v Speaker 3>effectively infinite complexity that change is based on every tiny

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<v Speaker 3>clump of matter.

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<v Speaker 2>So by enforcing this assumption that the universe is homogeneous

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<v Speaker 2>and isotropic on large scales, cosmologists can basically treat the

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<v Speaker 2>whole universe as a smooth, perfectly fluid simple thing.

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<v Speaker 3>That's the trick. That assumption allows them to apply a specific,

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<v Speaker 3>highly constrained mathematical description space time, one that provides the

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<v Speaker 3>maximum possible symmetry. This specific structure is called the FLRW description.

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<v Speaker 2>Named after the scientists who developed.

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<v Speaker 3>It right Friedman, La Madra, Robertson, and Walker. They developed

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<v Speaker 3>it throughout the early twentieth century.

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<v Speaker 2>And the FLRW description is really the core mathematical engine

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<v Speaker 2>of the model. It takes that unmanageable complexity of general

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<v Speaker 2>relativity and turns it into a set of differential equations

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<v Speaker 2>that you can actually solve.

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<v Speaker 3>And that you can use to capture things like the

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<v Speaker 3>expansion rate of space.

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<v Speaker 2>It's the whole basis for the LAMB to CDM, the

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<v Speaker 2>entire thing.

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<v Speaker 3>It successfully captures the observed expansion, the geometry of space,

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<v Speaker 3>whether it's flat, open or closed, and it allows us

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<v Speaker 3>to insert the components we think are in there, like

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<v Speaker 3>dark energy and cold dark matter.

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<v Speaker 2>So if you lose the florw description, if.

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<v Speaker 3>The universe has proven to be fundamentally asymmetrical, the entire

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<v Speaker 3>foundation of LAMB to CDM just collapses. It forces a

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<v Speaker 3>complete mathematical overhaul. This is why it's so well sacred

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<v Speaker 3>to the field.

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<v Speaker 2>Okay, so cosmologists are already dealing with a pretty major

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<v Speaker 2>problem in the model, one that often dominates the news,

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<v Speaker 2>the Hubble tension, and that tells us the model is

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<v Speaker 2>already under some strain.

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<v Speaker 3>That's correct. The Hubble tension is the most widely publicized

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<v Speaker 3>issue right now. It all centers on determining the Hubble constant,

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<v Speaker 3>the exact rate at which the universe is currently expanding.

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<v Speaker 2>And the conflict here is rooted in a disagreement between

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<v Speaker 2>two different sets of measurements.

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<v Speaker 3>Precisely, you have measurements of the expansion rate taken from

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<v Speaker 3>the early universe.

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<v Speaker 2>Which is mainly from the cosmic microwave.

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<v Speaker 3>Back right, using data from the CMB, and then predicting

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<v Speaker 3>what the current rate should be, and that prediction doesn't

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<v Speaker 3>match the measurements we take from the nearby or more recent.

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<v Speaker 2>Universe, where we're using things like type ia, supernovae and

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<v Speaker 2>other local distance indicators exactly.

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<v Speaker 3>And there's a disagreement roughly eight to ten percent. It's

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<v Speaker 3>a conflict between early universe physics says X and late

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<v Speaker 3>universe observation says why so.

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<v Speaker 2>The Hubble tension suggests the problem with maybe what the

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<v Speaker 2>universe is made of, maybe dark energy behaves differently, or

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<v Speaker 2>there's a new relativistic particle we don't know about.

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<v Speaker 3>Or a problem with how the universes evolves.

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<v Speaker 2>Right, But the dipole anomaly, the subject of today, challenges

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<v Speaker 2>something much much.

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<v Speaker 3>Deeper it does, and this is the crucial distinction. The

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<v Speaker 3>Hubble tension challenges the parameters and the contents of LAMB

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<v Speaker 3>to CDM. It says, maybe the ingredients in our recipe

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<v Speaker 3>are slightly wrong, but.

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<v Speaker 2>The cosmic dipole anomaly.

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<v Speaker 3>It challenges the very geometric basis the FFLRW description upon

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<v Speaker 3>which LAMB to CDM is built. If the foundation itself

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<v Speaker 3>is flawed, if the universe is fundamentally asymmetric, then trying

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<v Speaker 3>to patch the cracks in the walls like the Hubble

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<v Speaker 3>tension because the secondary issue.

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<v Speaker 2>We're forced to ask a bigger question.

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<v Speaker 3>Is the universe simply not symmetric enough for the flor

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<v Speaker 3>W equations to even apply in the first place.

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<v Speaker 2>Okay, so to understand how scientists actually test that core

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<v Speaker 2>symmetry assumption, we have to look at the universe's baby picture,

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<v Speaker 2>the cosmic microwave background or CMB. The cmba burelic radiation

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<v Speaker 2>left over from the Big Bang.

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<v Speaker 3>It's essentially the universe's first light. It was released about

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<v Speaker 3>three hundred and eighty thousand years after the Big Bang,

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<v Speaker 3>which is when the cosmos finally cooled down enough for

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<v Speaker 3>electrons and protons to form neutral hydrogen atoms.

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<v Speaker 2>And before that, the universe was just an opaque plasma.

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<v Speaker 3>Completely opaque. You couldn't see through it, but after that moment,

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<v Speaker 3>light could stream freely, and we observe that light today.

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<v Speaker 3>It's been stretched by cosmic expansion over thirteen point eight

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<v Speaker 3>billion years. Now it appears as a faint, uniform glow

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<v Speaker 3>of microwaves baiting the entire sky.

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<v Speaker 2>And when cosmologists first measured this glow with real precision,

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<v Speaker 2>especially with satellites like WMAP and later PLANK, they were

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<v Speaker 2>just stunned by its uniformity.

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<v Speaker 3>Absolutely stunned. I mean, the CMB is uniform over the

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<v Speaker 3>entire sky to within one part in one hundred thousand.

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<v Speaker 4>Wow.

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<v Speaker 3>That is an astonishing degree of smoothness, and that uniformity

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<v Speaker 3>is the single biggest reason why cosmologists felt so confident

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<v Speaker 3>in the perfectly symmetric FLRW model.

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<v Speaker 2>The thinking being if the universe looked this smooth thirteen

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<v Speaker 2>point eight billion years ago, it seems safe to assume

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<v Speaker 2>it adheres to the rules of large scale homogeneity and

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<v Speaker 2>isotropy precisely.

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<v Speaker 3>But even this relic radiation has variations.

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<v Speaker 2>The little ripples that eventually seated galaxy formation right.

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<v Speaker 3>But the largest temperature difference we find is what we

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<v Speaker 3>call the CMB dipole. Anisotropye.

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<v Speaker 2>Okay, so anisotropy just means not isotropic, looks different in

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<v Speaker 2>different directions exactly.

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<v Speaker 3>And the CMB dipole anisotropy is the largest temperature trast

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<v Speaker 3>we see. It's a slight but very measurable difference where

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<v Speaker 3>one side of the sky is hotter and the opposite

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<v Speaker 3>side is cooler.

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<v Speaker 2>And the magnitude of this difference is about one part

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<v Speaker 2>in a thousand. That's a huge signal compared to the

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<v Speaker 2>overall smoothness.

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<v Speaker 3>It is a very big signal. You don't even need

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<v Speaker 3>super advanced equipment to detect it. But and this is crucial,

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<v Speaker 3>this specific large variation does not challenge LAMB to CDM

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<v Speaker 3>on its own.

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<v Speaker 2>In fact, it's expected.

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<v Speaker 3>It's entirely expected and necessary within the standard model.

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<v Speaker 2>Okay, So why is a huge hot spot and a

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<v Speaker 2>huge cold spot in the CMB actually expected in a

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<v Speaker 2>symmetrical universe. That sounds counterintuitive, it.

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<v Speaker 3>Does, but it comes down to the principle of relativity

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<v Speaker 3>in our own motion. The standard interpretation of the CMB

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<v Speaker 3>dipole anisotropy is that it's entirely due to our local

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<v Speaker 3>motion through the universe's rest frame.

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<v Speaker 2>The rest frame being the frame in which the CMB

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<v Speaker 2>would appear perfectly isotropic exactly. Let's use that classic analogy

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<v Speaker 2>running in the rain.

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<v Speaker 3>Right, So if you are standing still, the rain seems

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<v Speaker 3>to hit you perfectly vertically from straight above.

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<v Speaker 2>But if you start running forward.

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<v Speaker 3>The drops in front of you hit your face faster

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<v Speaker 3>and more frequently. That's the relativistic Doppler effect. As our

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<v Speaker 3>solar system and the Milky Way galaxy move relative to

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<v Speaker 3>the cmb's universal reference frame, the light from the CMB

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<v Speaker 3>in the direction of our motion gets blue shifted.

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<v Speaker 2>So it's crammed together and making it seem slightly hotter right.

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<v Speaker 3>And conversely, the light from the opposite direction, the direction

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<v Speaker 3>we're running away from, gets red shifted or stretched out,

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<v Speaker 3>making it seem slightly cooler.

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<v Speaker 2>Yeah, we can actually calculate our speed from that.

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<v Speaker 3>We can. The strength of this dipole signal allows cosmologists

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<v Speaker 3>to calculate our absolute velocity relative to the rest frame

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<v Speaker 3>of the early universe. The consensus result derived from the

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<v Speaker 3>precise Plank satellite data is that our local group of

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<v Speaker 3>galaxies is cruising through space at roughly three hundred and

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<v Speaker 3>seventy kilometers per second.

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<v Speaker 2>Wow per second per.

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<v Speaker 3>Second towards a specific point in the sky near the

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<v Speaker 3>constellation Hydra.

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<v Speaker 2>So, just to be clear, the small the only symmetry

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<v Speaker 2>we see in the CMB is entirely attributed to the

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<v Speaker 2>fact that we are moving. Yes, it's an observational effect

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<v Speaker 2>tied to us the observers, not a fundamental flaw in

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<v Speaker 2>the universe's geometric structure.

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<v Speaker 3>That's the consensus interpretation, and it holds up beautifully for

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<v Speaker 3>the CMB data. However, here's where the deep philosophical question

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<v Speaker 3>comes in. Okay, if the universe is truly governed by

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<v Speaker 3>the symmetric FLRW description, then every large scale observable component

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<v Speaker 3>of the cosmos must adhere to the same physical rules

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<v Speaker 3>dictated by that symmetry.

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<v Speaker 2>So the core test then is whether the rest of

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<v Speaker 2>the universe agrees with that imposed asymmetry.

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<v Speaker 3>That is the ultimate consistency check. If we are truly

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<v Speaker 3>moving at three hundred and seventy kilometers per second relative

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<v Speaker 3>to the early universe, we should see all truly distant structures,

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<v Speaker 3>the distribution of galaxies, the brightness of quasars respond to

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<v Speaker 3>that speed in a predictable, uniform.

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<v Speaker 2>And quantifiable way, and if they don't.

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<v Speaker 3>If they don't, then our movement isn't the whole story

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<v Speaker 3>or the GMAC model we're using the cat aculate these

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<v Speaker 3>effects is fundamentally broken.

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<v Speaker 2>And this realization that the CMB dipole mandates a corresponding

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<v Speaker 2>dipole in the matterfield is what leads us directly into

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<v Speaker 2>the most critical experiment designed to test cosmic symmetry. So

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<v Speaker 2>now we get to the specific scientific challenge designed to

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<v Speaker 2>test this required cosmic consistency, the Elis Baldwin test.

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<v Speaker 3>Right back in nineteen eighty four, George Ellis and John Baldwin,

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<v Speaker 3>two figures known for their really rigorous application of general

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<v Speaker 3>relativity to cosmology, proposed this specific check.

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<v Speaker 2>And the question was sharp and simple.

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<v Speaker 3>Very if the symmetric FLRW framework is correct, then the

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<v Speaker 3>variations we observe in the early Universe's light the CMB

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<v Speaker 3>dipole must be perfectly reflected by a similar dipole anisotropy

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<v Speaker 3>in the sky distribution of distant astronomical sources.

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<v Speaker 2>The matter dipole, the matter dipole.

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<v Speaker 3>They weren't just proposing a measurement, they were proposing a

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<v Speaker 3>mandatory relationship. It puts the light field and the matterfield

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<v Speaker 3>into direct confrontation with that core FLRW assumption.

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<v Speaker 2>It's the ultimate benchmark test for the standard model's geometric foundation.

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<v Speaker 3>I think. So you have the radiation field, this pristine

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<v Speaker 3>information from thirteen point eight billion years ago telling us

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<v Speaker 3>our velocity, and then you have the matter field, the

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<v Speaker 3>distribution of trillions of galaxies stretching across vast cosmic distances,

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<v Speaker 3>which should, in theory react in a very calculated way

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<v Speaker 3>to that velocity.

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<v Speaker 2>Now, to perform this test correctly, the data has to

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<v Speaker 2>satisfy a really strict requirement. The astronomical sources you use

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<v Speaker 2>must be very distant.

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<v Speaker 3>This point cannot be overstated. We need to look far

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<v Speaker 3>enough out that the universe has smoothed out that it

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<v Speaker 3>meets that large scale homogeneity assumption.

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<v Speaker 2>So if you use sources that are too nearby.

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<v Speaker 3>If you use sources that are too nearby, say within

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<v Speaker 3>our local superpluster, which might be a few hundred million

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<v Speaker 3>light years across, you run the risk of measuring what

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<v Speaker 3>we call a spurious clustering dipole.

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<v Speaker 2>Okay, let's break that down. Spurrious is meaning what exactly.

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<v Speaker 3>Spurrious just means false or misleading in the nearby universe.

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<v Speaker 3>Gravity hasn't finished its work yet. You know, galaxies are

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<v Speaker 3>still clumped together into filaments and walls and these immense voids.

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<v Speaker 2>The cosmic web, the cosmic web.

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<v Speaker 3>So if we just happen to be sitting on the

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<v Speaker 3>edge of a massive over density of galaxies, we might

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<v Speaker 3>measure an apparent dipole simply because there are more galaxies

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<v Speaker 3>to our left than to our right.

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<v Speaker 2>And that asymmetry would just be a local effect exactly.

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<v Speaker 3>It would be tied to the small scale clumpiness of matter,

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<v Speaker 3>not a universal effect dictated by our motion through the

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<v Speaker 3>CMB frame.

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<v Speaker 2>So to truly test the universe's foundational structure in its symmetry,

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<v Speaker 2>we need sources so remote that we're averaging over many,

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<v Speaker 2>many billions of light years.

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<v Speaker 3>That's the only way it ensures that any dipole signal

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<v Speaker 3>we see reflects the deep, large scale structure of the

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<v Speaker 3>cosmos rather than some local fluctuation.

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<v Speaker 2>And this is why researchers focus on things like quasars.

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<v Speaker 3>Quasars and distant radio galaxies. They're excellent deep space probes

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<v Speaker 3>because they're so incredibly luminous. They allow us to gain

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00:16:57.320 --> 00:17:00.519
<v Speaker 3>the statistical power necessary to average out those local in

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<v Speaker 3>homogeneities and see what the universe is really doing on

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00:17:03.519 --> 00:17:07.079
<v Speaker 3>scales large enough to satisfy that FLRW.

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<v Speaker 2>Premis so, the hypothesis is actually elegantly simple. It is,

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<v Speaker 2>if the FLRW metric is correct, the dipole amplitude calculated

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<v Speaker 2>from the distant matter field must quantitatively match the dipole

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<v Speaker 2>amplitude observed in the CMB.

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<v Speaker 3>They have to be consistent in both direction and magnitude.

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<v Speaker 2>And conversely, if there's discord a measurable mismatch between the

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<v Speaker 2>two dipole signals, that would directly challenge the fundamental FLRW.

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<v Speaker 3>Description and put the entire standard model into question.

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<v Speaker 2>It's an incredible test, and it's worth noting too the

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<v Speaker 2>huge gap in time between the proposal of this test

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<v Speaker 2>in nineteen eighty four and its actual execution.

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<v Speaker 3>Oh absolutely. When Ellis in Baldwin proposed it, it was almost

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<v Speaker 3>a theoretical challenge, a thought experiment. The observational data simply

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<v Speaker 3>didn't exist to reach the necessary statistical precision.

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<v Speaker 2>We just couldn't see far enough or wide enough, right.

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<v Speaker 3>We didn't have all sky surveys is with high enough

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<v Speaker 3>sensitivity and enough depth to measure hundreds of thousands of

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<v Speaker 3>truly distant, statistically independent sources. It has only been in

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<v Speaker 3>the last what five or six years, thanks to modern

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<v Speaker 3>radio telescopes and deep infra red surveys, that we finally

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<v Speaker 3>accumulated the precise catalogs required to run this critical check.

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<v Speaker 2>So we're truly moving from the theoretical foundation to the

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<v Speaker 2>actual measured reality we are, and the results of that

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<v Speaker 2>measured reality, according to the research, are not kind to

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<v Speaker 2>the standard model.

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<v Speaker 3>So let's just state the core finding as clearly as

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<v Speaker 3>possible as it's synthesized in this review. The universe fails

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<v Speaker 3>the Ellis Baldwin test.

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<v Speaker 2>These it completely.

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<v Speaker 3>The variation observed in distant matter does not match the

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<v Speaker 3>variation observed in the CMB, and this mismatch is what

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<v Speaker 3>we call the cosmic dipole anomaly.

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<v Speaker 2>And it's a quantitative failure, right, and not just a

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<v Speaker 2>vague feel.

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<v Speaker 3>Oh, absolutely quantitative. If we calculate the expected dipole anisotropy

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<v Speaker 3>in matter based purely on the velocity we get from

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<v Speaker 3>the CMB, that three hundred and seventy kilometers per secon movement, and.

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<v Speaker 2>Then we measure the actual dipole anisotropy from the distribution

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<v Speaker 2>of distant radio galaxies.

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<v Speaker 3>The expected and the measured numbers simply don't align, and.

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<v Speaker 2>They mismatch in a very specific and telling way.

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<v Speaker 3>They do. The directional data is the direction of the

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<v Speaker 3>dipole is generally consistent. The hot side of the CMB,

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<v Speaker 3>the direction we're moving into it aligns roughly with the

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<v Speaker 3>direction where the distant matter sources seem to be slightly

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<v Speaker 3>more clustered.

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<v Speaker 2>Okay, so that part makes sense.

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<v Speaker 3>That directional consistency makes sense if our local motion is

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<v Speaker 3>part of the explanation.

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00:19:33.160 --> 00:19:36.319
<v Speaker 2>But it's the amplitude, the strength of the signal that's

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<v Speaker 2>where the failure lies.

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<v Speaker 3>Precisely, the measured amplitude of the matter dipole is consistently

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<v Speaker 3>across multiple studies and different source catalogs, found to be

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<v Speaker 3>several times larger than the amplitude predicted purely by our

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00:19:49.480 --> 00:19:50.519
<v Speaker 3>CMB derived motion.

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<v Speaker 2>So, just to put that in perspective, if the CMB

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<v Speaker 2>dipole says you are moving at three hundred and seventy

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<v Speaker 2>kilometers per second, the distant matter dipole is essentially shouting

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<v Speaker 2>back no. Based on how lopsided I look, you should

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00:20:03.200 --> 00:20:06.119
<v Speaker 2>be moving at something like fifteen hundred kilometers per second.

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00:20:05.920 --> 00:20:08.559
<v Speaker 3>Or even two thousand. That's a perfect way to visualize

401
00:20:08.559 --> 00:20:11.200
<v Speaker 3>the discord. The fact that the amplitude is so off

402
00:20:11.519 --> 00:20:13.880
<v Speaker 3>means the universe doesn't look the same in all directions

403
00:20:13.920 --> 00:20:16.440
<v Speaker 3>in the way the standard model forces it to predict.

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00:20:16.759 --> 00:20:20.759
<v Speaker 2>It's a profound quantitative failure of cosmic symmetry, and.

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00:20:20.799 --> 00:20:24.119
<v Speaker 3>It indicates that our local motion is not the sole

406
00:20:24.240 --> 00:20:29.000
<v Speaker 3>factor determining the dipole observed in the large scale matter distribution.

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00:20:29.759 --> 00:20:30.799
<v Speaker 3>Something else is going on.

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00:20:31.119 --> 00:20:33.720
<v Speaker 2>And here's where it gets really interesting, because when you

409
00:20:33.799 --> 00:20:37.480
<v Speaker 2>have conflicting results like this, the first and most scientific

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00:20:37.519 --> 00:20:40.160
<v Speaker 2>reaction is always to blame your equipment.

411
00:20:39.839 --> 00:20:42.039
<v Speaker 3>Of course systematic errors.

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00:20:42.200 --> 00:20:46.240
<v Speaker 2>But the research review emphasizes just how robust this finding is.

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00:20:46.480 --> 00:20:50.279
<v Speaker 3>The scientific confidence in this anomaly is extremely high, and

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00:20:50.319 --> 00:20:55.680
<v Speaker 3>that's because the result holds up across diverse instruments, diverse wavelengths,

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00:20:55.720 --> 00:20:58.960
<v Speaker 3>and independent catalogs of distant sources. We are not talking

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00:20:59.000 --> 00:21:01.799
<v Speaker 3>about a single telescope malfunctioning here, Okay.

417
00:21:01.519 --> 00:21:04.440
<v Speaker 2>So give us some specifics on that. What confirms this confidence?

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00:21:04.759 --> 00:21:08.240
<v Speaker 3>Well, consider the data being used. Researchers obtain the same

419
00:21:08.359 --> 00:21:12.680
<v Speaker 3>dipole anomaly result that mismatch in amplitude using instruments observing

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00:21:12.720 --> 00:21:15.680
<v Speaker 3>it fundamentally different parts of the electromagnetic.

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00:21:14.960 --> 00:21:17.039
<v Speaker 2>Spectrum, so not just one type of light.

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00:21:17.440 --> 00:21:21.440
<v Speaker 3>No, it's been seen using terrestrial radio telescopes that are

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00:21:21.440 --> 00:21:25.079
<v Speaker 3>mapping millions of distant radio galaxies, and it has been

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00:21:25.119 --> 00:21:29.119
<v Speaker 3>confirmed using separate satellite instruments that are observing galaxies at

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00:21:29.160 --> 00:21:30.920
<v Speaker 3>mid infrared wavelengths, so.

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00:21:30.839 --> 00:21:35.400
<v Speaker 2>Those are completely independent ways of surveying the distant cosmos completely.

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00:21:35.720 --> 00:21:38.880
<v Speaker 3>Radio surveys are looking primarily at the emission from supermassive

428
00:21:38.920 --> 00:21:42.079
<v Speaker 3>black holes and active galaxies, while the infrared surveys are

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00:21:42.079 --> 00:21:44.599
<v Speaker 3>looking at the overall thermal emission from dust and star

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00:21:44.680 --> 00:21:45.920
<v Speaker 3>formation in galaxies.

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00:21:46.119 --> 00:21:48.920
<v Speaker 2>And if two fundamentally different ways of measuring the distant

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00:21:48.960 --> 00:21:52.680
<v Speaker 2>cosmos give you the same unexpected asymmetry.

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00:21:51.920 --> 00:21:55.960
<v Speaker 3>It rules out simple observational bias or dust absorption or

434
00:21:55.960 --> 00:21:59.880
<v Speaker 3>atmospheric interference. The problem almost certainly lies in the model

435
00:22:00.039 --> 00:22:03.920
<v Speaker 3>are using to interpret the data the FLRW geometry.

436
00:22:03.359 --> 00:22:07.200
<v Speaker 2>Itself, so that strengthens the conclusion that the problem isn't observational.

437
00:22:07.599 --> 00:22:11.359
<v Speaker 2>The problem is inherent to our current cosmological description. The

438
00:22:11.440 --> 00:22:14.079
<v Speaker 2>universe is genuinely lopsided when we look at it with

439
00:22:14.160 --> 00:22:15.519
<v Speaker 2>enough precision, and.

440
00:22:15.400 --> 00:22:18.279
<v Speaker 3>This is why the anomaly is so severe. If the

441
00:22:18.319 --> 00:22:22.519
<v Speaker 3>standard model symmetry assumption is correct, the CMB derived velocity

442
00:22:22.720 --> 00:22:26.599
<v Speaker 3>must create a predictable dipole in the distant matterfield. The

443
00:22:26.680 --> 00:22:31.279
<v Speaker 3>failure implies that the fundamental symmetry assumptions underpinning the FLRW

444
00:22:31.400 --> 00:22:33.759
<v Speaker 3>framework are simply inadequate.

445
00:22:33.960 --> 00:22:35.880
<v Speaker 2>This isn't just about tweaking a parameter.

446
00:22:36.319 --> 00:22:39.440
<v Speaker 3>Note it suggests there's a preferred frame or a directionality

447
00:22:39.480 --> 00:22:41.720
<v Speaker 3>to the universe that the current model cannot account for

448
00:22:41.799 --> 00:22:42.160
<v Speaker 3>at all.

449
00:22:42.400 --> 00:22:46.319
<v Speaker 2>But you mentioned earlier that despite this severity, the astronomical

450
00:22:46.319 --> 00:22:50.559
<v Speaker 2>community has largely chosen to ignore it, compared to say,

451
00:22:50.680 --> 00:22:53.680
<v Speaker 2>the attention given to the Hubble tension. Why would there

452
00:22:53.680 --> 00:22:57.440
<v Speaker 2>be hesitation to tackle a flaw that seems so foundational.

453
00:22:57.759 --> 00:23:00.319
<v Speaker 3>I think the difficulty lies in the sheer severe of

454
00:23:00.319 --> 00:23:03.400
<v Speaker 3>the solution required, or, to put it a bit less charitably,

455
00:23:03.440 --> 00:23:05.160
<v Speaker 3>the fear of mathematical chaos.

456
00:23:05.359 --> 00:23:05.920
<v Speaker 2>What do you mean?

457
00:23:06.000 --> 00:23:09.400
<v Speaker 3>The Hubble tension, while it's a serious problem, still allows

458
00:23:09.400 --> 00:23:14.519
<v Speaker 3>cosmologists to play within the existing lambda CDM structure. Maybe

459
00:23:14.519 --> 00:23:16.799
<v Speaker 3>they can change the equation of state for dark energy,

460
00:23:16.880 --> 00:23:19.480
<v Speaker 3>or they introduce a new particle. It requires a patch

461
00:23:19.599 --> 00:23:20.079
<v Speaker 3>a fix.

462
00:23:20.559 --> 00:23:25.319
<v Speaker 2>But the cosmic dipole anomaly challenges the geometric premis itself exactly.

463
00:23:25.359 --> 00:23:28.559
<v Speaker 3>It's like discovering that the mathematical ruler you use to

464
00:23:28.599 --> 00:23:31.799
<v Speaker 3>design the foundation of your house was actually curved and uneven,

465
00:23:32.160 --> 00:23:35.359
<v Speaker 3>but the blueprints mandated that it had to be perfectly straight.

466
00:23:35.519 --> 00:23:37.839
<v Speaker 2>You can't just repaint the walls.

467
00:23:37.480 --> 00:23:40.319
<v Speaker 3>You have to rebuild the entire foundation. If the universe

468
00:23:40.359 --> 00:23:45.799
<v Speaker 3>isn't sufficiently homogeneous or isotropic to be described by FLRW,

469
00:23:46.279 --> 00:23:49.319
<v Speaker 3>then we lose the ability to use those vastly simplified

470
00:23:49.319 --> 00:23:52.640
<v Speaker 3>Einstein equations, And that's why it's often relegated to the sidelines.

471
00:23:52.880 --> 00:23:57.160
<v Speaker 3>It's just too painful and too disruptive to fundamental physics.

472
00:23:57.200 --> 00:24:00.559
<v Speaker 2>So the insight here is crucial. The dipole and is

473
00:24:00.599 --> 00:24:03.680
<v Speaker 2>more fundamental than the Hubble tension because it directly attacks

474
00:24:03.720 --> 00:24:07.319
<v Speaker 2>that geometric assumption. Right we are talking about rewriting the

475
00:24:07.359 --> 00:24:10.960
<v Speaker 2>mathematics that describe spacetime itself, not just the stuff floating

476
00:24:10.960 --> 00:24:14.240
<v Speaker 2>around within it. It's really the highest stakes tension in

477
00:24:14.279 --> 00:24:15.400
<v Speaker 2>cosmology right now.

478
00:24:15.680 --> 00:24:18.880
<v Speaker 3>It forces us to confront the possibility that the universe

479
00:24:18.920 --> 00:24:22.440
<v Speaker 3>is genuinely anisotropic, that when you look in one direction,

480
00:24:22.960 --> 00:24:26.359
<v Speaker 3>you are fundamentally seeing something different than when you look

481
00:24:26.359 --> 00:24:28.920
<v Speaker 3>in the opposite direction, even after you account for our

482
00:24:28.920 --> 00:24:33.680
<v Speaker 3>own motion, and that would overturn the very philosophical basis

483
00:24:33.680 --> 00:24:38.160
<v Speaker 3>of modern cosmology, the cosmological principle, which holds that our

484
00:24:38.200 --> 00:24:40.759
<v Speaker 3>location and our direction are not special.

485
00:24:41.240 --> 00:24:43.359
<v Speaker 2>So what does this all mean for the future of physics?

486
00:24:43.440 --> 00:24:46.839
<v Speaker 2>I mean, if we take the cosmic dipole anomaly seriously,

487
00:24:47.279 --> 00:24:50.680
<v Speaker 2>what is the profound consequence and what are the possible

488
00:24:50.720 --> 00:24:51.920
<v Speaker 2>paths forward from here?

489
00:24:52.160 --> 00:24:55.039
<v Speaker 3>Well, the profound consequence is the need to abandon the

490
00:24:55.079 --> 00:24:59.319
<v Speaker 3>convenience of the FLRW description. There's just no easy way

491
00:24:59.359 --> 00:25:02.359
<v Speaker 3>to patch up this problem within the existing framework that

492
00:25:02.440 --> 00:25:03.559
<v Speaker 3>assumes perfect symmetry.

493
00:25:03.720 --> 00:25:05.799
<v Speaker 2>So solving the dipole anomaly.

494
00:25:05.400 --> 00:25:08.480
<v Speaker 3>It may require moving beyond LAMB to CDM entirely and

495
00:25:08.519 --> 00:25:11.000
<v Speaker 3>going back to square one to construct a new cosmological

496
00:25:11.079 --> 00:25:13.720
<v Speaker 3>model based on asymmetric space time solutions.

497
00:25:13.839 --> 00:25:15.960
<v Speaker 2>Going back to square one, that means we have to

498
00:25:15.960 --> 00:25:18.599
<v Speaker 2>find a whole new mathematical description of the large scale

499
00:25:18.680 --> 00:25:21.480
<v Speaker 2>universe that does not assume perfect symmetry but still accounts

500
00:25:21.480 --> 00:25:22.599
<v Speaker 2>for everything else we see.

501
00:25:22.799 --> 00:25:25.160
<v Speaker 3>Right, It still has to account for the observed expansion

502
00:25:25.559 --> 00:25:29.440
<v Speaker 3>and the near uniformity of the CMB everywhere else. It

503
00:25:29.519 --> 00:25:32.079
<v Speaker 3>sounds like an intimidating amount of complex mathematics.

504
00:25:32.119 --> 00:25:33.160
<v Speaker 2>It sounds terrifying.

505
00:25:33.240 --> 00:25:36.599
<v Speaker 3>It is an enormous undertaking. When you remove those symmetry constraints,

506
00:25:37.000 --> 00:25:41.519
<v Speaker 3>Einstein's equations just explode in complexity. We'd have to look

507
00:25:41.559 --> 00:25:45.400
<v Speaker 3>at what are called non FLRWS solutions, you know, models

508
00:25:45.440 --> 00:25:50.480
<v Speaker 3>like the Lametrotolman Bondi or LTB solution, which describes an

509
00:25:50.519 --> 00:25:55.039
<v Speaker 3>inhomogeneous but spherically symmetric space time, or the various Biyonkey

510
00:25:55.160 --> 00:25:57.920
<v Speaker 3>models which allow for global anisotropy.

511
00:25:58.200 --> 00:26:01.359
<v Speaker 2>And why are these non symmetric solution so much harder to.

512
00:26:01.319 --> 00:26:04.359
<v Speaker 3>Work with Because they introduce variables that change depending on

513
00:26:04.440 --> 00:26:07.680
<v Speaker 3>direction and location, and they don't provide the tidy, closed

514
00:26:07.720 --> 00:26:12.480
<v Speaker 3>form solutions that FLRW gives us. They require massive computational power.

515
00:26:12.200 --> 00:26:13.799
<v Speaker 2>And fitting them to all the data we have.

516
00:26:14.079 --> 00:26:18.319
<v Speaker 3>It becomes computationally crippling. The elegance of FLRW is that

517
00:26:18.359 --> 00:26:21.799
<v Speaker 3>it explained ninety percent of the universe with these simple equations.

518
00:26:22.440 --> 00:26:27.200
<v Speaker 3>These new models might require solving differential equations numerically across

519
00:26:27.279 --> 00:26:30.759
<v Speaker 3>every single point in space. It's why symmetry was assumed

520
00:26:30.799 --> 00:26:33.680
<v Speaker 3>for so long it was a practical necessity.

521
00:26:33.720 --> 00:26:36.359
<v Speaker 2>So the implication is clear. The universe is telling us

522
00:26:36.440 --> 00:26:40.720
<v Speaker 2>that reality is just messier than our idealized math.

523
00:26:40.839 --> 00:26:41.880
<v Speaker 3>That's a great way to put it.

524
00:26:42.079 --> 00:26:45.400
<v Speaker 2>But even as this conceptual challenge is forcing us backward,

525
00:26:45.680 --> 00:26:49.279
<v Speaker 2>technology is rushing forward giving us the tools to map

526
00:26:49.319 --> 00:26:50.640
<v Speaker 2>that messiness, and.

527
00:26:50.519 --> 00:26:53.799
<v Speaker 3>That new data avalanche is critical. It's going to provide

528
00:26:53.839 --> 00:26:57.720
<v Speaker 3>the necessary constraints for constructing any new asymmetrical model. We're

529
00:26:57.799 --> 00:27:00.319
<v Speaker 3>entering a golden age of cosmology where the PRIs decision

530
00:27:00.359 --> 00:27:03.359
<v Speaker 3>of our observation is finally yielding results that actively break

531
00:27:03.359 --> 00:27:03.960
<v Speaker 3>our best.

532
00:27:03.720 --> 00:27:06.759
<v Speaker 2>Theories, which forces a shift, a necessary one. Okay, let's

533
00:27:06.759 --> 00:27:09.319
<v Speaker 2>look specifically at the projects mentioned in the research that

534
00:27:09.359 --> 00:27:11.839
<v Speaker 2>will contribute to charting this asymmetry right.

535
00:27:12.359 --> 00:27:15.559
<v Speaker 3>First, on the satellite front, we have Euclid and SPHEREx.

536
00:27:16.440 --> 00:27:19.160
<v Speaker 3>Euclid is already up there and it's focused on mapping

537
00:27:19.240 --> 00:27:22.920
<v Speaker 3>the dark universe. Its primary mission is to create a

538
00:27:23.000 --> 00:27:26.960
<v Speaker 3>massive three D map of billions of galaxies over a

539
00:27:27.079 --> 00:27:28.079
<v Speaker 3>vast extent.

540
00:27:27.799 --> 00:27:30.640
<v Speaker 2>Of the sky, so that will dramatically improve our census

541
00:27:30.640 --> 00:27:31.920
<v Speaker 2>of distant matter exactly.

542
00:27:32.000 --> 00:27:34.200
<v Speaker 3>It will allow us to map the cosmic web with

543
00:27:34.400 --> 00:27:38.839
<v Speaker 3>unprecedented fidelity. If the universe is lopsided, EUCLID will see

544
00:27:38.880 --> 00:27:42.359
<v Speaker 3>those directional differences in the galaxy clustering with stunning precision.

545
00:27:42.880 --> 00:27:45.559
<v Speaker 3>It's going to refine the results of the Ellis Baldwin test.

546
00:27:45.960 --> 00:27:47.119
<v Speaker 2>And what about SPHEREx.

547
00:27:47.359 --> 00:27:50.880
<v Speaker 3>SPHEREx is a planned all sky spectroscopic survey. It's going

548
00:27:50.920 --> 00:27:54.000
<v Speaker 3>to map the entire near infrared sky, which is crucial

549
00:27:54.039 --> 00:27:57.559
<v Speaker 3>because it gives us highly accurate distances in compositions for

550
00:27:57.680 --> 00:27:58.640
<v Speaker 3>millions of galaxies.

551
00:27:58.680 --> 00:28:00.400
<v Speaker 2>So another independent confirmation.

552
00:28:00.200 --> 00:28:02.640
<v Speaker 3>Right, It will help us confirm whether this discrepancy is

553
00:28:02.640 --> 00:28:05.319
<v Speaker 3>consistent across even deeper cosmological volumes.

554
00:28:05.440 --> 00:28:07.640
<v Speaker 2>And then we have the ground based powerhouses, the ones

555
00:28:07.680 --> 00:28:09.480
<v Speaker 2>that deal with just pure volume.

556
00:28:09.119 --> 00:28:12.200
<v Speaker 3>Of data exactly. We have telescopes like the ver Ruben

557
00:28:12.200 --> 00:28:16.240
<v Speaker 3>Observatory in Chile. It's poised to conduct the legacy survey

558
00:28:16.279 --> 00:28:19.640
<v Speaker 3>of space and time. Ruben will observe nearly the entire

559
00:28:19.759 --> 00:28:23.720
<v Speaker 3>southern hemisphere sky every few nights, creating these incredible time

560
00:28:23.799 --> 00:28:25.359
<v Speaker 3>lapse movies of the cosmos.

561
00:28:25.599 --> 00:28:29.200
<v Speaker 2>Its sheer volume of data on galaxy distribution and clustering

562
00:28:29.480 --> 00:28:33.079
<v Speaker 2>is going to provide unprecedented detail on cosmic structure.

563
00:28:32.680 --> 00:28:37.039
<v Speaker 3>And potentially reveal non FLRW effects on scales we've never

564
00:28:37.079 --> 00:28:38.759
<v Speaker 3>been able to measure consistently before.

565
00:28:38.839 --> 00:28:40.680
<v Speaker 2>And then there's the big one, at least for the

566
00:28:40.920 --> 00:28:45.359
<v Speaker 2>radio astronomers, the Square Kilometer Array the SKA.

567
00:28:45.640 --> 00:28:49.839
<v Speaker 3>The SKA is an immense revolutionary radio telescope project. It

568
00:28:49.880 --> 00:28:53.279
<v Speaker 3>spans two continents in South Africa and Australia. When it's

569
00:28:53.319 --> 00:28:56.200
<v Speaker 3>fully operational, the SKA will be sensitive enough to detect

570
00:28:56.200 --> 00:28:59.039
<v Speaker 3>the faintest radio galaxy, stretching almost all the way back

571
00:28:59.039 --> 00:29:00.079
<v Speaker 3>to the CMBs.

572
00:29:00.079 --> 00:29:02.279
<v Speaker 2>That will extend the range and the precision of the

573
00:29:02.359 --> 00:29:05.240
<v Speaker 2>Ellis Baldwin test far beyond what we can do now, and.

574
00:29:05.160 --> 00:29:07.359
<v Speaker 3>It will allow us to see if this dipole anomaly

575
00:29:07.440 --> 00:29:11.119
<v Speaker 3>evolves or maybe disappears at earlier epochs in the universe's history.

576
00:29:11.319 --> 00:29:14.279
<v Speaker 2>So these projects won't just confirm the anomaly, they will

577
00:29:14.279 --> 00:29:17.640
<v Speaker 2>hopefully characterize it. They'll tell us where the lack of

578
00:29:17.680 --> 00:29:20.599
<v Speaker 2>symmetry is most pronounced and perhaps how it changes over

579
00:29:20.640 --> 00:29:21.359
<v Speaker 2>cosmic time.

580
00:29:21.599 --> 00:29:25.839
<v Speaker 3>And you know, managing this data floodmapping asymmetry across billions

581
00:29:25.839 --> 00:29:29.279
<v Speaker 3>of data points is an enormous task. It's one that

582
00:29:29.279 --> 00:29:32.519
<v Speaker 3>will require harnessing new tools that don't rely on our

583
00:29:32.599 --> 00:29:34.240
<v Speaker 3>simple assumptions.

584
00:29:33.920 --> 00:29:37.799
<v Speaker 2>Which brings us to computational tools. The review suggests it's

585
00:29:37.880 --> 00:29:41.279
<v Speaker 2>conceivable that new insights will come through recent advances in

586
00:29:41.400 --> 00:29:44.440
<v Speaker 2>artificial intelligence, specifically machine learning.

587
00:29:44.720 --> 00:29:48.839
<v Speaker 3>Well, if you're forced to abandon the simple, elegant FLRW geometry,

588
00:29:49.359 --> 00:29:52.799
<v Speaker 3>you need computational tools that are robust enough to analyze complex,

589
00:29:52.880 --> 00:29:56.680
<v Speaker 3>asymmetrical and highly detailed data sets without relying on human

590
00:29:56.720 --> 00:29:58.160
<v Speaker 3>imposed symmetrical assumptions.

591
00:29:58.240 --> 00:30:01.039
<v Speaker 2>Humans tend to search for patterns we expect defined right.

592
00:30:01.319 --> 00:30:04.079
<v Speaker 3>AI can search for patterns we haven't even conceived.

593
00:30:03.599 --> 00:30:06.200
<v Speaker 2>Of yet, So machine learning algorithms could be the key

594
00:30:06.279 --> 00:30:09.880
<v Speaker 2>to cracking this non symmetric universe. They are excellent at

595
00:30:09.880 --> 00:30:14.000
<v Speaker 2>spotting subtle nonlinear correlations within massive data sets that a

596
00:30:14.079 --> 00:30:17.480
<v Speaker 2>human eye or even a standard statistical model would just miss.

597
00:30:17.799 --> 00:30:20.359
<v Speaker 3>I think it might be the only viable pathway forward

598
00:30:21.039 --> 00:30:25.200
<v Speaker 3>constructing a replacement cosmological model, a lopsided one that is

599
00:30:25.240 --> 00:30:28.119
<v Speaker 3>still consistent with the near perfect uniformity of the CMB,

600
00:30:28.559 --> 00:30:31.880
<v Speaker 3>yet accommodates the measured matter dipole. That may depend on

601
00:30:31.960 --> 00:30:35.799
<v Speaker 3>AI finding the underlying non symmetric equations that govern the

602
00:30:35.880 --> 00:30:36.880
<v Speaker 3>universe's true.

603
00:30:36.640 --> 00:30:39.799
<v Speaker 2>Geometry, and that would usher in an entirely new era

604
00:30:40.000 --> 00:30:41.279
<v Speaker 2>of physics, one.

605
00:30:41.200 --> 00:30:45.359
<v Speaker 3>Driven by observation and computation rather than purely by theoretical elegance.

606
00:30:45.519 --> 00:30:48.160
<v Speaker 2>So what does this all mean. Really, the impact would

607
00:30:48.160 --> 00:30:51.839
<v Speaker 2>be well truly huge on fundamental physics. It means rewriting

608
00:30:51.839 --> 00:30:54.920
<v Speaker 2>the basic laws that govern the cosmosis structure. It means

609
00:30:54.920 --> 00:30:58.000
<v Speaker 2>potentially accepting a much more complex, non uniform reality.

610
00:30:58.160 --> 00:31:00.759
<v Speaker 3>It means that the next generation of cosmolayists might have

611
00:31:00.799 --> 00:31:02.960
<v Speaker 3>to learn a completely different set of equations for the

612
00:31:03.079 --> 00:31:05.960
<v Speaker 3>universe than the ones we teach today. It's a moment

613
00:31:06.039 --> 00:31:08.680
<v Speaker 3>of intellectual crisis, yes, but it's also a moment of

614
00:31:08.720 --> 00:31:12.319
<v Speaker 3>profound opportunity. The universe is telling us that our simplifying

615
00:31:12.359 --> 00:31:15.119
<v Speaker 3>assumption the very basis of the entire land to CDM

616
00:31:15.160 --> 00:31:18.240
<v Speaker 3>framework was just too convenient, and now we have to

617
00:31:18.279 --> 00:31:21.680
<v Speaker 3>embrace the messy reality of a cosmos that doesn't obey

618
00:31:21.720 --> 00:31:23.200
<v Speaker 3>our knee for perfect symmetry.

619
00:31:23.279 --> 00:31:26.000
<v Speaker 2>We started this discussion asking about the shape of the universe,

620
00:31:26.319 --> 00:31:30.680
<v Speaker 2>and the standard answer was smooth and uniform. We've learned

621
00:31:30.680 --> 00:31:33.640
<v Speaker 2>that this symmetry is rooted in the practical necessity of

622
00:31:33.720 --> 00:31:36.799
<v Speaker 2>solving Einstein's equations via the FLRW metric.

623
00:31:37.160 --> 00:31:40.880
<v Speaker 3>And now we leave with the confirmed possibility that the

624
00:31:40.960 --> 00:31:46.039
<v Speaker 3>universe is fundamentally lopsided. The failure of the Ellis Baldwin test,

625
00:31:46.160 --> 00:31:50.440
<v Speaker 3>confirmed across multiple wavelengths and instruments, shows a measurable discord

626
00:31:50.680 --> 00:31:54.359
<v Speaker 3>between the CMB, the relic radiation, and the distribution of

627
00:31:54.400 --> 00:31:56.160
<v Speaker 3>matter from distant sources.

628
00:31:55.920 --> 00:31:59.039
<v Speaker 2>And this demands a fundamental shift away from the FLRW

629
00:31:59.200 --> 00:32:01.160
<v Speaker 2>description and the la LAMB to a CDM model.

630
00:32:01.200 --> 00:32:02.200
<v Speaker 3>There's no escaping it.

631
00:32:02.279 --> 00:32:04.480
<v Speaker 2>And this isn't just an academic detail for you to

632
00:32:04.519 --> 00:32:07.599
<v Speaker 2>think about. This is about the underlying rules that dictate

633
00:32:07.680 --> 00:32:10.640
<v Speaker 2>everything from the clustering of galaxies to the expansion rate

634
00:32:10.640 --> 00:32:14.519
<v Speaker 2>of space. Understanding this tension is a shortcut to understanding

635
00:32:14.559 --> 00:32:17.640
<v Speaker 2>the cutting edge of physics today, the precise moment where

636
00:32:17.720 --> 00:32:21.119
<v Speaker 2>our most successful theory is actively being broken by reality.

637
00:32:21.519 --> 00:32:25.039
<v Speaker 2>It's exhilarating to watch a scientific paradigm potentially collapse and

638
00:32:25.079 --> 00:32:26.039
<v Speaker 2>evolve in real time.

639
00:32:26.240 --> 00:32:28.319
<v Speaker 3>And that leads us to the final provocative thought we'd

640
00:32:28.359 --> 00:32:31.759
<v Speaker 3>like to leave you with. If the universe is fundamentally asymmetric,

641
00:32:32.160 --> 00:32:35.839
<v Speaker 3>if it truly is lopsided, what new forces or spatial

642
00:32:35.880 --> 00:32:39.000
<v Speaker 3>geometries must exist that we haven't even begun to account

643
00:32:39.039 --> 00:32:42.119
<v Speaker 3>for in our symmetrical math. What happens when we finally

644
00:32:42.160 --> 00:32:45.319
<v Speaker 3>build a model that doesn't assume symmetry, but rather predicts

645
00:32:45.319 --> 00:32:49.119
<v Speaker 3>it on local scales while embracing a global asymmetry. The

646
00:32:49.200 --> 00:32:52.039
<v Speaker 3>new rules for the universe might be far stranger, far

647
00:32:52.079 --> 00:32:55.200
<v Speaker 3>more complex, and ultimately far more truthful than we ever.

648
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<v Speaker 4>Imagined us

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<v Speaker 2>Says
