WEBVTT

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

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

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

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

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

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<v Speaker 1>slumber under the night sky.

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<v Speaker 2>So I want you to imagine something for a second.

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<v Speaker 2>Try to, like, picture looking at a photograph of a galaxy.

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<v Speaker 2>Oka like a massive swirling vortex of billions of stars,

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<v Speaker 2>you know, laced with those glowing veins of purple gas

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<v Speaker 2>and thick dark rivers of cosmic dust.

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<v Speaker 3>Write something like a classic image beamed back from the

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<v Speaker 3>James Webb Space Telescope.

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<v Speaker 2>Exactly, a stunning high definition space image. Now imagine a

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<v Speaker 2>second photograph right next to it, and it looks completely

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<v Speaker 2>identical down to the pixel right, the same complex spiral arms,

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<v Speaker 2>the same chaotic star forming regions, the exact same distribution

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<v Speaker 2>of light and shadow. But there's a fundamental difference between

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<v Speaker 2>these two images.

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<v Speaker 3>And it's a pretty massive difference.

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<v Speaker 2>Yeah, because one is a photograph of our actual universe, right,

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<v Speaker 2>the product of fourteen billion years of messy, chaotic natural evolution, right,

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<v Speaker 2>But the other one is essentially a hallucination. It is

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<v Speaker 2>a product of pure math running on silicon chips in

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<v Speaker 2>a basement somewhere here on Earth. It's incredible to think

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<v Speaker 2>about it really is. So what if we could build

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<v Speaker 2>a universe inside a computer so mathematically perfect, like, so

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<v Speaker 2>unfathomably detailed that if you put those two images side

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<v Speaker 2>by side, even professional PhD holding astronomers couldn't tell you

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<v Speaker 2>which one was real.

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<v Speaker 3>I mean, it sounds completely like science fiction, but it

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<v Speaker 3>is the current, very real frontier of computational astrophysics.

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<v Speaker 2>Today, which is just wild to me.

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<v Speaker 3>It is we are no longer just sketching rough approximations

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<v Speaker 3>of how galaxies might form. We are synthesizing entire cosmoses

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<v Speaker 3>from absolute scratch.

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<v Speaker 2>Wow.

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<v Speaker 3>Yeah, the boundary between observed physical reality and simulated digital

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<v Speaker 3>reality is becoming well incredibled porous.

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<v Speaker 2>Okay, let's unpack this because simulating an entire universe from

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<v Speaker 2>the literal Big Bang all the way to the present

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<v Speaker 2>day sounds like a task that would just melt any

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<v Speaker 2>computer on Earth.

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<v Speaker 3>It definitely pushes the absolute limits of our current hardware.

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<v Speaker 2>I bet. Yet this massive, decade long scientific effort has

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<v Speaker 2>just achieved exactly this. We are looking at a project

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<v Speaker 2>that successfully simulated the evolution of galaxies by tracking the

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<v Speaker 2>absolute smallest like microscopic specs of cosmic.

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<v Speaker 3>Dust, down to the fundamental chemistry.

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<v Speaker 2>Right, and in doing so, they essentially rescued the entire

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<v Speaker 2>standard model of the universe from being thrown in the

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<v Speaker 2>scientific garbage bin.

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<v Speaker 3>They really did. It was a close call for a

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<v Speaker 3>minute there.

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<v Speaker 2>Plus they figured out a way for us to literally

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<v Speaker 2>hear this virtual universe, which we will definitely get into.

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<v Speaker 3>Oh, the sonification stuff is fascinating, but the scope of

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<v Speaker 3>the simulation itself is genuine only difficult to wrap your

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<v Speaker 3>head around, even for the people actively.

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<v Speaker 2>Working on it, I can imagine.

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<v Speaker 3>But this endeavor really highlights a core philosophy of science,

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<v Speaker 3>which is that knowledge is most valuable when it is

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<v Speaker 3>rigorously applied to solve a crisis.

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<v Speaker 2>And there was definitely a crisis.

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<v Speaker 3>Oh absolutely. For decades, astrophysicists have understood the broad theoretical

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<v Speaker 3>strokes of how the.

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<v Speaker 2>Universe expands, that the big picture stuff, right.

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<v Speaker 3>But whenever they tried to actually build a digital model

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<v Speaker 3>of it. The simulated galaxies always looked well, they just looked.

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<v Speaker 2>Wrong, like how wrong.

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<v Speaker 3>They were too clunky, the colors were off, the sizes

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<v Speaker 3>just didn't match reality at all. The breakthrough here from

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<v Speaker 3>this massive international initiative known as the Collibo project is

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<v Speaker 3>that it proves something fundamental, which is, if you want

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<v Speaker 3>to get the massive billion light year macro universe right,

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<v Speaker 3>you have to perfect the microscopic physics first.

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<v Speaker 2>See. And that's the part that gets me because for

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<v Speaker 2>the longest time we weren't just struggling with the microphysics right,

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<v Speaker 2>we were actively blatantly ignoring them.

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<v Speaker 3>Yeah, that's as one way to put it.

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<v Speaker 2>I want to talk about this concept of the heat

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<v Speaker 2>barrier in early simulations because when I first learned about this,

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<v Speaker 2>it sounded completely absurd.

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<v Speaker 3>It is a bit counterintuitive until you understand the math behind.

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<v Speaker 2>It, right. But in all the older legacy simulations of

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<v Speaker 2>the universe, scientists put a hard floor on the temperature

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<v Speaker 2>of their virtual space.

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<v Speaker 3>Didn't They They did a very strict temperature limit.

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<v Speaker 2>They artificially prevented the gas inside their virtual galaxies from

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<v Speaker 2>cooling down below about ten thousand degrees fahrenheit.

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<v Speaker 3>Which just to put that into perspective, for you, is

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<v Speaker 3>significantly hotter than the surface of our sun.

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<v Speaker 2>Wait? Really?

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<v Speaker 3>Oh yeah? So imagine trying to code an entire virtual

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<v Speaker 3>universe where literally nothing, no cloud of gas, no planetary nebula,

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<v Speaker 3>no empty void, is allowed to be cooler than a

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<v Speaker 3>raging stellar surface.

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<v Speaker 2>It sounds like trying to study how a delicate French

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<v Speaker 2>pastry is baked, but your oven only have one setting,

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<v Speaker 2>and that setting is blowtorch.

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<v Speaker 3>That's a great way to describe it, Like, how do.

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<v Speaker 2>You expect to bake a croissant, or in this case,

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<v Speaker 2>forge a star if every ingredient in your digital kitchen

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<v Speaker 2>is instantly vaporized into superheated plasma.

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<v Speaker 3>Well, you don't. You simply don't. And that was the

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<v Speaker 3>glaring flaw of late twentieth and early twenty first century cosmology.

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<v Speaker 2>It seems like such an obvious oversight, it does.

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<v Speaker 3>But to be fair to those early pioneers, it wasn't

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<v Speaker 3>that astronomers didn't want their.

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<v Speaker 2>Universes to be cold, Okay, so why do it?

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<v Speaker 3>It was that modeling cold gas was computationally lethal to

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<v Speaker 3>their machines.

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<v Speaker 2>Lethal How like, is cold gas harder to calculate than

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<v Speaker 2>hot gas. I would assume hot things are more chaotic.

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<v Speaker 3>It's actually the exact opposite. Modeling cold gas is exponentially harder. Really, Yeah,

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<v Speaker 3>when we talk about gas moving through space, we were

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<v Speaker 3>really talking about hydrodynamics. In astrophysics, we treat these massive

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<v Speaker 3>clouds of hydrogen and helium.

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<v Speaker 2>Like a fluid, like water flowing in a river.

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<v Speaker 3>Sort of. Yeah, we have to calculate their pressure, their viscosity,

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<v Speaker 3>how they flow, and crucially, how they react to the

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<v Speaker 3>gravitational pull of dark matter.

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<v Speaker 2>Okay, that makes sense.

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<v Speaker 1>Now.

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<v Speaker 3>When gas is kept artificially hot at ten thousand degrees,

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<v Speaker 3>it has a lot of thermal pressure. It's smooth, it

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<v Speaker 3>expands outward evenly. It predictable exactly. The math to track

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<v Speaker 3>a smooth expanding balloon of hot fluid is relatively straightforward.

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<v Speaker 3>For a supercomputer, it can handle that easily. But what

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<v Speaker 3>happens to a gas when you cool it down?

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<v Speaker 2>It condenses, right, It shrinks and gets thicker, exactly.

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<v Speaker 3>It loses all that outward thermal pressure. So gravity suddenly

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<v Speaker 3>takes over and the gas starts clumping together into microscopic,

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<v Speaker 3>incredibly dense pockets. Oh I see, it becomes chaotic. And

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<v Speaker 3>highly nonlinear. To calculate the hydrodynamics of cold, clumpy gas,

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<v Speaker 3>your computer grid needs a massive, massive increase in resolution.

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<v Speaker 2>Because there's more stuff happening in a smaller area.

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<v Speaker 3>Right, You have to track millions of tiny, independent, highly

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<v Speaker 3>dense collapsing now instead of just one big smooth cloud.

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<v Speaker 2>So the computers just couldn't handle the math exactly.

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<v Speaker 3>If older supercomputers tried to let the gas drop below

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<v Speaker 3>ten thousand degrees, the simulation would essentially choke on the

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<v Speaker 3>math and crash. The algorithm simply couldn't handle the resolution

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<v Speaker 3>required to track all those tiny clumps.

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<v Speaker 2>But the physical reality we actually live in completely relies

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<v Speaker 2>on that cold gas.

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<v Speaker 3>It lies entirely on it.

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<v Speaker 2>Right, Like, if the real universe couldn't cool down, the

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<v Speaker 2>gas would never clump, stars would never form, and you

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<v Speaker 2>and I wouldn't be sitting here talking about it.

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<v Speaker 3>No, we wouldn't. And this is the grand irony of

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<v Speaker 3>early cosmological simulations. Stars only form in molecular clouds that

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<v Speaker 3>are incredibly cold. We are talking just a few degrees

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<v Speaker 3>above absolute zero.

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<v Speaker 2>Wow, that cold.

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<v Speaker 3>Yes, at those freezing temperatures, the gas has virtually zero

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<v Speaker 3>thermal pressure.

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<v Speaker 2>Pushing outward, so gravity just completely takes over.

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<v Speaker 3>Precisely without that outward push, the inward pull of gravity

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<v Speaker 3>finally wins the tug of war. The cold gas collapses

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<v Speaker 3>in on itself, becoming denser and denser until the pressure

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<v Speaker 3>at the core is so extreme that it ignites nuclear fusion.

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<v Speaker 2>And boom, a star is born.

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<v Speaker 3>Exactly, But if your virtual universe is artificially locked at

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<v Speaker 3>ten thousand degrees, the gas is just moving too fast.

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<v Speaker 3>It has too much kinetic.

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<v Speaker 2>Energy, so it just zips right past itself right.

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<v Speaker 3>Gravity can never grab onto it long enough to forge

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<v Speaker 3>a star. What's fascinating here is how this forced scientists

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<v Speaker 3>to reevaluate their entire approach.

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<v Speaker 2>So wait, if the physics in those older simulations physically

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<v Speaker 2>prevented stars from format like mathematically made it impossible, how

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<v Speaker 2>do they get galaxies? Do they just hack the code? H?

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<v Speaker 1>Yeah?

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<v Speaker 3>Essentially, they used a conceptual band aid called subgrid physics.

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<v Speaker 2>Subgrid physics it sounds like a polite way of saying

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<v Speaker 2>we made it.

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<v Speaker 3>Up, well, kind of. Because the computer grid couldn't zoom

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<v Speaker 3>in far enough to simulate actual cooling and collapsing, they

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<v Speaker 3>wrote a statistical workaround an arbitrary rule.

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<v Speaker 2>How did that work?

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<v Speaker 3>The code basically said, Hey, if a pocket of hot

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<v Speaker 3>gas reaches a certain density threshold, just pretend it magically

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<v Speaker 3>cooled down, delete the gas, and spawn a star particle

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<v Speaker 3>in its place.

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<v Speaker 2>Wow. So they were just spawning in stars like items

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<v Speaker 2>in a video game based on a rough guess.

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<v Speaker 3>Exactly, just dropping them in when the math looked close enough.

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<v Speaker 2>That means for years an enormous chunk of our understanding

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<v Speaker 2>of galaxy evolution was built on a giant blind.

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<v Speaker 3>Spot, a huge blind spot.

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<v Speaker 2>We were trying to map the cosmos while completely ignoring

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<v Speaker 2>the actual environment where galaxies build themselves.

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<v Speaker 3>Right, it was an educated guest, But you can only

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<v Speaker 3>rely on statistical band aids for so long before your

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<v Speaker 3>virtual universe diverges so far from reality that it just

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<v Speaker 3>stops being scientifically useful.

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<v Speaker 2>Right, Eventually the cracks are going to show.

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<v Speaker 3>Absolutely Eventually you have to find a way to break

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<v Speaker 3>that heat barrier and let the virtual cosmos freeze.

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<v Speaker 2>And breaking that barrier wasn't just a matter of like

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<v Speaker 2>waiting for Apple or IBM to build a faster microchip, right,

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<v Speaker 2>You actually had to write new physics into the simulation.

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<v Speaker 3>Yes, entirely new physics.

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<v Speaker 2>And this is where the claw reproject completely changes the game.

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<v Speaker 2>To cool the universe down, they had to introduce two

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<v Speaker 2>highly specific ingredients that had never been successfully modeled on

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<v Speaker 2>this scale before, right, right, molecular hydrogen and cosmic dust.

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<v Speaker 3>Yes, and let me stop you there, because it is

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<v Speaker 3>vital to understand why those two things go hand in hand.

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<v Speaker 3>You cannot have cold molecular hydrogen in space without cosmic

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<v Speaker 3>dust rate. Dust is the great enabler of the universe.

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<v Speaker 2>Which is such a wild paradigm shift because normally, if

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<v Speaker 2>you ask an amateur astronomer about dust, they'll just groan.

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<v Speaker 3>Oh, they hate it.

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<v Speaker 2>Right, dust is the annoying haze that blocks the light

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<v Speaker 2>from the beautiful glowing nebulae behind it. It's an obstacle.

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<v Speaker 2>But here dust is essentially the vip of the universe.

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<v Speaker 2>So what does this all mean? Why is it so important?

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<v Speaker 3>Well, because the vacuum of space is an incredibly hostile

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<v Speaker 3>place to build a molecule. The primary ingredient for a

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<v Speaker 3>star is molecular hydrogen, which is just two hydrogen atoms

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<v Speaker 3>bonded together.

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<v Speaker 2>Okay, simple enough.

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<v Speaker 3>In the vast empty expanse of an early galaxy. Trying

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<v Speaker 3>to get two single hydrogen atoms to bump into each

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<v Speaker 3>other and bond is nearly impossible.

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<v Speaker 2>Because space is just too big.

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<v Speaker 3>The space is too vast, the atoms are moving too fast,

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<v Speaker 3>and if they do happen to collide, they usually just

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<v Speaker 3>bounce off each other. Why do they bounce because they

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<v Speaker 3>have nowhere to dump their excess kinetic energy. They hit

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<v Speaker 3>and the energy just pushes them right back apart.

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<v Speaker 2>It's like trying to get two pieces of velcro to

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<v Speaker 2>stick together by firing them out of cannons at each

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<v Speaker 2>other across an empty football stadium.

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<v Speaker 3>That is Yes, that is a brilliant way to visualize it.

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<v Speaker 3>They're just going to ricochet exactly. They need a mediator,

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<v Speaker 3>They need a surface to slow them down. And this

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<v Speaker 3>is exactly where a microscopic grain of cosmic dust comes in. Okay, Now,

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<v Speaker 3>when we say dust in astrophysics, we aren't talking about

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<v Speaker 3>the dust bunnies under your couch.

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<v Speaker 2>Right, It's not skin cells and lint.

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<v Speaker 3>No, No, we are talking about microscopic solid particles of

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<v Speaker 3>silicates or carbon, Essentially tiny grains of sand or soot

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<v Speaker 3>forged in the dying breaths of older stars.

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<v Speaker 2>Okay, so stellar's soot.

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<v Speaker 3>Yes, and these solid grains act as a catalytic docking station.

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<v Speaker 2>So a single hydrogen atom is flying through the stadium

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<v Speaker 2>and instead of hitting another atom, it crashes into this giant,

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<v Speaker 2>well relatively speaking, grain of soot yes.

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<v Speaker 3>It hits the dust grain and actually sticks to its surface.

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<v Speaker 3>The dust grain absorbs the atom's kinetic energy, acting as

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<v Speaker 3>a thermal sink.

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<v Speaker 2>Oh, so it bleeds off the speed exactly.

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<v Speaker 3>Then another hydrogen atom hits that exact same dust grain.

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<v Speaker 3>It wanders around the solid surface until it finds the

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<v Speaker 3>first atom.

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<v Speaker 2>And because they're both slowed down, they bond.

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<v Speaker 3>They form molecular hydrogen and then drift off the dust

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<v Speaker 3>grain together into space.

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<v Speaker 2>So the dust is literally acting like a cosmic anvil

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<v Speaker 2>where the fuel for stars is hammered together.

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<v Speaker 3>It is the factory floor of star formation. But its

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<v Speaker 3>job doesn't end there.

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<v Speaker 2>There's more.

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<v Speaker 3>Oh yeah. Once that molecular hydrogen forms, it is incredibly fragile.

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<v Speaker 3>A galaxy is a violent place, fle with harsh, destructive

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<v Speaker 3>ultraviolet radiation pouring out of young hot stars.

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<v Speaker 2>So it's basically a hostile environment for these new molecules.

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<v Speaker 3>Very hostile if that UV radiation hits our newly formed

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<v Speaker 3>molecular hydrogen, it excites the molecule, heats it up, and

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<v Speaker 3>literally blasts it apart. Oh, it destroys the fuel supply

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<v Speaker 3>for any future stars. It just sterilizes the whole region precisely,

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<v Speaker 3>unless the dust steps in again.

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<v Speaker 2>The VIP returns exactly.

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<v Speaker 3>Cosmic dust is incredibly effective at absorbing ultraviolet light. It

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<v Speaker 3>blankets these cold molecular clouds, acting as a physical shield,

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<v Speaker 3>so it takes the hit right. The UV radiation hits

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<v Speaker 3>the dust on the outside of the cloud, while the

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<v Speaker 3>fragile hydrogen gas safely nestled deep inside remains freezing cold.

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<v Speaker 2>It's like the universe's own SBF ten thousand sunscreen.

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<v Speaker 3>That's a perfect analogy.

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<v Speaker 2>The dust takes the hit so the baby stars can

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<v Speaker 2>incubate in the dark cold center. And the clean Aber

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<v Speaker 2>project was the first time anyone managed to mathematically track

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<v Speaker 2>these microscopic sit grains, like their chemical reactions and their

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<v Speaker 2>shielding effects across an entire simulated.

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<v Speaker 3>Universe on this massive of a scale.

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<v Speaker 2>Yes, that is mind blowing.

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<v Speaker 3>And what's fascinating here is that introducing dust didn't just

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<v Speaker 3>fix the physics. It completely revolutionized the visuals of the

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<v Speaker 3>simulation too. How so, Well, think about it. If the

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<v Speaker 3>dust is absorbing all that intense ultraviolet starlight, that energy

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<v Speaker 3>can't just vanish. The laws of thermodynamics dictate it has

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<v Speaker 3>to go somewhere.

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<v Speaker 2>Right, energy cannot be created or destroyed. So the dust

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<v Speaker 2>heats up and starts glowing in a different wavelength exactly.

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<v Speaker 2>It re emits the energy as intrared light.

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<v Speaker 3>Exactly, and that completely alters how a simulated galaxy appears

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<v Speaker 3>when we look at it. Yeah, for the first time,

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<v Speaker 3>researchers were creating virtual galaxies that didn't just have the

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<v Speaker 3>right mass or gravity.

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<v Speaker 2>They actually looked real.

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<v Speaker 3>They actually look like the galaxies we observed through infrared telescopes.

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<v Speaker 2>I was actually looking at the visual outputs the Collier

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<v Speaker 2>team published. They showed a rendering of a virtual disk

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<v Speaker 2>galaxy structurally very similar to our ow Milky Way, right,

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<v Speaker 2>from two different perspectives.

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<v Speaker 3>Yes, the face on on edge on views right.

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<v Speaker 2>When you look at it face on from the top down,

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<v Speaker 2>it is this brilliant glowing spiral of starlight. But when

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<v Speaker 2>they rotate the simulation and show it to you edge

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<v Speaker 2>on from the side, the starlight is suddenly choked out

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<v Speaker 2>by this dense, dark, suffocating band of dust slicing right

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<v Speaker 2>through the galactic equator.

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<v Speaker 3>It's a dramatic visual shift, it really is.

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<v Speaker 2>It perfectly mimics the real optical telescope images we get

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<v Speaker 2>of edge on galaxies, and that.

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<v Speaker 3>Visual fidelity is what makes this a monumental achievement. We

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<v Speaker 3>are no longer limited to comparing abstract graphs of theoretical mass.

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<v Speaker 2>You know, we're comparing actual pictures exactly.

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<v Speaker 3>We can take a real observed image from a space telescope,

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<v Speaker 3>put it next to a simulated image from collar, run

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<v Speaker 3>both images through the exact same analytical software, and test

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<v Speaker 3>if they match. We can measure the exact obscuration of light.

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<v Speaker 2>But hold on. The sheer computational brute force required to

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<v Speaker 2>do that is I mean, I can't even process it.

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<v Speaker 3>It's staggering.

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<v Speaker 2>You are asking a computer to track microscopic grains of soot,

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<v Speaker 2>calculate the fluid dynamics of freezing gas, apply the gravitational

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<v Speaker 2>pull of billions of dark matter halos, and compute the

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<v Speaker 2>radiation physics of starlight, all across a volume of space

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<v Speaker 2>that spans hundreds of millions of light years.

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<v Speaker 3>It's a lot of math.

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<v Speaker 2>What kind of machine is actually capable of calculating that matrix?

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00:16:25.120 --> 00:16:28.600
<v Speaker 3>Well, it requires an architecture that is almost as complex

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<v Speaker 3>as the simulation itself. The physical engine running this was

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<v Speaker 3>the cost Am Supercomputer, which is hosted by the DRAC

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<v Speaker 3>National Facility at Durham University in the UK. Oh but

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<v Speaker 3>hardware alone isn't enough. You can have the absolute fastest

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<v Speaker 3>supercomputer in the world and if your code is inefficient,

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<v Speaker 3>it will still crash when trying to simulate a freezing.

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<v Speaker 2>Galaxy, right because of that resolution bottleneck we talked about

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<v Speaker 2>earlier Exactly.

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<v Speaker 3>The real hero here is the software code they wrote,

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<v Speaker 3>which is called swift.

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<v Speaker 2>Swift Okay, so how does swift handle the math differently

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<v Speaker 2>then the older codes that used to crash when the

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<v Speaker 2>gas got cold.

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<v Speaker 3>Older cosmological codes usually operated on rigid time steps.

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<v Speaker 2>What does that mean?

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<v Speaker 3>It means the computer would calculate the gravity, temperature, and

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<v Speaker 3>velocity of every single particle in the entire universe, move

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<v Speaker 3>the simulation forward by one tick of the cosmic clock,

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<v Speaker 3>and then recalculate everything all over again.

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<v Speaker 2>Oh wow, So which means the computer has to wait

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<v Speaker 2>for the absolute slowest, most complicated calculation to finish before

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<v Speaker 2>the whole universe is allowed to move forward one second exactly.

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<v Speaker 3>It creates massive processing.

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<v Speaker 2>Bottlenecks like a traffic jam.

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<v Speaker 3>Very much like a traffic jam, Swift entirely abandoned that model.

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<v Speaker 3>It uses task based asynchronous parallelism, meaning it breaks the

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<v Speaker 3>universe down into millions of independent tasks. If a cold,

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<v Speaker 3>dense cloud of gas in one corner of the simulation

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<v Speaker 3>is highly chaotic and needs to be calculated in incredibly

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<v Speaker 3>tiny fractions of a second, the processor handles that.

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<v Speaker 2>Locally without making the rest of the universe.

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<v Speaker 3>Wait right, without forcing a quiet, empty void on the

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<v Speaker 3>other side of the virtual universe to slow down and

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<v Speaker 3>wait for it. The code dynamically shifts computational power exactly

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<v Speaker 3>where it is needed the millisecond it is needed.

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<v Speaker 2>So it's essentially a self optimizing universe. It is, And

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<v Speaker 2>even with that hyper efficient code, the scale of the

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<v Speaker 2>simulation they ran is just staggering. I want you, the listener,

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<v Speaker 2>to really internalize these numbers for a second. The largest

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<v Speaker 2>simulation in the Calibra suite required seventy two million CPU

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<v Speaker 2>hours to complete.

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<v Speaker 3>That's seventy two million hours of continuous processing.

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<v Speaker 2>Seventy two million. If you somehow manage to install this

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<v Speaker 2>swift code onto a top of the line twenty twenty

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<v Speaker 2>six gaming laptop and you hit run, your computer would

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<v Speaker 2>have to sit there processing it one hundred percent maximum

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<v Speaker 2>capacity twenty four hours a day for over eight thousand

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<v Speaker 2>years before it finished calculating what calls an A eight did.

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<v Speaker 3>And that seventy two million hours produced a volume of

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<v Speaker 3>space that is unprecedented in its resolution. They build multiple

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<v Speaker 3>simulated universes, but their largest box is a side length

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<v Speaker 3>of four hundred coup moving megaparsex.

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00:19:00.079 --> 00:19:03.920
<v Speaker 2>Now wait, co moving megaparsex. A megaparsec is about three

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<v Speaker 2>point twenty six million light years. But what does comoving mean?

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00:19:08.160 --> 00:19:09.839
<v Speaker 2>Why not just say a billion light years?

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00:19:09.880 --> 00:19:12.680
<v Speaker 3>Well, because the universe is expanding, right. If you measure

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00:19:12.720 --> 00:19:16.519
<v Speaker 3>the distance between two galaxies today and then wait a

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00:19:16.559 --> 00:19:19.799
<v Speaker 3>billion years, the distance between them will be larger, even

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00:19:19.839 --> 00:19:22.920
<v Speaker 3>if the galaxies themselves haven't actually traveled through space.

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00:19:23.039 --> 00:19:24.720
<v Speaker 2>The space itself stretched.

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00:19:24.359 --> 00:19:28.119
<v Speaker 3>Exactly, space is self stretched. Co moving is a coordinate

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00:19:28.119 --> 00:19:30.279
<v Speaker 3>system that expands along with the universe.

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00:19:30.440 --> 00:19:31.200
<v Speaker 2>How does that work?

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00:19:31.359 --> 00:19:34.440
<v Speaker 3>It's like drawing two dots on a deflated balloon. As

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00:19:34.480 --> 00:19:37.079
<v Speaker 3>you blow the balloon up, the dots get further apart,

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00:19:37.160 --> 00:19:41.160
<v Speaker 3>but their comoving distance, their relative position on the rubber,

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00:19:41.480 --> 00:19:42.720
<v Speaker 3>stays exactly the same.

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00:19:42.799 --> 00:19:43.720
<v Speaker 2>Oh, it's a great visual.

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00:19:43.920 --> 00:19:47.039
<v Speaker 3>Using co moving MEGAPARSEX allows the simulation to track the

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00:19:47.079 --> 00:19:50.440
<v Speaker 3>evolution of matter without the math getting distorted by the

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00:19:50.480 --> 00:19:51.960
<v Speaker 3>expansion of space itself.

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00:19:52.160 --> 00:19:55.039
<v Speaker 2>That is deeply counterintuitive, right, but it makes perfect sense

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00:19:55.079 --> 00:19:58.279
<v Speaker 2>for a simulation tracking fourteen billion years of history. It's

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00:19:58.319 --> 00:20:01.359
<v Speaker 2>a SEX. So this massive bos over a billion light

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00:20:01.480 --> 00:20:06.240
<v Speaker 2>years across, is just relentlessly churning through these equations. And

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00:20:06.279 --> 00:20:10.279
<v Speaker 2>there's a quote about this process from Carlos Frank he's

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<v Speaker 2>the Ogden Professor of Fundamental physics and a core member

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00:20:13.559 --> 00:20:15.680
<v Speaker 2>of this team that I found deeply profound.

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00:20:15.759 --> 00:20:17.119
<v Speaker 3>Yeah, he summed it up perfectly.

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00:20:17.279 --> 00:20:20.559
<v Speaker 2>He pointed out that they didn't paint these galaxies. They

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00:20:20.599 --> 00:20:23.960
<v Speaker 2>didn't tell the computer, hey, put a spiral galaxy over here,

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00:20:24.000 --> 00:20:25.720
<v Speaker 2>in an elliptical galaxy over there.

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00:20:25.839 --> 00:20:27.359
<v Speaker 3>No no hard coating shapes.

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00:20:27.440 --> 00:20:31.920
<v Speaker 2>They literally just inputted the raw fundamental equations of gravity, thermodynamics,

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00:20:31.960 --> 00:20:34.640
<v Speaker 2>and chemistry, hit play on the Big Bang, and the

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00:20:34.680 --> 00:20:35.880
<v Speaker 2>galaxies built themselves.

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00:20:35.920 --> 00:20:39.400
<v Speaker 3>It is the ultimate testament to the emergent complexity of physics.

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00:20:39.519 --> 00:20:40.240
<v Speaker 2>It really is.

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00:20:40.400 --> 00:20:43.799
<v Speaker 3>When you finally provide the equations with sufficient resolution, when

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00:20:43.839 --> 00:20:46.880
<v Speaker 3>you respect the dust and the cold gas, reality naturally

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00:20:46.880 --> 00:20:50.680
<v Speaker 3>emerges from the math. Wow, the simulated galaxy spontaneously grew

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00:20:50.720 --> 00:20:53.599
<v Speaker 3>to have the exact same masses, the exact same colors,

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00:20:53.599 --> 00:20:57.759
<v Speaker 3>and the exact same chemical compositions, what astronomers call metallicity

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00:20:58.160 --> 00:20:59.799
<v Speaker 3>as the real galaxies we observe.

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00:21:00.119 --> 00:21:03.359
<v Speaker 2>Let's actually define metallicity real quick, because astronomers use that

433
00:21:03.400 --> 00:21:05.000
<v Speaker 2>word very differently than normal people do.

434
00:21:05.119 --> 00:21:06.000
<v Speaker 3>That's true, they do.

435
00:21:06.240 --> 00:21:09.039
<v Speaker 2>If I say metal, people think of iron or aluminum, right.

436
00:21:09.079 --> 00:21:12.319
<v Speaker 3>But to an astrophysicist, the periodic table is incredibly simple.

437
00:21:12.559 --> 00:21:16.079
<v Speaker 3>There is hydrogen, there is helium, and literally every other

438
00:21:16.119 --> 00:21:20.279
<v Speaker 3>element in the universe carbon, oxygen, nitrogen, Iron is considered.

439
00:21:19.880 --> 00:21:21.839
<v Speaker 2>A metal, So oxygen is a metal.

440
00:21:21.920 --> 00:21:25.599
<v Speaker 3>In astronomy, yes, these heavy metals are forged in the

441
00:21:25.680 --> 00:21:29.119
<v Speaker 3>nuclear furnaces of early stars and then blasted out into

442
00:21:29.119 --> 00:21:32.720
<v Speaker 3>space when those stars die in supernovae.

443
00:21:31.920 --> 00:21:34.839
<v Speaker 4>And then that seeds the next generation exactly that metal

444
00:21:34.920 --> 00:21:38.440
<v Speaker 4>rich dust then seeds the next generation of stars caliber

445
00:21:38.559 --> 00:21:42.559
<v Speaker 4>track that exact chemical enrichment process over billions of years.

446
00:21:42.680 --> 00:21:46.079
<v Speaker 2>Okay, so building this ultimate virtual laboratory is an absolute

447
00:21:46.200 --> 00:21:50.559
<v Speaker 2>marvel of human engineering. But the critical question is what

448
00:21:50.720 --> 00:21:51.400
<v Speaker 2>do we do with it?

449
00:21:51.599 --> 00:21:52.960
<v Speaker 3>Right? Application is key?

450
00:21:53.279 --> 00:21:57.039
<v Speaker 2>Did spending seventy two million CPU hours actually solve any

451
00:21:57.160 --> 00:22:00.759
<v Speaker 2>real world problems? Because right around the time the supercomputer

452
00:22:00.920 --> 00:22:04.880
<v Speaker 2>was redlining, the actual astronomy community was undergoing a massive

453
00:22:04.920 --> 00:22:06.400
<v Speaker 2>existential crisis, weren't they.

454
00:22:06.559 --> 00:22:09.680
<v Speaker 3>They were in an absolute panic, and that panic was

455
00:22:09.960 --> 00:22:13.200
<v Speaker 3>entirely courtesy of the James Web Space Telescope.

456
00:22:13.240 --> 00:22:17.160
<v Speaker 2>I remember this. When JWST finally launched and sent back

457
00:22:17.240 --> 00:22:21.799
<v Speaker 2>its first deep field images, it pointed its incredibly sensitive

458
00:22:21.880 --> 00:22:26.279
<v Speaker 2>infrared sensors at the very edge of the observable universe, right, yes,

459
00:22:26.519 --> 00:22:29.079
<v Speaker 2>peering into the first few hundred million years, right after

460
00:22:29.119 --> 00:22:32.240
<v Speaker 2>the Big Bang. Because you know, light takes time to travel,

461
00:22:32.440 --> 00:22:35.200
<v Speaker 2>so looking far away is literally looking back in time.

462
00:22:35.319 --> 00:22:38.640
<v Speaker 3>Yes, it's a time machine. And the established standard model

463
00:22:38.640 --> 00:22:42.240
<v Speaker 3>of cosmology, which is called the Lambda CDM model, incorporating

464
00:22:42.319 --> 00:22:46.160
<v Speaker 3>dark energy and cold dark matter, had very specific predictions

465
00:22:46.160 --> 00:22:48.319
<v Speaker 3>for what the universe should look like in that early era.

466
00:22:48.440 --> 00:22:49.440
<v Speaker 2>What were those predictions?

467
00:22:49.599 --> 00:22:53.279
<v Speaker 3>The model predicted that really, galaxies should be small, chaotic,

468
00:22:53.559 --> 00:22:57.759
<v Speaker 3>ragged little clumps of stars slowly building themselves up over

469
00:22:57.839 --> 00:23:01.559
<v Speaker 3>billions of years, like stepping stones exactly. But when JWST

470
00:23:01.720 --> 00:23:04.240
<v Speaker 3>looked back at the dawn of time, it didn't find

471
00:23:04.359 --> 00:23:05.359
<v Speaker 3>ragged little clumps.

472
00:23:05.480 --> 00:23:05.640
<v Speaker 2>No.

473
00:23:05.839 --> 00:23:10.200
<v Speaker 3>No, it found massive, incredibly bright, fully formed galaxies.

474
00:23:10.640 --> 00:23:13.640
<v Speaker 2>They were way too big, way too fast. I remember.

475
00:23:13.640 --> 00:23:18.240
<v Speaker 2>The headlines were everywhere. JWST breaks the universe, The Big

476
00:23:18.279 --> 00:23:19.319
<v Speaker 2>Bang theory is wrong.

477
00:23:19.880 --> 00:23:21.799
<v Speaker 3>It was a very dramatic few months.

478
00:23:21.880 --> 00:23:24.640
<v Speaker 2>It was as if an archaeologist dug down into a

479
00:23:24.680 --> 00:23:28.880
<v Speaker 2>Bronze Age settlement and found a fully functional nuclear reactor.

480
00:23:29.440 --> 00:23:33.000
<v Speaker 2>It violated the established timeline of reality. You could feel

481
00:23:33.039 --> 00:23:34.599
<v Speaker 2>the tension in the scientific community.

482
00:23:34.680 --> 00:23:36.720
<v Speaker 3>People were genuinely terrified, right.

483
00:23:36.799 --> 00:23:40.519
<v Speaker 2>People were terrified that the fundamental blueprint of cosmology, which

484
00:23:40.640 --> 00:23:43.960
<v Speaker 2>thousands of scientists had dedicated their entire lives to, was

485
00:23:43.960 --> 00:23:44.960
<v Speaker 2>fundamentally broken.

486
00:23:45.079 --> 00:23:47.720
<v Speaker 3>The dread was very real. If the standard model was wrong,

487
00:23:47.799 --> 00:23:51.200
<v Speaker 3>it meant we basically understood nothing about dark matter or

488
00:23:51.279 --> 00:23:51.920
<v Speaker 3>dark energy.

489
00:23:52.039 --> 00:23:53.640
<v Speaker 2>We have to start from scratch, essentially.

490
00:23:53.759 --> 00:23:56.839
<v Speaker 3>Yes, and this is exactly where the Khaliber project proved

491
00:23:56.880 --> 00:23:59.079
<v Speaker 3>its immense, undeniable.

492
00:23:58.480 --> 00:24:00.480
<v Speaker 2>Value because they could test it right.

493
00:24:00.960 --> 00:24:03.480
<v Speaker 3>Doctor of Yenni Chaikin, the lead author of several of

494
00:24:03.519 --> 00:24:07.559
<v Speaker 3>the major calabor papers, used this brand new virtual universe

495
00:24:07.720 --> 00:24:12.559
<v Speaker 3>to test the crisis. The team essentially acted as virtual astronomers.

496
00:24:13.039 --> 00:24:16.039
<v Speaker 3>They aimed a digital version of the James Web Telescope

497
00:24:16.079 --> 00:24:18.920
<v Speaker 3>into the deep past of their simulated universe to see

498
00:24:18.920 --> 00:24:19.640
<v Speaker 3>what they would find.

499
00:24:20.000 --> 00:24:23.519
<v Speaker 2>And here's where it gets really interesting. The standard model

500
00:24:23.559 --> 00:24:26.240
<v Speaker 2>wasn't broken at all, was it. We just had terrible

501
00:24:26.319 --> 00:24:27.319
<v Speaker 2>rendering software.

502
00:24:27.519 --> 00:24:30.759
<v Speaker 3>That is exactly what they proved when doctor Chakin ran

503
00:24:30.799 --> 00:24:35.839
<v Speaker 3>the virtual observation. The Caliber simulation effortlessly produced those exact

504
00:24:35.880 --> 00:24:40.359
<v Speaker 3>same massive, hyper bright early galaxies that the real JWST

505
00:24:40.519 --> 00:24:44.400
<v Speaker 3>was seeing. Wow, they naturally emerged within the strict confines

506
00:24:44.400 --> 00:24:46.400
<v Speaker 3>of the standard Lambda CDM model.

507
00:24:46.680 --> 00:24:50.039
<v Speaker 2>Wait, if the standard model allowed for these massive galaxies

508
00:24:50.079 --> 00:24:53.000
<v Speaker 2>the whole time, why did our previous predictions say they

509
00:24:53.000 --> 00:24:53.720
<v Speaker 2>shouldn't exist?

510
00:24:53.759 --> 00:24:56.920
<v Speaker 3>Because the previous predictions were based on legacy simulations that

511
00:24:56.960 --> 00:24:59.039
<v Speaker 3>couldn't model cold gas and dust.

512
00:24:59.319 --> 00:25:01.799
<v Speaker 2>Oh the ten thousand degree floor.

513
00:25:02.079 --> 00:25:06.559
<v Speaker 3>Remember that heat barrier. If your simulated universe artificially prevents

514
00:25:06.599 --> 00:25:09.920
<v Speaker 3>gas from cooling, you are artificially suppressing the rate at

515
00:25:09.920 --> 00:25:11.319
<v Speaker 3>which stars can form, So.

516
00:25:11.319 --> 00:25:13.039
<v Speaker 2>You're stunting their growth in the simulation.

517
00:25:13.319 --> 00:25:17.960
<v Speaker 3>Precisely, your virtual early universe will look sluggish and dim,

518
00:25:18.319 --> 00:25:21.279
<v Speaker 3>not because the fundamental laws of cosmology dictate it, but

519
00:25:21.400 --> 00:25:24.000
<v Speaker 3>because your computer code is stifling the chemistry.

520
00:25:24.240 --> 00:25:27.039
<v Speaker 2>So the moment Cobbra added the microscopic dust and let

521
00:25:27.079 --> 00:25:30.119
<v Speaker 2>the gas freeze, the early galaxies suddenly had the fuel

522
00:25:30.160 --> 00:25:34.000
<v Speaker 2>they needed to ignite massive firestorms of rapid star formation,

523
00:25:34.519 --> 00:25:36.640
<v Speaker 2>matching the JWST data perfectly.

524
00:25:36.839 --> 00:25:41.960
<v Speaker 3>Yes, And furthermore, caullibly successfully modeled the intense explosive outflows

525
00:25:41.960 --> 00:25:45.039
<v Speaker 3>of energy driven by those early stars and super massive

526
00:25:45.039 --> 00:25:45.680
<v Speaker 3>black holes.

527
00:25:45.960 --> 00:25:47.240
<v Speaker 2>It all just clicked into place.

528
00:25:47.440 --> 00:25:50.279
<v Speaker 3>It proved that the universe didn't need entirely new physics,

529
00:25:50.519 --> 00:25:54.200
<v Speaker 3>It just needed us to model the messy microscopic chemistry correctly.

530
00:25:54.759 --> 00:25:57.359
<v Speaker 3>If we connect this to the bigger picture, it shows

531
00:25:57.440 --> 00:26:00.000
<v Speaker 3>the standard cosmological model is perfectly sound.

532
00:26:00.200 --> 00:26:03.839
<v Speaker 2>I can just imagine the collective exhale across university physics

533
00:26:03.839 --> 00:26:04.920
<v Speaker 2>departments worldwide.

534
00:26:05.039 --> 00:26:07.039
<v Speaker 3>Oh, the relief was palpable.

535
00:26:07.119 --> 00:26:10.359
<v Speaker 2>It's a profound lesson When a new, shiny piece of

536
00:26:10.400 --> 00:26:14.720
<v Speaker 2>technology like JWST gives you observations that contradict your life's work.

537
00:26:15.200 --> 00:26:18.240
<v Speaker 2>The immediate reaction shouldn't be to throw out the physics textbook.

538
00:26:18.279 --> 00:26:18.400
<v Speaker 1>Right.

539
00:26:18.480 --> 00:26:22.200
<v Speaker 2>Sometimes the overarching theory is perfectly fine, but your ability

540
00:26:22.200 --> 00:26:26.279
<v Speaker 2>to model its intricate emergent behaviors is just lacking.

541
00:26:26.559 --> 00:26:29.960
<v Speaker 3>It is a massive victory for the standard model. And

542
00:26:30.000 --> 00:26:33.000
<v Speaker 3>there's a but here. The universe still has secrets that

543
00:26:33.079 --> 00:26:37.680
<v Speaker 3>even seventy two million CPU hours couldn't decipher. Because as

544
00:26:37.759 --> 00:26:40.799
<v Speaker 3>brilliantly as coll A solve the crisis of the massive

545
00:26:40.839 --> 00:26:44.599
<v Speaker 3>early galaxies, it ran into an absolute brick wall when

546
00:26:44.599 --> 00:26:48.359
<v Speaker 3>it came to another of Jawst's most bizarre discoveries.

547
00:26:48.440 --> 00:26:51.799
<v Speaker 2>You're talking about the phenomena that astrophysicists are currently referring

548
00:26:51.880 --> 00:26:55.000
<v Speaker 2>to as the ghosts in the machine. Yes, the little red.

549
00:26:54.880 --> 00:26:58.480
<v Speaker 3>Dots and little red dots. It is such an unassuming,

550
00:26:58.799 --> 00:27:02.559
<v Speaker 3>cute name for what are essentially the most terrifying cosmic

551
00:27:02.599 --> 00:27:03.799
<v Speaker 3>monsters in the early universe.

552
00:27:03.880 --> 00:27:04.759
<v Speaker 2>What exactly are they?

553
00:27:05.039 --> 00:27:05.279
<v Speaker 1>Well?

554
00:27:05.400 --> 00:27:11.240
<v Speaker 3>Jwst discovered these highly compact, heavily obscured, intensely red sources

555
00:27:11.279 --> 00:27:13.960
<v Speaker 3>of light buried deep in the first billion years of

556
00:27:14.000 --> 00:27:17.200
<v Speaker 3>the cosmos. The current consensus is that we're looking at

557
00:27:17.200 --> 00:27:20.519
<v Speaker 3>the foundational seeds of supermassive black holes.

558
00:27:20.319 --> 00:27:23.599
<v Speaker 2>Right because we know that almost every large galaxy today,

559
00:27:23.640 --> 00:27:26.720
<v Speaker 2>including our Milky Way, has a supermassive black hole at

560
00:27:26.720 --> 00:27:29.720
<v Speaker 2>its dead center. We're orbiting one right now exactly. Some

561
00:27:29.799 --> 00:27:32.279
<v Speaker 2>of them are billions of times the mass of our Sun.

562
00:27:33.720 --> 00:27:36.559
<v Speaker 2>But the mystery has always been, Yeah, how did they

563
00:27:36.599 --> 00:27:40.880
<v Speaker 2>get so monstrously huge so early in the universe's timeline.

564
00:27:40.920 --> 00:27:42.319
<v Speaker 3>It's a massive timing problem.

565
00:27:42.400 --> 00:27:44.960
<v Speaker 2>There simply wasn't enough time for a normal sized black

566
00:27:45.000 --> 00:27:48.759
<v Speaker 2>hole to slowly eat enough gas to get that big.

567
00:27:48.920 --> 00:27:53.680
<v Speaker 3>And this is where the grand perfect colliber simulation basically

568
00:27:53.720 --> 00:27:56.039
<v Speaker 3>throws its hands in the air and gives up. Really,

569
00:27:56.119 --> 00:28:00.599
<v Speaker 3>the simulation cannot mathematically predict or naturally form these early

570
00:28:00.799 --> 00:28:02.759
<v Speaker 3>supermassive black hole seeds.

571
00:28:02.839 --> 00:28:06.720
<v Speaker 2>This shocked me. Wait, so after a decade of international collaboration,

572
00:28:06.839 --> 00:28:09.680
<v Speaker 2>writing millions of lines of the most advanced physics code

573
00:28:09.720 --> 00:28:12.359
<v Speaker 2>ever conceived, and letting a supercomputer chew on it for

574
00:28:12.400 --> 00:28:16.000
<v Speaker 2>eight thousand computational years, the scientists still have to manually

575
00:28:16.039 --> 00:28:18.799
<v Speaker 2>plant black holes in the simulation like they're planting trees

576
00:28:18.839 --> 00:28:19.799
<v Speaker 2>in a digital garden.

577
00:28:19.920 --> 00:28:22.880
<v Speaker 3>We do, We literally have to do that. The simulation

578
00:28:22.960 --> 00:28:25.480
<v Speaker 3>assumes the black hole seeds already exist at a certain

579
00:28:25.519 --> 00:28:28.000
<v Speaker 3>mass and manually injects them into the centers of the

580
00:28:28.119 --> 00:28:29.440
<v Speaker 3>virtual early galaxies.

581
00:28:29.720 --> 00:28:32.920
<v Speaker 2>That feels like a cheat code. Why can we perfectly

582
00:28:32.960 --> 00:28:36.680
<v Speaker 2>simulate the fluid dynamics of a cold dust cloud condensing

583
00:28:36.720 --> 00:28:39.519
<v Speaker 2>into a star? Now, we can't simulate the genesis of

584
00:28:39.559 --> 00:28:40.559
<v Speaker 2>a black hole.

585
00:28:40.480 --> 00:28:44.920
<v Speaker 3>Because the birth of these specific supermassive seeds requires physics

586
00:28:44.960 --> 00:28:47.000
<v Speaker 3>that humanity does not fully understand yet.

587
00:28:47.039 --> 00:28:48.599
<v Speaker 2>We just don't have the equations right.

588
00:28:48.839 --> 00:28:52.079
<v Speaker 3>Simulating a star is incredibly complex, but we know the

589
00:28:52.160 --> 00:28:55.519
<v Speaker 3>rules of thermodynamics and nuclear fusion. But the origin of

590
00:28:55.559 --> 00:28:58.359
<v Speaker 3>these little red dots is a theoretical frontier.

591
00:28:58.680 --> 00:28:59.599
<v Speaker 2>So what are the theories?

592
00:29:00.119 --> 00:29:03.559
<v Speaker 3>Well, some cosmologists hypothesize that they form from the direct

593
00:29:03.559 --> 00:29:07.480
<v Speaker 3>collapse of massive, pristine, metal free gas clouds, meaning.

594
00:29:07.319 --> 00:29:10.279
<v Speaker 2>The gas cloud gets so heavy it just entirely skips

595
00:29:10.319 --> 00:29:13.240
<v Speaker 2>the process of becoming a star and immediately crushes itself

596
00:29:13.279 --> 00:29:14.599
<v Speaker 2>into a black hole singularity.

597
00:29:14.720 --> 00:29:18.759
<v Speaker 3>Yes, just an instant massive collapse. Other theories suggest they

598
00:29:18.759 --> 00:29:22.880
<v Speaker 3>are formed from runaway chain reaction collisions inside unbelievably dense

599
00:29:23.000 --> 00:29:24.680
<v Speaker 3>early star clusters.

600
00:29:24.160 --> 00:29:25.720
<v Speaker 2>Like a cosmic demolition derby.

601
00:29:26.000 --> 00:29:29.839
<v Speaker 3>Essentially, yes, but the gravity and density involved in these

602
00:29:29.880 --> 00:29:34.400
<v Speaker 3>events approach the singularity, the point where our current mathematical

603
00:29:34.400 --> 00:29:38.759
<v Speaker 3>equations for general relativity literally break down and output infinities.

604
00:29:38.960 --> 00:29:41.160
<v Speaker 2>The math just stops working exactly.

605
00:29:41.319 --> 00:29:46.079
<v Speaker 3>To model those events natively without manual human intervention, will

606
00:29:46.119 --> 00:29:50.400
<v Speaker 3>require grid resolutions that make Colliber look primitive and entirely

607
00:29:50.440 --> 00:29:53.359
<v Speaker 3>new equations of quantum gravity written into the code.

608
00:29:53.799 --> 00:29:57.240
<v Speaker 2>It is a phenomenal reality check. The simulation is a

609
00:29:57.319 --> 00:30:01.039
<v Speaker 2>flawless mirror of nature, right up until the exact millimeter

610
00:30:01.440 --> 00:30:03.799
<v Speaker 2>where human knowledge itself hits a cliff.

611
00:30:03.920 --> 00:30:05.440
<v Speaker 3>It is a very stark boundary.

612
00:30:05.480 --> 00:30:07.559
<v Speaker 2>But the team isn't just packing up their bags, are

613
00:30:07.559 --> 00:30:07.920
<v Speaker 2>they not?

614
00:30:08.000 --> 00:30:11.119
<v Speaker 3>At all? While the foundational Colliber runs were completed recently,

615
00:30:11.240 --> 00:30:15.079
<v Speaker 3>some of the absolute highest resolution simulations are currently running

616
00:30:15.160 --> 00:30:18.559
<v Speaker 3>right now, eating up more processor hours trying to push

617
00:30:18.599 --> 00:30:21.680
<v Speaker 3>that boundary further. The work continues, oh absolutely, And the

618
00:30:21.720 --> 00:30:25.200
<v Speaker 3>data they've already generated is so vast, petabytes upon petabytes

619
00:30:25.200 --> 00:30:28.400
<v Speaker 3>of information that it will take the global scientific community

620
00:30:28.440 --> 00:30:31.359
<v Speaker 3>a decade just to fully read and analyze it.

621
00:30:31.480 --> 00:30:34.279
<v Speaker 2>And while the supercomputers grind away at the next era

622
00:30:34.400 --> 00:30:38.880
<v Speaker 2>of frontier physics, the scientists have developed a radical, entirely

623
00:30:39.000 --> 00:30:42.240
<v Speaker 2>new way for humans to experience the petabytes of data

624
00:30:42.279 --> 00:30:44.720
<v Speaker 2>we already have. This might be my favorite part, which

625
00:30:44.720 --> 00:30:48.119
<v Speaker 2>brings us to the final and visually, or rather sensorily,

626
00:30:48.240 --> 00:30:51.839
<v Speaker 2>most fascinating aspect of this endeavor. We aren't just looking

627
00:30:51.880 --> 00:30:54.759
<v Speaker 2>at the virtual universe anymore. We are hearing it.

628
00:30:55.079 --> 00:30:58.039
<v Speaker 3>This is a truly innovative approach led by doctor James

629
00:30:58.119 --> 00:31:00.000
<v Speaker 3>Treyford at the University of Portsmouth.

630
00:31:00.200 --> 00:31:00.440
<v Speaker 2>Right.

631
00:31:00.599 --> 00:31:04.039
<v Speaker 3>He was the lead developer of Climber's complex dust model,

632
00:31:04.279 --> 00:31:06.960
<v Speaker 3>but he also spearheaded the creation of what they call

633
00:31:07.119 --> 00:31:11.680
<v Speaker 3>sonified videos. They are creating a multisensory cosmos.

634
00:31:11.920 --> 00:31:16.119
<v Speaker 2>Normally, astrophysics is entirely visual. We look at scatterplots, line graphs,

635
00:31:16.160 --> 00:31:19.720
<v Speaker 2>and beautiful false color renderings of nebulae. But doctor Treyford

636
00:31:19.759 --> 00:31:24.599
<v Speaker 2>took this dense, mathematically terrifying digital universe and applied sonification,

637
00:31:24.920 --> 00:31:28.200
<v Speaker 2>essentially encoding physical astronomical data into sound.

638
00:31:28.480 --> 00:31:31.480
<v Speaker 3>And let's be clear about what sonification is not. They

639
00:31:31.519 --> 00:31:34.680
<v Speaker 3>aren't just overlaying a pretty Beethoven symphony onto a video

640
00:31:34.720 --> 00:31:35.759
<v Speaker 3>of a galaxy spinning.

641
00:31:35.839 --> 00:31:37.000
<v Speaker 2>It's not just a soundtrack.

642
00:31:37.279 --> 00:31:41.559
<v Speaker 3>No, they are mapping highly specific physical properties of the

643
00:31:41.599 --> 00:31:44.240
<v Speaker 3>simulated universe directly to acoustic parameters.

644
00:31:44.279 --> 00:31:46.160
<v Speaker 2>You give an example, sure.

645
00:31:46.319 --> 00:31:49.599
<v Speaker 3>For instance, the velocity of stars orbiting the galactic center

646
00:31:49.759 --> 00:31:52.119
<v Speaker 3>might be mapped to the pitch of the sound. The

647
00:31:52.240 --> 00:31:54.880
<v Speaker 3>rate at which new stars are forming the star formation

648
00:31:55.039 --> 00:31:57.759
<v Speaker 3>rate might be mapped to rhythm or volume.

649
00:31:57.920 --> 00:32:01.079
<v Speaker 2>So instead of trying to read a chaotic line graph,

650
00:32:01.359 --> 00:32:04.440
<v Speaker 2>you could listen to a galaxy and the pitch would

651
00:32:04.440 --> 00:32:09.079
<v Speaker 2>literally rise and fall as the galaxy's rotation speeds up

652
00:32:09.200 --> 00:32:10.759
<v Speaker 2>or slows down precisely.

653
00:32:10.960 --> 00:32:13.920
<v Speaker 3>Or imagine listening to the sonified data of a galaxy's

654
00:32:13.960 --> 00:32:15.160
<v Speaker 3>cold gas reserves.

655
00:32:15.279 --> 00:32:16.519
<v Speaker 2>Okay, what would that sound like?

656
00:32:16.599 --> 00:32:20.000
<v Speaker 3>You hear a steady, low frequency hum representing the molecular

657
00:32:20.079 --> 00:32:24.160
<v Speaker 3>hydrogen the fuel right then suddenly the hum is violently

658
00:32:24.160 --> 00:32:28.359
<v Speaker 3>interrupted by sharp, staccato, high pitched rhythmic bursts.

659
00:32:28.599 --> 00:32:29.400
<v Speaker 2>What's that?

660
00:32:29.400 --> 00:32:32.920
<v Speaker 3>That represents the thermal shock waves of supernovae exploding as

661
00:32:32.960 --> 00:32:34.680
<v Speaker 3>a burst of star formation occurs.

662
00:32:35.039 --> 00:32:37.960
<v Speaker 2>Wow, it's like atoustic diagnostics if you think about it.

663
00:32:38.000 --> 00:32:39.799
<v Speaker 2>Human beings do this all the time in everyday life.

664
00:32:39.880 --> 00:32:40.200
<v Speaker 3>We do.

665
00:32:40.519 --> 00:32:43.160
<v Speaker 2>Yeah. If you are sitting in traffic and your car's

666
00:32:43.240 --> 00:32:47.519
<v Speaker 2>engine suddenly starts making a subtle rhythmic ticking noise, your

667
00:32:47.559 --> 00:32:51.480
<v Speaker 2>brain detects that anomaly instantly, often long before a warning

668
00:32:51.559 --> 00:32:52.960
<v Speaker 2>light flashes on your dashboard.

669
00:32:53.039 --> 00:32:56.440
<v Speaker 3>That is exactly the cognitive mechanism doctor Treyford is tapping into.

670
00:32:56.839 --> 00:32:59.680
<v Speaker 3>This rate is an important question about how we process data.

671
00:33:00.200 --> 00:33:04.559
<v Speaker 3>Human hearing evolved to be extraordinarily sensitive to patterns, rhythms,

672
00:33:04.599 --> 00:33:06.799
<v Speaker 3>and subtle changes in frequency.

673
00:33:06.359 --> 00:33:07.480
<v Speaker 2>Much more so than our eyes.

674
00:33:07.480 --> 00:33:11.400
<v Speaker 3>Sometimes exactly, our auditory processing can often pick out a

675
00:33:11.480 --> 00:33:15.240
<v Speaker 3>single anomalous data point in a chaotic environment much faster

676
00:33:15.319 --> 00:33:18.000
<v Speaker 3>than our visual processing can spot a rogue dot on

677
00:33:18.079 --> 00:33:19.359
<v Speaker 3>a crowded scatterplot.

678
00:33:19.559 --> 00:33:22.440
<v Speaker 2>So if a simulated galaxy undergoes a violent merger with

679
00:33:22.480 --> 00:33:25.960
<v Speaker 2>another galaxy, the visual data on a screen might just

680
00:33:26.000 --> 00:33:29.119
<v Speaker 2>look like a messy, blindingly bright blob of light hard

681
00:33:29.160 --> 00:33:32.079
<v Speaker 2>to decipher right, But the Sonifi data would hit your

682
00:33:32.079 --> 00:33:35.559
<v Speaker 2>ears as a distinct, chaotic acoustic crash followed by a

683
00:33:35.599 --> 00:33:39.839
<v Speaker 2>settling resonance as the two gravitational fields finally merge and stabilize.

684
00:33:39.960 --> 00:33:43.599
<v Speaker 3>By making the data multisensory, they are effectively training human intuition.

685
00:33:43.799 --> 00:33:44.720
<v Speaker 2>That is so cool.

686
00:33:45.000 --> 00:33:48.119
<v Speaker 3>Science isn't just the cold collection of numbers, It is

687
00:33:48.200 --> 00:33:52.319
<v Speaker 3>the human comprehension of those numbers. By allowing researchers to

688
00:33:52.359 --> 00:33:55.839
<v Speaker 3>sit in the lab with headphones on and interactively fly

689
00:33:56.039 --> 00:33:59.599
<v Speaker 3>through the calabor universe, feeling the rhythm of star formation

690
00:33:59.759 --> 00:34:02.480
<v Speaker 3>and daring the pitch of dark matter gravity. They are

691
00:34:02.519 --> 00:34:07.160
<v Speaker 3>building a deeper, almost subconscious instinct for how galaxies evolve.

692
00:34:07.559 --> 00:34:11.239
<v Speaker 2>It bridges the gap between the incredibly abstract math of

693
00:34:11.280 --> 00:34:15.119
<v Speaker 2>an expanding universe and the physical sensory experience of the

694
00:34:15.199 --> 00:34:15.840
<v Speaker 2>human body.

695
00:34:16.000 --> 00:34:17.920
<v Speaker 3>It makes the math tangible.

696
00:34:17.440 --> 00:34:20.480
<v Speaker 2>It really does. It is an absolutely wild journey. When

697
00:34:20.480 --> 00:34:22.639
<v Speaker 2>you zoom out and look at the sheer scope of

698
00:34:22.679 --> 00:34:24.039
<v Speaker 2>what we've explored today, it.

699
00:34:24.039 --> 00:34:25.880
<v Speaker 3>Is a testament to how far we have come in

700
00:34:25.920 --> 00:34:27.039
<v Speaker 3>such a short amount of time.

701
00:34:27.280 --> 00:34:30.679
<v Speaker 2>We started with crude, legacy simulations that were literally too

702
00:34:30.719 --> 00:34:33.840
<v Speaker 2>hot to handle, restricted by an artificial ten thousand degree

703
00:34:33.840 --> 00:34:36.760
<v Speaker 2>floor that completely blinded us to the true nature of

704
00:34:36.760 --> 00:34:37.400
<v Speaker 2>star formation.

705
00:34:37.679 --> 00:34:40.280
<v Speaker 3>We couldn't see the forest for the fire, basically.

706
00:34:40.599 --> 00:34:45.559
<v Speaker 2>Right then, scientists painstakingly cracked the mathematical code of cosmic dust,

707
00:34:46.039 --> 00:34:49.639
<v Speaker 2>proving that the tiniest, most microscopic spects of soot are

708
00:34:49.639 --> 00:34:53.119
<v Speaker 2>the ultimate architects and thermal protectors of the largest galaxies

709
00:34:53.159 --> 00:34:56.360
<v Speaker 2>in existence, the cousin of VIPs. The VIPs, we unleashed

710
00:34:56.360 --> 00:34:59.920
<v Speaker 2>the unfathomable brute force of the cosm. A eight supercomputer

711
00:35:00.119 --> 00:35:04.159
<v Speaker 2>or burning through seventy two million asynchronous CPU hours to

712
00:35:04.199 --> 00:35:07.480
<v Speaker 2>synthesize a one to one scale universe out of pure

713
00:35:07.599 --> 00:35:11.159
<v Speaker 2>fluid dynamics in gravity, a digital triumphs, and in doing

714
00:35:11.239 --> 00:35:14.440
<v Speaker 2>so we essentially saved the standard model of the cosmos

715
00:35:14.599 --> 00:35:18.519
<v Speaker 2>from the terrifying reality bending early observations of the James

716
00:35:18.519 --> 00:35:19.760
<v Speaker 2>Webs based telescope.

717
00:35:19.960 --> 00:35:22.679
<v Speaker 3>And yet we are main profoundly humbled by the limitations

718
00:35:22.719 --> 00:35:25.199
<v Speaker 3>of our own knowledge, staring into the abyss of the

719
00:35:25.239 --> 00:35:27.960
<v Speaker 3>little red dots, waiting for the next generation of physics

720
00:35:28.000 --> 00:35:30.559
<v Speaker 3>to explain how the universe's ultimate monsters are born.

721
00:35:31.000 --> 00:35:34.199
<v Speaker 2>It really is a story of human audacity. And I

722
00:35:34.239 --> 00:35:36.519
<v Speaker 2>want to leave you with one final mind bending thought

723
00:35:36.639 --> 00:35:38.559
<v Speaker 2>to ponder as you go about the rest of your day.

724
00:35:38.719 --> 00:35:42.480
<v Speaker 2>We just spent this entire time dissecting how human beings

725
00:35:42.840 --> 00:35:47.400
<v Speaker 2>right now, in the twenty twenties, have built computers capable

726
00:35:47.400 --> 00:35:51.440
<v Speaker 2>of generating a digital universe so physically accurate, so perfectly rendered,

727
00:35:51.639 --> 00:35:55.480
<v Speaker 2>that even our best professional astronomers cannot distinguish its virtual

728
00:35:55.519 --> 00:35:56.760
<v Speaker 2>galaxies from reality.

729
00:35:57.079 --> 00:35:57.920
<v Speaker 3>That is a fact.

730
00:35:58.199 --> 00:36:00.480
<v Speaker 2>If we could achieve that level of simulation to what

731
00:36:00.559 --> 00:36:03.519
<v Speaker 2>happens in a century. What happens after a thousand years

732
00:36:03.519 --> 00:36:04.840
<v Speaker 2>of computational advancement.

733
00:36:04.960 --> 00:36:06.480
<v Speaker 3>It's almost scary to think about.

734
00:36:06.960 --> 00:36:11.000
<v Speaker 2>Is it entirely possible that the grand, beautiful, chaotic universe

735
00:36:11.039 --> 00:36:14.119
<v Speaker 2>you and I are currently observing the stars, the dust,

736
00:36:14.360 --> 00:36:17.960
<v Speaker 2>the massive early galaxies we see through our telescopes is

737
00:36:18.039 --> 00:36:22.000
<v Speaker 2>actually just a highly detailed, perfect simulation running on someone

738
00:36:22.000 --> 00:36:22.960
<v Speaker 2>else's supercomputer.

739
00:36:23.159 --> 00:36:24.719
<v Speaker 3>The ultimate simulation there is

740
00:36:24.800 --> 00:36:27.800
<v Speaker 2>Exactly Keep looking up at the stars, everyone, and maybe

741
00:36:27.880 --> 00:36:29.800
<v Speaker 2>if you listen closely enough, you can hear the hum

742
00:36:29.800 --> 00:36:30.559
<v Speaker 2>of the processor
