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<v Speaker 1>Welcome to the quart Side Quantum Physics Podcast, an exploration

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<v Speaker 1>of the fundamental structure of reality, where quantum laws govern matter, energy,

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<v Speaker 1>and information. Here, uncertainty is a feature, not a flaw,

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<v Speaker 1>and understanding begins at the smallest scales.

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<v Speaker 2>I want you to imagine, just for a second, stepping

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<v Speaker 2>outside on a really crisp, clear night. You look up

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<v Speaker 2>and you see the night sky in all its glory.

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<v Speaker 3>Right, it's completely breathtaking here.

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<v Speaker 2>Yeah, you see the stars twinkling, maybe the faint smudge

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<v Speaker 2>of a distant galaxy, or the glowing dust of the

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<v Speaker 2>Milky Way stretching right across the horizon. It feels incredibly vast,

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<v Speaker 2>it really does. It feels like you are looking at

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<v Speaker 2>the entire universe. Yeah, but here is the mind bending reality.

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<v Speaker 2>Everything you can see, I mean everything emitting light, absorbing light,

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<v Speaker 2>or reflecting light. It's just a tiny microscopic fraction of

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<v Speaker 2>what is actually out there.

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<v Speaker 3>Yeah, it's wild. The vast, overwhelming majority of our universe

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<v Speaker 3>is completely invisible to our eyes and well to our

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<v Speaker 3>telescopes too, completely invisible. Exactly. We only know this unseen

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<v Speaker 3>matter exists because we can observe its gravity pulling on

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<v Speaker 3>the luminous structures, we actually can.

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<v Speaker 2>See, like, we can literally see its effects without seeing it.

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<v Speaker 3>Right. We watch galaxies rotating at speeds that you know,

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<v Speaker 3>frankly you should tear them apart, yet they hold together,

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<v Speaker 3>basically bound by the immense weight of this invisible scaffolding.

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<v Speaker 2>We are talking about dark matter, of course. It's the

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<v Speaker 2>universe's ultimate.

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<v Speaker 3>Ghost, the ultimate ghost, yeah, because it just.

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<v Speaker 2>Doesn't interact with electromagnetism at all. It drifts right through everything,

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<v Speaker 2>and for decades the physics community has been completely obsessed

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<v Speaker 2>with trying to catch it.

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<v Speaker 1>Oh.

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<v Speaker 3>Absolutely, everyone wants to figure out what it is made of,

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<v Speaker 3>and you know, to detect it directly right here on Earth, which.

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<v Speaker 2>Is why we are currently living through this incredible boom

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<v Speaker 2>in quantum technology. Like physicists are building these hyper sensitive,

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<v Speaker 2>cutting edge quantum machines designed specifically to hunt for this

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<v Speaker 2>ghostly matter.

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<v Speaker 3>And that technological leap that's what sets the stage for

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<v Speaker 3>a really fascinating paradise paradox. Yeah, because a groundbreaking new

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<v Speaker 3>study analyzing how these detectors interact with dark matter has

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<v Speaker 3>revealed this profound cosmic irony.

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<v Speaker 2>Okay, I love a good cosmic irony.

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<v Speaker 3>Well, the fundamental quantum nature of dark matter is completely

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<v Speaker 3>fundamentally undetectable to us.

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<v Speaker 2>Wait really, yeah.

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<v Speaker 3>The universe is actively hiding its quantum mechanics from our machines.

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<v Speaker 2>Wow. Okay, so here is where we are going today.

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<v Speaker 2>We're going to explore the mechanics of why the universe

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<v Speaker 2>is burying its quantum secrets, how this massive realization actually works,

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<v Speaker 2>and why surprisingly this seemingly impassable wall is actually brilliant news.

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<v Speaker 3>It really is great news for science.

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<v Speaker 2>But to really grasp why the quantum nature of dark

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<v Speaker 2>matter is playing hide and seek with our most advanced technology,

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<v Speaker 2>we need to talk about what physicists actually think this

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<v Speaker 2>ghost is made of.

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<v Speaker 3>Right, We have to start with the suspects.

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<v Speaker 2>Exactly, because for a long time we've had a roster

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<v Speaker 2>of theoretical candidates.

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<v Speaker 3>We have because dark matter refuses to interact with normal

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<v Speaker 3>matter in any meaningful way, you basically have to build

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<v Speaker 3>theoretical models of particles that fit that extreme ghostly profile.

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<v Speaker 3>And one of the leading theoretical candidates right now is

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<v Speaker 3>a particle called the axion.

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<v Speaker 2>The axion, Okay, I know this is a front runner,

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<v Speaker 2>but how does it differ from the heavy bulky dark

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<v Speaker 2>matter particles people used to theorize about.

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<v Speaker 3>So the axion is what we call an ultra light particle.

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<v Speaker 2>Ultra light How light is ultra light?

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<v Speaker 3>Well, to give you a sense of scale, its mass

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<v Speaker 3>is so vanishingly small that it might be a trillionth

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<v Speaker 3>of a trillionth the mass of a single electron.

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<v Speaker 2>A trillionth of a trillion that's I mean, that's barely

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<v Speaker 2>even a thing exactly.

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<v Speaker 3>Because each individual axion carries almost zero mass. The only

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<v Speaker 3>way they could account for the immense gravitational weight of

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<v Speaker 3>dark matter in our galaxy is if there is an

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<v Speaker 3>unimaginably large number of them.

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<v Speaker 2>Way a completely absurd amount, Right.

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<v Speaker 3>We're talking about a density so high that they just

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<v Speaker 3>permeate every single inch of the universe around us.

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<v Speaker 2>Okay, let's unpack this. Yeah, because trying to visualize a

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<v Speaker 2>swarm of invisible, almost weightless particles making up a quarter

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<v Speaker 2>of the universe is honestly hurting my brain a bit.

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<v Speaker 3>It's definitely not easy to picture.

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<v Speaker 2>So I want to picture this correctly. When scientists model axions,

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<v Speaker 2>they don't treat them like a hail storm of tiny

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<v Speaker 2>individual bullets, do they. They treat them as a classical field.

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<v Speaker 3>Right they do. Yeah, And it really comes down to

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<v Speaker 3>a fundamental principle of quantum mechanics called the Dobroglei.

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<v Speaker 2>Wavelength the de Brogli wavelength. Right.

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<v Speaker 3>In quantum physics, every particle can also be described as

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<v Speaker 3>a wave, and the lighter the particle, the longer its

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<v Speaker 3>wave stretches out.

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<v Speaker 2>Okay, that makes sense. The lighter equals longer.

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<v Speaker 3>Exactly because because the axion is so incredibly light, it's

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<v Speaker 3>quantum wavelength is just huge compared to standard sub atomic particles.

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<v Speaker 2>So you have these massive, stretched out waves, and because

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<v Speaker 2>you need trillions upon trillions of them packed into the

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<v Speaker 2>exact same space just to make up a tiny bit

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<v Speaker 2>of gravity, they all sort of crowd together.

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<v Speaker 3>And when they crowd together, those elongated quantum waves overlap,

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<v Speaker 3>they sync.

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<v Speaker 2>Up, they sink up.

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<v Speaker 3>Yeah. Instead of acting like a bunch of erratic individual

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<v Speaker 3>particles bouncing around, they behave collectively, they just wash over

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<v Speaker 3>the Earth as a single macroscopic.

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<v Speaker 2>Wave, oscillating it as specific frequency.

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<v Speaker 3>Precisely, that smooth, continuous sloshing that is the classical field model.

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<v Speaker 2>I think I've got it. It's like the difference between

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<v Speaker 2>looking at dark matter as a massive invisible ocean current,

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<v Speaker 2>that macroscopic classical field versus you know, focusing on the

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<v Speaker 2>individual microscopic drops of water that make up the current.

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<v Speaker 3>That is a perfect way to look at it.

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<v Speaker 2>So currently we're just constantly swimming in this smooth ocean

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<v Speaker 2>current of dark matter.

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<v Speaker 3>Yeah, that ocean current analogy perfectly captures the classical view,

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<v Speaker 3>and it works flawlessly for predicting how galaxies form and

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<v Speaker 3>how gravity behaves on a large cosmological scale.

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<v Speaker 2>Here's where it gets really interesting, though, because if axioans

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<v Speaker 2>are technically sub atomic particles, you know, these tiny drops

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<v Speaker 2>of water, shouldn't they behave by the bizarre rules of

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<v Speaker 2>quantum mechanics. When we look closely.

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<v Speaker 3>Enough, you would think so.

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<v Speaker 2>Yes. If you zoom in on anything with a powerful

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<v Speaker 2>enough microscope, the smooth illusion usually breaks down, right and

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<v Speaker 2>you see the discrete quantum pieces.

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<v Speaker 3>And that logical leap is the exact foundation of the

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<v Speaker 3>current push to build highly sensitive dark matter detectors.

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<v Speaker 2>Okay, so that's what we're trying to do, right.

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<v Speaker 3>Physicists have developed these instruments called haloscopes taloscopes. Yeah, they

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<v Speaker 3>use incredibly powerful magnetic fields and superconducting quantum sensors. They

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<v Speaker 3>are attempting to coax a single axion to interact with

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<v Speaker 3>the magnetic field and basically canvert into a detectable microwave photon.

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<v Speaker 2>So we're trying to build machines that can detect the

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<v Speaker 2>absolute faintest whispers of energy, the absolute faintest. Yes, we

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<v Speaker 2>basically want the machine to go click when a single

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<v Speaker 2>drop of water from that dark matter ocean hits it.

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<v Speaker 3>Exactly. The scientific community assumed that by utilizing detectors that

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<v Speaker 3>operate on strict quantum principles, we would naturally be able

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<v Speaker 3>to detect the underline, discrete quantum nature of the dark

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<v Speaker 3>matter itself.

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<v Speaker 2>We just expected it to happen, right.

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<v Speaker 3>We anticipated seeing the erratic particle like behavior, those individual

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<v Speaker 3>clicks of quantum interactions you just mentioned.

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<v Speaker 2>And this is where a team of physicists Lion Tao

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<v Speaker 2>Wang and his colleagues from the University of Chicago, Lawrence

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<v Speaker 2>Berkeley National Lab, and UC Berkeley stepped in and realized

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<v Speaker 2>a major piece of the puzzle was simply missing.

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<v Speaker 3>A huge piece.

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<v Speaker 2>Yeah, because we were using all this advanced quantum math

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<v Speaker 2>to engineer the inner workings of the detectors, but researchers

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<v Speaker 2>hadn't actually applied strict quantum mechanics to describe the dark

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<v Speaker 2>matter itself at the exact moment it interacts with the machine.

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<v Speaker 3>Which reveals a really fascinating blind spot in the theoretical framework.

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<v Speaker 2>A huge blind spot.

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<v Speaker 3>Yeah, the models dictating how the detector operates were entirely quantum,

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<v Speaker 3>but the input in a dark matter expected to hit

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<v Speaker 3>the detector was still largely being fed in as a

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<v Speaker 3>smooth classical wave.

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<v Speaker 2>Okay, I really have to push back on the logic

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<v Speaker 2>of the scientific community here.

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<v Speaker 3>Oh, fair enough, go ahead.

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<v Speaker 2>Why would physicists spend decades at like millions of dollars

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<v Speaker 2>building highly sensitive quantum heloscopes without first checking the fundamental

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<v Speaker 2>math to see if the dark matter they are looking

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<v Speaker 2>for actually acts like a quantum particle when it strikes

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<v Speaker 2>the sensor. I know, I know. It feels like building

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<v Speaker 2>an ultra sensitive microphone to record a bat's echo location

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<v Speaker 2>without I don't know, checking if bats actually make noise

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<v Speaker 2>in that frequency.

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<v Speaker 3>It really seems like a massive oversight when you frame

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<v Speaker 3>it that way, but it stems from how theoretical physics

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<v Speaker 3>practically evolves. You mean, well, the classical field model that

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<v Speaker 3>smooth ocean current. It explained all the gravitational effects we

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<v Speaker 3>could observe perfectly.

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<v Speaker 2>Okay, so it worked right.

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<v Speaker 3>So when experimentalists began designing quantum level detectors, they relied

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<v Speaker 3>on a standard assumption. It is incredibly common in physics

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<v Speaker 3>to assume that if you push your magnification deep enough

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<v Speaker 3>into the microscopic realm, the classical limits will naturally break down.

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<v Speaker 2>And the quantum stuff will just sort of pop out exactly.

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<v Speaker 3>They assumed the discrete quantum signatures would just emerge. They

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<v Speaker 3>didn't rigorously calculate the dark matter's quantum state during detection

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<v Speaker 3>because honestly, that assumption just felt mathematically safe.

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<v Speaker 2>Safe, until Wang and his team decided it was time

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<v Speaker 2>to stop assuming and actually run the numbers exactly.

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<v Speaker 3>They wanted to see what a quantum axion would mathematically

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<v Speaker 3>look like to a modern quantum detector.

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<v Speaker 2>So what did they do.

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<v Speaker 3>They built a brand new, entirely quantum mechanical framework from

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<v Speaker 3>the ground up, modeling both the detector and the dark

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<v Speaker 3>matter as interacting quantum entities.

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<v Speaker 2>They put the whole system into the quantum math.

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<v Speaker 3>Right. They set out to mathematically prove whether an experiment

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<v Speaker 3>could distinguish the hidden quantum states, those discrete particle like

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<v Speaker 3>clicks from the continuous, smooth, classical wave state we've always modeled.

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<v Speaker 2>And the findings they publish, which are incredible by the way,

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<v Speaker 2>they found that the intrinsically quantum effects of axions are

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<v Speaker 2>completely fundamentally undetectable.

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<v Speaker 3>Undetectable.

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<v Speaker 2>Yes, when the detector looks at the dark matter, it

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<v Speaker 2>basically only sees the classical.

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<v Speaker 3>Wave, right, The discrete quantum nature just vanishes.

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<v Speaker 2>But why why does a fundamental particle just lose its

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<v Speaker 2>quantum identity like that?

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<v Speaker 3>The disappearance of the quantum nature basically comes down to

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<v Speaker 3>the relationship between the mean and the variance of the

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<v Speaker 3>signal mean invariance.

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<v Speaker 2>Okay, let's break that down.

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<v Speaker 3>So when a detector measures the axion field, it is

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<v Speaker 3>measuring the average strength of the wave over time. That

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<v Speaker 3>is the mean.

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<v Speaker 2>Got it. The average is the mean.

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<v Speaker 3>But the quantum quarks, the individual particle interactions we are

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<v Speaker 3>actually looking for, they live in the variance.

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<v Speaker 2>The variants.

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<v Speaker 3>Yeah, the tiny statistical fluctuations away from that average.

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<v Speaker 2>Okay, so the fluctuations are the discrete.

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<v Speaker 3>Clicks precisely, And there are two major physical factors working

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<v Speaker 3>in tandem here to completely suppress those fluctuations.

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<v Speaker 2>What's the first one?

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<v Speaker 3>First, the sheer weakness of the interaction heavily penalizes our

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<v Speaker 3>ability to see anything other than the massive.

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<v Speaker 2>Average because it's a ghost.

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<v Speaker 3>Right, Because the axion interacts so faintly with the magnetic

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<v Speaker 3>fields in our haloscopes to begin with, the overall signal

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<v Speaker 3>strength is incredibly low. It's super quiet, exactly so to

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<v Speaker 3>see tiny variances inside an already microscopic signal requires just

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<v Speaker 3>an impossible level of precision.

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<v Speaker 2>Wait, earlier we established that there are trillions upon trillions

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<v Speaker 2>of these axions permeating everything, Right, doesn't the sheer volume

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<v Speaker 2>of particles make up for the weak interaction, Like, if

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<v Speaker 2>enough of them are flowing through the detector, shouldn't the

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<v Speaker 2>sheer quantity amplify those little quantum fluctuations.

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<v Speaker 3>See, that is the intuitive assumption, but statistically the exact

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<v Speaker 3>opposite happens.

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<v Speaker 2>The opposite.

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<v Speaker 3>Yeah, the immense density of the axions is actually the

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<v Speaker 3>primary mechanism hiding their quantum nature.

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<v Speaker 2>You're kidding, No, It is an.

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<v Speaker 3>Extreme example of the central limit theorem in statistics.

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<v Speaker 2>The central limit theorem. Okay, let's try to visualize this.

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<v Speaker 2>Imagine you are standing in the middle of a massive stadium, Okay,

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<v Speaker 2>a stadium, and there are one hundred thousand people in

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<v Speaker 2>the stands, and they are all humming the exact same

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<v Speaker 2>continuous note.

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<v Speaker 3>Okay, so the humming represents the mean the macroscopic classical

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<v Speaker 3>dark matter wave rolling over the Earth.

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<v Speaker 2>Right now. In the quantum world, things are a little unpredictable.

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<v Speaker 2>So maybe one person over in section one oh four

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<v Speaker 2>has their voice cracked for a split second. Okay, that

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<v Speaker 2>tiny vocal fluctuation, that little anomaly, That is your quantum variance.

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<v Speaker 2>That's the discrete particle click we want to hear.

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<v Speaker 3>But here's the problem. If you are standing in the

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<v Speaker 3>center of the field holding a microphone, you aren't just

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<v Speaker 3>recording that one person in section one o four.

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<v Speaker 2>You're recording the other ninety nine hundred ninety nine people

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<v Speaker 2>constantly humming that perfect, overwhelming note exactly. The sheer volume

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<v Speaker 2>of the massive crowd completely drowns out the anomaly. The

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<v Speaker 2>massive number of axions hitting the detector means those tiny

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<v Speaker 2>quantum variances just average out into the smooth, continuous roar

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<v Speaker 2>of the classical wave.

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<v Speaker 3>It is physically impossible to hear the voice crack wow

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<v Speaker 3>because the detector is absorbing energy from so many overlapping

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<v Speaker 3>axion waves simultaneously. The quantum fluctuations just smooth themselves over.

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<v Speaker 2>They just blur together, right.

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<v Speaker 3>The mathematics of the wangpaper prove that these quantum signatures

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<v Speaker 3>would only manifest as extremely slight changes to what statisticians

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<v Speaker 3>call higher order statistics.

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<v Speaker 2>Higher order statistics, So we are talking about analyzing the

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<v Speaker 2>shape of the data curve itself.

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<v Speaker 3>Yes, you're looking at things like the skewness of the

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<v Speaker 3>signal or the variance of the variants. You are basically

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<v Speaker 3>trying to find correlations in the noise.

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<v Speaker 2>Of the data, which sounds impossible.

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<v Speaker 3>It essentially is because as the number of particles in

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<v Speaker 3>the field approaches the astronomical numbers required for dark matter,

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<v Speaker 3>the central limit theorem dictates that the variance grows much

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<v Speaker 3>much slower than.

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<v Speaker 2>The mean, So the signal just disappears.

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<v Speaker 3>The quantum signal essentially gets pushed to zero relative to

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<v Speaker 3>the classical wave.

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<v Speaker 2>It becomes a statistical whisper lost in a hurricane.

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

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<v Speaker 3>to the most staggering calculation in their entire paper. With that, well,

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<v Speaker 3>the researchers wanted to know the absolute limit. They assumed

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<v Speaker 3>an optimally designed, theoretically perfect experiment utilizing the absolute pinnacle

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<v Speaker 3>of quantum technology, running without any background noise whatsoever.

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<v Speaker 2>A perfect machine, and to find those higher order statistics,

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<v Speaker 2>you know, to hear that single voice crack in a

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<v Speaker 2>stadium of trillions, How long would this perfect machine need

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<v Speaker 2>to run?

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<v Speaker 3>The experiment would have to run for significantly longer than

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<v Speaker 3>the age of the universe.

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<v Speaker 2>Significantly longer than the thirteen point eight billion years our

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<v Speaker 2>universe has even existed, just to catch a single statistical

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<v Speaker 2>glimpse of a quantum axion doing something quantum that is,

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<v Speaker 2>I mean, that is the universe firmly closing a door.

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<v Speaker 2>It's a hard physical limit, it really is.

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<v Speaker 3>It forces us to confront a profound boundary on what

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<v Speaker 3>is observable in our reality. Yeah, the sheer density required

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<v Speaker 3>for the axion to be dark matter makes us underlying

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<v Speaker 3>quantum mechanics eternally inaccessible to us.

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<v Speaker 2>So what does this all mean? Because learning that an

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<v Speaker 2>experiment would take fourteen billion years sounds like a massive

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<v Speaker 2>crushing failure for physics. If the quantum effects are totally invisible,

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<v Speaker 2>doesn't that render all our highly sensitive quantum heloscopes and

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<v Speaker 2>sensors completely useless.

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<v Speaker 3>It's so crucial to make the distinction between the quantum

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<v Speaker 3>nature of the dark matter and the quantum sensitivity of the.

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<v Speaker 2>Detector, because they aren't the same thing.

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<v Speaker 3>Exactly, because the immediate reaction is often disappointment, like you said,

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<v Speaker 3>But the detectors we are building are not useless at all.

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<v Speaker 2>They aren't.

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<v Speaker 3>No. In fact, establishing this physical limit is a massive victory.

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<v Speaker 3>It clears a dense fog of uncertainty for experimental physicists.

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<v Speaker 2>Okay, how does hitting a fourteen billion year wall help

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<v Speaker 2>the people building the machines?

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<v Speaker 3>It resolves a massive amount of theoretical anxiety.

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<v Speaker 2>In the field, anxiety about what Well.

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<v Speaker 3>Returning to your ocean analogy, our quantum detectors are absolutely

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<v Speaker 3>phenomenal at feeling the push of the massive ocean current.

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<v Speaker 3>The high sensitivity is still required because the classical wave

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<v Speaker 3>itself interacts so weakly with standard matter. Oh, I see,

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<v Speaker 3>we need quantum level precision just to detect the macroscopic wave.

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<v Speaker 2>Ah, so we need the ultrasensitive quantum microphone just to

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<v Speaker 2>hear the crowd humming in the first place.

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<v Speaker 3>Yes, what the study definitively proves is simply that we

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<v Speaker 3>don't need to worry about trying to calibrate our machines

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<v Speaker 3>to isolate the individual drops.

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<v Speaker 2>Of water, because we literally can't.

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<v Speaker 3>Right. Prior to this mathematical proof, physicists were actively debating

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<v Speaker 3>whether intrinsic quantum fluctuations in the dark matter field might

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<v Speaker 3>be skewing our data or creating strange interferences that were

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<v Speaker 3>causing us to miss the signal entirely.

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<v Speaker 2>So people were actually stressing out that the quantum quirks

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<v Speaker 2>of the axions were throwing off the calibration of the.

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<v Speaker 3>Traps exactly, and Wang and his team rigorously demonstrated that

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<v Speaker 3>we can completely ignore those quantum.

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<v Speaker 2>Effects because they average out to zero.

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<v Speaker 3>Because they average out to zero, they will not interfere

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<v Speaker 3>with the classical detection. This validates our historical models so easy.

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<v Speaker 3>It proves that treating axion dark matter as a classical

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<v Speaker 3>macroscopic wavefield works flawlessly on an experimental level, even when

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<v Speaker 3>using quantum instruments. We can trust the classical models when

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<v Speaker 3>we are hunting for the dark matter signal.

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<v Speaker 2>So it's basically the universe giving us permission to simplify

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<v Speaker 2>our approach pretty much. We don't have to account for

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<v Speaker 2>the unpredictable discrete quantum behavior on the dark matter side

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<v Speaker 2>because the universe naturally smooths it out for us. We

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<v Speaker 2>just focus our quantum detectors on catching the big wave.

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<v Speaker 3>It's correctly what signal profile we are looking for.

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<v Speaker 2>Now. That is a huge relief, it is.

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<v Speaker 3>And what makes this realization even more impactful is that

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<v Speaker 3>this averaging out phenomenon isn't restricted to just axions.

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<v Speaker 2>Wait, this applies to other areas of physics.

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<v Speaker 3>It does. The exact same quantum hiding logic applies to

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<v Speaker 3>the detection of gravitational waves.

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<v Speaker 2>Gravitational waves. Oh, that makes perfect sense, because we detect

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<v Speaker 2>gravitational waves using massive interferometers like Lego.

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<v Speaker 3>Right.

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<v Speaker 2>And theoretically gravity is composed of subatomic quantum particles called gravitons.

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<v Speaker 3>Exactly, But a gravitational wave generated by say two black

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<v Speaker 3>holes colliding it contains such an astronomically immense number of

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<v Speaker 3>gravitons that their individual quantum quirks average.

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<v Speaker 2>Out entirely, just like the axions.

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<v Speaker 3>Just like the axiom field, the variance vanishes, and our

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<v Speaker 3>detectors only observe the smooth classical ripple in space time

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<v Speaker 3>virtual limit theorem and forces classical physics on any ultra light,

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<v Speaker 3>highly abundant particle field.

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<v Speaker 2>The bigger the crowd, the smooth than noise.

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<v Speaker 3>I perfectly said, and this mathematical framework provides a real

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<v Speaker 3>launch pad for future engineering.

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<v Speaker 2>How so well.

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<v Speaker 3>The researchers noted that their ongoing work involves developing a

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<v Speaker 3>complete end to end quantum mechanical description of the detection process.

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<v Speaker 2>But I thought we just said we can't see the

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<v Speaker 2>quantum stuff.

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<v Speaker 3>We can't. They aren't doing this to look for the

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<v Speaker 3>impossible quantum quirks of the axion. They are using that

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<v Speaker 3>deep mathematical understanding to search for entirely new quantum techniques

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<v Speaker 3>to build better traps for the classical wave.

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<v Speaker 2>Oh wow.

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<v Speaker 3>They are utilizing the hard limits of what we can't

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<v Speaker 3>see to optimize how we search for what we can see.

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<v Speaker 2>A closed door just forces you to engineer a better window.

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<v Speaker 3>I love that exactly.

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<v Speaker 2>So let's recap the journey here. We started with the

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<v Speaker 2>universe's most delusive ghost, dark matter right. We zoomed in,

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<v Speaker 2>assuming that our incredible new quantum technology would reveal the

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<v Speaker 2>microscope discrete quantum secrets of the axion, But instead we

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<v Speaker 2>found that it's overwhelming abundance moves out all its quantum fluctuations.

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<v Speaker 3>It's all about the averages.

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<v Speaker 2>The central limit theorem basically hides its discrete nature behind

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<v Speaker 2>the roar of the crowd, leaving us with a continuous

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<v Speaker 2>classical wave.

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<v Speaker 3>A wave we are now better equipped to find, precisely

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<v Speaker 3>because we are no longer distracted by the search for

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<v Speaker 3>its quantum.

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00:20:22.759 --> 00:20:25.559
<v Speaker 2>Ripples, which is just so fascinating, and it leaves me

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<v Speaker 2>with this lingering thought. You know what's that? Well, we

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<v Speaker 2>are so used to thinking of the quantum realm as

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<v Speaker 2>the true fundamental base.

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<v Speaker 3>Of reality, right the bottom level of everything.

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<v Speaker 2>Exactly. We assume that if you strip away the illusion

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<v Speaker 2>of our macroscopic world, the microscopic truth is always discrete

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<v Speaker 2>in quantum. But if the most abundant form of matter

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<v Speaker 2>in the universe hides its fundamental quantum nature simply because

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<v Speaker 2>there's too much of it crowding together, it makes you wonder,

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<v Speaker 2>wonder what what other mind bending quantum realities are happening?

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<v Speaker 2>All around you right now, perfectly hidden in plain sight,

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<v Speaker 2>just because the universe is too noisy for you to

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<v Speaker 2>hear them.

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<v Speaker 3>That's a profound point. We navigate a macroscopic reality entirely

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<v Speaker 3>smoothed over by averages. The discrete truths are just buried

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<v Speaker 3>under the weight of sheer numbers.

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<v Speaker 2>Exactly so you know, the next time you step outside

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<v Speaker 2>and look up at that vast night sky and you

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<v Speaker 2>realize you're only seeing a tiny fraction of what is

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<v Speaker 2>out there, remember that even the invisible things have secrets

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<v Speaker 2>they will never tell they really do. The universe is loud,

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<v Speaker 2>it is crowded, and sometimes the most profound mysteries are

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<v Speaker 2>the ones that simply refuses to let us hear
