WEBVTT

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

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

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

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

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

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<v Speaker 1>slumber under the night sky.

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<v Speaker 2>Imagine just for a second, standing at the absolute edge

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<v Speaker 2>of existence.

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<v Speaker 3>Well, that is a pretty terrifying place to start, right.

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<v Speaker 2>But just humor me. Here you are hovering just millimeters

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<v Speaker 2>away from a boundary that is so profound and you know,

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<v Speaker 2>so final that right before everything goes dark forever, the

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<v Speaker 2>universe itself actually.

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<v Speaker 3>Rings like a bell, a cosmic bell.

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<v Speaker 2>Yeah, exactly, because it's basically a fundamental law of physics

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<v Speaker 2>and well a massive pop culture cliche at this point

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<v Speaker 2>that in the vacuum of space, no one.

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<v Speaker 3>Can hear you scream because there's no air.

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<v Speaker 2>Right, there is no medium for acoustic sound to travel through.

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<v Speaker 2>Space is just this silent void. But there's this massive

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<v Speaker 2>paradox sitting right at the center of modern astrophysics right now.

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<v Speaker 2>Oh absolutely, we actually know that there is a way

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<v Speaker 2>to quote unquote here the violent cataclysmic crash of two

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<v Speaker 2>black holes colliding.

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<v Speaker 3>Which is such a profound contradiction when you really think

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<v Speaker 3>about it. I mean, we're talking about the darkest, most

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<v Speaker 3>invisible objects in the universe. Yeah, and they are creating

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<v Speaker 3>the most energetic outburst of noise imaginable, but not a

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<v Speaker 3>sound moving through the air of course, right right, It's

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<v Speaker 3>a sound moving through the very geometry of reality.

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<v Speaker 2>Okay, So let's unpack this because what we are embarking

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<v Speaker 2>on today is basically a journey to decode the loudest

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<v Speaker 2>gravitational wave ever recorded by human beings.

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<v Speaker 3>It really is a milestone.

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<v Speaker 2>It is. Our mission here is to transport you, the listener,

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<v Speaker 2>right to the edge of an event horizon during a

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<v Speaker 2>cosmic collision, and we're gonna explore what this totally unprecedented

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<v Speaker 2>signal tell us about, well, the most impenetrable boundary in

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<v Speaker 2>the entire cosmos.

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<v Speaker 3>And we really should establish right away that we aren't

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<v Speaker 3>just talking about a loud noise in some abstract or

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<v Speaker 3>you know, theoretical sense. Right when a signal of this

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<v Speaker 3>magnitude hits our detectors, we're essentially unlocking space time's deepest secrets.

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<v Speaker 3>We're peeling back the layers of physics that govern how

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<v Speaker 3>the universe operates at its absolute extreme limits.

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<v Speaker 2>The places where things get weird.

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<v Speaker 3>Exactly, the places where our standard equations actually start to

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<v Speaker 3>break down.

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<v Speaker 2>So to really grasp the gravity of this, and yes,

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<v Speaker 2>that pun is fully intended, nice, thank you, we have

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<v Speaker 2>to look at the signal that started it all. This

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<v Speaker 2>was basically a cosmic alarm bell ringing across the universe.

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<v Speaker 2>The event is centered around a signal designated as GW

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<v Speaker 2>two five zero one one.

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<v Speaker 3>Fifteen, recorded just last year, right in twenty twenty five.

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<v Speaker 2>YEP twenty twenty five by the two laser interferometer Gravitational

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<v Speaker 2>Wave Observatories or you know LEGO as most people know

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<v Speaker 2>it here in the United States. And the major our

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<v Speaker 2>headline here is that it is the loudest binary black

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<v Speaker 2>hole signal observed to.

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<v Speaker 3>Date, which is staggering.

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<v Speaker 2>It really is. I mean, we are talking roughly three

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<v Speaker 2>times louder than the very first gravitational wave ever detected

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<v Speaker 2>just a decade ago.

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<v Speaker 3>In the concept of loudness and gravitational wave astronomy, it

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<v Speaker 3>kind of requires us to completely discard our biological experience

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<v Speaker 3>of hearing. Yeah, there are no sound waves right right.

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<v Speaker 3>When astrophysicists say loud, they're actually referring to amplitude. Amplitude, okay, Yeah,

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<v Speaker 3>gravitational waves are physical ripples in the actual fabric of

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<v Speaker 3>space time. And you always hear people compare spacetime to

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<v Speaker 3>a flat trampoline, which.

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<v Speaker 2>Oh, the bowling ball on the trampoline analogy, Yes.

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<v Speaker 3>And it is a terrible over used analogy that completely

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<v Speaker 3>fails to capture the three dimensional nature of the universe.

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<v Speaker 2>So what's a better way to picture it?

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<v Speaker 3>Think of space time instead as a massive solid block

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<v Speaker 3>of dense, clear gelatine.

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<v Speaker 2>Okay, a giant block of cosmic jello. I can work

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<v Speaker 2>with that, A.

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<v Speaker 3>Giant block of cosmic jell exactly. So if you take

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<v Speaker 3>two dense, heavy marbles and embed them deep inside that gelatin, right,

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<v Speaker 3>and then you start spinning them around each other at

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<v Speaker 3>a significant fraction of the speed of light, they are

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<v Speaker 3>going to violently churn that material.

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<v Speaker 2>Oh, I see.

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<v Speaker 3>And when they finally smash together, that massive collision sends

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<v Speaker 3>these severe pressure waves rippling outward through the gelatine in

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<v Speaker 3>all three dimensions at once.

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<v Speaker 2>Okay, So when those ripples finally reach Earth after traveling

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<v Speaker 2>outward for you know, maybe billions of years, they are

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<v Speaker 2>actually physically stretching and squeezing the space that we occupy.

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<v Speaker 3>That's exactly what's happening.

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<v Speaker 2>So, like, think about where you are sitting right now

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<v Speaker 2>listening to this, as this specific wave passed through Earth,

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<v Speaker 2>the room you're in, the chair you're sitting on, and

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<v Speaker 2>literally your own body were physically stretched and squeezed, like

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<v Speaker 2>oscillating back and forth.

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<v Speaker 3>You were. But we do need to emphasize that this

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<v Speaker 3>is on a microscopic.

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<v Speaker 2>Scale, right, Nobody actually felt it.

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<v Speaker 3>No, No, we are talking about distortions that alter the

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<v Speaker 3>distance between here in the nearest star by roughly the

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<v Speaker 3>width of a human hair.

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<v Speaker 2>That is, I mean, that's almost impossible to even conceptualize.

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<v Speaker 3>Or to bring it locally. It's like changing the length

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<v Speaker 3>of logos four kilometer long vacuum tubes by just a

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<v Speaker 3>fraction of the width of a single proton.

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<v Speaker 2>Which honestly makes the engineering behind LIGO sound completely impossible.

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<v Speaker 2>I mean, we aren't just talking about building a really

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<v Speaker 2>big telescope here, not at all. These facilities they're in

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<v Speaker 2>Washington State and Louisiana.

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<v Speaker 3>Right, Yes, those are the two.

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<v Speaker 2>They are shooting lasers down these four kilometer long vacuum tubes,

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<v Speaker 2>bouncing them off perfectly suspended mirrors and basically measuring how

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<v Speaker 2>long it takes for the light to return.

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<v Speaker 3>And the precision required to pull that off is just

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<v Speaker 3>difficult to overstate. I mean, to measure a distortion smaller

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<v Speaker 3>than a proton. You have to isolate those mirrors from

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<v Speaker 3>the seismic noise of the Earth itself.

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<v Speaker 2>Right, because everything vibrates.

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<v Speaker 3>Everything a truck driving down a highway miles away, or

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<v Speaker 3>a wave crashing on some distant shoreline, even the microscope

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<v Speaker 3>thermal vibrations of the actual atoms inside the mirrors themselves.

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<v Speaker 2>Wait, really, the heat of the atoms in the mirror

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<v Speaker 2>can mess up the reading.

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<v Speaker 3>Well absolutely all that creates background noise. Yeah, so Lego

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<v Speaker 3>has to mathematically and physically cancel out the ambient vibration

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<v Speaker 3>of the entire planet just to hear the universe whisper.

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<v Speaker 2>That is just wild. And you know, that rapid progression

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<v Speaker 2>of our technological ability over just the last ten years

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<v Speaker 2>is mind blowing to me.

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<v Speaker 3>It's been incredibly fast.

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<v Speaker 2>Like a decade ago, just confirming that these ripples existed

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<v Speaker 2>at all. Was this monumental Nobel Prize winning priumph. And

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<v Speaker 2>now just ten years later, we capture a signal three

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<v Speaker 2>times as powerful, and we're using it as this incredibly

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<v Speaker 2>precise surgical instrument to probe the black holes themselves well.

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<v Speaker 3>And the amplitude is what allows for that surgical precision

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<v Speaker 3>because it's louder, Right, A louder signal means that the

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<v Speaker 3>stretching and squeezing of space time was significantly more pronounced.

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<v Speaker 3>It implies immense energy, and crucially, it implies proximity.

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<v Speaker 2>Proximity, so GW two five zero one one teen was

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<v Speaker 2>close to.

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<v Speaker 3>Us relatively speaking on a cosmic scale. Yes, it happened

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<v Speaker 3>relatively close to us.

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<v Speaker 2>Okay, let me throw out an analogy here to see

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<v Speaker 2>if I'm visualizing the impact of this amplitude correctly. Sure

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<v Speaker 2>it so if the first gravitational wave we detected a

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<v Speaker 2>decade ago was kind of like feeling the faint rhythmic

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<v Speaker 2>rumble of a distant train through the soles of your

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<v Speaker 2>shoes while you're standing, I don't know, five miles away, Okay,

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<v Speaker 2>is GW two five zero one to one tour more

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<v Speaker 2>like standing right next to the tracks as a massive

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<v Speaker 2>freight train blasts its horn and just rattles your ribcage.

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<v Speaker 3>I like that. But let's actually take that train and

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<v Speaker 3>analogy a step further. Okay, when you're five miles away,

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<v Speaker 3>you really only feel the lowest, deepest base frequencies of

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<v Speaker 3>that rumble.

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<v Speaker 2>Right, Yeah, just the heavy vibrations exactly.

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<v Speaker 3>The higher, more delicate frequencies, yeah, like the middle wheels

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<v Speaker 3>clacking on the rails. Those are completely lost to the

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<v Speaker 3>intervening distance and the soil.

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<v Speaker 2>That makes sense.

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<v Speaker 3>But by standing right next to the tracks, you don't

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<v Speaker 3>just feel as stronger rumble. Your ear can suddenly pick

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<v Speaker 3>up the complex, subtle harmonics of the machinery itself.

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<v Speaker 2>Oh. I see. So the volume doesn't just make the

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<v Speaker 2>main event easier to notice. The high volume actually allows

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<v Speaker 2>us to hear entirely different layers of the collision.

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<v Speaker 3>It unveils the harmonics. It's like in music, you know,

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<v Speaker 3>a piano key doesn't just produce one pure mathematical tone

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<v Speaker 3>when you strike it. It produces a fundamental frequency, but

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<v Speaker 3>alongside dozens of overtones. These are higher, quieter frequencies resonating

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<v Speaker 3>simultaneously and.

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<v Speaker 2>That's what makes it sound like a piano and not

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<v Speaker 2>a computer beep.

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<v Speaker 3>Precisely, those overtones give the instrument its character. So in

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<v Speaker 3>gravitational waves, the main roar is the bulk of the collision.

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<v Speaker 2>The huge smash, But a profoundly.

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<v Speaker 3>Loud signal like GW two five zero one fourteen has

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<v Speaker 3>such an incredibly high signal to noise ratio that the

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<v Speaker 3>faint overtones of the collision finally rise above the background

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<v Speaker 3>static of the universe.

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<v Speaker 2>Wow, which brings just a completely new layer of data

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<v Speaker 2>to the table. We aren't just hearing this anymore. We're

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<v Speaker 2>actually hearing the subtle vibrations of the new black hole

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<v Speaker 2>settling down, Yes, the ring down, and that shifts our

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<v Speaker 2>focus directly to the true protagonist of this whole cosmic drama,

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<v Speaker 2>which is the event horizon, the point of no return exactly,

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<v Speaker 2>this is the universe's ultimate point of no return. We

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<v Speaker 2>know the basics, right, It's the boundary around a black

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<v Speaker 2>hole where absolutely nothing, not even light, can escape. But

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<v Speaker 2>for anyone familiar with the basic physics of gravity, the

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<v Speaker 2>mechanics of this boundary get incredibly.

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<v Speaker 3>Strange, oh very strange. And the strangeness really comes from

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<v Speaker 3>the absolute finality of the universal.

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<v Speaker 2>Speed limit the speed of light.

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<v Speaker 3>Right, we know that as mass increases, the escape velocity,

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<v Speaker 3>which is the speed required to break free of an

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<v Speaker 3>object's gravitational pull, that increases too.

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<v Speaker 2>Like how it's harder to launch a rocket from Jupiter

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<v Speaker 2>than from.

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<v Speaker 3>Earth exactly, and at a certain point of mass density,

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<v Speaker 3>that required escape velocity hits exactly two hundred and ninety

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<v Speaker 3>nine thousand, seven hundred and ninety two kilometers per.

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<v Speaker 2>Second, which is the speed of light in a vacuum. Yes,

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<v Speaker 2>and since Einstein equations dictate that nothing can travel faster

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<v Speaker 2>than the speed of light, anything that crosses that mathematical

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<v Speaker 2>boundary is just permanently trapped.

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<v Speaker 3>It is a one way door in the universe information, matter, light,

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<v Speaker 3>It goes in and it never comes out.

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<v Speaker 2>Which presents a pretty profound paradox for observational astronomy, doesn't

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<v Speaker 2>it a huge one? Because how do you observe an

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<v Speaker 2>object that, by its very definition completely forbids observation. If

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<v Speaker 2>no light, no radiation, and literally no information can cross

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<v Speaker 2>from the inside of the event horizon to the outside universe,

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<v Speaker 2>you're essentially trying to study a shadow by like turning

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<v Speaker 2>off all the lights.

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<v Speaker 3>Yeah, that paradox is really what trips up a lot

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<v Speaker 3>of people when they first look at the data from

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<v Speaker 3>GW two five zero one one day.

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<v Speaker 2>I know, it tripped me up. I was like, if

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<v Speaker 2>it's the ultimate trap, how did scientists witness it? We

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<v Speaker 2>literally can't see the black hole itself.

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<v Speaker 3>Well, the key is that we aren't seeing what comes

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<v Speaker 3>out of it, because nothing does. Instead, we are witnessing

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<v Speaker 3>the severe agonizing warping of the space time directly adjacent

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<v Speaker 3>to the horizon and in the exact millisecond it is forming.

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<v Speaker 2>Oh so it's the space around it.

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<v Speaker 3>Yes. When two black holes merge, their individual event horizons deform,

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<v Speaker 3>they stretch toward each other, and they finally fuse to

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<v Speaker 3>form a single, larger and highly chaotic event horizon.

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<v Speaker 2>Highly chaotic. So for a fraction of a second, this

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<v Speaker 2>newly born remnant black hole is not a perfect sphere.

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<v Speaker 3>Far from it. It is violently asymmetrical. Really, Oh yeah,

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<v Speaker 3>it is wobbling, ringing, and shedding immense amounts of energy

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<v Speaker 3>in the form of gravitational waves as it desperately attempts

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<v Speaker 3>to settle down into a stable spherical state. Wow, it's

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<v Speaker 3>that dynamic turbulent boundary the space time actively reacting to

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<v Speaker 3>the violent birth of the horizon that we are observing.

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<v Speaker 3>We are essentially catching the shadow just before the door

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<v Speaker 3>slam shut forever.

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<v Speaker 2>That is such a cool way to freeze it. Catching

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<v Speaker 2>the shadow before the door slam shut, and the method

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<v Speaker 2>scientists used to actually capture that fleeting moment before the

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<v Speaker 2>eternal dark is just a brilliant piece of analytical detective work.

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<v Speaker 3>It really is.

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<v Speaker 2>And this research was led by doctor Lingsn and PhD

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<v Speaker 2>candidate Neil Lou. They're over at OSGREV and the Australian

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<v Speaker 2>National University, right.

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<v Speaker 3>Yes, working with an international coalition spanning Canada, at the

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<v Speaker 3>US and Spain.

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<v Speaker 2>Just a massive global effort, and they managed to basically

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<v Speaker 2>isolate the last sound these black holes made.

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<v Speaker 3>And the secret to measuring this last sound lies in

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<v Speaker 3>a very specific, notoriously elusive component of this signal called

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<v Speaker 3>direct waves direct waves. Okay, yeah. Prior to this analysis,

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<v Speaker 3>direct waves were theoretically understood but frankly impossible to extract

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<v Speaker 3>from the noise. They were just buried exactly. But Neil

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<v Speaker 3>Lu's new analytical framework essentially deciphered them. It pulled completely

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<v Speaker 3>unique data from incredibly close to the event horizon.

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<v Speaker 2>Okay, so let's dig into the how of that extraction.

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<v Speaker 2>Because they couldn't just use like a standard audio filter

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<v Speaker 2>to clean up the track. I was looking into the

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<v Speaker 2>computational mechanics behind this, and the process of mathematical dissection

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<v Speaker 2>is just staggering.

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<v Speaker 3>It's intense.

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<v Speaker 2>They had to rely heavily on something called numerical relativity, right.

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<v Speaker 3>They did, And numerical relativity is basically the unsung hero

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<v Speaker 3>of gravitational wave astronomy. Oh so well, Einstein's equations of

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<v Speaker 3>general relativity. They are nonlinear partial differential.

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<v Speaker 2>Equations, which means they're a nightmare to solve.

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<v Speaker 3>They are famously brutally difficult to solve for decades, physicists

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<v Speaker 3>could really only solve them for highly simplified, idealized scenarios.

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<v Speaker 3>You cannot just write down the exact solution for two

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<v Speaker 3>black holes merging.

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<v Speaker 2>On a chop breaks mean a supercomputer.

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<v Speaker 3>You need massive clusters of supercomputers running for months just

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<v Speaker 3>to simulate a fraction of a second of a black

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<v Speaker 3>hole merger.

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<v Speaker 2>Months for a fraction of a second.

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<v Speaker 3>Yes, the research team had to model millions of potential

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<v Speaker 3>merger scenarios. They simulate the exact masses, the spins, and

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<v Speaker 3>the orbital trajectories of the two black holes, and then

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<v Speaker 3>the computer's crunch Einstein's equations to predict exactly what the

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<v Speaker 3>main gravitational wave that dominant roar should look like.

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<v Speaker 2>Okay, so if the main crash, the bulk collision is

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<v Speaker 2>a deafening orchestral symbol smash happening right in front of you,

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<v Speaker 2>these direct waves are like a tiny specific vibration of

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<v Speaker 2>one single violin string happening at the exact same millisecond.

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<v Speaker 3>That's a great way to picture it.

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<v Speaker 2>So to find the violin string, they use the supercomputer

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<v Speaker 2>to map out the exact acoustic profile of the symbol smash, right,

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<v Speaker 2>and then they mathematically subtract it from the raw lego data.

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<v Speaker 3>That's exactly what they do, but that subtraction requires an

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<v Speaker 3>unprecedented level of precision. I can imagine if your numerical

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<v Speaker 3>relativity model is off by even a fraction of a percent,

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<v Speaker 3>the leftover data will just be statistical garbage.

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<v Speaker 2>Oh, because you didn't subtract the right thing.

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<v Speaker 3>Right. But by meticulously modeling and subtracting the dominant signal,

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<v Speaker 3>which is the inspiral and the immediate merger. What they

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<v Speaker 3>were left with was a tiny residual vibration, the ring.

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<v Speaker 2>Down phase, the violin string.

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<v Speaker 3>The direct waves, and the origin of those direct waves

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<v Speaker 3>is really what makes them so and valuable to us.

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<v Speaker 2>Why is that? Where do they come from?

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<v Speaker 3>They don't come from the distant orbiting phase of the

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<v Speaker 3>black holes. They are emitted right at the throat of

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<v Speaker 3>the beasts. Wow. They carry the untainted fingerprint of the

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<v Speaker 3>extreme gravity immediately adjacent to the newly formed event horizon.

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<v Speaker 2>It's kind of like standing at a massive party with

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<v Speaker 2>one hundred conversations happening, heavy music playing, glasses clinking, and

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<v Speaker 2>you're trying to hear a specific whisper from across the

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<v Speaker 2>room exactly except here, the team is filtering out the

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<v Speaker 2>noise of the universe itself to hear a single whisper

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<v Speaker 2>from billions of light years away.

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<v Speaker 3>And the effort to isolate that single voice is driven

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<v Speaker 3>by the totally unique physical environment it originates.

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<v Speaker 2>From the event horizon itself.

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<v Speaker 3>Yes, black holes are the ultimate extreme laboratories. They sit

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<v Speaker 3>precisely at the intersection of our two most successful, yet

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<v Speaker 3>fundamentally incompatible frameworks of physics.

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<v Speaker 2>Oh right, general relativity and quantum theory exactly. This is

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<v Speaker 2>where the physics gets incredibly tense because we have these

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<v Speaker 2>two rule books. Right. General relativity is the master theory

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<v Speaker 2>of the massive. It explains gravity orbits and the smooth,

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<v Speaker 2>continuous fabric of space and time.

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<v Speaker 3>Correct.

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<v Speaker 2>But then we have quantum mechanics, which is the master

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<v Speaker 2>theory of the microscopic. It explains atoms, subatomic particles, and

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<v Speaker 2>it treats the universe as chunky like it's made of

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<v Speaker 2>discrete packets.

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<v Speaker 3>Of energy and under normal circumstances in the universe, those

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<v Speaker 3>two rule books never have to speak to each.

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<v Speaker 2>Other, right, because things are either huge or tiny.

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<v Speaker 3>Exactly. You use relativity for stars and you use quantum

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<v Speaker 3>mechanics for electrons. But at the event horizon of a

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<v Speaker 3>black hole, the mass is so immense and the space

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<v Speaker 3>it occupies is so compact that the gravity violently warps

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<v Speaker 3>space time on a microscopic quantum level.

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<v Speaker 2>It forces them together.

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<v Speaker 3>It is the singular place in the cosmos where the

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<v Speaker 3>rules of the massive crash headlong into the rules of

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<v Speaker 3>the microscopic.

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<v Speaker 2>So, okay, if these two frameworks fundamentally disagree on how

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<v Speaker 2>the universe works. What does it actually mean for doctor

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<v Speaker 2>Son and you'll lou to use these direct waves to

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<v Speaker 2>test general relativity.

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<v Speaker 3>Well, it's a huge deal.

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<v Speaker 2>Are we essentially using this super loud gravitational wave to

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<v Speaker 2>see if Einstein's equations finally break down? Like, are we

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<v Speaker 2>trying to prove him wrong?

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<v Speaker 3>We'll consider the implications of a breakdown. I mean, every

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<v Speaker 3>single time physicists have tested general relativity over the last century,

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<v Speaker 3>from the bending of starlight around the Sun to the

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<v Speaker 3>time dilation in GPS satellite, it's always right. Einstein has

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<v Speaker 3>been proven flawlessly correct every time. But theorists know the

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<v Speaker 3>theory is incomplete.

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<v Speaker 2>Because it produces infinities right right at the very center

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<v Speaker 2>of a black hole.

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<v Speaker 3>The singularity relativity predicts infinite density and infinite.

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<v Speaker 2>Curvature, which doesn't make sense no.

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<v Speaker 3>Because nature abhors in infinity and an infinity usually just

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<v Speaker 3>means your math stopped working. Yeah, So theorists suspect that

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<v Speaker 3>right at the boundary, right at the event horizon, general

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<v Speaker 3>relativity might begin to fray, revealing subtle quantum effects.

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<v Speaker 1>Oh.

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<v Speaker 3>By isolating these direct waves, these little whispers from the

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<v Speaker 3>absolute edge, the team is gathering the raw data needed

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<v Speaker 3>to run the ultimate stress test. They are checking if

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<v Speaker 3>Einstein's rulebook actually holds up under the most extreme pressure

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<v Speaker 3>the universe can generate.

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<v Speaker 2>Man that is fascinating. So to run those stress tests,

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<v Speaker 2>the team had to pull incredibly specific measurements from that

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<v Speaker 2>leftover whisper very specific. They had to essentially take the

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<v Speaker 2>vitals of the newly born black hole, and the analysis

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00:18:28.519 --> 00:18:31.559
<v Speaker 2>of GW two five zero one one four allowed them

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<v Speaker 2>to measure two fundamental properties of the remnant, its rotation

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00:18:36.000 --> 00:18:37.839
<v Speaker 2>frequency and its surface gravity.

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<v Speaker 3>And those two properties basically define the entire existence of

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<v Speaker 3>the remnant.

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00:18:41.839 --> 00:18:44.200
<v Speaker 2>And the remnant. Just to be clear, is the single

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<v Speaker 2>black hole left behind after the chaotic fusion.

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<v Speaker 3>Yes, And in that fusion process, a substantial percentage of

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<v Speaker 3>the two parent black holes combined mass is converted instantaneously

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00:18:54.480 --> 00:18:55.319
<v Speaker 3>into pure energy.

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00:18:55.440 --> 00:18:59.079
<v Speaker 2>Oh, and that energy is the gravitational waves ligo detected.

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00:18:58.799 --> 00:19:02.039
<v Speaker 3>Exactly e equals ms squared. In its most violent form.

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00:19:01.960 --> 00:19:04.680
<v Speaker 2>The mass just turns into a ripple in space, right.

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00:19:04.920 --> 00:19:07.720
<v Speaker 3>And what remains after that burst is a new entity.

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00:19:08.079 --> 00:19:11.319
<v Speaker 3>And when we measure its rotation frequency, we are measuring.

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00:19:10.960 --> 00:19:12.400
<v Speaker 2>Its spin, because they spin.

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00:19:12.640 --> 00:19:16.119
<v Speaker 3>Black holes are rarely static stationary objects. I mean, almost

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00:19:16.160 --> 00:19:21.000
<v Speaker 3>everything in the universe possesses angular momentum. Stars spin, galaxy spin.

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00:19:21.279 --> 00:19:24.640
<v Speaker 3>When two massive black holes orbit each other e merge,

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00:19:25.680 --> 00:19:29.240
<v Speaker 3>all that tremendous orbital energy has to go somewhere. The

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00:19:29.359 --> 00:19:33.519
<v Speaker 3>law of conservation of angular momentum dictates that the rotational

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00:19:33.640 --> 00:19:35.319
<v Speaker 3>energy is inherited by.

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00:19:35.240 --> 00:19:38.640
<v Speaker 2>The remnant, meaning the resulting black hole can be spinning

400
00:19:38.640 --> 00:19:41.279
<v Speaker 2>at like a significant fraction of the speed of light.

401
00:19:41.359 --> 00:19:44.640
<v Speaker 3>Oh, absolutely speeds we can barely comprehend. And the second

402
00:19:44.720 --> 00:19:47.759
<v Speaker 3>vital sign they measured the surface gravity. That requires a

403
00:19:47.759 --> 00:19:51.119
<v Speaker 3>bit of a conceptual adjustment. Why is that Because, as

404
00:19:51.160 --> 00:19:54.160
<v Speaker 3>we established earlier, a black hole doesn't have a physical

405
00:19:54.240 --> 00:19:55.519
<v Speaker 3>solid surface, right.

406
00:19:55.599 --> 00:19:57.400
<v Speaker 2>You can't land a rover on it. It's just a

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00:19:57.480 --> 00:19:58.559
<v Speaker 2>boundary exactly.

408
00:19:59.359 --> 00:20:02.920
<v Speaker 3>The term gravity is really barred from planetary physics for

409
00:20:02.960 --> 00:20:05.839
<v Speaker 3>a black hole. Surface gravity refers to the strength of

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00:20:05.880 --> 00:20:09.480
<v Speaker 3>the gravitational pull precisely at the mathematical boundary of the

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00:20:09.519 --> 00:20:12.160
<v Speaker 3>event horizon, just right at the edge. Right. It is

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00:20:12.200 --> 00:20:15.920
<v Speaker 3>a measure of how sharply, how steeply space time is

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<v Speaker 3>curved exactly at the point of no return.

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00:20:18.440 --> 00:20:21.079
<v Speaker 2>You know, the mathematical reality here is actually stranger than

415
00:20:21.119 --> 00:20:23.759
<v Speaker 2>fiction it usually is. I mean, think about it. We

416
00:20:23.799 --> 00:20:27.359
<v Speaker 2>are taking the vitals, the spin, and the gravity of

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00:20:27.400 --> 00:20:32.039
<v Speaker 2>a completely invisible light trapping void sitting billions of light

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00:20:32.119 --> 00:20:36.559
<v Speaker 2>years away, purely by mathematically dissecting the invisible ripples it

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00:20:36.640 --> 00:20:38.000
<v Speaker 2>cast off during its birth.

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00:20:38.319 --> 00:20:41.200
<v Speaker 3>It is poetry, and those two properties give us a

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00:20:41.240 --> 00:20:44.640
<v Speaker 3>complete picture because a concept known as the no hair theorem.

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00:20:44.720 --> 00:20:48.720
<v Speaker 3>The no hair theorem, yes, it postulates that from the outside,

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00:20:48.759 --> 00:20:52.599
<v Speaker 3>an astrophysical black hole is incredibly simple. It has no

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00:20:52.720 --> 00:20:55.000
<v Speaker 3>complex identifying features. No hair.

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00:20:55.160 --> 00:20:56.000
<v Speaker 2>Oh, I get it.

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00:20:56.079 --> 00:20:58.480
<v Speaker 3>If you know it's mass and its spin, you know

427
00:20:58.680 --> 00:21:01.599
<v Speaker 3>absolutely everything there is to know about its macroscopic state.

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00:21:01.759 --> 00:21:02.920
<v Speaker 3>It is fully identified.

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00:21:03.000 --> 00:21:06.000
<v Speaker 2>Okay, let's do it. So the basic definition is that

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00:21:06.079 --> 00:21:10.240
<v Speaker 2>a spinning black hole literally drags the fabric of space

431
00:21:10.359 --> 00:21:14.640
<v Speaker 2>time nearby along with it, creating an environment where absolutely

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<v Speaker 2>nothing can remain stationary relative to a distant observer. That's

433
00:21:17.960 --> 00:21:20.279
<v Speaker 2>a definition, yeah, But to actually visualize that, I think

434
00:21:20.319 --> 00:21:22.200
<v Speaker 2>we have to go back to our Gelatin analogy.

435
00:21:22.319 --> 00:21:27.319
<v Speaker 3>Definitely. We intuitively think of space as a static, rigid

436
00:21:27.400 --> 00:21:31.039
<v Speaker 3>stage where events happen like a three dimensional grid, right.

437
00:21:30.960 --> 00:21:32.319
<v Speaker 2>Yeah, an empty room.

438
00:21:32.680 --> 00:21:35.400
<v Speaker 3>But Einstein taught us that space time is a dynamic,

439
00:21:35.519 --> 00:21:39.480
<v Speaker 3>tangible medium. So if you place a perfectly smooth, massive

440
00:21:39.599 --> 00:21:42.960
<v Speaker 3>stationary ball in our block of clear gelatin, it just

441
00:21:42.960 --> 00:21:46.240
<v Speaker 3>sits there. It displaces the material around it, but that's it.

442
00:21:46.599 --> 00:21:47.680
<v Speaker 3>That is standard gravity.

443
00:21:47.720 --> 00:21:50.119
<v Speaker 2>But if you start spinning that ball, the friction of

444
00:21:50.119 --> 00:21:53.240
<v Speaker 2>the ball surface grips the gelatin, it doesn't just sit

445
00:21:53.279 --> 00:21:53.920
<v Speaker 2>still anymore.

446
00:21:54.000 --> 00:21:56.519
<v Speaker 3>The gelatin begins to swirl in a vortex around the

447
00:21:56.559 --> 00:21:57.799
<v Speaker 3>spinning object.

448
00:21:57.480 --> 00:21:59.119
<v Speaker 2>Like twisting a spoon and a bowl of honey.

449
00:21:59.279 --> 00:22:02.599
<v Speaker 3>Yes, the material closest to the ball is dragged the fastest,

450
00:22:02.799 --> 00:22:05.039
<v Speaker 3>and the effect tapers off the further way you get.

451
00:22:05.240 --> 00:22:07.519
<v Speaker 2>But wait again. A black hole doesn't have a physical

452
00:22:07.559 --> 00:22:08.960
<v Speaker 2>surface to create friction.

453
00:22:08.920 --> 00:22:12.359
<v Speaker 3>And the beauty of general relativity is that it doesn't

454
00:22:12.400 --> 00:22:12.839
<v Speaker 3>need one.

455
00:22:13.000 --> 00:22:13.519
<v Speaker 2>It doesn't.

456
00:22:13.720 --> 00:22:17.599
<v Speaker 3>No, the mass itself, just by twisting through the geometry

457
00:22:17.599 --> 00:22:21.599
<v Speaker 3>of the universe, drags the coordinate system of space.

458
00:22:21.279 --> 00:22:23.599
<v Speaker 2>Along with it the coordinate system itself.

459
00:22:23.680 --> 00:22:27.440
<v Speaker 3>Yes, the swirling vortex of space time around a spinning

460
00:22:27.519 --> 00:22:32.559
<v Speaker 3>mass is the lens thirring effect or frame dragging. The

461
00:22:32.680 --> 00:22:36.359
<v Speaker 3>mathematical reference frame of space itself is literally being pulled

462
00:22:36.400 --> 00:22:37.359
<v Speaker 3>into a whirlpool.

463
00:22:37.400 --> 00:22:39.799
<v Speaker 2>Okay, let me push this to its logical extreme. To

464
00:22:39.839 --> 00:22:42.400
<v Speaker 2>make sure I am truly grasping the physics here. Because

465
00:22:42.480 --> 00:22:45.279
<v Speaker 2>this is wild, go for it. Say I have an

466
00:22:45.319 --> 00:22:50.079
<v Speaker 2>indestructible spaceship. I have infinite fuel and infinite thruster power.

467
00:22:50.279 --> 00:22:52.279
<v Speaker 3>Okay, a magical spaceship.

468
00:22:51.880 --> 00:22:54.000
<v Speaker 2>Right, And I fly right up to this newly born,

469
00:22:54.160 --> 00:22:56.759
<v Speaker 2>rapidly spinning black hole. And I cross into the region

470
00:22:57.200 --> 00:22:59.319
<v Speaker 2>just outside the event horizon, which is an area called

471
00:22:59.319 --> 00:23:00.000
<v Speaker 2>the ergosphere.

472
00:23:00.400 --> 00:23:01.279
<v Speaker 3>Yes, the aerosphere.

473
00:23:01.440 --> 00:23:05.039
<v Speaker 2>So I get there, and I fire my thrusters perfectly

474
00:23:05.079 --> 00:23:08.079
<v Speaker 2>to hover in one exact mathematical coordinate. I am trying

475
00:23:08.079 --> 00:23:10.480
<v Speaker 2>to stand completely still. Okay, do I stay still.

476
00:23:10.599 --> 00:23:13.240
<v Speaker 3>If you do that, you are fighting a losing battle

477
00:23:13.279 --> 00:23:14.799
<v Speaker 3>against the geometry of the universe.

478
00:23:15.200 --> 00:23:17.240
<v Speaker 2>Really, even with infinite power.

479
00:23:17.079 --> 00:23:20.720
<v Speaker 3>Even with infinite power inside the ergosphere, the frame dragging

480
00:23:20.799 --> 00:23:24.880
<v Speaker 3>effect is so severe that space time itself is being

481
00:23:24.960 --> 00:23:27.880
<v Speaker 3>dragged around the black hole faster than the speed of light.

482
00:23:27.960 --> 00:23:30.920
<v Speaker 2>Wait wait, wait, nothing can move faster than light. That

483
00:23:31.039 --> 00:23:33.759
<v Speaker 2>is the fundamental rule we just established for the event horizon.

484
00:23:33.880 --> 00:23:38.119
<v Speaker 3>Ah, nothing can move through space faster than light, but

485
00:23:38.279 --> 00:23:41.240
<v Speaker 3>space itself has no speed limit. Really, think about the

486
00:23:41.279 --> 00:23:46.319
<v Speaker 3>expansion of the universe, the universe itself expands faster than light. Right, Okay,

487
00:23:46.480 --> 00:23:49.880
<v Speaker 3>so in the ergosphere, the local space is swirling so

488
00:23:50.079 --> 00:23:55.279
<v Speaker 3>violently that to remain stationary relative to me, Like if

489
00:23:55.279 --> 00:23:58.279
<v Speaker 3>I'm an observer back on Earth watching your spaceship through

490
00:23:58.279 --> 00:24:01.480
<v Speaker 3>a telescope, Yeah, to stay still relative to me, you

491
00:24:01.480 --> 00:24:03.839
<v Speaker 3>would have to travel through your local space faster than

492
00:24:03.880 --> 00:24:05.759
<v Speaker 3>the light just to hold your ground.

493
00:24:05.519 --> 00:24:07.759
<v Speaker 2>Which is physically impossible.

494
00:24:07.160 --> 00:24:10.799
<v Speaker 3>Exactly impossible. Therefore, even with your infinite fuel and your

495
00:24:10.839 --> 00:24:14.240
<v Speaker 3>infinite thruster power, you are inevitably swept along in the

496
00:24:14.240 --> 00:24:18.400
<v Speaker 3>cosmic whirlpool. To you, inside the cockpit of the spaceship,

497
00:24:18.839 --> 00:24:21.079
<v Speaker 3>you might feel like you are pushing as hard as

498
00:24:21.079 --> 00:24:24.240
<v Speaker 3>you can in one direction, you are burning fuel at

499
00:24:24.400 --> 00:24:28.440
<v Speaker 3>maximum capacity. But to me looking at you from Earth,

500
00:24:28.880 --> 00:24:34.079
<v Speaker 3>your spaceship is being irresistibly swept sideways in a cosmic hurricane.

501
00:24:34.160 --> 00:24:36.200
<v Speaker 2>So you literally cannot stand still.

502
00:24:36.319 --> 00:24:39.039
<v Speaker 3>You cannot stand still because the stillness of space no

503
00:24:39.119 --> 00:24:40.079
<v Speaker 3>longer exists. There.

504
00:24:40.160 --> 00:24:43.160
<v Speaker 2>Think about the absolute wildness of that concept. The very

505
00:24:43.200 --> 00:24:46.160
<v Speaker 2>fabric of where you are is moving. It sounds like pure,

506
00:24:46.480 --> 00:24:47.920
<v Speaker 2>unfiltered science fiction.

507
00:24:47.880 --> 00:24:48.519
<v Speaker 3>It really does.

508
00:24:48.640 --> 00:24:52.400
<v Speaker 2>But this is a measurable, mathematically proven reality happening in

509
00:24:52.400 --> 00:24:55.000
<v Speaker 2>our universe right now. And the true triumph of the

510
00:24:55.000 --> 00:24:57.799
<v Speaker 2>research led by doctor Son and Neil Lou is that

511
00:24:57.839 --> 00:25:00.519
<v Speaker 2>their analytical technique actually allows us to e isolate the

512
00:25:00.519 --> 00:25:04.720
<v Speaker 2>specific signatures of this frame dragging from those tiny direct waves.

513
00:25:04.920 --> 00:25:08.480
<v Speaker 3>Yes, we are transitioning from merely cataloging the existence of

514
00:25:08.519 --> 00:25:11.759
<v Speaker 3>black holes to actually charting the fluid dynamics of an

515
00:25:11.799 --> 00:25:15.559
<v Speaker 3>invisible universe. We are mapping the whirlpools of space time

516
00:25:15.839 --> 00:25:17.400
<v Speaker 3>with excruciating precision.

517
00:25:17.480 --> 00:25:20.319
<v Speaker 2>It is truly staggering. So let's trace the arc of

518
00:25:20.400 --> 00:25:21.400
<v Speaker 2>what we've explored today.

519
00:25:21.440 --> 00:25:22.200
<v Speaker 3>It's been journey.

520
00:25:22.440 --> 00:25:25.720
<v Speaker 2>We started with the sheer violence of GW two five

521
00:25:25.880 --> 00:25:29.839
<v Speaker 2>zero one fourteen, a cosmic crash so massive it sent

522
00:25:29.880 --> 00:25:33.160
<v Speaker 2>the loudest ripples ever recorded through the gelatin of space time.

523
00:25:33.519 --> 00:25:36.000
<v Speaker 2>And we looked at how an international team of scientists

524
00:25:36.200 --> 00:25:41.799
<v Speaker 2>used supercomputers and numerical relativity to mathematically subtract the deafening

525
00:25:41.880 --> 00:25:43.400
<v Speaker 2>noise of that crash.

526
00:25:43.119 --> 00:25:46.039
<v Speaker 3>Which revealed the tiny, hidden direct waves.

527
00:25:45.920 --> 00:25:49.599
<v Speaker 2>Right and those faint, lingering vibrations allowed us to bypass

528
00:25:49.640 --> 00:25:52.880
<v Speaker 2>the paradox of the event horizon. We use those whispers

529
00:25:52.920 --> 00:25:55.839
<v Speaker 2>to measure the spin and surface gravity of a newborn.

530
00:25:55.519 --> 00:25:58.319
<v Speaker 3>Remnant, taking the vitals of an invisible ghost.

531
00:25:58.119 --> 00:26:01.279
<v Speaker 2>Exactly, and in doing so we uncover the reality of

532
00:26:01.319 --> 00:26:04.480
<v Speaker 2>frame dragging, where the sheer rotational force of a black

533
00:26:04.480 --> 00:26:07.880
<v Speaker 2>hole twists spacetime itself into a cosmic treadmill where nothing

534
00:26:07.920 --> 00:26:08.920
<v Speaker 2>can ever stand still.

535
00:26:09.039 --> 00:26:09.720
<v Speaker 3>It's beautiful.

536
00:26:09.799 --> 00:26:12.599
<v Speaker 2>It really highlights the absolute beauty of human ingenuity. I mean,

537
00:26:12.640 --> 00:26:14.720
<v Speaker 2>we are sitting here on a pale blue dot, orbiting

538
00:26:14.759 --> 00:26:18.400
<v Speaker 2>a totally average star, yet with our minds, our supercomputers

539
00:26:18.680 --> 00:26:21.759
<v Speaker 2>and you know, lasers shooting down four kilometer vacuum tubo.

540
00:26:21.880 --> 00:26:25.160
<v Speaker 2>I forget the vacuum tubes, right, we can mathematically dissect

541
00:26:25.160 --> 00:26:27.799
<v Speaker 2>the most extreme bizarre environments in reality.

542
00:26:28.200 --> 00:26:32.640
<v Speaker 3>It is a remarkable perspective. The universe is incredibly vast

543
00:26:32.680 --> 00:26:37.839
<v Speaker 3>and violently chaotic, yet it remains profoundly intelligible. It follows rules,

544
00:26:37.839 --> 00:26:41.160
<v Speaker 3>It follows rules, and piece by piece, frequency by frequency,

545
00:26:41.480 --> 00:26:43.599
<v Speaker 3>we are learning to read the rule book.

546
00:26:43.319 --> 00:26:45.839
<v Speaker 2>Which leaves me with one final provocative thought for you

547
00:26:45.960 --> 00:26:49.160
<v Speaker 2>to consider. We have established today that the event horizon

548
00:26:49.279 --> 00:26:51.279
<v Speaker 2>is the ultimate eraser.

549
00:26:50.759 --> 00:26:52.720
<v Speaker 3>Of information, the ultimate trap.

550
00:26:52.799 --> 00:26:57.240
<v Speaker 2>It permanently swallows all light, sound and matter. Once something

551
00:26:57.319 --> 00:26:59.960
<v Speaker 2>crosses that boundary, it is gone from the observable uth

552
00:27:00.079 --> 00:27:04.920
<v Speaker 2>universe forever. Right yet, right before that eraser activates, right

553
00:27:05.079 --> 00:27:07.759
<v Speaker 2>in the millisecond before the door slams shut for eternity,

554
00:27:08.200 --> 00:27:12.039
<v Speaker 2>the violent collision broadcasts its most intimate secrets, its mass,

555
00:27:12.079 --> 00:27:15.759
<v Speaker 2>its spin, its gravity across the cosmos via these gravitational

556
00:27:15.799 --> 00:27:16.480
<v Speaker 2>direct waves.

557
00:27:16.559 --> 00:27:17.480
<v Speaker 3>It's quite send off.

558
00:27:17.519 --> 00:27:20.799
<v Speaker 2>The universe essentially screams its identity precisely at the moment

559
00:27:20.799 --> 00:27:23.359
<v Speaker 2>of its erasure. Is this the universe is built in

560
00:27:23.400 --> 00:27:26.559
<v Speaker 2>mechanism for ensuring that nothing is ever truly erased without

561
00:27:26.599 --> 00:27:29.960
<v Speaker 2>living a trace. If the universe rings like a bell

562
00:27:30.039 --> 00:27:34.160
<v Speaker 2>right before it goes dark, what other invisible boundaries are

563
00:27:34.160 --> 00:27:36.200
<v Speaker 2>out there right now, just waiting for us to figure

564
00:27:36.200 --> 00:27:37.000
<v Speaker 2>out how to listen.

565
00:27:37.440 --> 00:27:40.960
<v Speaker 3>It is a beautiful contradiction to end on the darkness

566
00:27:41.039 --> 00:27:43.559
<v Speaker 3>announces its arrival with absolute clarity.

567
00:27:43.680 --> 00:27:46.119
<v Speaker 2>It truly does. Keep looking up and keep listening until

568
00:27:46.119 --> 00:27:46.519
<v Speaker 2>next time.
