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Speaker 1: Imagine stepping back from everything you know. I mean everything,

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every city, every mountain, every single star you've ever seen,

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the whole thing, the whole thing. Now, imagine taking all

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of cosmic history, that entire thirteen point seven billion years

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we've so carefully mapped out, and just shrinking it all down,

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reducing every particle, every photon down to a single, tiny,

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insignificant point. What if that point, our entire universe is

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just a sub atomic particle in a system that we

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can't even begin to grasp.

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Speaker 2: It's the ultimate exercise in humility, isn't it the idea

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that our vast, mysterious cosmos, the very thing we think

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of as infinity, might actually be contained inside something else,

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something even bigger, an unimaginable, larger structure. It's a concept

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that basically demands we throw out our most fundamental assumptions

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about well about reality itself.

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Speaker 1: Welcome back to the deep dive Today. We're diving into

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a frontier of theoretical physics that, and I'm not exaggerating here,

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genuinely challenges the most basic principles of modern cosmology. We

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are exploring the stunning, pretty radical possibility that our entire

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observable universe is encapsulated within an unimaginably gigantic black hole.

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Speaker 2: And this isn't just you know, some thought experiment. This

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is a hypothesis that's actually gaining traction because of some

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very curious, very hard to explain astronomical observations.

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Speaker 1: Right, But we have to tackle the central contradiction right away.

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Speaker 2: We have to on one hand, every measurement we have,

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from the red shift of distant galaxies to cosmic microwave background,

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it all defines our universe.

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Speaker 1: By expansion, everything is moving away from.

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Speaker 2: Everything else exactly, everything is charging outward. Space itself is stretching.

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But a black hole, by its very definition, is all

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about relentless crushing compression gravity pulling everything inward to a

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single point.

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Speaker 1: So that's the tension. How can something be expanding at

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these incredible speeds while also being held captive inside a

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system defined by inescapable inward gravitational collapse.

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Speaker 2: For this to be true, these two completely opposing forces

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expansion and containment, have to somehow coexist, And we're going.

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Speaker 1: To dive into the clues that suggests this impossible harmony

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might actually be our reality.

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Speaker 2: Okay, so let's start with the official story the Standard.

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Speaker 1: Model, right the Big Bang. It's the clinerstone of all

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of cosmology. It's the model that governs everything from how

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atoms formed to the ultimate fate of reality.

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Speaker 2: And the Standard Model requires us to go back thirteen

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point seven billion years, when all matter, all energy, space

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and time, we're all compressed into this infinitely small, infinitely

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hot point the singularity, the singularity, which is a state

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of infinite density that right off the bat breaks all

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the known laws.

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Speaker 1: Of physics, and then suddenly came the Bang, or more accurately,

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this cataclysmic process of expansion. I think people hear explosion

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and get the wrong idea.

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Speaker 2: Oh. Absolutely, an explosion sends stuff flying through space that's

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already there.

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Speaker 1: Okay. The Big Bang, and especially that first moment called

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cosm inflation, was the expansion of space time itself. In

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a tiny, tiny fraction of a second, the universe inflated

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faster than the speed of light.

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Speaker 2: And that's not matter moving, that's the ruler of space

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itself stretching out exactly.

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Speaker 1: It's why the universe seems so uniformly flat and homogeneous

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to us today.

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Speaker 2: The scale of that is just it's impossible to visualize.

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We're talking about the volume of the universe increasing by

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a factor of ten to the seventy eighth power in

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a sliver of a second.

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Speaker 1: It's just short circuits your brain trying to imagine it.

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Speaker 2: It does. My go to analogy is it's not like

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blowing up a balloon where air goes into it. It's

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like having lines drawn on the balloon, and then you

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stretch the rubber itself. The lines just get further apart.

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Speaker 1: That's a much better way to think about it. Yeah,

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and the Big Bang relies very heavily on something we

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have to talk about, the cosmological principle. It's sort of

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the non negotiable assumption that lets us do cosmology in

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the first place.

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Speaker 2: Okay, so define that for us again, because this is

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the specific idea that the black hole hypothesis just just shatters.

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The principle basically states that on very large scales, the

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universe is both isotropic and homogenous.

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Speaker 1: Okay, what do those mean.

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Speaker 2: Isotropic means it looks the same in all directions from

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any point. There's no up or down in the cosmos.

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Homogeneous means it looks the same everywhere no matter where

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you go. The density and distribution of galaxies are roughly uniform.

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Speaker 1: So if the universe is truly uniform, the matter should

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be spread out like a well mixed soup. And more

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importantly for today, things like the spin of galaxies should

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be totally random.

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Speaker 2: Completely random. You should see just as many galaxies spinning

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clockwise as you do counterclockwise, a perfect fifty to fifty.

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Speaker 1: Split, because the initial chaos of the bang should lead

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to random orientations.

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Speaker 2: Exactly. But here's the fundamental clash. If we are contained

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within a black hole, a structure defined by gravity, rotation,

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and compression, that cosmological principle is immediately violated.

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Speaker 1: Because a black hole is the opposite of uniform. It's

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a single central eye structure, it has a boundary the

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event horizon center, and probably a dominant rotation.

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Speaker 2: Precisely, black holes compress things inward. The gravity is relentless.

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So if we accept that we're contained, we have to

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challenge this idea of uniform expansion, and the challenge is huge.

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How can this rapid, faster than light expansion happen against

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the crushing gravity of the container.

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Speaker 1: We're looking for a loophole, a way for expansion to

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be possible, maybe even caused by the physics of the

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black hole we're supposedly in.

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Speaker 2: And the exciting part is that this isn't just the

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thought experiment. It's being driven by actual astronomical observations that

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are starting to show these little cracks in the idea

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of uniformity.

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Speaker 1: Okay, let's get into that. Let's talk about the specific

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observation that really shook things up recently. It came from

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a pretty fascinating science paper using the James Webs based

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telescope the GWST right.

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Speaker 2: A researcher used its deep field capabilities to zero in

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on a huge patch of the sky and they were

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looking specifically at the rotational dynamics of spiral galaxies, the

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beautiful cosmic pinwheels the very same and if the universe

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were perfectly uniform, like the cosmological principles says it should be,

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the spins of these galaxies should be completely random. But

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that's not what they found, not even close. They found

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a definitive, statistically significant bias. In that huge region. They

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observed roughly two thirds of the spiral galaxies appeared to

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be rotating clockwise and the other third counterclockwise.

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Speaker 1: Wait a two to one preference for clockwise rotation. That is,

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that's not random at all, not in the slightest. That

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means there's a preferred directionality, a cosmic axis or spin

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that's influencing matter across these immense distances. That observation alone,

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if it holds up, fundamentally challenges the idea that the

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universe is the same everywhere.

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Speaker 2: It creates what physicists sometimes call an access of evil problem.

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It's a kind of a dramatic term for any finding

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that suggests the universe has a preferred.

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Speaker 1: Direction, the axis of evil.

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Speaker 2: I like that, and if it is real, it implies

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that some massive external structure as imposing its own rotation,

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its own spin, onto the stuff inside it.

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Speaker 1: Here's the connection. What massive singular structures are defined by

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immense gravity and crucially rotation.

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Speaker 2: Black holes. A large rotating black hole has this property

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called frame dragging, the lens thiring effect.

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Speaker 1: All right, It literally drags space time around of it.

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Speaker 2: It does. And while we usually think of that effect

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as being really strong close to the event horizon, if

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our container is a black hole of stupendous scale, its

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sheer mass and rotation could introduce this this subtle long

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range alignment effect on the galaxies inside.

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Speaker 1: It is like we're inside a cosmic washing machine, and

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all the clothes the galaxies are eventually going to start

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swirling in the same direction.

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Speaker 2: That's a great analogy for it.

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Speaker 1: Okay, but let me play skeptic for a second. The

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paper itself notes that this observation hasn't been confirmed yet

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by larger surveys. Why is that so hard to do?

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Why can't we just point more telescopes in check?

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Speaker 2: It's a vital question. Confirmation is tricky for a couple

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of reasons. First, there's observational bias. When you're looking at

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galaxies billions of light years away, you have to account

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for how they're tilted relative to you. Dust getting in

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the way, lots of things.

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Speaker 1: So it's a messy signal to clean up.

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Speaker 2: Very messy. And second, the cosmological principle is a really

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deeply ingrained assumption. Scientists often design surveys that kind of

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average out these anomalies by default because they expect them

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to disappear with a large enough sample size.

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Speaker 1: So we need new surveys that are specifically designed to

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look for this asymmetry instead of just assuming it away precisely.

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Speaker 2: So until then, this anomaly. Is this crucial, tantalizing piece

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of evidence, and it leads us to the second truly

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mind bending clue, the mathematical alignment known as the radius coincidence.

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Speaker 1: I still find this one staggering. Explain how this mathematical

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coincidence works?

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Speaker 2: Okay, So we use the short shelled radius formula to

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calculate the size of a black hole's event horizon. Is

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actually quite simple. The radius is directly proportional to the mass.

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Speaker 1: More mass, bigger event horizon exactly.

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Speaker 2: So, to figure out the size of the black hole

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that could contain our universe, we take the total estimated

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mass and energy of the observable universe everything we can see,

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detect or measure, and we plug that number into the formula.

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Speaker 1: And what is it spit up?

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Speaker 2: It spits out a radius that is mathematically incredibly close

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to the actual measured size of our observable universe.

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Speaker 1: How close is incredibly close?

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Speaker 2: A calculated radius matches the observable size to within about

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ten to fifteen percent. In cosmology, that is an unnervingly

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small discrepancy.

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Speaker 1: Hold on, let me pause there. When I think about

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cosmic math, the uncertainty margins can be huge. We argue

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over the hubble constant dark energy measurements. Sometimes the air bars.

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Speaker 2: Are massive, they can be yes.

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Speaker 1: But here you're telling me that a theoretical calculation for

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a black hole containing all of our universe's mass matches

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the actual distance to the edge of what we can

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see within fifteen percent.

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Speaker 2: That's why it's such an aha moment for this theory.

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It's really hard to dismiss a coincidence when you're dealing

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with numbers of this magnitude.

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Speaker 1: So what does that mean for the age of our universe.

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We've always been taught that the edge is just defined

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by how far light has had time to travel to

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us since the Big Bang.

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Speaker 2: Right about forty six billion light years away when you

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account for expansion. But if this mathematical alignment is a

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physical reality, then the edge of our observable universe isn't

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just a time limit.

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Speaker 1: It's the event horizon.

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Speaker 2: It's the event horizon of the massive black hole we

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are inside.

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Speaker 1: That's why we can't see beyond it. The event horizon

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is the ultimate firewall, the boundary where nothing, not even light,

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can escape Exactly.

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Speaker 2: The universe looks finite to us because we're locked inside

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its boundary. It's a clean, elegant explanation for why our

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cosmic vision has a hard stop. We aren't just looking

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out into space. We're looking right up to the point

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of no return of our cosmic prison.

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Speaker 1: Okay, that sounds existentially terrifying, but you said earlier that

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our day to day lives wouldn't change. We don't feel

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like we're being crushed or spaghettified. Why not.

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Speaker 2: It all comes down to scale. The tidal forces, the

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things that stretch you apart. They only become destructive when

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there's a huge difference in gravity over a small.

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Speaker 1: Distance, like near a small stellar mass black hole.

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Speaker 2: Right, It's gravity changes dramatically over just a few meters,

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so it would tear you apart. But if the black

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hole containing us is stupendously large, the radius of curvature

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is immense.

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Speaker 1: So the gravitational field is almost uniform over say the

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size of our.

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Speaker 2: Solar system, the difference in the pole on your head

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versus your feet would be so small it would be

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completely negligible. We're safe because our container is just too

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big for us to feel the squeeze.

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Speaker 1: So if this is true, the black hole we're in

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isn't just big. It's got to be a whole new

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class of object.

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Speaker 2: It does. We need to talk about the scale required.

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The black hole containing our universe would have to be

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what theoretical physicists have called, quite bluntly, a stupid hendously

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large black hole. A slab, A slab.

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Speaker 1: I love it. It's a fitting name, it is. Let's

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really appreciate the scale here by doing a quick tour

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of black hole sizes, just to show how far off

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the charts this thing would be. Let's start small.

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Speaker 2: Okay, we can start with primordial black holes. These are

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hypothetical objects formed in the first few moments after the

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Big Bang from collapsing pockets of super dense plasma. No

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bigger they They could range from the mass of an

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asteroid to maybe tens of thousands of times the mass

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of the Sun. They're fascinating, but obviously way too small

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to hold the universe.

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Speaker 1: Okay, next up the common ones, stellar mass black holes.

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These form when a single massive star collapses.

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Speaker 2: And the key here is always density. If you took

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our entire planet Earth and somehow compressed it down into.

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Speaker 1: A black hole, how big would be.

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Speaker 2: Its Schwitz Child radius would be about one centimeter. The

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size of.

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Speaker 1: A marble one centimeter. When I try to picture the

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entire mass of the Earth, the oceans, the mountains, the

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molten core all crush into a marble. My brain just

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it starts to fizz. The density is incomprehensible.

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Speaker 2: And if that one centimeter object holds all of Earth,

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a stellar black hole is clearly not going to hold

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the universe.

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Speaker 1: Laughably too small, okay.

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Speaker 2: Moving up next are the intermediate mass black holes or imbhs,

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the elusive middle children, ranging from one hundred to maybe

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a million solar masses, still just mediocre by cosmic standards, which.

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Speaker 1: Brings us to the giants. We actually see super massive

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black holes. The SMBH is at the center of nearly

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every galaxy.

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Speaker 2: Right, weighing in at millions or even billions of times

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the mass of our Sun. A lot of people hear

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this theory and they immediately think, oh, so we're inside

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one of those.

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Speaker 1: But even they aren't big enough.

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Speaker 2: Not even close. Let's take one of the biggest ones

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we've ever measured, something truly terrifying, maybe ten billion times

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the mass of our sun. Okay, if you calculate the

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size of its event horizon, its diameter is only about

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two hundred astronomical units across two hundred AUG.

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Speaker 1: For context, that's roughly the diameter of our soul system,

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including the Orc Cloud. It's enormous, but it's still just

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our little stellar neighborhood exactly.

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Speaker 2: It's astronomically large, but it's not cosmologically large. The relationship

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between mass and radius is linear, so to get a

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radius of forty six billion light years, you need a

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correspondingly gigantic increase in mass.

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Speaker 1: So we have to go way beyond the billions of

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solar masses of an SMBH. We need a stell ab

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whose mass is precisely the mass of the entire observable universe.

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That's the only thing that works for the radius coincidence.

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Speaker 2: And that raises another huge question. Where would something like

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that even come from. We think SMBHs grow by eating

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gas and stars or merging with other black holes, but

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a slab am that would have to have been born

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in an even older, even more massive parent universe.

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Speaker 1: It feels like every answer we find just opens up

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three more, even bigger questions.

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Speaker 2: That's cosmology for you.

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Speaker 1: Okay, So let's tackle the biggest conceptual headache again, expansion

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versus compression. If our universe is inside a cell, abb

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how does the Big Bang, the expansion even happen.

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Speaker 2: We have to redefine what the big Bang is. Instead

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of the absolute beginning of everything, it becomes a sub event.

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Speaker 1: A chapter, and a bigger story exactly.

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Speaker 2: The big Bang model still works perfectly to describe the

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physics inside our space time, the rapid expansion, the cooling,

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the formation of elements. But the event that create our

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singularity happened outside.

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Speaker 1: So it's the moment a black hole and apparent universe collapsed,

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and that singularity somehow birth the whole new, sealed off

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bubble of space time, and that bubble is us.

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Speaker 2: This is a concept in quantum gravity called ficcun universes

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or baby universes. The idea is that when matter collapses

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into a singularity, the extreme conditions could effectively create a new,

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separate volume of space. Our big Bang is just the

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moment that new singularity began its own rapid inflationary expansion.

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Speaker 1: So we are expanding, but only within the sealed off

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boundaries of our container. The container itself is an exit.

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It's just doing what black holes do in the parent universe.

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Speaker 2: Right it connects our universe to this potentially infinite chain

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of creation where black holes are basically the portals for

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new space times. But this idea immediately competes with other

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alternative theories to the standard Big.

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Speaker 1: Bang, like the Big Bounce.

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Speaker 2: Like the Big Bounce, which is a really popular one,

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it suggests that our universe didn't start from nothing, but

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that it's cyclical.

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Speaker 1: Our current expansion is just the rebound from the collapse

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of a previous universe.

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Speaker 2: Yes, so the universe could be infinitely old, just expanding

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and contracting, rebooting itself over and over. It's an elegant

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way to get rid of that pesky beginning problem.

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Speaker 1: But the Big Bounce runs into huge trouble if we're

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inside a black hole.

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Speaker 2: Huge trouble because a black hole acts like a giant

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pit of quicksand not a trampoline. It's not going to

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bounce back, not easily. The analogy is powerful because it

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captures the immense gravitational resistance. A black hole's gravity is

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an inward pulling force. The Big Bounce needs some kind

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of immense, organized out what word rebound force to overcome

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the final collapse.

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Speaker 1: And if that collapse happened inside a cess lab its

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own gravity is now fighting against the gravity of the

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entire container.

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Speaker 2: It's a double ammy. The big bounced theories often rely

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on some kind of quantum mechanical repulsive force that only

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kicks in at extreme densities. For that to work inside

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a cess lab, that quantum force would have to be

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strong enough to overcome both the internal gravity and the

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external compressive force of the container.

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Speaker 1: That's a huge hurdle to clear. It seems like you'd

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need some kind of new physics, maybe something about gravity

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leaking into other dimensions, to allow that initial inflation to

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punch out against the containment pressure you would.

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Speaker 2: One idea that gets discussed is the role of negative pressure.

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We already know our universe has dark energy, which acts

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as a kind of negative pressure to drive.

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Speaker 1: Expansion, pushing things apart right.

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Speaker 2: So one wild idea is that if the parent universe

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is somehow leaking high energy exotic matter across the event

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horizon into our universe, that could provide the case continuous

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negative pressure we need to keep inflating even while we're contained.

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Speaker 1: There's a huge leap of faith assuming physics from outside

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our own.

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Speaker 2: Reality it is, but it shows the kind of radical

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thinking you need to reconcile these two massive observations. We're expanding,

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but we might also be contained.

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Speaker 1: Okay, so regardless of how we got here, if we

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are inside asl lab, that container has to influence our

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ultimate fate. So what are the possibilities for the end

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of the universe.

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Speaker 2: Well, we've got four major cosmological endgame scenarios, and being

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inside a black hole makes some of them much more

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likely and others well nearly impossible.

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Speaker 1: Let's start with the one that feels most natural for

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being stuck inside a gravitational prison.

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Speaker 2: That would be scenario one, The Big Crunch.

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Speaker 1: The Great Collapse. The universe stops expanding, gravity takes over,

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and everything comes crashing back together.

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Speaker 2: In this scenario, matter starts accelerating inward again, Galaxies collide,

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black holes merge, and everything culminates in this violent, insanely

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collapse back into a singularity.

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Speaker 1: And being inside a cell lab would just accelerate that process, right.

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The container's gravity would be amplifying our own universe as

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gravity just speeding up the collapse almost certainly.

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Speaker 2: Yes. The good news, if you can call it that,

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is that the contraction would take billions of years, just

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like the expansion did, but the end state is this

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single monsterized black hole swallowing everything.

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Speaker 1: Okay, now, let's go to the opposite end of the spectrum,

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the one that seems like the biggest challenge for this.

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Speaker 2: Hypothesis, Scenario two, the big freeze or heat death.

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Speaker 1: This is the quiet cold ending.

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Speaker 2: Right, driven by maximum entropy, The universe expands forever, energy

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spreads out perfectly evenly, the temperature drops toward absolute zero,

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and all organized structures dissolve. It just becomes dark, cold

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and empty.

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Speaker 1: But the problem, as we've said, yeah, is that requires

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endless expansion that just seems impossible.

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Speaker 2: If you're inside a black hole, it's fundamentally opposed. The

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big freeze relies on stuff being able to spread out forever,

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But if we're the cess lab's gravity is constantly trying

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to pull all that dispersed energy back in. To achieve

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heat death, the outward energy of every particle would have

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to overcome the total gravitational pull of the entire sl ab,

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which seems unlikely, mathematically, very unlikely. So the s Lab

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hypothesis pretty much rules out the quiet cold death in

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favor of a more violent end.

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Speaker 1: Okay, let's get violent scenario three, the Big Rip.

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Speaker 2: This is where expansion goes completely off the rails. It's

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driven by dark energy, that mysterious force that's already accelerating

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the expansion of our universe.

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Speaker 1: It's like a negative pressure pushing space time itself apart.

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Speaker 2: And in the big Rip scenario, the strength of that

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expansionary force keeps increasing over time.

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Speaker 1: And eventually it gets so strong it overcomes everything else.

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Speaker 2: Everything First it tears galaxies apart, then solar systems, then planets,

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and finally the expansion force becomes stronger than the fundamental

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forces holding atoms together.

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Speaker 1: So it literally rips apart matter itself. Instant vaporization it does.

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Speaker 2: And if if the Big Rip is possible inside a

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CIS lab, it means that dark energy is strong enough

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to completely overwhelm the colossal gravity of the container.

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Speaker 1: So dark energy would have to be this intrinsic property

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of our space time bubble, powerful enough to just ignore

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the external gravity and destroy us from within.

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Speaker 2: That's the idea, so it remains a viable, terrifying, and

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extremely violent option even from the inside.

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Speaker 1: And finally, the weirdest one scenario four, the big slurf.

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Speaker 2: Scientifically, this is called vacuum decay. It comes from quantum

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field theory, and it suggests that the vacuum of space

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we live in might only be a false vacuum, like a.

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Speaker 1: Ball resting on a high shelf but not on the floor.

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It's stable, but it could fall to a more stable state.

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Speaker 2: Perfect analogy and a random quantum event could cause a

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small region of space to collapse into a true vacuum,

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a state of even lower energy. This creates a bubble

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that expands at.

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Speaker 1: The speed of light, and it changes the laws of

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physics as it goes. If that bubble.

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Speaker 2: Hits us, all existing matter and forces would just cease

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to exist. But the big SLURP is probably the least

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likely scenario if we're in a black hole. Why is

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that black holes are the opposite of a vacuum. They're

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defined by extreme density. A constant influx of matter and energy.

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That high energy, densely packed environment would make an expanding

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bubble of true vacuum incredibly.

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Speaker 1: Unstable, so the conditions inside the s lab would probably

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pop the bubble before it could even get started, or.

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Speaker 2: Prevent it from forming in the first place. So, in

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a weird way, being inside a black hole might actually

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be protecting us from the threat of vacuum decay.

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Speaker 1: It's fascinating how our potential prison dictates our potential doom.

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It seems to favor the crunch or the rip while

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shielding us from the slurp in the freeze.

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Speaker 2: It really narrows down the possibilities.

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Speaker 1: So we've talked about the container this s lab. But

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if our universe is inside a black hole, that black

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hole must be part of another bigger parent universe.

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Speaker 2: Right, And that parent universe must have its own black holes,

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which could contain other universes, and.

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Speaker 1: On and on. It's the ultimate infinite cosmic nesting doll.

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Speaker 2: This is the concept of a fractal universe, a multiverse

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system born directly out of black hole physics. Every time

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a massive star collapses in one universe, it could seed

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a new separate space time bubble. Our universe, as vast

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as it is, might just be a seed for the

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next generation.

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Speaker 1: The implications for parallel realities are just they're dizzying. If

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there are infinite nested universes, each one could have been

476
00:23:31,599 --> 00:23:34,559
born from a different type of singularity, meaning each could

477
00:23:34,559 --> 00:23:36,279
have completely different laws of physics.

478
00:23:36,400 --> 00:23:39,279
Speaker 2: Think about the fundamental constants that rule our reality. The

479
00:23:39,279 --> 00:23:42,720
speed of light, the strength of gravity, planks constant. They

480
00:23:42,759 --> 00:23:45,160
could all be different in an adjacent universe. You could

481
00:23:45,200 --> 00:23:47,480
have a universe where gravity is a repulsive force, not

482
00:23:47,519 --> 00:23:48,519
an attractive one.

483
00:23:48,640 --> 00:23:52,519
Speaker 1: The variation is literally endless, you know. I sometimes try

484
00:23:52,559 --> 00:23:55,920
to ground these huge ideas in a personal way. When

485
00:23:56,359 --> 00:23:58,519
I look up at the stars, I think about how

486
00:23:58,519 --> 00:24:03,160
those photons travel for millions of years just to reach

487
00:24:03,240 --> 00:24:06,200
my eye. To think that all of that staggering depth,

488
00:24:06,359 --> 00:24:10,319
all those galaxies are contained within something else, and that

489
00:24:10,400 --> 00:24:13,880
something else is contained again, it just breaks my sense

490
00:24:13,920 --> 00:24:18,480
of objective reality. It moves from science into philosophy. It

491
00:24:18,519 --> 00:24:20,720
makes me wonder if there's an exact copy of me

492
00:24:20,799 --> 00:24:24,200
in an adjacent universe, having this exact same conversation right now.

493
00:24:24,440 --> 00:24:27,319
Speaker 2: Well, if the nesting is truly infinite, then probability says

494
00:24:27,359 --> 00:24:29,440
there must be. There's a version of you who became

495
00:24:29,440 --> 00:24:32,279
a concert pianist, a version who took that dream job

496
00:24:32,319 --> 00:24:33,039
you passed up in.

497
00:24:33,039 --> 00:24:35,240
Speaker 1: A version who married their high school crush.

498
00:24:35,279 --> 00:24:38,119
Speaker 2: And the sobering flip side is that for every success,

499
00:24:38,279 --> 00:24:41,119
there are millions of versions of us facing failure or

500
00:24:41,160 --> 00:24:43,240
living in a universe where the laws of physics are

501
00:24:43,279 --> 00:24:46,359
so hostile that complex life never even had a chance

502
00:24:46,400 --> 00:24:46,799
to form.

503
00:24:46,920 --> 00:24:50,640
Speaker 1: It's the ultimate reflection of cosmic possibility and absurdity all

504
00:24:50,680 --> 00:24:51,079
at once.

505
00:24:51,480 --> 00:24:54,680
Speaker 2: It gives you perspective. It reminds you that the specific

506
00:24:54,799 --> 00:24:58,279
fine tune conditions that led to our existence are probably

507
00:24:58,519 --> 00:25:01,559
just one luck key roll of the dice in an

508
00:25:01,599 --> 00:25:03,079
immense cosmic casino.

509
00:25:03,400 --> 00:25:05,759
Speaker 1: But let's bring it back to the hard evidence, to

510
00:25:05,799 --> 00:25:09,160
that rotational anomaly that started all this. Where does the

511
00:25:09,400 --> 00:25:11,319
hypothesis actually stand right now?

512
00:25:11,480 --> 00:25:16,400
Speaker 2: It remains a crucial but unconfirmed hypothesis. That JWST observation

513
00:25:16,599 --> 00:25:20,960
is incredibly tantalizing, but large scale cosmological surveys have not

514
00:25:21,079 --> 00:25:26,480
yet definitively confirmed that global rotational pattern. The cosmological principle,

515
00:25:26,559 --> 00:25:29,599
though it has some cracks, is still the dominant framework.

516
00:25:30,000 --> 00:25:33,119
Speaker 1: So we're left with these compelling clues, the spin bias

517
00:25:33,200 --> 00:25:36,400
and that uncanny mathematical alignment of the radius, but no

518
00:25:36,519 --> 00:25:37,920
smoking gun just yet.

519
00:25:37,960 --> 00:25:40,039
Speaker 2: That's the nature of this kind of science. We still

520
00:25:40,039 --> 00:25:42,160
have so much to learn, especially about things like dark

521
00:25:42,279 --> 00:25:45,200
energy and what really happens inside of singularity. But the

522
00:25:45,279 --> 00:25:48,079
knowledge regaining whether it proves this s lab theory or

523
00:25:48,160 --> 00:25:50,960
refutes it. It forces us to ask these profound questions.

524
00:25:51,000 --> 00:25:53,200
We're learning how to even search for the impossible.

525
00:25:53,519 --> 00:25:57,039
Speaker 1: This has been an incredibly deep exploration into something truly

526
00:25:57,119 --> 00:26:01,240
mind bending. We've wrestled with that fundamental tension between expansion

527
00:26:01,240 --> 00:26:04,119
and compression, realizing that for us to be inside a

528
00:26:04,119 --> 00:26:07,000
black hole, the Big Bang has to be redefined as

529
00:26:07,119 --> 00:26:09,559
just one event in a much larger story.

530
00:26:09,839 --> 00:26:13,039
Speaker 2: We looked at the key pieces of evidence that jwst

531
00:26:13,279 --> 00:26:16,880
observation of a weird rotational preference in galaxies, and that

532
00:26:17,039 --> 00:26:20,839
uncanny mathematical alignment of our universe's size with the theoretical

533
00:26:20,880 --> 00:26:23,880
event horizon of a stupendously large black hole, the s LAB.

534
00:26:24,240 --> 00:26:27,599
Speaker 1: We toured the cosmic scales and realized that this hypothetical

535
00:26:27,680 --> 00:26:30,559
s LAB would be exponentially larger than any supermassive black

536
00:26:30,559 --> 00:26:32,920
hole we've ever seen, and we mapped out our potential

537
00:26:32,960 --> 00:26:36,640
cosmic endings, finding that being contained likely steers us toward

538
00:26:36,680 --> 00:26:39,119
a violent big crunch or an extreme big rip.

539
00:26:39,279 --> 00:26:42,200
Speaker 2: So if the universe really is a nesting doll and

540
00:26:42,359 --> 00:26:44,880
black holes are the portals creating new space times, what

541
00:26:44,920 --> 00:26:47,319
does that really imply about the limits of scale? If

542
00:26:47,319 --> 00:26:49,759
the event horizon is the absolute limit of what we

543
00:26:49,839 --> 00:26:53,039
can see, what entirely new kind of physics must apply

544
00:26:53,160 --> 00:26:56,599
to the parent universe just beyond our boundary, And that

545
00:26:56,680 --> 00:26:59,599
leaves us with the ultimate question. Is there a true

546
00:26:59,640 --> 00:27:02,119
limit scale a biggest thing and the smallest thing, or

547
00:27:02,160 --> 00:27:05,440
is reality truly fractal and infinite in both directions. That's

548
00:27:05,480 --> 00:27:07,319
the challenge we'll leave you to contemplate.

