Latest / The Quark Side - Quantum Physics Podcast / Breakthrough Quantum Material Conducts Electricity With Zero Energy Loss
Transcript
- 0:01Speaker 1: Welcome to the quart Side Quantum Physics Podcast, an exploration
- 0:05Speaker 1: of the fundamental structure of reality, where quantum laws govern matter, energy,
- 0:11Speaker 1: and information. Here, uncertainty is a feature, not a flaw,
- 0:16Speaker 1: and understanding begins at the smallest scales.
- 0:27Speaker 2: Hello everyone, and welcome back. It is Thursday, February twelfth,
- 0:31Speaker 2: twenty twenty six. I want to start today's exploration with
- 0:36Speaker 2: a feeling, a sensation that I guarantee every single one
- 0:39Speaker 2: of you has felt. It's that very specific kind of annoyance.
- 0:43Speaker 2: You're sitting there, maybe you're on a long video call,
- 0:45Speaker 2: or you're rendering a video, or maybe you're just you know,
- 0:48Speaker 2: scrolling on your phone with the brightness all the way up,
- 0:51Speaker 2: and then you feel it, the heat, the heat. Your
- 0:54Speaker 2: phone starts to feel like a hot little brick. Your
- 0:57Speaker 2: laptop fan suddenly kicks in, and it's like a tiny
- 1:01Speaker 2: jet engine is about to take off from your desk.
- 1:03Speaker 3: And your battery percentage just plummets.
- 1:05Speaker 2: It's just nose dives. Yeah, and we treat this as normal.
- 1:07Speaker 2: We just think, oh, my device is working hard. But
- 1:10Speaker 2: when you really stop and think about the physics of it, yeah,
- 1:13Speaker 2: that heat is just failure, isn't it.
- 1:15Speaker 3: It's pure failure. It is waste. In physics, we call
- 1:18Speaker 3: it dissipation. And it is, without a doubt, the single
- 1:21Speaker 3: biggest bottleneck in modern electronics.
- 1:23Speaker 2: So that heat is just energy that's not doing what
- 1:25Speaker 2: I wanted to do exactly.
- 1:27Speaker 3: That heat is literally your batteries, precious energy being turned
- 1:31Speaker 3: into useless themal vibration. Instead of you know, running the
- 1:34Speaker 3: app you just opened, it's just gone.
- 1:36Speaker 2: It's like paying for a gallon of gas and just
- 1:37Speaker 2: pour and have it in the ground before you even
- 1:39Speaker 2: start the car. So the reason we're talking about this,
- 1:42Speaker 2: this very fundamental problem, is because of a paper that
- 1:45Speaker 2: just dropped, I mean just dropped two days ago February tenth,
- 1:48Speaker 2: twenty twenty six in the journal Nature Physics. It's from
- 1:52Speaker 2: a team at the University of Washington led by researcher
- 1:55Speaker 2: name Shaodong Shoo.
- 1:56Speaker 3: And it is a monster of a paper, truly, it
- 1:59Speaker 3: really is.
- 2:00Speaker 2: Because they are claiming to have well essentially solved the
- 2:04Speaker 2: heat problem. Yeah, and not in some small incremental we
- 2:08Speaker 2: made the copper wiring slightly better kind of way.
- 2:11Speaker 3: So this is a fundamental shift.
- 2:13Speaker 2: They have engineered a material where electricity flows with zero
- 2:16Speaker 2: heat loss.
- 2:17Speaker 3: Effectively zero no dissipation. It is the first practical, verified
- 2:23Speaker 3: realization of what's called a dissipationless fractional churn insulator.
- 2:27Speaker 2: Okay, dissipationless fractional churn insulator. That's a mouthful. I feel
- 2:33Speaker 2: like we need to put a giant pin in that
- 2:34Speaker 2: phrase because there is a lot of physics jargon packed
- 2:37Speaker 2: into those forwards. There is will unpack it all you will,
- 2:41Speaker 2: but the headline, the big takeaway here is that they
- 2:44Speaker 2: have created a state of matter where electrons just flow
- 2:48Speaker 2: without resistance. And this is the kicker. They've done it
- 2:52Speaker 2: without the massive, room sized magnetic fields that you usually
- 2:56Speaker 2: need for this kind of quantum magic, and.
- 2:59Speaker 3: That is the holy part of this. We've known about
- 3:01Speaker 3: zero resistance states for a long time, but they always
- 3:04Speaker 3: always required these insane lab conditions that made them totally
- 3:08Speaker 3: impractical for say a microchip. Right this paper, it completely
- 3:12Speaker 3: changes the playing field.
- 3:13Speaker 2: So here's our roadmap for this analysis. Yeah, first we
- 3:16Speaker 2: have to start with the physics of the impossible. You know,
- 3:18Speaker 2: how do you even get electrons to stop bumping into things?
- 3:21Speaker 2: We need to talk about this whole family of quantum hall.
- 3:23Speaker 3: Effects, right, the basics.
- 3:25Speaker 2: Then we need to get into the drama of the engineering,
- 3:28Speaker 2: because this isn't the first time this team has tried this.
- 3:31Speaker 2: They actually took a swing at it back in twenty
- 3:32Speaker 2: twenty three and it didn't quite work.
- 3:35Speaker 3: It was a fascinating failure, though, one of those successful
- 3:38Speaker 3: failures that pushes science forward exactly.
- 3:41Speaker 2: So we'll talk about what went wrong then and the
- 3:44Speaker 2: incredibly specific, almost artisanal changes they made to the crystal
- 3:50Speaker 2: growth and this twisting mechanism to finally make it work
- 3:54Speaker 2: this year.
- 3:54Speaker 3: And then there's the mystery.
- 3:55Speaker 2: Yes, we have to talk about the mystery, because there's
- 3:58Speaker 2: a section at the end of this paper that base
- 4:00Speaker 2: sickly says, Okay, we built it. It works perfectly, but
- 4:02Speaker 2: now it's behaving in a way that makes absolutely no
- 4:04Speaker 2: sense to us.
- 4:05Speaker 3: The thermal activation gap mystery. It's a genuine plot twist
- 4:08Speaker 3: in the data.
- 4:09Speaker 2: So let's dive in section one, the physics of the impossible.
- 4:12Speaker 2: I want you to explain resistance to me, like I'm well,
- 4:16Speaker 2: let's say a smart high school student, Why does my
- 4:19Speaker 2: fane get hot? What is actually happening at the atomic level?
- 4:22Speaker 3: Okay? Sure, To really get resistance, you have to visualize
- 4:25Speaker 3: the life of a single electron trying to get through
- 4:28Speaker 3: a wire. We have this mental picture of electricity as
- 4:32Speaker 3: like water flowing smoothly through a pipe, a.
- 4:34Speaker 2: Nice, clean, continuous stream, right.
- 4:36Speaker 3: But at the atomic level, a copper wire is a
- 4:39Speaker 3: complete nightmare. It is a chaotic, crowded, messy obstacle course.
- 4:44Speaker 2: So the electron isn't just gliding along, not.
- 4:47Speaker 3: At all, not even close. Imagine you're on a highway,
- 4:49Speaker 3: but this highway has no lanes, no speed limit, and
- 4:51Speaker 3: it's just filled with giant, vibrating boulders. The boulders are
- 4:55Speaker 3: the atoms of the copper and the highway is also
- 4:57Speaker 3: full of other cars, which are all the other electrons.
- 5:00Speaker 3: The electron hits the gas that's the voltage you apply,
- 5:03Speaker 3: and it zooms forward, but almost immediately whack it smacks
- 5:08Speaker 3: into an impurity in the metal. It recovers, zooms again, Whack,
- 5:12Speaker 3: it hits an atom that's just vibrating because of temperature.
- 5:15Speaker 3: It recovers again, whack, it collides with another electron.
- 5:18Speaker 2: In every single one of those collisions, that's the heat.
- 5:21Speaker 3: That is the heat precisely in physics we call it scattering.
- 5:25Speaker 3: The electron has kinetic energy, energy of motion. When it
- 5:28Speaker 3: crashes into an atom, it transfers some of that energy,
- 5:31Speaker 3: making the atom vibrate even more violently. That collective violent
- 5:35Speaker 3: vibration of all the atoms is what we feel and
- 5:38Speaker 3: measure as heat. So resistance is really just a measure
- 5:41Speaker 3: of how often your electrons are crashing.
- 5:43Speaker 2: It's friction, It's electrical friction.
- 5:45Speaker 3: It is the exact same principle. Now, for decades, physicists
- 5:48Speaker 3: have been absolutely obsessed with one question, how do we
- 5:52Speaker 3: stop the crashing? How can we build a highway where
- 5:55Speaker 3: it's physically impossible for the electrons to hit anything?
- 5:58Speaker 2: Which sounds well impossible, and that brings us to the
- 6:01Speaker 2: quantum hall effect. Okay, I've heard this term thrown around
- 6:04Speaker 2: usually when people are talking about Nobel prizes, but what
- 6:06Speaker 2: is it actually?
- 6:07Speaker 3: Okay, so let's take that chaotic highway, your normal copper wire.
- 6:12Speaker 3: The first thing we do is we cool it way
- 6:14Speaker 3: way down to near absolute zero, so.
- 6:17Speaker 2: Like a few degrees above the coldest possible temperature in.
- 6:20Speaker 3: The universe exactly. That slows down the vibrating atoms. It's
- 6:24Speaker 3: like clearing most of the boulders off the road. The
- 6:26Speaker 3: road is now much smoother, Okay.
- 6:28Speaker 2: Smooth road. But the electrons the other cars are still there.
- 6:32Speaker 2: They can still crash into each other.
- 6:34Speaker 3: They can. So next we turn on a magnet, and
- 6:37Speaker 3: not just any magnet, a massive magnet. We're talking about
- 6:40Speaker 3: magnetic fields of ten, maybe twenty tesla. These are monsters.
- 6:46Speaker 2: Just for context, a hospital MRI machine is what one
- 6:49Speaker 2: point five or maybe three tesla.
- 6:51Speaker 3: Right, So we were talking about fields that would rip
- 6:54Speaker 3: a metal chair across the room. It's an incredibly strong field. Now,
- 6:58Speaker 3: when you apply that kind of magnetic force perpendicular to
- 7:01Speaker 3: an electron's motion, the electrons path curves.
- 7:05Speaker 2: It doesn't go straight anymore, it can't.
- 7:06Speaker 3: The field forces it to move in a circle. This
- 7:09Speaker 3: is a fundamental principle called cyclotron motion.
- 7:11Speaker 2: So now instead of all the cars driving straight down
- 7:13Speaker 2: the highway, they're all just driving in tiny little circles
- 7:15Speaker 2: in place that doesn't seem very useful.
- 7:17Speaker 3: In the middle of the material, what we call the bulk, yes,
- 7:20Speaker 3: they're just spinning in pla is completely trapped going nowhere.
- 7:22Speaker 3: But think about what happens at the very edge of
- 7:26Speaker 3: the material. Think about the guard rail on the side
- 7:28Speaker 3: of the highway.
- 7:29Speaker 2: Okay, so I'm an electron near the edge. I try
- 7:32Speaker 2: to spin in a circle to my right, but before
- 7:35Speaker 2: I can complete the circle, I hit the wall.
- 7:38Speaker 3: You hit the wall, so you bounce off it. You
- 7:40Speaker 3: try to spin again, You hit the wall again, You
- 7:42Speaker 3: bounce again. What ends up happening is this beautiful skipping motion.
- 7:48Speaker 3: The electrons skip jump along the boundary of the material.
- 7:52Speaker 2: Okay, I can picture that.
- 7:53Speaker 3: And here is the magic part. Because the magnetic field
- 7:56Speaker 3: forces everything to try and turn, let's say to the right,
- 8:00Speaker 3: all the electrons on that one edge are forced to
- 8:02Speaker 3: move in exactly the same direction.
- 8:04Speaker 2: It creates a one way street.
- 8:06Speaker 3: A perfect one way dissipationless super highway. There's no oncoming traffic.
- 8:11Speaker 3: An electron can't scatter backwards because to do that, it
- 8:14Speaker 3: would have to turn left, and the magnetic field makes
- 8:16Speaker 3: that physically impossible.
- 8:17Speaker 2: So it literally can't crash.
- 8:19Speaker 3: It can't. And this is what we call a topological
- 8:21Speaker 3: property topology.
- 8:23Speaker 2: That's the branch of math about shapes. Right, the whole
- 8:26Speaker 2: donut and coffee mug thing exactly.
- 8:28Speaker 3: In topology, a coffee mug and a doughnut are considered
- 8:32Speaker 3: the same because they both have one hole. You can
- 8:34Speaker 3: squish and stretch one into the other. Without tearing it.
- 8:37Speaker 3: In the quantum Hall effect, the flow of electrons along
- 8:41Speaker 3: the edge is protected by the topology of the system's
- 8:44Speaker 3: quantum state.
- 8:45Speaker 2: So even if there's a bump, like a defect in
- 8:48Speaker 2: the material.
- 8:48Speaker 3: The electron just flows smoothly around it. It can't scatter backwards.
- 8:52Speaker 3: It's robust. The resistance along that edge just vanishes. It
- 8:56Speaker 3: goes to zero.
- 8:57Speaker 2: Wow.
- 8:57Speaker 3: And when you measure it, the Hall resistance doesn't increase smoothly.
- 9:00Speaker 3: It goes up in these perfect quantized steps, like a staircase,
- 9:04Speaker 3: step one, step two. It's this beautiful, perfect order emerging
- 9:08Speaker 3: from total chaos.
- 9:10Speaker 2: Okay, so that's the quantum Hall effect that the paper
- 9:13Speaker 2: we're discussing today. It's not just about that. It's about
- 9:15Speaker 2: the fractional quantum Hall effect. And this is where my
- 9:18Speaker 2: brain starts to hurt a little bit. How can you
- 9:20Speaker 2: have a fraction of a step? How on Earth can
- 9:22Speaker 2: you have a fraction of an electron?
- 9:24Speaker 3: This is one of the coolest, most mind bending concepts
- 9:27Speaker 3: in all of physics. And you're right. An electron is
- 9:30Speaker 3: a fundamental particle. It's an elementary particle. You can't take
- 9:33Speaker 3: a tiny knife and slice it into thirds, right, but
- 9:36Speaker 3: you can get a group of electrons to act collectively
- 9:40Speaker 3: as if they are fractional particles.
- 9:41Speaker 2: Okay, explain that what does that even mean?
- 9:44Speaker 3: It all comes down to collective behavior. Think about it
- 9:47Speaker 3: like this. Imagine you're in a crowded room. If everyone
- 9:51Speaker 3: is just milling about randomly, you just have a collection
- 9:53Speaker 3: of individuals. But what if everyone links arms and starts
- 9:57Speaker 3: moving together in a very specific, comp plex braided dance.
- 10:01Speaker 2: Then the crowd itself becomes a thing. The entity is
- 10:04Speaker 2: the pattern of the dance, not the individual person.
- 10:07Speaker 3: That's a perfect way to put it. In the fractional
- 10:09Speaker 3: quantum Hall effect or FQHG, the conditions are so extreme,
- 10:13Speaker 3: the magnetic field is even stronger, the material is even cleaner,
- 10:17Speaker 3: that the electrons can't ignore each other anymore. Their mutual
- 10:20Speaker 3: repulsion becomes the dominant force. There's force to interact intensely.
- 10:25Speaker 3: They organize themselves into this incredibly delicate correlated quantum liquid.
- 10:30Speaker 2: A liquid made of electrons, a.
- 10:32Speaker 3: Quantum liquid, yes, And the tiny ripples in this liquid,
- 10:36Speaker 3: the little vortices or excitations they behave mathematically exactly like
- 10:42Speaker 3: particles with a fractional charge, like one third of an electrons.
- 10:46Speaker 2: Chart or two thirds, so we're not splitting the particle.
- 10:49Speaker 2: We are creating a quasi particle out of the collective
- 10:53Speaker 2: dance of the crowd.
- 10:54Speaker 3: You've nailed it. That's the can reuse. These are quasi particles.
- 10:58Speaker 3: They're often called enians, and they are incredibly important for
- 11:02Speaker 3: the future of technology. Why because they're stable, because they're topological.
- 11:05Speaker 3: They're born out of this global collective dance, which makes
- 11:08Speaker 3: them super robust. If you poke one individual electron, the
- 11:13Speaker 3: overall dance just continues. The fractional quasi particle remains intact.
- 11:17Speaker 2: And this is the link to quantum computing, right, This
- 11:20Speaker 2: is why everyone gets so excited.
- 11:21Speaker 3: This is the holy grail of quantum computing. A normal
- 11:24Speaker 3: quantum bit aquibit is ridiculously fragile. The slightest vibration a
- 11:29Speaker 3: little bit of heat, and the quantum information is lost.
- 11:32Speaker 3: It's called decoherence. But if you could build a quibit
- 11:35Speaker 3: out of these fractional stakes bulletproof, it would be topologically protected.
- 11:39Speaker 3: The idea is you could literally braid these quasi particles
- 11:43Speaker 3: around each other to perform calculations, and because the information
- 11:47Speaker 3: is stored in the global topology of the braid local
- 11:50Speaker 3: noise couldn't mess it up.
- 11:51Speaker 2: So a fault tolerant quantum computer.
- 11:54Speaker 3: The dream of a fault tolerant quantum computer.
- 11:56Speaker 2: Yes, okay, so let's just recap the stakes here. We
- 11:59Speaker 2: want this fractional quantum hall state because it's dissipationless, no heat,
- 12:04Speaker 2: and it's topologically stable, which is great for computing. But
- 12:07Speaker 2: there has always been this one giant show stoffing catch
- 12:12Speaker 2: the magnet, the giant room size credit card erasing magnet.
- 12:16Speaker 3: Exactly, you cannot put a fifteen tesla magnet inside your iPhone.
- 12:19Speaker 3: It's just not going to happen. So for forty years
- 12:21Speaker 3: this has been this beautiful laboratory curiosity. Look what amazing
- 12:26Speaker 3: things nature can do. Moment, but not a Let's build
- 12:28Speaker 3: a product with this moment.
- 12:29Speaker 2: Which brings us to the churn insulator. This is the
- 12:32Speaker 2: proposed solution to the magnet problem, at least in theory.
- 12:35Speaker 3: In theory, yes, a churn insulator is a type of
- 12:39Speaker 3: material that, through its own internal quantum mechanics, essentially creates
- 12:44Speaker 3: its own magnetic environment. The specific arrangement of the atoms
- 12:48Speaker 3: and the way the electrons wave functions interact. It generates
- 12:51Speaker 3: an effective magnetic field.
- 12:53Speaker 2: So it's like virtual reality for electrons. They think they're
- 12:57Speaker 2: in a massive magnetic field. Yeah, so they start doing
- 12:59Speaker 2: the quant the Hall dance even though there's no external magnet.
- 13:02Speaker 3: That is a fantastic analogy. Yes, a property of the
- 13:06Speaker 3: material's electronic structure called Barry curvature acts just like a
- 13:10Speaker 3: magnetic field. So you get the protected edge states, you
- 13:12Speaker 3: get the one way super highway, you get the zero
- 13:15Speaker 3: resistance all at zero external magnetic field.
- 13:19Speaker 2: And that's the anomalous part of the name quantum anomalous
- 13:21Speaker 2: Hall effect anomalists because the magnet is missing.
- 13:24Speaker 3: Correct. So bringing it all back to this week's paper,
- 13:27Speaker 3: Sue and his team have been chasing the ultimate prize,
- 13:30Speaker 3: not just a quantum anomalous Hall effect, but a fractional
- 13:33Speaker 3: quantum anomalist Hall effect.
- 13:35Speaker 2: Right. They want the material that has the fractional charges,
- 13:38Speaker 2: the one third steps and works with no magnet.
- 13:41Speaker 3: That is the goal, a dissipationless fractional churn insulator.
- 13:45Speaker 2: And they actually tried to publish this before, didn't they.
- 13:47Speaker 2: I was looking at the timeline back in twenty twenty three.
- 13:49Speaker 2: They had a paper that claimed they found it, but
- 13:52Speaker 2: looking back now, it seems like that was a close
- 13:55Speaker 2: but no cigar moment.
- 13:56Speaker 3: Oh, it was a heartbreaking moment for the field. Honestly, Ujin,
- 14:00Speaker 3: you're a scientist. You spend years designing and building this
- 14:03Speaker 3: incredibly complex device. Cool it down. You measure it, and
- 14:07Speaker 3: you see it. You see the plateau and the Hall
- 14:10Speaker 3: resistance that screams one third fractional charges here.
- 14:14Speaker 2: You pop the fambage, you.
- 14:15Speaker 3: Pop the champagne. But then then you look at the
- 14:18Speaker 3: other measurement. You measure the longitudinal resistance.
- 14:21Speaker 2: Okay, remind us again. Hall resistance is the measurement across
- 14:24Speaker 2: the current, the one that gives you the nice steps.
- 14:25Speaker 3: Longitudinal resistance is it's the resistance along the direction of
- 14:29Speaker 3: the current flow. In a perfect dissipationless state. This number
- 14:34Speaker 3: should be zero, a flat line at the bottom of
- 14:37Speaker 3: your graph, no question.
- 14:38Speaker 2: And in their twenty twenty three experiment.
- 14:40Speaker 3: It wasn't zero. It was something. It was small, but
- 14:43Speaker 3: it was definitely measurably not zero.
- 14:46Speaker 2: So the pipe was leaky.
- 14:47Speaker 3: The pipe was leaky, exactly. They had the right general idea.
- 14:50Speaker 3: The electrons were trying to do the collective dance, but
- 14:53Speaker 3: the dance floor was too messy. They were tripping. They
- 14:56Speaker 3: were bumping into things. Energy was leaking out as heat.
- 14:59Speaker 3: It was not dipationless.
- 15:00Speaker 2: I imagine for a physicist in this field, kind of
- 15:03Speaker 2: dissipationless is like being kind of pregnant. It's a binary thing.
- 15:08Speaker 2: It's either zero or it isn't.
- 15:10Speaker 3: Absolutely in this game, if there's any resistance, it means
- 15:13Speaker 3: the topological protection is broken. It means there are what
- 15:17Speaker 3: we call dissipative channels that the electrons are finding. So
- 15:21Speaker 3: for the last three years, big question in the community
- 15:23Speaker 3: hasn't been is the theory wrong? The question has been
- 15:27Speaker 3: is our sample just too dirty?
- 15:28Speaker 2: Too dirty? I love that we're talking about the most
- 15:31Speaker 2: esoteric quantum mechanics imaginable, and the problem comes down to
- 15:34Speaker 2: basically dirt.
- 15:36Speaker 3: Atomic scale dirt disorder in the crystal.
- 15:38Speaker 2: Okay, so let's move on to that section three engineering
- 15:42Speaker 2: the solution. How did they clean up the dirt? Because
- 15:45Speaker 2: this is where the story shifts from abstract physics to
- 15:48Speaker 2: really hardcore hands on material science. It really does They
- 15:52Speaker 2: used of material called molybdenum detailur ride or multi two
- 15:55Speaker 2: to two? Why this particular stuff? Why not good Old's silk?
- 16:00Speaker 3: Well, silicon is great for what it does, but it's
- 16:02Speaker 3: electronically kind of boring for this kind of work. MOTI
- 16:06Speaker 3: two to two is part of a class of materials
- 16:08Speaker 3: called transition metal decocogenis or TMDs, And the key thing
- 16:13Speaker 3: about them is that they're layered materials like graphite. You
- 16:16Speaker 3: can literally peel them apart into sheets that are just
- 16:19Speaker 3: a few atoms thick.
- 16:21Speaker 2: So they're effectively two dimensional.
- 16:22Speaker 3: Exactly two D. And the real magic happens when you
- 16:25Speaker 3: take two of these atomically thin sheets and stack them
- 16:28Speaker 3: on top of each other. But you don't just stack
- 16:31Speaker 3: them like two pieces of paper. You twist them.
- 16:33Speaker 2: This is the famous tristronics.
- 16:35Speaker 3: This is twistronics. It sounds like a nineteen eighties dance move,
- 16:38Speaker 3: but it's one of the hottest fields in physics right now.
- 16:41Speaker 3: When you rotate that top layer relative to the bottom
- 16:43Speaker 3: layer by a very specific tiny angle, in this case
- 16:46Speaker 3: somewhere around three degrees, you create something called a more pattern.
- 16:49Speaker 2: I've seen this in the real world. If you look
- 16:51Speaker 2: through two layers of fine mash, like two window screens,
- 16:55Speaker 2: and you move your head, you see these weird, bigger,
- 16:59Speaker 2: wavy patterns that aren't in the original mesh.
- 17:01Speaker 3: Yes, that is an optical more pattern. In these stacked crystals,
- 17:06Speaker 3: the twisting creates an electronic maree pattern. It's a giant
- 17:11Speaker 3: periodic superlattice for the electrons, and this pattern fundamentally changes
- 17:16Speaker 3: the energy landscape they live in. It creates what physicists
- 17:20Speaker 3: call flat bands.
- 17:21Speaker 2: Okay, flat bands, This feels like a key concept. We
- 17:25Speaker 2: really need to nail down. What does a flat energy
- 17:27Speaker 2: band do to an electron? Right?
- 17:30Speaker 3: So, in a normal material, the energy band is curved.
- 17:33Speaker 3: That means an electron can have a wide range of
- 17:35Speaker 3: kinetic energies. It can zoom around at all.
- 17:37Speaker 2: Different speeds, free to move.
- 17:38Speaker 3: It's free to move, and it's kinetic energy dominates its life.
- 17:41Speaker 3: It's running around so fast that it doesn't really have
- 17:43Speaker 3: time to interact or care about the electron next to it.
- 17:46Speaker 2: Too busy running to chat with the neighbors.
- 17:48Speaker 3: Exactly. But in a flat band, the more superlattice essentially
- 17:52Speaker 3: traps the electrons. It dramatically quenches or flattens their kinetic energy.
- 17:57Speaker 3: They slow down to a crawl. They all have roughly
- 17:59Speaker 3: the same very low energy, and because they aren't zooming
- 18:03Speaker 3: around anymore, suddenly the most important force in their life
- 18:06Speaker 3: isn't their own speed, it's the electrostatic repulsion from all
- 18:10Speaker 3: their neighbors.
- 18:11Speaker 2: The chat with the neighbors becomes the loudest thing in
- 18:13Speaker 2: the room.
- 18:14Speaker 3: The interaction energy becomes dominant, and that is the absolute
- 18:18Speaker 3: prerequisite for the fractional quantum hall state. You need strong
- 18:22Speaker 3: interactions to force the electrons into that collective correlated dance.
- 18:27Speaker 3: The twist creates the flat band, and the flat band
- 18:30Speaker 3: turns on the interactions.
- 18:31Speaker 2: Okay, so they knew they need a twisted mo call
- 18:32Speaker 2: two too. Back in twenty twenty three, they had that recipe.
- 18:35Speaker 2: So what change between then and now? What was the
- 18:38Speaker 2: big breakthrough?
- 18:39Speaker 3: It was two things. First, they realized their starting ingredients,
- 18:42Speaker 3: the crystals themselves, just weren't good enough. Even though they
- 18:45Speaker 3: looked perfect under a normal microscope at the atomic level,
- 18:48Speaker 3: they were full of defects the dirt. So they changed
- 18:51Speaker 3: the recipe for how they grew the crystals. And this
- 18:54Speaker 3: is where we have to give huge credit to the
- 18:56Speaker 3: materials scientists on the team, specifically Ginhachu post doc Chohwehu.
- 19:02Speaker 3: They switch to a different growth method called horizontal flux growth.
- 19:06Speaker 2: How is that different from the usual way they make
- 19:08Speaker 2: these things?
- 19:08Speaker 3: Well, the more common way is something called chemical vapor transport.
- 19:12Speaker 3: You basically heat up the raw powder, it turns into
- 19:14Speaker 3: a gas, It drifts down a tube to a cooler spot,
- 19:17Speaker 3: and it crystallizes on a surface. It's fast and it's
- 19:20Speaker 3: pretty efficient, but it's a bit chaotic. Atoms can kind
- 19:24Speaker 3: of slam into place. Sometimes they land in the wrong spot,
- 19:27Speaker 3: creating a defect.
- 19:28Speaker 2: It sounds like the fast food version of crystal growth.
- 19:31Speaker 3: That's not a bad analogy. Horizontal flex growth is the
- 19:34Speaker 3: slow cooked, artisanal, farm to table version. You dissolve the
- 19:38Speaker 3: raw molybdenum and tellurium powder and a molten solvent, a
- 19:41Speaker 3: liquid salt called a flux. It's a big liquid bath,
- 19:44Speaker 3: and then you cool that entire bath down incredibly slowly.
- 19:47Speaker 3: We are talking fractions of a degree over many hours
- 19:50Speaker 3: or even days.
- 19:51Speaker 2: It's like making perfectly clear ice for a fancy cocktail.
- 19:54Speaker 2: If you freeze water really fast, it gets cloudy and
- 19:58Speaker 2: full of imperfections. If you freeze is it super super slowly,
- 20:01Speaker 2: it comes out crystal clear.
- 20:03Speaker 3: That is the perfect analogy. By cooling it so slowly
- 20:07Speaker 3: that atoms have time to find their absolute lowest energy position,
- 20:11Speaker 3: they can wiggle around and slot themselves perfectly into the
- 20:14Speaker 3: crystal lattice, no vacancies, no misaligned atoms, just perfection.
- 20:20Speaker 2: And did it actually make a difference in the final product.
- 20:22Speaker 3: A monumental difference. They measured a property called charge carrier mobility,
- 20:26Speaker 3: which is basically a measure of how easily electrons can
- 20:29Speaker 3: move through the material without scattering. It's a proxy for
- 20:32Speaker 3: crystal quality. It increased by more than an order of magnitude,
- 20:36Speaker 3: more than ten times better than the crystals they were
- 20:38Speaker 3: using in twenty twenty three.
- 20:40Speaker 2: Wow. All from just being more patient during the growth process.
- 20:43Speaker 3: All from improving the fundamental ingredients. But that was only
- 20:46Speaker 3: half the battle. You can have a perfect, flawless crystal,
- 20:49Speaker 3: but you still have to perform the twist and the
- 20:52Speaker 3: act of peeling, cutting and stacking these three atom thick
- 20:55Speaker 3: layers is well, it's violent.
- 20:58Speaker 2: I can't even imagine trying to twist some thing that
- 21:00Speaker 2: thin without getting wrinkles and folds all over it.
- 21:02Speaker 3: It's an absolute nightmare. And this was the second major
- 21:05Speaker 3: problem in twenty twenty three twist angle disorder. Imagine you
- 21:09Speaker 3: need that magic more pattern, which requires say exactly three
- 21:14Speaker 3: point seven degrees of twist. But in the twenty twenty
- 21:17Speaker 3: three devices, the twist angle wasn't uniform across the whole sample.
- 21:20Speaker 3: One corner might have been at three point six degrees,
- 21:23Speaker 3: the middle at three point seven, and the other corner at
- 21:25Speaker 3: three point eight.
- 21:26Speaker 2: So the flat band isn't actually flat everywhere it's warped.
- 21:29Speaker 3: It's warped. The physics changes from one spot to the next.
- 21:33Speaker 3: So an electron moving across the device hits these patches
- 21:36Speaker 3: of the wrong angle and it scatters. It breaks the magic,
- 21:38Speaker 3: it ruins the topological protection.
- 21:40Speaker 2: So how did they iron out the wrinkles? Literally?
- 21:42Speaker 3: A student on the team he on June Park gets
- 21:45Speaker 3: the credit here. They refine the fabrication technique. They developed
- 21:47Speaker 3: a new stamping method that uses specific polymers to handle
- 21:50Speaker 3: the layers, reducing mechanical stress and ensuring the tension is
- 21:54Speaker 3: perfectly uniform as the pop layer is laid down.
- 21:56Speaker 2: So, okay, let's put it all together. They have the
- 21:59Speaker 2: slow frozen eyes, ice perfect crystal, and they have the
- 22:02Speaker 2: perfectly ironed out uniform twist. This is the twenty twenty
- 22:06Speaker 2: six device. The moment of truth arrives.
- 22:09Speaker 3: The moment of truth they put the new device in
- 22:12Speaker 3: the cryostat, they cool it down to base temperature just
- 22:15Speaker 3: millikelvin above absolute zero. They apply the gate voltage to
- 22:19Speaker 3: tune the electron density to exactly two thirds filling.
- 22:23Speaker 2: Why two thirds specifically.
- 22:25Speaker 3: That just happens to be one of the known sweet
- 22:27Speaker 3: spots where these fractional states are predicted to be most stable.
- 22:30Speaker 3: It means, for every three units of magnetic flux in
- 22:33Speaker 3: the Maire super lattice, you have two electrons. It's a
- 22:36Speaker 3: particular stable configuration for the dance.
- 22:39Speaker 2: Okay, two thirds filling. They flip the switch, they start
- 22:41Speaker 2: measuring the resistance.
- 22:42Speaker 3: What happens, The hall resistance jumps up and forms a
- 22:45Speaker 3: perfect quantized placateau, exactly where theory says the two thirds
- 22:50Speaker 3: fractional state should be. That's the good news, same.
- 22:52Speaker 2: As twenty twenty three so far. But what about the
- 22:54Speaker 2: other one, the longitudinal resistance, the heat loss.
- 22:57Speaker 3: It drops to zero, a flat line, fixed flat line.
- 23:01Speaker 3: It vanishes into the noise floor of their measurement equipment.
- 23:05Speaker 3: In the twenty twenty three paper, there was a clear bump,
- 23:08Speaker 3: a peak of resistance there. In the twenty twenty six paper,
- 23:12Speaker 3: it is a beautiful flat line at.
- 23:15Speaker 2: Zero they did it. A dissipationless fractional churn insulator.
- 23:18Speaker 3: They did it, and the significance of this really cannot
- 23:21Speaker 3: be overstated. They have proven definitively that you do not
- 23:25Speaker 3: need an external magnetic field to get this exotic quantum state.
- 23:30Speaker 3: They've proven that the key variable was always material quality.
- 23:34Speaker 2: It validates the entire field of twistronics completely.
- 23:37Speaker 3: It shows that by engineering these more a patterns, we
- 23:40Speaker 3: can create and control some of the most bizarre and
- 23:43Speaker 3: wonderful phases of matter imaginable.
- 23:45Speaker 2: So if I'm a listener at home, I'm probably asking, Okay,
- 23:47Speaker 2: this is super cool physics, but when does this get
- 23:49Speaker 2: into my laptop and stop it from burning my legs?
- 23:51Speaker 3: Well, we should be clear there are still some major hurdles.
- 23:53Speaker 3: The biggest one is temperature.
- 23:55Speaker 2: Right, this is still all happening at near absolute zero.
- 23:57Speaker 3: It is we are not at room temperature yet, but
- 24:00Speaker 3: the size of the energy gap they measured is promising.
- 24:04Speaker 3: It suggests that with further improvements we could push that
- 24:07Speaker 3: operating temperature up. But the more immediate application isn't about
- 24:11Speaker 3: power lines or laptops, not yet.
- 24:13Speaker 2: It's the quantum computer.
- 24:15Speaker 3: It's the quantum computer. Remember the braiding the enions.
- 24:18Speaker 2: The topologically protected quivots.
- 24:20Speaker 3: Yes, now that we have a physical platform where these
- 24:24Speaker 3: enians demonstrably exist without needing a giant magnet, we can
- 24:28Speaker 3: start to actually design circuits. You could, in principle, etch
- 24:32Speaker 3: tiny pathways on this Maditude two chip and use electric
- 24:35Speaker 3: fields to shuttle these fractional quasi particles around, braid them
- 24:40Speaker 3: around each other, and perform a computation.
- 24:42Speaker 2: A computation that doesn't just collapse into dust when you
- 24:44Speaker 2: look at.
- 24:44Speaker 3: It's funny exactly. This transforms topological quantum computing from a
- 24:48Speaker 3: beautiful theory on a blackboard into a tangible hardware platform.
- 24:52Speaker 3: It's a chip, it exists, it's sitting in a lab
- 24:54Speaker 3: in Seattle right now.
- 24:55Speaker 2: That is just incredible butt. And there's always a butt
- 24:58Speaker 2: in these big discovery stories. As I was reading through
- 25:00Speaker 2: the notes here, there's a section labeled the scientific mystery.
- 25:04Speaker 3: Ah. Yes, the thermal activation Gap.
- 25:06Speaker 2: It sounds like the title of a Robert Ludlam thriller,
- 25:09Speaker 2: The thermal activation Gap.
- 25:11Speaker 3: It is a thriller, at least for the condensed matter theorists,
- 25:14Speaker 3: because what they found when they dug deeple into the
- 25:16Speaker 3: data makes absolutely no sense. Based on the old rules
- 25:20Speaker 3: of the game.
- 25:21Speaker 2: So set the scene for us. They have the device,
- 25:23Speaker 2: it's working, zero resistance. The champagne has been popped, and
- 25:28Speaker 2: then they decide to just mess with it.
- 25:30Speaker 3: Scientists always mess with it, that's the job. They asked
- 25:33Speaker 3: a very logical question. Okay, this state is perfect at
- 25:36Speaker 3: zero magnetic field, but what happens if we add a
- 25:39Speaker 3: small magnetic field?
- 25:40Speaker 2: Now, based on everything we just talked about with the
- 25:42Speaker 2: original quantum Hall effect, the magnet is the friend. The
- 25:46Speaker 2: magnet is what creates the state in the first place,
- 25:49Speaker 2: So adding more magnet should make the state even stronger, right,
- 25:53Speaker 2: more robust.
- 25:54Speaker 3: That is exactly the intuition everyone had in a standard
- 25:57Speaker 3: fractional quantum Hall system in say alium arsenide, if you
- 26:01Speaker 3: increase the magnetic field, you increase the gap.
- 26:03Speaker 2: Okay, define gap for us again quickly. Yeah, the thermal
- 26:06Speaker 2: activation gap.
- 26:07Speaker 1: Right.
- 26:08Speaker 3: Think of the gap as the width of a moat
- 26:10Speaker 3: protecting a castle. Inside the castle, all the electrons are
- 26:14Speaker 3: safe and sound in their perfect fractional state. Outside the
- 26:18Speaker 3: moat is chaos. To destroy the state, an enemy like
- 26:22Speaker 3: thermal energy has to kick an electron all the way
- 26:25Speaker 3: across the moat.
- 26:26Speaker 2: So a wider moat, a larger energy gap is better. Yeah,
- 26:29Speaker 2: it means the castle is more secure, the state is
- 26:31Speaker 2: more stable.
- 26:32Speaker 3: Precisely, so, they turn on the magnetic field, expecting the
- 26:35Speaker 3: moat to get wider. It got narrower.
- 26:37Speaker 2: It shrank. The magnet made the state weak.
- 26:39Speaker 3: It collapsed. As they slowly cranked up the magnetic field
- 26:43Speaker 3: from zero, the thermal activation gap dropped rapidly. It became
- 26:47Speaker 3: easier to destroy the state. The magnet, their old friend
- 26:50Speaker 3: was actively attacking the stability of this new state.
- 26:53Speaker 2: That is completely backwards from how it's supposed to work.
- 26:56Speaker 3: It is profoundly counterintuitive. There's a line in the paper
- 26:59Speaker 3: where you and the team right to our surprise, which
- 27:02Speaker 3: is you know, scientists code for we were completely baffled.
- 27:05Speaker 3: And this makes no sense. The gap decreased quickly and
- 27:07Speaker 3: then eventually plateaued at a lower value.
- 27:10Speaker 2: So what is the theory. Why if the magnet is
- 27:13Speaker 2: supposed to help, why is it hurting. Here?
- 27:16Speaker 3: The leading hypothesis, and it is just a hypothesis at
- 27:19Speaker 3: this point, involves a kind of civil war inside the
- 27:23Speaker 3: quantum state itself.
- 27:24Speaker 2: A civil war, yes.
- 27:25Speaker 3: A competition between different quantum properties of the electrons. In
- 27:30Speaker 3: these TMD materials, electrons don't just have charge and spin
- 27:34Speaker 3: up or down. They also have another property called valley valley.
- 27:37Speaker 2: What's that.
- 27:38Speaker 3: In the momentum energy landscape of the crystal, there are
- 27:40Speaker 3: two distinct lowest energy valleys where electrons can live. They're
- 27:44Speaker 3: called the K and K prime valleys. You can think
- 27:47Speaker 3: of it as another quantum number, like another flavor of spin.
- 27:50Speaker 2: So electrons have spin and they have flavor basically. Yes.
- 27:53Speaker 3: Now, the magnetic field is very good at one thing.
- 27:56Speaker 3: It loves to align spin. A magnetic field wants all
- 27:58Speaker 3: the electrons spins to point in one direction. That's the Zeman effect.
- 28:01Speaker 2: Okay, that makes sense. It's aligning all the little internal magnets, right.
- 28:05Speaker 3: But the theorists think that the stability of the fractional
- 28:09Speaker 3: state in this specific twisted material might depend on a
- 28:13Speaker 3: very particular arrangement of the valleys. It might want the
- 28:16Speaker 3: valleys to be polarized or mixed in a certain way
- 28:19Speaker 3: that has nothing to do with spin.
- 28:20Speaker 2: And the magnet comes in and messes up that valley
- 28:23Speaker 2: arrangement exactly.
- 28:23Speaker 3: The magnet storms in and says, attention, everyone, aligned by
- 28:26Speaker 3: your spin. But the delicate fractional state says no, wait,
- 28:31Speaker 3: we need to be aligned by our valley to maintain
- 28:33Speaker 3: this collective dance. The two orders are competing. The magnet
- 28:37Speaker 3: is forcing the system into a spin configuration that is
- 28:41Speaker 3: not the optimal configuration for the valley based fractional state.
- 28:45Speaker 2: So the mote shrinks because the very foundation of the
- 28:48Speaker 2: castle is shaking from this internal conflict.
- 28:50Speaker 3: That is a brilliant way to put it. The shrinking
- 28:52Speaker 3: gap is the experimental evidence that the topology of this
- 28:55Speaker 3: new state is much more complex and richer than the
- 28:58Speaker 3: simple quantum hollow effect. It's born from this weird interplay
- 29:02Speaker 3: of spin, valley and the more physics.
- 29:05Speaker 2: So does this new mystery Does it ruin the discovery
- 29:09Speaker 2: at all?
- 29:10Speaker 3: Not at all. In many ways, it makes it even
- 29:12Speaker 3: more exciting. It's a giant sign post that says new
- 29:15Speaker 3: physics here. It means we don't fully understand what we've created,
- 29:19Speaker 3: and that's the best place to be in science.
- 29:21Speaker 2: It's not a bug, it's a feature.
- 29:23Speaker 3: It's a new discovery that's come along for the ride.
- 29:26Speaker 3: It gives us a new knob to turn and a
- 29:28Speaker 3: new puzzle to solve.
- 29:29Speaker 2: This brings us to the final section the future outlook,
- 29:33Speaker 2: Shaodong Shoe seems incredibly optimistic. In the paper's conclusion, he
- 29:37Speaker 2: has this great quote, the quantum hall community has made
- 29:41Speaker 2: repeated breakthroughs by improving sample quality over the last forty years.
- 29:45Speaker 3: That's the clean lens philosophy of science.
- 29:48Speaker 2: Explain what you mean by that.
- 29:49Speaker 3: Think of early astronomers looking at the sky through a dirty,
- 29:52Speaker 3: low quality telescope. You see a faint, fuzzy blur. You
- 29:56Speaker 3: might think that blur is a single star. But then
- 29:58Speaker 3: you spend years grinding a better lens, making it cleaner
- 30:02Speaker 3: and more perfect. Okay, you look through the new clean
- 30:05Speaker 3: lens and you realize that blaur wasn't a star at all.
- 30:08Speaker 3: It was an entire galaxy, or it was binary star system.
- 30:11Speaker 3: The dirt in your instrument was hiding the true, more
- 30:14Speaker 3: complex reality.
- 30:16Speaker 2: The dirt hides the details.
- 30:18Speaker 3: For forty years, the atomic scale, dirt and disorder in
- 30:21Speaker 3: our materials has been hiding the true bizarre nature of
- 30:25Speaker 3: interacting electrons. As we clean the lens with these incredible
- 30:29Speaker 3: techniques like horizontal flux growth and low disorder fabrication, we
- 30:34Speaker 3: aren't just making things more efficient, We are revealing new
- 30:37Speaker 3: laws of physics that were hidden in the noise.
- 30:40Speaker 2: Zoo follows that up by saying, we hope that the
- 30:42Speaker 2: progress on this new platform will be even faster.
- 30:45Speaker 3: And I think he's right to be optimistic, because now
- 30:47Speaker 3: we have a recipe. It's not a mystery anymore. We
- 30:49Speaker 3: know the key ingredients. High purity MOTI two two, the
- 30:52Speaker 3: flux growth method, the low disorder twist. Any lab in
- 30:55Speaker 3: the world with the right equipment can now start making
- 30:57Speaker 3: these high quality devices and exploring.
- 31:00Speaker 2: So the floodgates are about to open.
- 31:01Speaker 3: People can try different twist angles, different layer fominations, different
- 31:05Speaker 3: TMD materials. It really feels like we are standing on
- 31:08Speaker 3: the beach of a new continent and we've just figured
- 31:10Speaker 3: out how to build the boats.
- 31:11Speaker 2: I want to circle all the way back to where
- 31:13Speaker 2: we started this conversation. That hot phone in your pocket,
- 31:16Speaker 2: that roaring data center.
- 31:17Speaker 3: The radiator world we live in.
- 31:19Speaker 2: It really feels like we are living in the steam
- 31:22Speaker 2: age of computing. It's loud, it's hot, it's incredibly inefficient.
- 31:26Speaker 3: We absolutely are. We are brute forcing electrons through solid
- 31:29Speaker 3: rock and just dealing with the heat as a waste product.
- 31:32Speaker 2: In this research, this dissipationless fractional churn insulator. This feels
- 31:38Speaker 2: like the first real glimpse of the solid state silent electric.
- 31:43Speaker 3: Future it is. It's a future where electrical current flows
- 31:46Speaker 3: like a superfluid, where heat becomes an engineering choice, not
- 31:50Speaker 3: an inevitable byproduct, where quantum information isn't stored on a material,
- 31:55Speaker 3: but is braided into the very fabric of the material itself.
- 31:59Speaker 2: It's just mind blowing stuff, and the fact that this
- 32:01Speaker 2: is happening now in twenty twenty six makes me incredibly
- 32:04Speaker 2: excited to see what the landscape looks like by twenty thirty.
- 32:07Speaker 3: The pace of discovery here is just breathtaking.
- 32:10Speaker 2: I think I want to leave our listener with one
- 32:11Speaker 2: final thought, tom all over. We often look for the
- 32:13Speaker 2: next big thing in a new app or a new
- 32:15Speaker 2: gadget design, but sometimes the biggest revolutions are completely invisible.
- 32:20Speaker 2: They're happening at the atomic scale inside a tiny flake
- 32:23Speaker 2: of crystal that has been twisted just right.
- 32:25Speaker 3: The twist is the key.
- 32:27Speaker 2: Thank you so much for walking us through this. I
- 32:29Speaker 2: feel like I finally actually understand what a churn insulator is.
- 32:32Speaker 3: It was my absolute pleasure. This is the kind of
- 32:34Speaker 3: stuff that makes being a physicist fun and.
- 32:36Speaker 2: To everyone listening, thank you for being part of this exploration.
- 32:40Speaker 2: Keep your devices cool, stay curious, and we will see
- 32:43Speaker 2: you in the next deep dive.