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>I want you to start by visualizing a scene with me.

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<v Speaker 2>We are on land. We aren't looking up at the

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<v Speaker 2>sky from some mountaintop. We are deep, deep, underwater, really

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<v Speaker 2>due We're at the bottom of the Mediterranean Sea. It

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<v Speaker 2>is it's pitch black. Obviously the sunlight gave up trying

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<v Speaker 2>to reach this depth a long, long time ago.

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<v Speaker 3>The pressure is immense, crushing.

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<v Speaker 2>It's silent and down there, anchored to the seabed. Is

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<v Speaker 2>this well, this strange vertical forest.

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

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<v Speaker 2>It's a forest of cables, strings of sensors, just floating

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<v Speaker 2>upright in the dark, stretching up from the mud, just

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<v Speaker 2>watching the water.

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<v Speaker 3>This is the domain of the KM three net Neutrino telescope,

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<v Speaker 3>and it's an incredibly eerie and frankly beautiful piece of engineering.

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<v Speaker 2>Right, and they're waiting for a flash, a tiny, faint

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<v Speaker 2>blue flash of light that signals something is crashed into

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<v Speaker 2>the water from space.

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<v Speaker 3>A cosmic ray, a neutrino, something from out there.

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<v Speaker 2>Now, usually this happens occasionally, you know, we catch a

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<v Speaker 2>ghost particle here and there. It's part of the background noise.

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<v Speaker 3>Of the universe, exactly, just the normal hum of reality.

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<v Speaker 2>But I want you to take us back to twenty

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<v Speaker 2>twenty three, because something happened in the data that well

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<v Speaker 2>it really shouldn't have happened.

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<v Speaker 3>It was an anomaly that woke a lot of people up,

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<v Speaker 3>a real wake up call in the data streams.

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<v Speaker 2>Bam, a single particle slams into the atmosphere, It interacts,

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<v Speaker 2>and it sends a signal down to the depths. But

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<v Speaker 2>this wasn't just a polite knock at the door, Oh no,

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<v Speaker 2>this was a battering ram. The energy level of this

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<v Speaker 2>single subatomic particle was.

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<v Speaker 3>Frankly, when I first read the briefing, I thought it

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<v Speaker 3>was a typo. It just sounds made up.

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<v Speaker 2>It does sound like science fiction, or you know, an

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<v Speaker 2>error in the spreadsheet. But it wasn't.

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<v Speaker 3>I looked at the numbers. This single particle carried in

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<v Speaker 3>energy level roughly one hundred thousand times higher than the

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<v Speaker 3>most powerful collision human beings have ever produced.

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<v Speaker 2>And just to put that into context for you, we're

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<v Speaker 2>talking about the Large Hadron Collider, the LHC, The.

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<v Speaker 3>LHC, that twenty seven kilometer ring buried under the border

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<v Speaker 3>of Friends in Switzerland.

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<v Speaker 2>The most expensive, most complex machine our species is ever built.

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<v Speaker 2>We use the power gred of a small country just

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<v Speaker 2>to turn it on. We accelerate protons to ninety nine

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<v Speaker 2>point nine nine percent of the speed of light.

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<v Speaker 3>We smashed them together to try and recreate the conditions

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<v Speaker 3>right after the Big.

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<v Speaker 2>Bang, and nature just casually threw a rock at us

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<v Speaker 2>that was one hundred thousand times stronger than our absolute

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<v Speaker 2>best effort.

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<v Speaker 3>That is the scale we're dealing with. Yeah, and the problem,

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<v Speaker 3>the whole reason we're having this conversation today is that

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<v Speaker 3>according to standard astrophysics, that particle shouldn't exist.

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<v Speaker 2>It shouldn't exist.

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<v Speaker 3>There is no gun in the known universe big enough

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<v Speaker 3>to fire that bullet.

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<v Speaker 2>So we have a ballistics report with no gun exactly.

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<v Speaker 3>We have the bullet hole, but no.

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<v Speaker 2>Weapon, and that leads us to the source material. For

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<v Speaker 2>today's analysis, we're looking at a fascinating new hypothesis from

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<v Speaker 2>a team at the University of Massachusetts Amherst, your mass Amherst,

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<v Speaker 2>and they're proposing that this wasn't a star, it wasn't

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<v Speaker 2>a supernova, it wasn't a gamma ray burst. They think

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<v Speaker 2>we witnessed a.

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<v Speaker 3>Death, a very specific and a very violent death.

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<v Speaker 2>I think we saw a black hole explode.

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<v Speaker 3>And not just any black hole, a quasi extremal, primordial

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<v Speaker 3>black hole.

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<v Speaker 2>Okay, hold on exploding black holes. I thought the number

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<v Speaker 2>one rule of black hole club was that you don't

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<v Speaker 2>talk about things coming out of them. Right, They're the

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<v Speaker 2>cosmic roach motel. You check in, you don't check out.

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<v Speaker 2>Things go in, nothing comes out. How do we get

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<v Speaker 2>an explosion?

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<v Speaker 3>That's the popular understanding, and you know, for big, stellar

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<v Speaker 3>mass black holes it's mostly true. But when you get

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<v Speaker 3>into the quantum physics of the very very small, the

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<v Speaker 3>rules they flip.

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<v Speaker 2>They flip.

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<v Speaker 3>We're going to find out that black holes aren't really black,

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<v Speaker 3>they're not perfectly stable, and they definitely don't stay quiet forever.

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<v Speaker 2>This is what I love about this topic. We're going

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<v Speaker 2>to peel back the layers here. We have a mystery

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<v Speaker 2>crash in twenty twenty three. We have a suspect, this

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<v Speaker 2>exploding black hole. But the researchers we're talking Andrea tam Jaqui,

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<v Speaker 2>Migua Juan, and Michael Baker, they aren't just trying to

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<v Speaker 2>solve one crash, are they.

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<v Speaker 3>No. No, that's why this paper is making such ways.

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<v Speaker 3>They're suggesting that this single impossible particle is a key,

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<v Speaker 3>aike to what a key that could unlock three of

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<v Speaker 3>the biggest locked doors in physics all at the same time.

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<v Speaker 2>A three for one deal.

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<v Speaker 3>If they're right, this explains the crash. It finally explains

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<v Speaker 3>dark matter, the invisible glue holding the universe together, and

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<v Speaker 3>maybe most excitingly, it gives us a way to find

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<v Speaker 3>particles that we haven't even discovered yet, a complete catalog

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<v Speaker 3>of reality.

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<v Speaker 2>That is a massive claim. So our mission today is

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<v Speaker 2>to really get into that. We need to understand the

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<v Speaker 2>crime scene, the weapon, and the motive. So it's good

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<v Speaker 2>let's start with the crime scene, the twenty twenty three event.

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<v Speaker 2>What exactly hit us? It was a neutrino, a newtrino,

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<v Speaker 2>the ghost particle.

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<v Speaker 3>For good reason, newtritos are notoriously antisocial particles. They have

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<v Speaker 3>almost no mass, no electric.

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<v Speaker 2>Charge, so they don't really interact with much.

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<v Speaker 3>They don't interact with the electromagnetic force, which means they're

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<v Speaker 3>invisible to light, radio X rays. They only really talk

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<v Speaker 3>to the universe via the weak nuclear force and gravity.

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<v Speaker 2>I've heard the stat that what trillions of them are

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<v Speaker 2>passing through my hand right.

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<v Speaker 3>Now, trillions, mostly from the Sun. They're streaming through your body,

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<v Speaker 3>through the chair you're sitting on, through the floor, through

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<v Speaker 3>the entire crust of the Earth.

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<v Speaker 2>All the way through the core, all the way through.

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<v Speaker 3>The molten core, and out the other side, without bumping

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<v Speaker 3>into a single atom to a newtrino. The Earth is

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<v Speaker 3>basically just a thin fog. It's barely there.

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<v Speaker 2>So if they're so ghostly, so hard to catch, how

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<v Speaker 2>did Cam three net that telescope in the Mediterranean, how

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<v Speaker 2>did it actually catch one?

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<v Speaker 3>It's all about probability. It's a numbers game. If you

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<v Speaker 3>have enough neutrinos passing through enough water, eventually, just by

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<v Speaker 3>sheer luck, one of them will smack head on into

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<v Speaker 3>the nucleus of a water molecule or an atom in

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<v Speaker 3>the sea bed.

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<v Speaker 2>A direct hit.

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<v Speaker 3>A direct hit, And when that happens, the kinetic energy

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<v Speaker 3>of that neutrino gets transferred to the wreckage. It creates

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<v Speaker 3>a cascade of other charged particles, mostly things like muons

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<v Speaker 3>or electrons, that then scream through the.

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<v Speaker 2>Water and they move incredibly fast.

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<v Speaker 3>They move faster than the speed of light in water.

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<v Speaker 2>Wait, faster than light? I thought Einstein put a start

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<v Speaker 2>to that. That's the universal speed limit.

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<v Speaker 3>Right, ah, But that's the key qualifier. Faster than light

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<v Speaker 3>in a vacuum is impossible. Nothing beats sea. But light

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<v Speaker 3>slows down when it goes through a medium like water

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<v Speaker 3>or glass, it drags a bit. These high energy particles

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<v Speaker 3>they don't slow down as much, so they actually outrun

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<v Speaker 3>the light they're creating. It's like a sonic boom for light.

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<v Speaker 2>And what does that look like?

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<v Speaker 3>It creates a cone of faint blue light called Chernkov radiation.

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<v Speaker 2>That's the blue flash.

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<v Speaker 3>That's the flash. The sensors in that underwater forest they

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<v Speaker 3>see that blue cone of light, and based on the

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<v Speaker 3>brightness and the angle of the cone, they can calculate

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<v Speaker 3>exactly where the neutrino came from and crucially how much

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<v Speaker 3>energy it had.

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<v Speaker 2>And this is where the twenty twenty three event just

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<v Speaker 2>goes completely off the rails because the energy was well,

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<v Speaker 2>it was off the chart completely.

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<v Speaker 3>We measure this energy in a unit called electron volts.

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<v Speaker 3>A visible photon particle of light you see with your

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<v Speaker 3>eyes is about two or three electron volts, Okay, very small.

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<v Speaker 3>The lac smashes protons together at around thirteen terra electron volts.

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<v Speaker 3>That's a TeV.

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<v Speaker 2>Trillions, thirteen trillion, Okay, that's a big number.

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<v Speaker 3>This neutrino was in the range of pav put electron

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<v Speaker 3>bolt heta. What's that? That's quadrillions a thousand trillion, So

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<v Speaker 3>it's orders of magnitude beyond what we can produce on Earth.

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<v Speaker 2>A thousand trillion electron vaults in one tiny particle. So

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<v Speaker 2>why can't it be a star? We have big stars,

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<v Speaker 2>We have supernovae, these massive explosions. Why can't a supernova

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<v Speaker 2>spit out a peavy neutrino.

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<v Speaker 3>It comes down to something called the energy ceiling. This

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<v Speaker 3>is a fascinating bit of cosmic.

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<v Speaker 2>Mechanically, the energy ceiling.

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<v Speaker 3>We know how magnetic fields and shock waves work in

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<v Speaker 3>space and things like supernovae remnants. To get a particle

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<v Speaker 3>up to that speed. You need to bounce it back

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<v Speaker 3>and forth in a magnetic field like a pinball machine,

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<v Speaker 3>gaining speed with airy bounce.

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<v Speaker 2>So it's like a natural particle accelerator in space. You

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<v Speaker 2>spin it up.

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<v Speaker 3>Exactly, but there's a problem. Eventually the particle gets so

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<v Speaker 3>fast and has so much momentum that the magnetic field

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<v Speaker 3>can't hold onto it anymore. It escapes, it flies off

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<v Speaker 3>the track.

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<v Speaker 2>Ah okay.

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<v Speaker 3>Standard astrophysical objects, supernova remnants, the jets from active galactic nuclei,

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<v Speaker 3>they all have a limit on how tightly they can

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<v Speaker 3>hold a particle while they're accelerating it. They leak, and

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<v Speaker 3>the math says they generally leak before they can reach

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<v Speaker 3>these peavy levels.

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<v Speaker 2>So you're saying the accelerator itself, it breaks before the

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<v Speaker 2>particle gets fast enough.

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<v Speaker 3>Precisely, so when we see a particle this hot, this energetic,

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<v Speaker 3>we know it didn't come from a pinball machine process

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<v Speaker 3>where it was gradually sped up over time.

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<v Speaker 2>It had to be a single shot process.

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<v Speaker 3>A single shot something that released all that energy in

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<v Speaker 3>one instantaneous event, like a bomb, like a decay or

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<v Speaker 3>an explosion. And that leads us right back to the

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<v Speaker 3>suspect the primordial black hole. Now I need you to

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<v Speaker 3>deprogram me a little bit here, because when I think

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<v Speaker 3>black hole, I have a very specific movie poster image

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<v Speaker 3>in my head.

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<v Speaker 2>Interstellar Gargantua. Yeah, a giant, swirling disk of doom, a

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<v Speaker 2>dead star that collapsed, spagheification, all that stuff.

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<v Speaker 3>And that's a perfect description of a stellar black hole.

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<v Speaker 3>That's the standard model. You take a star, say, twenty

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<v Speaker 3>times heavier than our sun, it burns through its fuel,

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<v Speaker 3>gravity wins the final battle, and it crushes down to

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<v Speaker 3>an infinitely dense point. Boom. You get a black.

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<v Speaker 2>Hole right the end of a star's life.

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<v Speaker 3>Primordial black holes or pdh are a completely different beast.

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<v Speaker 3>They're not dead stars, they're fossils. They are relics from

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<v Speaker 3>the very first moments of time, the Big Bang itself.

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<v Speaker 2>So these things are older than stars, older than galaxies.

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<v Speaker 3>Much older. Think about the universe. Just a fraction of

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<v Speaker 3>a second after time zero, It wasn't empty space with

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<v Speaker 3>stars sprinkled in it. It was a hot, dense, uniform

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<v Speaker 3>soup of plasma. Everything was grammed.

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<v Speaker 2>Together, the cosmic soup.

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<v Speaker 3>Now, usually this soup is thought to expand smoothly, but

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<v Speaker 3>Stephen Hawking and others back in the nineteen seventies proposed

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<v Speaker 3>a fascinating idea. What if it wasn't perfectly smooth? What

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<v Speaker 3>if there were lumps, lumps in the oatmeal exactly? What

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<v Speaker 3>if there were tiny regions that were, just by random chance,

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<v Speaker 3>slightly denser than the areas around them.

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<v Speaker 2>Lumps in the oatmeal of reality.

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<v Speaker 3>I like that if one of those lumps was dense enough,

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<v Speaker 3>just purely by the weight of the matter packed into

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<v Speaker 3>that small space, it would collapse under its own gravity.

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<v Speaker 3>It wouldn't need to wait billions of years to become

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<v Speaker 3>a star then die. It would just crunch, a direct

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<v Speaker 3>collapse into a black hole.

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<v Speaker 2>So you get a black hole created in the first

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<v Speaker 2>fraction of a second of the universe's existence.

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<v Speaker 3>Yes, and here is the absolutely crucial difference. A stellar

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<v Speaker 3>black hole has to be heavy. It has to be

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<v Speaker 3>heavier than the Sun because it came from a star

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<v Speaker 3>that was heavier than the Sun.

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<v Speaker 2>Right, that's the entry requirement.

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<v Speaker 3>But a primordial black hole it forms from a random

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<v Speaker 3>lump in the primordial soup. It could be any size.

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<v Speaker 2>How small are you talking?

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<v Speaker 3>It could be the mass of a mountain compressed into

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<v Speaker 3>the size of a proton. It could be the mass

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<v Speaker 3>of an asteroid compressed into the size of a single atom.

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<v Speaker 2>A black hole the size of an atom. That is

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<v Speaker 2>a genuinely terrifying thought, just floating around out there in.

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<v Speaker 3>Space, potentially trillions and trillions of them.

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<v Speaker 2>Yes, Oh, wait a minute, if there's the size of

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<v Speaker 2>an atom, wouldn't they just vanish? I mean, don't black

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<v Speaker 2>holes need to eat stuff to grow and survive? If

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<v Speaker 2>they're that tiny, can they even eat? Or do they starve?

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<v Speaker 3>That's the perfect question. They don't starve, they evaporate. And

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<v Speaker 3>this brings us to probably the most famous equation Stephen

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<v Speaker 3>Hawking ever wrote. It's called Hawking radiation.

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<v Speaker 2>I've definitely heard the term. It's the idea that black

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<v Speaker 2>holes aren't truly black, right, they leak?

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<v Speaker 3>Correct. In classical physics, nothing escapes a black hole's event horizon.

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<v Speaker 3>But quantum mechanics comes along and says, not so fast.

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<v Speaker 3>At the very edge of the black hole, space is

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<v Speaker 3>a weird, frothing foam. You have what are called virtual

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<v Speaker 3>particles popping in and out of existence constantly.

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<v Speaker 2>Quantum phone.

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<v Speaker 3>Right, it's happening everywhere all the time. Usually a particle

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<v Speaker 3>and its andy particle pop up, they find each other,

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<v Speaker 3>they annihilate, and they vanish back into the vacuum. It's

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<v Speaker 3>a zero sum game. But right at the edge of

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<v Speaker 3>a black hole, at the event horizon, sometimes a pair

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<v Speaker 3>pops into existence and one falls in and the other

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<v Speaker 3>one escapes out into space.

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<v Speaker 2>So the black hole just it actually spits something out effectively.

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<v Speaker 3>Yes, from an outside observer's point of view, it looks

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<v Speaker 3>like the black hole is blowing emitting particles. And because

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<v Speaker 3>of the conservation of energy, the energy for that escaping

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<v Speaker 3>particle has to come from somewhere. It comes from the

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<v Speaker 3>mass of the black hole itself.

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<v Speaker 2>So the black hole loses a tiny, tiny gooit of mass.

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<v Speaker 2>It's leaking.

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<v Speaker 3>It's leaking, it's evaporating. Now, for a big black hole

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<v Speaker 3>like Sagittarius A, the one in the center of our galaxy,

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<v Speaker 3>this leak is pathetic. It's colder than the background temperature

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<v Speaker 3>of the universe. It would take a trillion times the

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<v Speaker 3>current age of the universe for it to evaporate away.

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<v Speaker 3>It's completely negligible.

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<v Speaker 2>But we aren't talking about big ones.

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<v Speaker 3>No, we are talking about the tiny primordial ones. And

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<v Speaker 3>here is the completely counterintuitive rule of black hole thermodynamics,

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<v Speaker 3>The smaller the black hole, the hotter it is.

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<v Speaker 2>Wait, run that by me again. Smaller is hotter, that

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<v Speaker 2>feels backwards. Usually, you know, a big bonfire is hotter

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<v Speaker 2>than the single.

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<v Speaker 3>Match the quantum world of black holes, it's an inverse relationship.

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<v Speaker 3>A massive black hole is cosmically cold, and atam sized

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<v Speaker 3>black hole is a ferocious furnace. It radiates energy furiation.

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<v Speaker 2>Okay, okay, I think I see it. So if it

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<v Speaker 2>radiates energy furiously, it must be losing.

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<v Speaker 3>Mass faster correct, much faster.

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<v Speaker 2>And if it loses mass, it gets smaller. Correct, And

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<v Speaker 2>if it gets smaller, it gets even hotter.

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<v Speaker 3>You see where this is going.

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<v Speaker 2>It's a death spiral. It's a runaway reaction.

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<v Speaker 3>It's a runaway feedback loop. A primordial black hole might

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<v Speaker 3>spend billions of years slowly leaking, very quietly, not bothering anyone.

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<v Speaker 3>But as it gets smaller and smaller, it hits a

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<v Speaker 3>tipping point. The evaporation rates skyrockets. It starts screaming out particles.

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<v Speaker 2>So it shrinks faster, it gets hotter, screams louder.

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<v Speaker 3>The cycle accelerates until the last few seconds of its

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<v Speaker 3>life or just a catastrophic release of energy.

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<v Speaker 2>And that final moment when it hits zero mass, that's

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<v Speaker 2>the boom.

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<v Speaker 3>That is the explosion, a violent detonation that releases all

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<v Speaker 3>of its remaining mass energy into a flash of fundamental particles.

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<v Speaker 3>And according to the U mass researchers, that is what

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<v Speaker 3>hit our atmosphere in twenty twenty three. We didn't see

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<v Speaker 3>a star explode. We saw a microscopic, ancient black hole

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<v Speaker 3>finally reach the end of its multi billion year fuze.

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<v Speaker 2>That is actually kind of poetic. This thing has been

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<v Speaker 2>dying since the moment the universe began, and I finally

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<v Speaker 2>went out with a bang, right on our cosmic doorstep.

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<v Speaker 3>And the energy profile fits a dying black hole of

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<v Speaker 3>a certain mass, releases particles and exactly the kind of

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<v Speaker 3>energies that heavy scale that cam three net detected. The

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<v Speaker 3>shoe fits the crime scene perfectly.

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<v Speaker 2>But the UMAs team is saying it's not just about

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<v Speaker 2>the energy, it's about what comes out of the explosion.

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<v Speaker 2>They used a phrase in the paper that caught my eye,

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<v Speaker 2>a democratic explosion.

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<v Speaker 3>Yes, this is a fascinating part of the theory.

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<v Speaker 2>I assume they don't mean the black hole is you know,

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<v Speaker 2>holding elections before it blows up.

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<v Speaker 3>Hey. No. In particle physics, most interactions are biased, They

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<v Speaker 3>play favorites. For example, the electromagnetic force only talks to

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<v Speaker 3>particles that have an electric charge. It completely ignores neutrinos. Sure,

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<v Speaker 3>the strong nuclear force only talks to quarks. It holds

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<v Speaker 3>them together in protons and neutrons, but it doesn't care

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<v Speaker 3>about electrons at all.

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<v Speaker 2>Right, it's a click different forces for different particles exactly.

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<v Speaker 3>But gravity, gravity is the ultimate democrat. Gravity doesn't care

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<v Speaker 3>if you're a proton, a photon, a neutrino, or some

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<v Speaker 3>weird hypothetical dark matter particle. If you have mass or energy,

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<v Speaker 3>gravity treats you exactly the same, one particle, one vote, exactly.

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<v Speaker 3>So when a black hole explodes, which is fundamentally a

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<v Speaker 3>gravitational process, the unwinding of space time itself, it doesn't discriminate.

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<v Speaker 3>It doesn't just spit out light, It doesn't just spit

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<v Speaker 3>out electrons. It spits out everything, everything, everything that can

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<v Speaker 3>theoretically exist in nature. According to our laws of physics,

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<v Speaker 3>if a particle is possible in our universe, the evaporating

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<v Speaker 3>black hole will create it. It has no choice.

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<v Speaker 2>That is just wild. So in that final burst, it's

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<v Speaker 2>spitting out a shower of electrons, quarks, higgs, boson.

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<v Speaker 3>All the particles of the standard model. Yes, but it's

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<v Speaker 3>also spitting out things we haven't discovered yet.

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<v Speaker 2>I love the analogy you could use here. It's like

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<v Speaker 2>a pinata. You know, you hit a normal pinata star

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<v Speaker 2>and you get I don't know, a stream of light

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<v Speaker 2>beams a certain type of candy. But you crack open

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<v Speaker 2>a primordial black hole pinata and you get the entire

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<v Speaker 2>inventory of the candy factor. You get the standard lollipops

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<v Speaker 2>and chocolates, but you also get the secret prototype candies

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<v Speaker 2>that they haven't even released to the public yet.

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<v Speaker 3>That is a surprisingly accurate and useful analogy, and that's

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<v Speaker 3>why this theory is being called a potential Rosetta stone

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<v Speaker 3>for particle.

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<v Speaker 2>Physics, because it contains everything.

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<v Speaker 3>If we can analyze the debris from this explosion, like

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<v Speaker 3>that single high energy in neutrino, we saw, we're not

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<v Speaker 3>just seeing a crash, We're getting a data dump of

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<v Speaker 3>the entire universe's fundamental particle catalog.

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<v Speaker 2>So we had a better look at that twenty twenty

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<v Speaker 2>three event with more sensitive instruments we might have seen

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<v Speaker 2>what Derek, dark matter, particles, particles predicted by string theory, supersymmetry, all.

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<v Speaker 3>Of it in theory, it's all in the debris cloud.

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<v Speaker 3>It turns these explosions into the ultimate particle physics experiment.

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<v Speaker 3>It's better than the LHC.

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<v Speaker 2>Better than the LHC.

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<v Speaker 3>The LHC can only smash together what we put into it, protons,

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<v Speaker 3>lad ions. The black hole smashes spacetime itself and sees

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<v Speaker 3>what falls out. It's nature doing the experiment for us.

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<v Speaker 3>With energies, we could never dream of building on Earth.

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<v Speaker 2>Okay, I am completely sold on the concept. It's elegant,

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00:18:14.480 --> 00:18:18.079
<v Speaker 2>it explains the energy, it offers this incredible kresure trove

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00:18:18.160 --> 00:18:21.359
<v Speaker 2>of data. But here's the problem I'm seeing now. If

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<v Speaker 2>these things are exploding, how often does it happen? Is

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<v Speaker 2>this a once in a billion year's event.

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<v Speaker 3>You would think so, wouldn't you. But the UMass team

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<v Speaker 3>ran the numbers based on the standard primordial black hole models.

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<v Speaker 3>They calculated that these explosions should be happening within range

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<v Speaker 3>of our detectors surprisingly often. How often is often? Maybe

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<v Speaker 3>every decade or every decade?

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<v Speaker 2>Wait a minute, if a black hole blows up every

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<v Speaker 2>ten years, and it releases this insane amount of energy.

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<v Speaker 2>Why haven't we noticed this before? Why was twenty twenty

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<v Speaker 2>three the first time we all said, whoa look at that?

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<v Speaker 3>And that question brings us to the plot twist. This

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<v Speaker 3>is the detective story part of the paper because you

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00:18:58.279 --> 00:19:00.880
<v Speaker 3>are absolutely right. If they happen every decade, we should

401
00:19:00.880 --> 00:19:03.759
<v Speaker 3>have seen them. And more importantly, we have another detector

402
00:19:03.759 --> 00:19:06.799
<v Speaker 3>that should have seen them. Ice Cube. Ice cube the

403
00:19:07.079 --> 00:19:10.079
<v Speaker 3>absolute heavyweight champion of neutrino detections.

404
00:19:10.079 --> 00:19:11.960
<v Speaker 2>This is the one in Antarctica right bird in the

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00:19:12.000 --> 00:19:13.079
<v Speaker 2>ice yes.

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00:19:13.440 --> 00:19:16.720
<v Speaker 3>While CAM three net is in the Mediterranean Sea. Ice

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00:19:16.720 --> 00:19:19.440
<v Speaker 3>Cube is built into the solid, crystal clear ice of

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00:19:19.440 --> 00:19:22.839
<v Speaker 3>the South Pole. It's a full cubic kilometer of ice,

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00:19:23.119 --> 00:19:26.799
<v Speaker 3>instrumented with thousands of sensors. It has been running for years.

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00:19:27.079 --> 00:19:28.400
<v Speaker 3>It is incredibly sensitive.

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<v Speaker 2>So, okay, KM three neut saw the impossible particle. Did

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<v Speaker 2>ice cube see it?

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<v Speaker 3>No?

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00:19:33.880 --> 00:19:36.119
<v Speaker 2>It missed it. Bad luck, wrong part of the sky.

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00:19:36.279 --> 00:19:39.079
<v Speaker 3>It didn't register the event at all. But the problem

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00:19:39.200 --> 00:19:42.279
<v Speaker 3>is much deeper than just missing one flash. Because you're right,

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00:19:42.319 --> 00:19:44.799
<v Speaker 3>the geometry of the Earth means sometimes one detector sees

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00:19:44.839 --> 00:19:47.960
<v Speaker 3>something the other can't. That's fine. The problem is the history,

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00:19:48.240 --> 00:19:51.720
<v Speaker 3>the history. If these explosions happen every decade, the sky

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00:19:51.799 --> 00:19:54.160
<v Speaker 3>should be lit up with them. From ice cubes perspective,

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00:19:54.759 --> 00:19:56.799
<v Speaker 3>ice Cube has been staring at the northern sky where

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00:19:56.799 --> 00:19:59.079
<v Speaker 3>this event came from, for a very long time. It

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<v Speaker 3>has never seen anything like this, not even once. It's

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<v Speaker 3>never even seen an event one hundred as powerful.

425
00:20:03.599 --> 00:20:05.680
<v Speaker 2>So we have a huge contradiction.

426
00:20:05.559 --> 00:20:09.519
<v Speaker 3>A massive one. On one hand, the standard PBH theory says,

427
00:20:10.480 --> 00:20:14.039
<v Speaker 3>if primordial black holes explain the twenty twenty three CAM

428
00:20:14.039 --> 00:20:16.799
<v Speaker 3>three net event, then there should be thousands of them

429
00:20:16.799 --> 00:20:19.480
<v Speaker 3>exploding all the time, and we should be showered in

430
00:20:19.480 --> 00:20:20.839
<v Speaker 3>these high energy neutrinos.

431
00:20:21.200 --> 00:20:22.480
<v Speaker 2>And on the other hand, the.

432
00:20:22.440 --> 00:20:25.880
<v Speaker 3>Observational data from ice Cube says it's quiet out there,

433
00:20:26.079 --> 00:20:27.240
<v Speaker 3>eerially quiet.

434
00:20:27.599 --> 00:20:31.559
<v Speaker 2>So usually in science, when the prediction fails the observation test,

435
00:20:31.799 --> 00:20:33.599
<v Speaker 2>you throw out the theory. You say, well, I guess

436
00:20:33.640 --> 00:20:35.759
<v Speaker 2>it wasn't an exploding black hole after all, right.

437
00:20:36.200 --> 00:20:38.720
<v Speaker 3>You'd normally assume that CAM three net reading was a glitch,

438
00:20:39.319 --> 00:20:42.880
<v Speaker 3>a censor error, a weird fluke. But the UMass team

439
00:20:42.920 --> 00:20:45.279
<v Speaker 3>took a very different, very bold approach.

440
00:20:45.400 --> 00:20:46.039
<v Speaker 2>What did they do?

441
00:20:46.279 --> 00:20:49.240
<v Speaker 3>They said, Let's assume the data is correct. Let's assume

442
00:20:49.240 --> 00:20:51.720
<v Speaker 3>Cam three Nette did see a black hole explosion. What

443
00:20:51.799 --> 00:20:53.599
<v Speaker 3>would have to be true about black holes for that

444
00:20:53.640 --> 00:20:56.480
<v Speaker 3>to happen? While also explaining why ice CUE hasn't seen

445
00:20:56.559 --> 00:20:57.119
<v Speaker 3>hundreds of.

446
00:20:57.039 --> 00:21:00.319
<v Speaker 2>Them, They need a reason why the explosions are rare, rare.

447
00:21:00.519 --> 00:21:03.319
<v Speaker 3>Exactly, they need to turn the volume down on the explosions. Yeah,

448
00:21:03.319 --> 00:21:05.759
<v Speaker 3>you need a new model where these primordial black holes

449
00:21:05.799 --> 00:21:08.799
<v Speaker 3>exist in huge numbers, but they don't explode as easily

450
00:21:08.880 --> 00:21:10.920
<v Speaker 3>or as often as the standard model predicts.

451
00:21:11.079 --> 00:21:12.960
<v Speaker 2>They have to thread the needle. They need to allow

452
00:21:13.000 --> 00:21:16.400
<v Speaker 2>for one big boom in twenty twenty three, but prevent

453
00:21:16.519 --> 00:21:18.200
<v Speaker 2>a constant storm of booms.

454
00:21:18.319 --> 00:21:20.799
<v Speaker 3>And this is where they introduce the new physics, the

455
00:21:21.000 --> 00:21:21.920
<v Speaker 3>dark charge.

456
00:21:22.200 --> 00:21:24.519
<v Speaker 2>Okay, dark charge. That sounds like something straight out of

457
00:21:24.559 --> 00:21:26.039
<v Speaker 2>a sci fi movie? What is it?

458
00:21:26.160 --> 00:21:29.119
<v Speaker 3>This is the core of their new paper in Physical

459
00:21:29.119 --> 00:21:33.440
<v Speaker 3>Review Letters, the researchers, specifically Joachimiquis Juan and the team

460
00:21:34.000 --> 00:21:37.839
<v Speaker 3>proposed that these primordial black holes aren't just simple balls

461
00:21:37.839 --> 00:21:43.039
<v Speaker 3>of gravity. They possess a special property called quasi extremal status,

462
00:21:43.480 --> 00:21:46.039
<v Speaker 3>and that status is driven by a dark charge.

463
00:21:46.279 --> 00:21:49.519
<v Speaker 2>Quasi extremal that's a mouthful. Let's break that down. What

464
00:21:49.559 --> 00:21:52.319
<v Speaker 2>does extremal even mean in the context of a black hole.

465
00:21:52.359 --> 00:21:55.640
<v Speaker 3>An extremal black hole is a theoretical object where its

466
00:21:55.680 --> 00:21:58.839
<v Speaker 3>electric charge is so strong that it perfectly balances out

467
00:21:58.880 --> 00:21:59.440
<v Speaker 3>its gravity.

468
00:21:59.839 --> 00:22:01.799
<v Speaker 2>Arge balance is gravity. How does that work?

469
00:22:01.920 --> 00:22:04.240
<v Speaker 3>Think about it this way. Gravity is always attractive. It

470
00:22:04.279 --> 00:22:07.799
<v Speaker 3>pulls everything in. But electric charge. If you have a

471
00:22:07.880 --> 00:22:12.559
<v Speaker 3>lot of charges, say positive charges, packed together, it's repulsive.

472
00:22:12.599 --> 00:22:13.960
<v Speaker 3>It pushes everything out.

473
00:22:13.960 --> 00:22:16.920
<v Speaker 2>Like trying to push two positive ends of magnets together.

474
00:22:17.279 --> 00:22:20.119
<v Speaker 3>Exactly. So, if you could cram enough electric charge into

475
00:22:20.119 --> 00:22:23.039
<v Speaker 3>a black hole, the outward push from that charge would

476
00:22:23.079 --> 00:22:26.599
<v Speaker 3>fight the inward crush of gravity. An extremal black hole

477
00:22:26.680 --> 00:22:29.359
<v Speaker 3>is one where those two forces are perfectly balanced. It

478
00:22:29.400 --> 00:22:32.599
<v Speaker 3>stops evaporating, it stops shrinking, It becomes a stable remnant.

479
00:22:32.640 --> 00:22:34.359
<v Speaker 3>It gets cold and just sits there.

480
00:22:34.480 --> 00:22:36.640
<v Speaker 2>It hits the pause button on that death spiral we

481
00:22:36.640 --> 00:22:37.799
<v Speaker 2>talked about exactly.

482
00:22:38.039 --> 00:22:39.839
<v Speaker 3>Now, in the real world, you can't do this with

483
00:22:39.920 --> 00:22:43.200
<v Speaker 3>normal charge. Protons and electrons fly away too easily to

484
00:22:43.240 --> 00:22:46.720
<v Speaker 3>create this perfect balance. But the UMass team is suggesting

485
00:22:46.839 --> 00:22:49.759
<v Speaker 3>a new kind of charge, a dark charge.

486
00:22:49.799 --> 00:22:52.000
<v Speaker 2>What's the difference between that and regular charge?

487
00:22:52.119 --> 00:22:55.519
<v Speaker 3>Imagine our familiar force of electricity. You have positive and

488
00:22:55.599 --> 00:22:58.799
<v Speaker 3>negative charge, right, and that force governs how electrons and

489
00:22:58.839 --> 00:23:03.680
<v Speaker 3>protons interact. The dark charge is essentially a hypothetical copy

490
00:23:03.680 --> 00:23:07.240
<v Speaker 3>of that electric force, but it exists in what physicists

491
00:23:07.279 --> 00:23:09.839
<v Speaker 3>call the dark sector. The dark sector, the hidden part

492
00:23:09.880 --> 00:23:13.279
<v Speaker 3>of physics. We know dark matter exists, but it doesn't

493
00:23:13.279 --> 00:23:17.440
<v Speaker 3>interact with light or normal electricity. The theory suggests it

494
00:23:17.519 --> 00:23:20.240
<v Speaker 3>might have its own set of forces, its own version

495
00:23:20.279 --> 00:23:23.480
<v Speaker 3>of electromagnetism. And just like we have electrons that carry

496
00:23:23.480 --> 00:23:26.039
<v Speaker 3>our charge, this dark charge would be carried by a

497
00:23:26.200 --> 00:23:30.160
<v Speaker 3>dark electron, a dark electron, a hypothesized, very heavy and

498
00:23:30.200 --> 00:23:32.200
<v Speaker 3>completely invisible version of the electron.

499
00:23:32.359 --> 00:23:34.759
<v Speaker 2>Okay, so walk me through the mechanics of this. We

500
00:23:34.839 --> 00:23:39.079
<v Speaker 2>have these ancient tiny black holes. They're shrinking, they're getting hot,

501
00:23:39.519 --> 00:23:41.680
<v Speaker 2>but they're also carrying the secret dark charge.

502
00:23:41.759 --> 00:23:44.519
<v Speaker 3>What happens as they shrink and get hotter. They spit

503
00:23:44.559 --> 00:23:48.880
<v Speaker 3>out normal particles, photons, lutrinos, regular electrons pretty easily. But

504
00:23:48.960 --> 00:23:51.680
<v Speaker 3>if this dark electron is really really heavy, the black

505
00:23:51.680 --> 00:23:53.599
<v Speaker 3>hole can't spit it out yet. It doesn't have enough

506
00:23:53.680 --> 00:23:55.240
<v Speaker 3>energy at that temperature to create one.

507
00:23:55.319 --> 00:23:57.400
<v Speaker 2>So it's stuck with the dark charge.

508
00:23:57.160 --> 00:23:59.480
<v Speaker 3>Right, the charge can't escape. It's like trying to pay

509
00:23:59.480 --> 00:24:01.039
<v Speaker 3>one hundred dollar debt, but all you have in your

510
00:24:01.039 --> 00:24:03.160
<v Speaker 3>pocket or pennies, You can't get rid of the debt.

511
00:24:03.480 --> 00:24:06.319
<v Speaker 3>So the black hole holds onto the dark charge. As

512
00:24:06.319 --> 00:24:08.960
<v Speaker 3>the black hole gets smaller, that charge gets more and

513
00:24:09.000 --> 00:24:12.519
<v Speaker 3>more concentrated. The repulsive force builds up a Greakes kick

514
00:24:12.559 --> 00:24:16.880
<v Speaker 3>in exactly, the dark charge pushes back against gravity's crush.

515
00:24:16.960 --> 00:24:20.480
<v Speaker 3>It dramatically slows down the evaporation process. It prevents the

516
00:24:20.519 --> 00:24:24.440
<v Speaker 3>black hole from racing toward that final violent explosion. It

517
00:24:24.680 --> 00:24:25.640
<v Speaker 3>stabilizes it.

518
00:24:25.759 --> 00:24:28.440
<v Speaker 2>So instead of a universe filled with the constant pop

519
00:24:28.440 --> 00:24:31.759
<v Speaker 2>pop pop of these black holes exploding every decade, the

520
00:24:31.839 --> 00:24:34.079
<v Speaker 2>dark charge keeps most of them stable.

521
00:24:33.839 --> 00:24:36.640
<v Speaker 3>For a very very long time. It puts them into

522
00:24:36.680 --> 00:24:38.079
<v Speaker 3>a state of suspended animation.

523
00:24:38.440 --> 00:24:41.279
<v Speaker 2>But wait, if it stabilizes them, why did we see

524
00:24:41.279 --> 00:24:43.599
<v Speaker 2>an explosion in twenty twenty three? Why did that one

525
00:24:43.640 --> 00:24:43.960
<v Speaker 2>go off?

526
00:24:44.079 --> 00:24:48.880
<v Speaker 3>Because it's quasi extremal, not perfectly stable, just barely stable

527
00:24:49.160 --> 00:24:52.480
<v Speaker 3>on the edge. Eventually, after billions more years, the black

528
00:24:52.480 --> 00:24:55.440
<v Speaker 3>hole gets just small enough and just hot enough that

529
00:24:55.519 --> 00:24:59.039
<v Speaker 3>it can finally spit out those super heavy dark electrons.

530
00:24:58.480 --> 00:25:00.519
<v Speaker 2>Ah, so it can finally pay it's debt.

531
00:25:00.599 --> 00:25:03.559
<v Speaker 3>Once it starts shedding the charge, the brakes fail and

532
00:25:03.680 --> 00:25:07.440
<v Speaker 3>then the gravity is unopposed again. The collapse resumes with

533
00:25:07.519 --> 00:25:12.319
<v Speaker 3>a vengeance, the temperature spikes catastrophically, and boom, you get

534
00:25:12.319 --> 00:25:13.279
<v Speaker 3>the explosion we saw.

535
00:25:13.480 --> 00:25:16.400
<v Speaker 2>So the dark charge acts as a safety valve or

536
00:25:16.400 --> 00:25:20.839
<v Speaker 2>a regulator. It makes the explosions incredibly rare, but when

537
00:25:20.880 --> 00:25:23.680
<v Speaker 2>they do happen, they are unbelievably potent.

538
00:25:23.839 --> 00:25:27.519
<v Speaker 3>Precisely, it perfectly explains the ice cube discrepancy. Cam three

539
00:25:27.559 --> 00:25:31.000
<v Speaker 3>nets saw one of these rare catastrophic brake failures, but

540
00:25:31.079 --> 00:25:33.519
<v Speaker 3>ice Cube isn't seeing a constant rain of them because

541
00:25:33.519 --> 00:25:36.359
<v Speaker 3>the vast majority of these primordial black holes are sitting

542
00:25:36.440 --> 00:25:40.279
<v Speaker 3>out there, stabilized by their dark charge, quietly and invisibly waiting.

543
00:25:40.400 --> 00:25:43.200
<v Speaker 2>That is incredibly elegant. It doesn't throw out the data,

544
00:25:43.319 --> 00:25:46.200
<v Speaker 2>It saves the phenomenon. It allows the CAM three net

545
00:25:46.200 --> 00:25:48.799
<v Speaker 2>observation to be real without breaking all of our other

546
00:25:48.839 --> 00:25:50.079
<v Speaker 2>observations at the universe.

547
00:25:50.119 --> 00:25:52.119
<v Speaker 3>It does, and as Michael Baker, one of the co authors,

548
00:25:52.119 --> 00:25:54.799
<v Speaker 3>points out, this added complexity is actually a good thing.

549
00:25:55.160 --> 00:25:58.440
<v Speaker 3>Simpler models like the standard PBH model just don't fit

550
00:25:58.480 --> 00:26:01.519
<v Speaker 3>the reality we see. Need to add this dark sector

551
00:26:01.559 --> 00:26:03.119
<v Speaker 3>physics to make the math work out.

552
00:26:03.319 --> 00:26:05.720
<v Speaker 2>But the story doesn't end there, does it. Because once

553
00:26:05.759 --> 00:26:09.480
<v Speaker 2>you introduce this dark charge and these dark electrons, and

554
00:26:09.519 --> 00:26:13.680
<v Speaker 2>you theorize that there are trillions of these stable, tiny

555
00:26:13.720 --> 00:26:18.200
<v Speaker 2>black holes floating around the cosmos, you suddenly realize you

556
00:26:18.440 --> 00:26:21.599
<v Speaker 2>might have stumbled upon the solution to a much much

557
00:26:21.640 --> 00:26:23.000
<v Speaker 2>bigger problem.

558
00:26:22.759 --> 00:26:24.440
<v Speaker 3>The biggest problem in cosmology.

559
00:26:24.480 --> 00:26:25.720
<v Speaker 2>We're talking about dark matter.

560
00:26:25.839 --> 00:26:27.200
<v Speaker 3>We're talking about dark matter.

561
00:26:27.359 --> 00:26:30.119
<v Speaker 2>We mentioned dark matter in almost every investigation we do

562
00:26:30.200 --> 00:26:32.440
<v Speaker 2>on space. It's the ghost in the machine, it's the

563
00:26:32.519 --> 00:26:35.319
<v Speaker 2>elephant in every room in physics. But give us the

564
00:26:35.359 --> 00:26:38.319
<v Speaker 2>quick refresher. Why is it such a massive headache?

565
00:26:38.480 --> 00:26:41.480
<v Speaker 3>The headache is all about gravity. When we look at

566
00:26:41.519 --> 00:26:45.319
<v Speaker 3>galaxies like our own Milky Way, we can measure how

567
00:26:45.400 --> 00:26:48.279
<v Speaker 3>fast the stars on the outer edges are spinning around

568
00:26:48.279 --> 00:26:51.480
<v Speaker 3>the galactic center. And based on all the stars and

569
00:26:51.559 --> 00:26:54.119
<v Speaker 3>gas and dust that we can see, all the visible matter,

570
00:26:54.519 --> 00:26:58.599
<v Speaker 3>they're spinning way too fast. There's nearly enough gravitational pull

571
00:26:58.680 --> 00:27:00.920
<v Speaker 3>from the visible stuff to whole them in their orbits.

572
00:27:00.960 --> 00:27:03.799
<v Speaker 2>They should be flinging stars out into deep space.

573
00:27:03.960 --> 00:27:06.519
<v Speaker 3>Exactly like a carousel spinning too fast and the horse

574
00:27:06.599 --> 00:27:09.480
<v Speaker 3>is flying off. But they don't the galaxies hold together.

575
00:27:09.519 --> 00:27:12.559
<v Speaker 3>So there must be something else there, something invisible that

576
00:27:12.640 --> 00:27:15.160
<v Speaker 3>has a lot of mass and is providing the extra gravity.

577
00:27:15.359 --> 00:27:16.680
<v Speaker 2>We call it dark matter.

578
00:27:16.880 --> 00:27:18.759
<v Speaker 3>We call it dark matter. It seems to make up

579
00:27:18.759 --> 00:27:21.680
<v Speaker 3>about eighty five percent of all the matter in the universe,

580
00:27:22.039 --> 00:27:24.160
<v Speaker 3>and we have absolutely zero clue what it is.

581
00:27:24.319 --> 00:27:27.000
<v Speaker 2>And we've been looking for decades. Right, We've been looking

582
00:27:27.000 --> 00:27:29.480
<v Speaker 2>for these particles called WIMPs or axions.

583
00:27:29.680 --> 00:27:34.880
<v Speaker 3>We've built huge, incredibly sensitive detectors deep underground to shield

584
00:27:34.880 --> 00:27:38.359
<v Speaker 3>them from cosmic rays. We've looked for decades. We haven't

585
00:27:38.359 --> 00:27:42.440
<v Speaker 3>found a single wimp. The particle physics community is getting

586
00:27:42.480 --> 00:27:44.640
<v Speaker 3>a little nervous that we've been looking in the wrong place.

587
00:27:44.880 --> 00:27:47.079
<v Speaker 2>So enter the u mass hypothesis.

588
00:27:47.160 --> 00:27:49.319
<v Speaker 3>Look at the object we just built with this theory.

589
00:27:50.000 --> 00:27:54.599
<v Speaker 3>We have quasi extremal primordial black holes. They are heavy,

590
00:27:54.880 --> 00:27:57.359
<v Speaker 3>they are ancient, formed in the Big Bang. They're spread

591
00:27:57.400 --> 00:28:00.440
<v Speaker 3>all throughout the universe, and thanks to their dark shop charge,

592
00:28:00.839 --> 00:28:03.920
<v Speaker 3>they are stable. They don't explode often, they just sit there.

593
00:28:03.960 --> 00:28:07.079
<v Speaker 2>They are heavy, invisible objects that don't emit light and

594
00:28:07.160 --> 00:28:08.480
<v Speaker 2>only interact through gravity.

595
00:28:08.759 --> 00:28:13.079
<v Speaker 3>Which is the exact textbook definition of dark matter. Are

596
00:28:13.119 --> 00:28:16.920
<v Speaker 3>you saying the researchers are explicitly saying that these charge

597
00:28:16.960 --> 00:28:19.039
<v Speaker 3>primordial black holes are the dark matter.

598
00:28:19.240 --> 00:28:22.799
<v Speaker 2>So the dark matter holding our galaxy together. It isn't

599
00:28:22.839 --> 00:28:26.079
<v Speaker 2>a cloud of exotic gas. It's not some weird undiscovered

600
00:28:26.119 --> 00:28:31.240
<v Speaker 2>particle fluid. It's billions upon billions of tiny ancient ticking

601
00:28:31.319 --> 00:28:32.079
<v Speaker 2>time bombs.

602
00:28:32.240 --> 00:28:34.880
<v Speaker 3>Potentially, yes, it can. It's all the dots in one go.

603
00:28:35.519 --> 00:28:37.920
<v Speaker 3>The vast invisible halo of the Milky Way isn't a

604
00:28:37.920 --> 00:28:41.839
<v Speaker 3>cloud of whimps. It's a swarm of these charge primordial

605
00:28:41.880 --> 00:28:44.720
<v Speaker 3>black holes. They provide the extra gravity to keep our

606
00:28:44.759 --> 00:28:47.559
<v Speaker 3>galaxy from flying apart, Nywady. Once in a great while,

607
00:28:48.160 --> 00:28:51.240
<v Speaker 3>very rarely one of them finally loses its charge and debtonates,

608
00:28:51.440 --> 00:28:53.119
<v Speaker 3>sending out a particle like the one we saw in

609
00:28:53.119 --> 00:28:53.920
<v Speaker 3>twenty twenty three.

610
00:28:54.119 --> 00:28:56.519
<v Speaker 2>That is a staggering thought. The invisible glue of the

611
00:28:56.599 --> 00:28:59.720
<v Speaker 2>universe is actually made of the most destructive objects in nature,

612
00:29:00.160 --> 00:29:02.880
<v Speaker 2>held in check by a fundamental force we can't even see.

613
00:29:02.920 --> 00:29:05.559
<v Speaker 3>It unifies the micro and the macro in a beautiful way.

614
00:29:05.880 --> 00:29:08.440
<v Speaker 3>You have this subatomic particle detection deep in the ocean,

615
00:29:08.480 --> 00:29:11.799
<v Speaker 3>explaining the rotation of entire galaxies millions of light years across.

616
00:29:12.240 --> 00:29:15.279
<v Speaker 3>It is a potential grand unified moment for this specific

617
00:29:15.319 --> 00:29:16.240
<v Speaker 3>slice of physics.

618
00:29:16.480 --> 00:29:18.960
<v Speaker 2>It really makes you look at the empty space in

619
00:29:19.000 --> 00:29:22.039
<v Speaker 2>the night sky differently, doesn't it. It's not empty. It's

620
00:29:22.240 --> 00:29:25.119
<v Speaker 2>full of these dark charged seeds from the very beginning

621
00:29:25.200 --> 00:29:25.599
<v Speaker 2>of time.

622
00:29:26.000 --> 00:29:28.039
<v Speaker 3>And that brings us to the future of this research

623
00:29:28.559 --> 00:29:32.279
<v Speaker 3>because right now this is a hypothesis. It's a brilliant paper.

624
00:29:32.599 --> 00:29:35.279
<v Speaker 3>It fits the math beautifully, it fits the observational data

625
00:29:35.359 --> 00:29:37.920
<v Speaker 3>we have. But is it true?

626
00:29:38.160 --> 00:29:40.160
<v Speaker 2>How do we prove it? Do we just have to

627
00:29:40.200 --> 00:29:42.319
<v Speaker 2>sit back and wait another ten or twenty years for

628
00:29:42.359 --> 00:29:43.880
<v Speaker 2>another one of these things to explode?

629
00:29:43.920 --> 00:29:47.359
<v Speaker 3>That would certainly help. Another detection would be huge, but

630
00:29:47.440 --> 00:29:49.920
<v Speaker 3>we might not have to wait that long. The UMAs

631
00:29:49.960 --> 00:29:52.880
<v Speaker 3>team believes we are on the cusp of verifying hawking

632
00:29:52.960 --> 00:29:55.279
<v Speaker 3>radiation experimentally for the first time.

633
00:29:55.599 --> 00:29:58.440
<v Speaker 2>Verifying Hawking radiation would be a Nobel prize on its own.

634
00:29:58.559 --> 00:29:59.559
<v Speaker 2>That's a huge deal.

635
00:30:00.000 --> 00:30:02.839
<v Speaker 3>Sslutely, we have never actually seen a black hole evaporate.

636
00:30:02.880 --> 00:30:05.880
<v Speaker 3>It's been pure theory for fifty years. If this twenty

637
00:30:05.920 --> 00:30:09.000
<v Speaker 3>twenty three event is confirmed to be a PBH explosion.

638
00:30:09.480 --> 00:30:12.519
<v Speaker 3>It's the first proof that Hawking was right. But it

639
00:30:12.559 --> 00:30:13.279
<v Speaker 3>does more than that.

640
00:30:13.440 --> 00:30:15.200
<v Speaker 2>It proves the dark sector exists.

641
00:30:15.559 --> 00:30:17.920
<v Speaker 3>Yes, if we can get a better look at the

642
00:30:17.960 --> 00:30:21.519
<v Speaker 3>next event, or even reanalyze the twenty twenty three data

643
00:30:21.799 --> 00:30:24.400
<v Speaker 3>with more precision, we might be able to see the

644
00:30:24.440 --> 00:30:27.519
<v Speaker 3>specific fingerprint in the energy spectrum that points to the

645
00:30:27.519 --> 00:30:29.200
<v Speaker 3>decay of a dark electron.

646
00:30:29.359 --> 00:30:31.720
<v Speaker 2>Finding a brand new fundamental.

647
00:30:31.119 --> 00:30:33.599
<v Speaker 3>Particle, finding a particle that is not part of the

648
00:30:33.640 --> 00:30:37.599
<v Speaker 3>standard model of particle physics, it would fundamentally break physics

649
00:30:37.640 --> 00:30:39.799
<v Speaker 3>as we know it and open the door to a

650
00:30:39.839 --> 00:30:43.039
<v Speaker 3>whole new reality. As Michael Baker said in his interview,

651
00:30:43.359 --> 00:30:45.480
<v Speaker 3>it gave us a new window on the universe.

652
00:30:45.799 --> 00:30:48.279
<v Speaker 2>It's the joy of discovery, isn't it. I mean, think

653
00:30:48.279 --> 00:30:50.680
<v Speaker 2>about the journey we've just outlined here. We started with

654
00:30:50.720 --> 00:30:53.559
<v Speaker 2>a confusing blip on a sensor array at the bottom

655
00:30:53.559 --> 00:30:57.079
<v Speaker 2>of the Mediterranean Sea. What could have been dismissed as

656
00:30:57.200 --> 00:30:58.839
<v Speaker 2>a mistake in the data.

657
00:30:59.200 --> 00:31:00.920
<v Speaker 3>A simple outline, and by pulling on.

658
00:31:00.880 --> 00:31:04.079
<v Speaker 2>That single thread, these researchers have unraveled a theory that

659
00:31:04.119 --> 00:31:05.799
<v Speaker 2>goes all the way back to the first second of

660
00:31:05.799 --> 00:31:09.480
<v Speaker 2>the Big Bang, explains the glue holding galaxies together and

661
00:31:09.599 --> 00:31:11.559
<v Speaker 2>essentially invents a new force of nature.

662
00:31:11.839 --> 00:31:15.039
<v Speaker 3>It is the ultimate cosmic detective story. And the best

663
00:31:15.079 --> 00:31:17.880
<v Speaker 3>part is the evidence is literally raining down on us

664
00:31:17.880 --> 00:31:20.240
<v Speaker 3>from space. We just need to keep our eyes and

665
00:31:20.279 --> 00:31:21.599
<v Speaker 3>our dec sensors open.

666
00:31:21.880 --> 00:31:24.599
<v Speaker 2>So here is where we leave you today. We've talked

667
00:31:24.599 --> 00:31:27.319
<v Speaker 2>about the dark charge, We've talked about the dark electron.

668
00:31:27.359 --> 00:31:31.279
<v Speaker 2>It all sounds ominous, but it's really just hidden a

669
00:31:31.400 --> 00:31:33.880
<v Speaker 2>shadow version of our own reality.

670
00:31:34.039 --> 00:31:37.960
<v Speaker 3>And it raised as a final provocative question. If there

671
00:31:38.039 --> 00:31:42.359
<v Speaker 3>is a dark charge and a dark electron, what else

672
00:31:42.400 --> 00:31:43.119
<v Speaker 3>is in the shadow?

673
00:31:43.359 --> 00:31:45.200
<v Speaker 2>Right? If there's a dark version of the electron, is

674
00:31:45.240 --> 00:31:47.640
<v Speaker 2>their dark version of the proton? Is their dark hydrogen?

675
00:31:48.119 --> 00:31:51.000
<v Speaker 3>Are there dark atoms forming dark stars that burn with

676
00:31:51.039 --> 00:31:52.039
<v Speaker 3>a light we can't see.

677
00:31:52.119 --> 00:31:55.160
<v Speaker 2>Are there dark planets orbiting those dark stars with dark life?

678
00:31:55.200 --> 00:31:58.480
<v Speaker 3>It is entirely possible that there is a complex mirrored

679
00:31:58.519 --> 00:32:01.119
<v Speaker 3>structure to the universe that we we cannot interact with

680
00:32:01.519 --> 00:32:04.519
<v Speaker 3>except through gravity and on the very rare occasion when

681
00:32:04.599 --> 00:32:06.519
<v Speaker 3>one of their ancient black holes explodes.

682
00:32:06.720 --> 00:32:09.119
<v Speaker 2>That is a thought to chew on the idea that

683
00:32:09.119 --> 00:32:11.759
<v Speaker 2>we are only seeing half the movie and the other

684
00:32:11.839 --> 00:32:14.319
<v Speaker 2>half is playing out right next to us, all around

685
00:32:14.400 --> 00:32:17.200
<v Speaker 2>us completely invisible, just waiting for a crash to reveal

686
00:32:17.240 --> 00:32:17.839
<v Speaker 2>its existence.

687
00:32:17.920 --> 00:32:20.680
<v Speaker 3>The universe is far stranger than we can possibly imagine.

688
00:32:20.880 --> 00:32:24.200
<v Speaker 2>And on that note, keep looking up. You never know

689
00:32:24.519 --> 00:32:27.519
<v Speaker 2>what might crash into the atmosphere next. Thanks for listening

690
00:32:27.559 --> 00:32:29.160
<v Speaker 2>to this exploration, Stay curious.

691
00:33:05.000 --> 00:33:46.240
<v Speaker 1>Das sche
