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Audio · 2025-05-05 · 3h 7m · 12 moments

#468 – Janna Levin: Black Holes, Wormholes, Aliens, Paradoxes & Extra Dimensions

Janna Levin is a theoretical physicist and cosmologist specializing in black holes, cosmology of extra dimensions, topology of the universe, and gravitational waves. Thank you for listening ❤ Check out our sponsors: https://lexfridman.com/sponsors/ep468-sc See below for timestamps, transcript, and to give feedback, submit questions, contact Lex, etc. Transcript: https://lexfridman.com/janna-levin-transcript CONTACT LEX: Feedback – give feedback to Lex: https://lexfridman.com/survey AMA – ✦ AI generated

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01
Definition

A black hole is not the mass crushed to a point; it is the event horizon — a region of space-time that marks a causal separation where nothing inside can affect events outside.

Levin explains that the black hole is fundamentally the event horizon, not the singularity or the collapsed star. The event horizon is an empty region of space-time that marks a one-way causal boundary.

transcript

Janna Levin: The black hole is not the mass crushed to a point. The black hole is the event horizon. And the event horizon is really just a point in space-time or a region at space-time. It's actually, in this case, a surface in space-time. And it marks a separation in events, which is why it's called an event horizon. Everything outside is causally separated from the inside insofar as what's inside the event horizon can't affect events outside. What's outside can affect events inside. I can throw a probe into a black hole and cause something to happen on the inside. But the opposite isn't true. Somebody who fell in can't send a probe out. And this one-way aspect really is what's profound about the black hole.

02
Claim

Black holes are not dense objects; they are the event horizon — an empty region of spacetime that marks a one-way causal boundary.

Janna Levin explains that a black hole is not the super-dense matter crushed to a point, but rather the event horizon — an empty region of spacetime that causally separates inside from outside.

transcript

Janna Levin: The black hole is not the mass crushed to a point. The black hole is the event horizon. And the event horizon is really just a point in space-time or a region at space-time. It's actually, in this case, a surface in space-time. And it marks a separation in events, which is why it's called an event horizon. Everything outside is causally separated from the inside insofar as what's inside the event horizon can't affect events outside. What's outside can affect events inside. I can throw a probe into a black hole and cause something to happen on the inside. But the opposite isn't true. Somebody who fell in can't send a probe out. And this one-way aspect really is what's profound about the black hole. Sometimes we talk about the black holes being nothing because at the event horizon, there's really nothing there. Sometimes when we think about black holes, we want to imagine a really dense, dead star. But if you go up to the event horizon, it's an empty region of space-time. It's more of a place than it is a thing.

03
Context

The development of the atomic bomb by physicists fleeing Europe to the United States was historically the least harmful outcome, and the freedom of the American scientific system was essential to that concentration of talent.

Levin reflects on the Manhattan Project, noting that the concentration of refugee scientists in America was not a coincidence — they fled to the US for intellectual freedom. She argues that given the alternatives, the US developing the bomb first was the least harmful outcome, and that maintaining this intellectual freedom is essential today.

transcript

Janna Levin: I do believe that it wasn't a 31 third down the line because America was different. And I think that's something we have to think about right now in this particular climate. So many scientists fled here. They fled to here. Americans weren't fleeing to Nazi Germany. They came here and they were motivated by it's more than a patriotism, I mean, it was a patriotism, obviously, but it was sort of more than that. It was really understanding the threat of Europe, what was going on in Europe, and what that life, how quickly it turned, how quickly this free-spirited Berlin culture, you know, was suddenly in this repressive and terrifying regime. So I think that it was a much higher chance that it happened here in America... The world flocked here. And that won't be the case if we no longer have intellectual freedom.

04
Mechanism

Inside a black hole, space and time swap places: the singularity is not a location in space but a point in the future that the infalling observer cannot avoid.

Levin describes how for an infalling astronaut, the singularity becomes a point in their future, not a place in space. Space and time effectively swap roles inside the event horizon, making the singularity inevitable.

transcript

Janna Levin: One of the most beautiful things that we suspect happens on the inside of a black hole is that space and time, in some sense, swap places. So while I'm on the outside of the black hole, let's say I'm in a nice, comfortable space station. This black hole is maybe 10 times the mass of the sun, 60 kilometers across. I could be 100 kilometers out. That's very, very close. Orbiting quite safely. No big deal, you know, hanging out. I don't bug the black hole. Black hole doesn't bug me. It won't suck me up like a vacuum or anything crazy. But my astronaut friend jumps in. As they cross the event horizon, what I'm calling space, I'm looking on the outside at this spherical shadow of the black hole cast by maybe light around it. I think, oh, there's a center of a sphere. And in the center of the sphere is the singularity. It's a point in space from my perspective. But from the perspective of the astronaut who falls in, it's actually a point in time. So their notions of space and time have rotated so completely that what I'm calling a direction in space towards the center of the black hole, like the center of a physical sphere, they're going to tell me what they can't tell me, but they're going to come to the conclusion, oh no, that's not a location in space. That's a location in time. In other words, the singularity ends up in their future, and they can no more avoid the singularity than they can avoid time coming their way.

explains mechanism · 1

05
Mechanism

Inside a black hole, space and time swap places: the singularity becomes a point in the astronaut's future that cannot be avoided, not a location in space.

Levin describes how from the perspective of someone falling into a black hole, space and time swap roles — the singularity is not a location in space but a moment in their future, as unavoidable as tomorrow morning.

transcript

Janna Levin: One of the most beautiful things that we suspect happens on the inside of a black hole is that space and time, in some sense, swap places. So while I'm on the outside of the black hole, let's say I'm in a nice, comfortable space station. This black hole is maybe 10 times the mass of the sun, 60 kilometers across. I could be 100 kilometers out. That's very, very close. Orbiting quite safely. No big deal, you know, hanging out. I don't bug the black hole. Black hole doesn't bug me. It won't suck me up like a vacuum or anything crazy. But my astronaut friend jumps in. As they cross the event horizon, what I'm calling space, I'm looking on the outside at this spherical shadow of the black hole cast by maybe light around it. It's a shadow because everything gets too close, falls in. It's just this contrast against a bright sky. I think, oh, there's a center of a sphere. And in the center of the sphere is the singularity. It's a point in space from my perspective. But from the perspective of the astronaut who falls in, it's actually a point in time. So their notions of space and time have rotated so completely that what I'm calling a direction in space towards the center of the black hole, like the center of a physical sphere, they're going to tell me what they can't tell me, but they're going to come to the conclusion, oh no, that's not a location in space. That's a location in time. In other words, the singularity ends up in their future, and they can no more avoid the singularity than they can avoid time coming their way. So there's no shenanigans you can do once you're inside the black hole to try to skirt it, the singularity. You can't set yourself up in orbit around it. You can't try to fire rockets and stay away from it, because it's in your future. And there's an inevitable moment when you will hit it.

explains mechanism · 2

06
Mechanism

The purest experience of gravity is weightlessness — free fall is the natural state of following curved space-time, and the feeling of weight comes from atoms interfering with that fall.

Levin explains Einstein's equivalence principle: the purest experience of gravity is weightlessness in free fall. The Earth is in a constant free fall around the Sun, and the International Space Station simply falls along a curved path that closes on itself.

transcript

Janna Levin: That weightlessness is the purest experience of gravity. And so this idea of falling is actually fundamental. It's how we talk about it all the time. The earth is in a free fall around the sun. It's actually falling. It's not firing engines, right? It's just falling all the time, but it's just cruising so fast. So actually, yeah, oh God, you said so many profound things. So one of them is really one of the ways to experience space-time is to be falling. To be falling. That is the purest experience of gravity. The experience of gravity, unfettered, uninterrupted by atoms, is weightlessness.

07
Mechanism

The purest experience of gravity is weightlessness — free fall — and Einstein's equivalence principle reveals that falling bodies follow curved paths inscribed by mass in spacetime.

Levin explains Einstein's happiest thought — the equivalence principle — showing that when you cut the cable of an elevator, you experience weightlessness, which is the purest form of gravity. The Earth and space station are in constant free fall along curved paths in spacetime.

transcript

Janna Levin: One is to start with the equivalence principle, which he called the happiest thought of his life. And the equivalence principle comes pretty early on in his thinking. And it starts with something like this. Like right now, I think I'm feeling gravity 'cause I'm sitting in this chair and I feel the pressure of the chair and it's stopping me from falling and lie down in a bed and I feel heavy on the bed. And I think of that as gravity. And Einstein has a beautiful ability to remove all of these extraneous factors, including atoms. So let's imagine instead that you're in an elevator and you feel heavy on your feet 'cause the floor of the elevator's resisting your fall. But I want to remove the elevator. What does the elevator have to do with fundamental properties of gravity? So I cut the cable. Now I'm falling, but the elevator is falling at the same rate as me. So now I'm floating in the elevator. And if this happened to me, if I woke up in this state of falling or floating in the elevator, I might not know if I was in empty space, just floating. Or if I was falling around the earth, there would actually, they're equivalent situations. I would not be able to tell the difference. I'm actually, when I get rid of the elevator in this way by cutting the cable, I'm actually experiencing weightlessness. And that weightlessness is the purest experience of gravity. And so this idea of falling is actually fundamental. It's how we talk about it all the time. The earth is in a free fall around the sun. It's actually falling. It's not firing engines, right? It's just falling all the time, but it's just cruising so fast.

provides context · 1

08
Context

The scientist who will resolve the origin of life or consciousness will be like Einstein — bothered by a simple, unresolved tension that others have accepted, and willing to rethink fundamental assumptions.

Levin reflects that the next great breakthrough — whether on the origin of life, consciousness, or quantum gravity — will come from someone who, like Einstein and Newton before them, refuses to lie to themselves about a gap in understanding and keeps asking the simplest question.

transcript

Janna Levin: The best scientists I know often ask the simplest questions. They're really, first of all, there's probably some confidence there, but also they're never going to lie to themselves that they understand something that they don't understand. So even this idea that Newton didn't understand the apple falling from the tree, had he lived another couple hundred of years, he would have invented relativity, because he never would have lied to himself that he understood it. He would have kept asking this very simple question. And I think that there is this childlike beauty to that. I know a bunch of brilliant biologists, physicists, chemists that are thinking about the origin of life. They're like, this doesn't. I know how evolution works. I know how the biological systems work, how genetic information propagates, but this part, the singularity at the beginning doesn't make sense. We don't understand, we can't create in a lab, they're bothered, every single day they're bothered by it. And that being bothered by that tension, by that gap in knowledge is, yeah, that's the catalyst. That's the fuel for the discovery. The discovery is going to come because somebody couldn't sleep at night and couldn't rest.

09
Claim

Black holes are fundamentally flawless and featureless — defined only by mass, charge, and spin — making them more like fundamental particles than macroscopic objects.

Levin describes black holes as 'flawless' — you can completely describe one by just its mass, charge, and spin. Try to put any imperfection like Mount Everest on it, and it will radiate it away through gravitational waves. This makes them more like fundamental particles than anything else macroscopic in the universe.

transcript

Janna Levin: There's something flawless about black holes that makes them fundamental, unlike anything else. So they're flawless in the sense that you can completely understand a black hole by looking at just its charge, electric charge, its mass, and its spin. And every black hole with that charge, mass, and spin is identical to every other black hole. You can't be like, oh, that one's mine, I recognize it. Has this little feature, and that's how I know it's mine. They're featureless. You try to put Mount Everest on a black hole, and it will shake it off. These gravitational waves. It will radiate away this imperfection until it settles down to be a perfect black hole again. So there's something about them that is unlike, and another reason why I don't like to call them objects in a traditional sense, unlike anything else in the universe that's macroscopic. It's kind of a little bit more like a fundamental particle. So an electron is described by a certain short list of properties, charge, mass, spin, maybe some other quantum numbers. That's what it means to be an electron. There's no electron that's a little bit different. You can't recognize your electron. They're all identical in that sense. And so in some very abstract way, black holes share something in common with microscopic fundamental particles.

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10
Mechanism

Hawking radiation arises when virtual particle pairs are separated by the event horizon, causing the black hole to effectively steal one particle and force the other to become real and radiate away.

Levin explains Hawking's seminal insight: the quantum vacuum seethes with virtual particle pairs that normally cancel out. Near an event horizon, one particle can fall in while the other escapes, becoming real — the black hole radiates and loses mass, a process now known as Hawking radiation.

transcript

Janna Levin: One of the properties of the vacuum that is intriguing is this idea that you can never say the vacuum's actually completely empty. We talked about Heisenberg, but you know, the Heisenberg uncertainty principle really kicked off a lot of quantum mechanical thinking. It says that you can never exactly know a particle's position simultaneously with its motion, with its momentum. You can know one or the other pretty precisely, but not both precisely. And the uncertainty isn't a lack of ability that we'll technologically overcome. It's foundational. So it's that there's, in some sense, when it's in a precise location, it is fundamentally no longer in a precise motion. And that uncertainty principle means I can't precisely say a particle is exactly here, but it also means I can't say it's not. And so it led to this idea that what do I mean by a vacuum? Because I can't 100% precisely know. In fact, it's not really meaningful to say that there's zero particles here. And so what you can say, however, is you can say, well, maybe particles kind of froth around in this seething quantum sea of the vacuum. Maybe two particles come into existence and they're entangled in such a way that they cancel out each other's properties. So they have the properties of the vacuum. They don't destroy the kind of properties of vacuum because they cancel out each other's spin maybe, each other's charge maybe, things like that. But they kind of froth around. They come, they go, they come, they go. And that's what we really think is the best that empty space can do in a quantum mechanical universe. Now, if you add an event horizon, which as we said, is really fundamentally what a black hole is, that's the most important feature of a black hole. The event horizon, if the particles are created slightly on either side of that event horizon, now you have a real problem. Now, the pair has been separated by this event horizon. Now they can both fall in, that's okay. But if one falls in and the other doesn't, it's stuck. It can't go back into the vacuum because now it has a charge or it has a spin or it has something. It's no longer the property of that vacuum it came from. It needs its pair to disappear. Now it's stuck, it exists. It's like you've made it real. So in a sense, the black hole steals one of these virtual particles and forces the other to live. And if it'll escape, radiate out to infinity and look like to an observer far away that the black hole has actually radiated a particle. And the particle did not emanate from inside. It came from the vacuum. It stole it from empty space, from the nothingness that is the black hole.

11
Context

Black holes are 'flawless' and fundamental — like elementary particles, they are completely described by just mass, charge, and spin, with no individual features.

Levin explains that black holes are unlike any other macroscopic object in the universe: they are 'flawless' in that any imperfection is radiated away as gravitational waves, and they are completely characterized by just three properties, making them akin to fundamental particles.

transcript

Janna Levin: There's something flawless about black holes that makes them fundamental, unlike anything else. So they're flawless in the sense that you can completely understand a black hole by looking at just its charge, electric charge, its mass, and its spin. And every black hole with that charge, mass, and spin is identical to every other black hole. You can't be like, oh, that one's mine, I recognize it. Has this little feature, and that's how I know it's mine. They're featureless. You try to put Mount Everest on a black hole, and it will shake it off. These gravitational waves. It will radiate away this imperfection until it settles down to be a perfect black hole again. So there's something about them that is unlike, and another reason why I don't like to call them objects in a traditional sense, unlike anything else in the universe that's macroscopic. It's kind of a little bit more like a fundamental particle. So an electron is described by a certain short list of properties, charge, mass, spin, maybe some other quantum numbers. That's what it means to be an electron. There's no electron that's a little bit different. You can't recognize your electron. They're all identical in that sense.

extends · 1

12
Mechanism

Hawking radiation arises from quantum vacuum fluctuations near the event horizon: the black hole 'steals' one virtual particle from a pair, making the other real and causing the black hole to slowly evaporate.

Levin gives a detailed account of Hawking radiation: the quantum vacuum froths with virtual particle pairs that normally cancel out. When one falls into the black hole and the other escapes across the event horizon, the escaping particle becomes real, carrying energy away from the black hole.

transcript

Janna Levin: One of the properties of the vacuum that is intriguing is this idea that you can never say the vacuum's actually completely empty. We talked about Heisenberg, but you know, the Heisenberg uncertainty principle really kicked off a lot of quantum mechanical thinking... maybe particles kind of froth around in this seething quantum sea of the vacuum. Maybe two particles come into existence and they're entangled in such a way that they cancel out each other's properties. So they have the properties of the vacuum. They don't destroy the kind of properties of vacuum because they cancel out each other's spin maybe, each other's charge maybe, things like that. But they kind of froth around. They come, they go, they come, they go. And that's what we really think is the best that empty space can do in a quantum mechanical universe. Now, if you add an event horizon... if the particles are created slightly on either side of that event horizon, now you have a real problem. Now, the pair has been separated by this event horizon. Now they can both fall in, that's okay. But if one falls in and the other doesn't, it's stuck. It can't go back into the vacuum because now it has a charge or it has a spin or it has something. It's no longer the property of that vacuum it came from. It needs its pair to disappear. Now it's stuck, it exists. It's like you've made it real. So in a sense, the black hole steals one of these virtual particles and forces the other to live. And if it'll escape, radiate out to infinity and look like to an observer far away that the black hole has actually radiated a particle. And the particle did not emanate from inside. It came from the vacuum. It stole it from empty space, from the nothingness that is the black hole.

provides context · 1

Highlight slides
The Black Hole Is the Event Horizon✦ from: A black hole is not the mass crushed to a point; it is the event horizon — a region of space-time that marks a causal separation where nothing inside can affect events outside.The One-Way Causal Barrier✦ from: A black hole is not the mass crushed to a point; it is the event horizon — a region of space-time that marks a causal separation where nothing inside can affect events outside.Black holes are the event horizon, not the mass✦ from: Black holes are not dense objects; they are the event horizon — an empty region of spacetime that marks a one-way causal boundary.The one-way causal boundary✦ from: Black holes are not dense objects; they are the event horizon — an empty region of spacetime that marks a one-way causal boundary.Inside a black hole, space and time swap roles✦ from: Inside a black hole, space and time swap places: the singularity is not a location in space but a point in the future that the infalling observer cannot avoid.Why the singularity is unavoidable✦ from: Inside a black hole, space and time swap places: the singularity is not a location in space but a point in the future that the infalling observer cannot avoid.Inside a Black Hole, Space and Time Swap Places✦ from: Inside a black hole, space and time swap places: the singularity becomes a point in the astronaut's future that cannot be avoided, not a location in space.No Escape Once Inside✦ from: Inside a black hole, space and time swap places: the singularity becomes a point in the astronaut's future that cannot be avoided, not a location in space.
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