At the limits of astrophysics – with Katy Clough
Ringkasan
TLDRDr. Katy Clough discusses the intriguing overlap between mathematics and astrophysics in her talk, "At the Limits of Astrophysics." She centers on three ideas: black holes, wormholes, and warp drives, illustrating how such concepts, while appearing like science fiction, are rooted in scientific theory. By explaining spacetime curvature, she elaborates that gravity arises from this curvature rather than being merely a force. Clough uses historical anecdotes and demonstrations to address how theories can evolve and often seem improbable. Ultimately, she encourages a broad-minded outlook toward scientific exploration, highlighting the potential of ideas that can bridge theoretical physics and empirical science.
Takeaways
- 🌌 Gravity as curvature of spacetime
- 🌠 Black holes vs science fiction
- ⚛️ Importance of exotic matter
- 🌀 Wormholes as theoretical shortcuts
- ⭐ Warp drives and their challenges
- 📏 The universe is expanding
- 🔭 Evidence of black holes
- 🔑 Understanding spacetime is key
- 📜 History of scientific conflict
- 🧠 Open-mindedness in science
Garis waktu
- 00:00:00 - 00:05:00
Dr. Katy Clough addresses the audience at Queen Mary University of London, discussing the limits of astrophysics and presenting herself as a researcher situated between mathematics and astrophysics. She introduces her topic, hinting at the boundary between science and science fiction.
- 00:05:00 - 00:10:00
Setting the stage, Dr. Clough presents alternative titles for her talk, focusing on distinguishing between crazy and brilliant ideas in science. She mentions how historical misconceptions have often blurred the lines between the two, leading to unexpected scientific truths.
- 00:10:00 - 00:15:00
The discussion shifts to black holes, which Dr. Clough asserts are solid scientific entities despite their seemingly crazy nature. She introduces spacetime curvature, a fundamental aspect of Einstein's theory of general relativity, and illustrates how gravity operates differently in strong gravitational fields.
- 00:15:00 - 00:20:00
Using a two-dimensional model to explain spacetime, Dr. Clough elaborates on the nature of gravitational forces, emphasizing that what we perceive as gravitational attraction is actually the effect of spacetime curvature caused by massive objects like stars and planets.
- 00:20:00 - 00:25:00
Dr. Clough further illustrates spacetime curvature using an analogy involving two people walking on the surface of the Earth, explaining how their paths would converge due to the Earth's curvature. This analogy highlights the counterintuitive nature of gravity as understood through spacetime rather than traditional forces.
- 00:25:00 - 00:30:00
The talk transitions to the expansion of the universe, where Dr. Clough describes the Hubble Expansion. She explains how galaxies move apart due to the curvature of space and time rather than gravitational attraction, revealing insights into cosmic structures.
- 00:30:00 - 00:35:00
Dr. Clough dives into black holes, explaining their formation from collapsing massive stars as per Chandrasekhar's theory, which faced initial rejection due to prevailing scientific prejudices. She provides a modern confirmation of black holes through observational evidence, showcasing the first image of a black hole's event horizon.
- 00:35:00 - 00:40:00
Following her exploration of black holes, Dr. Clough introduces wormholes, describing them as theoretical shortcuts through spacetime. She discusses the challenges of conceptually and physically creating traversable wormholes due to the requirement for 'exotic matter' with negative energy, which poses several problems in modern physics.
- 00:40:00 - 00:45:00
The subject shifts to warp drives as another speculative concept from science fiction. Dr. Clough outlines how they draw from cosmological principles of space contraction and expansion while also facing challenges in terms of the need for exotic matter and potential paradoxes associated with time travel.
- 00:45:00 - 00:55:55
Finally, Dr. Clough concludes her discussion on the relationships between black holes, wormholes, and warp drives, reinforcing the importance of maintaining an open mind when approaching unconventional ideas in science, harkening back to the historical dismissal of innovative theories. She invites questions from the audience.
Peta Pikiran
Video Tanya Jawab
What is spacetime curvature?
Spacetime curvature is the concept that space and time are intertwined in a four-dimensional continuum, where the presence of mass can warp this fabric, leading to the effects we perceive as gravity.
What defines a black hole?
A black hole is defined as a region of spacetime from which nothing can escape, characterized by its event horizon.
What are wormholes?
Wormholes are hypothetical passages through spacetime that could create shortcuts for long journeys across the universe.
Do warp drives exist?
Warp drives are theoretical constructs that would allow faster-than-light travel by contracting and expanding spacetime, but they require exotic matter, which has not been proven to exist.
What is exotic matter?
Exotic matter is a type of matter that would have negative energy and density, necessary for stabilizing a traversable wormhole or warp drive.
How do black holes form?
Black holes form when massive stars collapse under their own gravity after exhausting their nuclear fuel.
What evidence supports the existence of black holes?
Recent observations such as the imaging of a black hole's event horizon and the detection of gravitational waves from merging black holes provide evidence for their existence.
What is the significance of the Hubble Expansion?
The Hubble Expansion refers to the observation that the universe is expanding, with galaxies moving away from each other over time.
How does time behave near a black hole?
Time behaves differently near a black hole due to the effects of strong gravity, leading to dilated time for objects at different distances from the event horizon.
What historical conflict related to black holes is mentioned?
The conflict between Chandrasekhar, who argued that massive stars must collapse into black holes, and Eddington, who dismissed this idea, illustrates how scientific biases can delay acceptance of valid theories.
Lihat lebih banyak ringkasan video
- 00:00:00(techno-style music)
- 00:00:04(audience applauding)
- 00:00:14- Wow.
- 00:00:17Hello. Thank you.
- 00:00:17And thank you especially for the promotion to professor.
- 00:00:22I am sadly only a doctor, but, yes, I'm nevertheless
- 00:00:26very happy to be here this evening.
- 00:00:28So yeah, as Hassan said, I'm Dr. Katy Clough.
- 00:00:31So I am an Earnest Rutherford fellow
- 00:00:33at Queen Mary University of London,
- 00:00:36which is just down the road.
- 00:00:37And this evening, I'm gonna be telling you
- 00:00:39about the limits of astrophysics.
- 00:00:41That's what I've promised to tell you.
- 00:00:43So the title, "At the Limits of Astrophysics,"
- 00:00:46so that's the title of my talk,
- 00:00:47but it's also a bit of a description of me and my research.
- 00:00:52So you'll notice from my slide,
- 00:00:54that I'm actually from the maths department
- 00:00:56at Queen Mary University.
- 00:00:57We've got some mathematicians in the audience.
- 00:01:01And so, actually,
- 00:01:04all the mathematicians think I'm an astrophysicist,
- 00:01:07but all the people in the astronomy unit
- 00:01:09who are real astrophysicists, think I'm a mathematician.
- 00:01:12But I actually sit in this very interesting and rich space
- 00:01:15that exists somewhere between the two things,
- 00:01:18especially for Einstein's theory
- 00:01:20of general relativity for gravity
- 00:01:22that I'm gonna tell you a bit about this evening.
- 00:01:24It's somewhat of a mathematical theory,
- 00:01:27and yet it has consequences in our universe,
- 00:01:30so it sits somewhere between the two things.
- 00:01:33So as Hassan was saying, this is actually the first
- 00:01:35in a series of talks that are gonna be given
- 00:01:37by Queen Mary researchers.
- 00:01:39And when I got the list
- 00:01:42of all of everyone else's abstracts and titles,
- 00:01:44I thought, "Wow, this is really amazing."
- 00:01:48So there's things like supernovae, exoplanets,
- 00:01:52beginning of the universe,
- 00:01:53dark energy, dark matter, all this kind of stuff.
- 00:01:56And I thought, "That sounds really impressive."
- 00:01:59It actually sounds like science fiction.
- 00:02:02And I thought, you know, if I wasn't working in this field,
- 00:02:05I might find it really difficult to know where the line is
- 00:02:09between science and science fiction.
- 00:02:12You know, if I can have, you know,
- 00:02:13all of these crazy supernovae
- 00:02:15and exoplanets and stuff like that,
- 00:02:17you know, why can't I have wormholes and warp drives
- 00:02:19and things like that?
- 00:02:20And so I thought it would be fun this evening,
- 00:02:22to try and explore with you where that boundary lies,
- 00:02:26which is also, as I say, kind of related to this space
- 00:02:28that I exist in for my research,
- 00:02:30somewhere between mathematics and astrophysics.
- 00:02:34Okay, so let's get started.
- 00:02:36So an alternative title for my talk is,
- 00:02:39"What is the Difference Between a Crazy Idea
- 00:02:41and a Brilliant One?"
- 00:02:44So it turns out, of course,
- 00:02:46you know, if you know anything about the history of science,
- 00:02:49that we're not very good at telling the difference
- 00:02:52between these two things.
- 00:02:53So often, we've thought that things were very good ideas
- 00:02:56and they turn out to be completely wrong, and vice versa,
- 00:02:59you know, things that we thought couldn't be true
- 00:03:01actually turn out to be reality,
- 00:03:03you know, the reality of the universe that we live in.
- 00:03:06And so I'm gonna focus on three crazy ideas
- 00:03:10for this evening,
- 00:03:11and I've sort of ranked them in order of craziness.
- 00:03:16So actually for the second and the third one,
- 00:03:18it's a bit of a matter of taste.
- 00:03:20Like it depends, you know, how you feel about these things,
- 00:03:23and it depends on the specific type of wormhole
- 00:03:26or warp drive that you wanna have.
- 00:03:28But definitely the first one, black holes, do exist.
- 00:03:31So black holes are really good science
- 00:03:33and not science fiction,
- 00:03:35which is surprising because they do, as I say,
- 00:03:38on the face of it, sound kind of completely mad.
- 00:03:41So before I tell you about these three types of objects,
- 00:03:45I have to tell you a bit about this really crazy
- 00:03:48but super brilliant idea, which is spacetime curvature.
- 00:03:52So I think for me, this is one of the most brilliant
- 00:03:55but also most crazy ideas in the history of physics.
- 00:03:58This is one of the things where when you first encounter it,
- 00:04:01you just can't accept it.
- 00:04:03Like deep in you, you're like,
- 00:04:05"No, that's not how the universe is."
- 00:04:07But it is, right?
- 00:04:08It's just that you don't have the right intuition
- 00:04:11because you were born and lived most of your life on,
- 00:04:14well, all of your life hopefully, on Earth.
- 00:04:18And, you know, you've never flown to a black hole
- 00:04:21or traveled at the speed of light.
- 00:04:22You know, as far as I know,
- 00:04:24you've all been here for your lives.
- 00:04:26So you just don't have the right intuition
- 00:04:28for these very strong gravity environments
- 00:04:31that you have, for example, around black holes.
- 00:04:35So at the core of this idea,
- 00:04:36is this idea of spacetime curvature,
- 00:04:38so let me break it down for you a bit.
- 00:04:41So the first part is spacetime.
- 00:04:43So this idea of spacetime is that somehow,
- 00:04:47space and time are not separate things,
- 00:04:52they're not independent, they somehow depend on each other,
- 00:04:55so they're part of this bigger thing called spacetime.
- 00:04:58So in this picture, this is probably how you,
- 00:05:00normally, we would think about space and time.
- 00:05:04So along the bottom, there's space,
- 00:05:06and going upwards, that's moving forward in time.
- 00:05:09And you would think that, you know,
- 00:05:10you flew off from your planet to a nearby black hole or star
- 00:05:14and, you know, everyone agrees
- 00:05:16that you left at seven o'clock in the evening
- 00:05:19and you arrived at 7:00 AM the next day
- 00:05:21in time for breakfast,
- 00:05:22and then you turn around and you fly back to your planet.
- 00:05:25And in this picture of time that we have,
- 00:05:27everyone agrees on the time
- 00:05:30which these events happened, right?
- 00:05:32There's like some big clock in the sky
- 00:05:35that everyone agrees on.
- 00:05:38But the reality is
- 00:05:39there is no such big clock on the sky, right?
- 00:05:41To measure the sequence of these events,
- 00:05:44you need to be the person at each one of them.
- 00:05:47You need to be the person traveling in the rocket,
- 00:05:49or sitting on the planet, or sitting at the black hole.
- 00:05:52And what you see on your watch
- 00:05:54will differ depending on where you are,
- 00:05:57and which of these events you are at,
- 00:05:58and how you're traveling through the space and the time.
- 00:06:02And that is, as I say, very counterintuitive,
- 00:06:04but it is really how our universe works.
- 00:06:08The second thing that you need to know, and this is,
- 00:06:10again, it's probably deep in you
- 00:06:12because it's one of the first things you learn
- 00:06:14when you're at school.
- 00:06:15Like I think really, the first science lesson you have,
- 00:06:17you have to learn forces, and you learn magnetism,
- 00:06:20and you learn gravity.
- 00:06:21So you say, "Name a force," and you say, "Gravity,"
- 00:06:24but that's wrong, okay?
- 00:06:25We shouldn't actually teach children this.
- 00:06:27I actually think we should just teach them
- 00:06:28spacetime coverture directly,
- 00:06:30but I'm apparently a minority view here.
- 00:06:33So, yeah, we teach them it's a force, which is okay,
- 00:06:36you know, it works on the surface of the Earth.
- 00:06:39But, you know, what is a force?
- 00:06:41So the idea of a force is that it's something
- 00:06:43that changes your speed or direction.
- 00:06:46So in this picture particularly,
- 00:06:48I'm thinking about a change of direction.
- 00:06:50So I'm flying my spaceship past a planet
- 00:06:53and it gets somehow pulled off course
- 00:06:56by this gravitational force.
- 00:06:58And we think of this as being like,
- 00:06:59you know, a kind of like a big magnet that sort of attracts
- 00:07:02the spaceship towards the Earth.
- 00:07:07But what I wanna tell you
- 00:07:08is that that's not what's really happening.
- 00:07:10So in fact, we would say actually,
- 00:07:12that there is no change of direction.
- 00:07:15So the picture that we should have is something like this,
- 00:07:18that it's not a force that's pulling us off course,
- 00:07:21it's spacetime curvature.
- 00:07:23So I have it up on this slide,
- 00:07:25but Hassan told me, "You have to do a demo."
- 00:07:29And I said, "There's a reason
- 00:07:30why I'm in the mathematics department
- 00:07:32and not in the engineering department anymore."
- 00:07:34But, okay, so he's responsible
- 00:07:36for anything that would happen.
- 00:07:38But, okay, so the idea is this...
- 00:07:40Oh, let me start with a small one.
- 00:07:42So the idea is basically,
- 00:07:43that you have to imagine that this two dimensional surface,
- 00:07:47this sheet here, is spacetime.
- 00:07:50So that's the first thing that's quite tricky
- 00:07:52in these pictures.
- 00:07:53So people always show this kind of picture
- 00:07:55when they explain spacetime.
- 00:07:57But this sheet has two dimensions,
- 00:08:01I can describe it by two coordinates,
- 00:08:04but it's supposed to represent spacetime,
- 00:08:06this unified space and time thing that I was talking about,
- 00:08:10and so it should really be four dimensional.
- 00:08:13So already, something three dimensional,
- 00:08:15you know, like a ball,
- 00:08:16is, okay, you can imagine that,
- 00:08:18but four dimensional, maybe not, right?
- 00:08:22It's okay, right?
- 00:08:24You don't have to imagine four dimensional spacetime.
- 00:08:26I actually challenge anyone
- 00:08:28who says that they can imagine four dimensional space time,
- 00:08:31I don't think they can, but it's okay.
- 00:08:34As I say, it's just kind of schematic,
- 00:08:35so just take it as being schematic.
- 00:08:38So if I...
- 00:08:39I mean, this is my rocket, this marble.
- 00:08:42If I roll it across spacetime,
- 00:08:44because it's quite light, it's quite small,
- 00:08:47it doesn't curve spacetime very much,
- 00:08:50and so it just travels in a straight line.
- 00:08:53So this is like in a space
- 00:08:54where I'm traveling through empty space, right?
- 00:08:56And I just always move in a straight line.
- 00:09:01But what if I then put a star
- 00:09:04in the center of my spacetime?
- 00:09:06Oh, that's not enough. I have to do a bigger star.
- 00:09:10Here's a bigger star.
- 00:09:13Okay, now my spacetime has been curved.
- 00:09:17So the nice thing about this picture is it tells you
- 00:09:19where does this curvature,
- 00:09:21this spacetime curvature, come from?
- 00:09:23It comes from energy and matter.
- 00:09:26So things like stars or planets
- 00:09:28curve the spacetime around them.
- 00:09:31And so then when I come in with my little rocket,
- 00:09:33what I can do if I...
- 00:09:35Well, so if I try and go in a straight line,
- 00:09:37I get deflected, right?
- 00:09:39I get pushed off course.
- 00:09:41And so we might describe this as being a force
- 00:09:44that's pulling this marble towards, whoop,
- 00:09:48towards the star.
- 00:09:50But you can see that's not really what's happening, right?
- 00:09:52So actually what it's doing
- 00:09:53is it's following the contours of the surface.
- 00:09:56And because it's a curved surface,
- 00:09:58those contours are not straight lines, right?
- 00:10:01They are curved.
- 00:10:02So there's no magnet in this ball
- 00:10:05pulling this ball towards it,
- 00:10:07it's really just following the curvature of my spacetime.
- 00:10:10So if I do it nicely... I'm not very good at this.
- 00:10:13If I make it do it like this,
- 00:10:15I can actually get it to go round in an orbit.
- 00:10:17And so this is actually what's happening
- 00:10:19with the Earth around the sun,
- 00:10:20and the planets around the sun, okay?
- 00:10:22We don't in-spiral so fast, don't worry.
- 00:10:26It takes a very long time for us to in-spiral
- 00:10:28towards the sun, and so we're all good.
- 00:10:33But, yeah, so this is the concept of spacetime curvature,
- 00:10:38and this is gonna be fundamental to all of the objects
- 00:10:40that I'm talking about.
- 00:10:41So I'm gonna show you lots of these
- 00:10:42two dimensional pictures, which you have to remember
- 00:10:45are kind of schematic representations
- 00:10:47of four dimensional spacetime.
- 00:10:50Sorry, I don't need my next two slides
- 00:10:52because I did it for you.
- 00:10:55Okay, but I have another picture that I really like to show.
- 00:10:59This is the one that I really like
- 00:11:01when I imagine spacetime.
- 00:11:04And the reason is that actually,
- 00:11:06most of the curvature is in the time direction,
- 00:11:10it's actually not in the space direction.
- 00:11:12So to quite a good approximation,
- 00:11:15it's time that's curved and not space.
- 00:11:18Okay, I said they were part of the same thing,
- 00:11:20so it's a bit subtle, but let me explain with my picture.
- 00:11:24So here are Sam and Lliebert,
- 00:11:27these are my two PhD students from Queen Mary University.
- 00:11:31And so I decide...
- 00:11:33Let's pretend that we live a long time ago, okay?
- 00:11:35Where we don't know if the surface of the Earth
- 00:11:37is flat or curved.
- 00:11:39And I decide to send my two PhD students to Africa
- 00:11:43to do an experiment that I can't be bothered to do myself.
- 00:11:47That's what you do with PhD students.
- 00:11:50And so I send them to Africa and I tell them,
- 00:11:54"Okay, we're gonna do an experiment.
- 00:11:56You need to start at the equator
- 00:11:59and you're gonna line yourselves up,
- 00:12:01so you're going parallel, right?"
- 00:12:03So one here, one here, and I tell them,
- 00:12:06"You're gonna walk in a straight line," right?
- 00:12:08"You're gonna just fix your eyes on the horizon
- 00:12:11and you're gonna head north," right?
- 00:12:12"You're just gonna walk always in a straight line.
- 00:12:15It doesn't matter if you're being chased by lions,
- 00:12:17you have to walk in a straight line."
- 00:12:18Okay, so off they go.
- 00:12:21And if the Earth was really flat,
- 00:12:25then this picture is what would happen, right?
- 00:12:27They would stay separated,
- 00:12:29they would stay a certain distance apart
- 00:12:31as they traveled north.
- 00:12:32And when they got to Europe, they would find
- 00:12:34that they were still the same distance apart.
- 00:12:37But of course you know,
- 00:12:38I hope you know that our Earth is in fact a ball
- 00:12:42and therefore, that's not what would happen.
- 00:12:44If they both kept going north, eventually they would find
- 00:12:47that they were getting closer together.
- 00:12:49They would actually find
- 00:12:50that when they got to the North Pole,
- 00:12:51they would actually meet there, right?
- 00:12:53They would find that they'd got together at the North Pole.
- 00:12:58And so they might sort of be kind of confused about that
- 00:13:03if they thought that the Earth was really flat.
- 00:13:05So the reason that we thought for a long time
- 00:13:08in the history of people, that these pictures were the same
- 00:13:11is because we live on this very tiny patch
- 00:13:13of the planet, right?
- 00:13:15So in a very small box, these two pictures look the same,
- 00:13:18people stay the same distance apart.
- 00:13:21It's only when you start to travel on distances
- 00:13:23that are similar to this curvature scale
- 00:13:26of the surface of the Earth,
- 00:13:28that you start to see differences
- 00:13:30that tell you that it's a curved surface.
- 00:13:33So, okay, here's a more schematic picture
- 00:13:36of what I just told you.
- 00:13:37You've got north in space,
- 00:13:40and Sam and Lliebert are going north.
- 00:13:44And in the left-hand picture, this is flat Earth,
- 00:13:47and in the right-hand picture
- 00:13:48is what would happen on the actual curved Earth.
- 00:13:51And if they were...
- 00:13:53But if they were really determined,
- 00:13:55you know, to hang onto this picture of a flat Earth,
- 00:13:59what they might say is,
- 00:14:00"Well, maybe there was some kind of mysterious force
- 00:14:04that pulled us off course.
- 00:14:06So we didn't go in a straight line,
- 00:14:08we got somehow pulled off course
- 00:14:10and that's why we met at the North Pole."
- 00:14:14So that would be wrong, but they could...
- 00:14:17You know, PhD students, what can you do?
- 00:14:21But, you know, they might reasonably conclude that,
- 00:14:24and in fact, they could probably build a model
- 00:14:26where these two things look the same.
- 00:14:29So what I'm sort of getting at indirectly, eventually,
- 00:14:33is that this is exactly what's happening
- 00:14:35with spacetime and gravity.
- 00:14:37So this mysterious attractive force, we call that gravity,
- 00:14:42but actually it's the fact that we are moving
- 00:14:44now through time, and time is curved.
- 00:14:48So instead of going north,
- 00:14:50I've replaced this north axis with time.
- 00:14:55So as I say, that's quite a hard concept to think of,
- 00:14:58time being curved, but that is indeed what happens.
- 00:15:02And so you might ask me at this point,
- 00:15:05"You know, okay, Katy, this is all very interesting,
- 00:15:09spacetime curvature, but to be honest,
- 00:15:11I've got to this point in my life,
- 00:15:13and I've never needed the concept of spacetime curvature.
- 00:15:16Like, just thinking of gravity as a force has worked okay,
- 00:15:20and frankly, what's wrong with just thinking of it
- 00:15:23as a force, if in fact they're just equivalent?"
- 00:15:27But the problem is that in some situations,
- 00:15:30they're not equivalent.
- 00:15:31In some situations, they're different.
- 00:15:33And in particular, in some situations,
- 00:15:36you just can't describe what you're seeing
- 00:15:38with gravity being a force.
- 00:15:41So a really good example of this
- 00:15:42is that the universe is expanding.
- 00:15:45So this is called the Hubble Expansion,
- 00:15:47perhaps you've heard of it,
- 00:15:50but what happens is that if you take two galaxies,
- 00:15:54so these two galaxies are something
- 00:15:55like a mega parsec apart.
- 00:15:57So maybe you don't know a mega parsec,
- 00:15:59but it's a really long distance.
- 00:16:01So this is such a long distance
- 00:16:03that they're individual curvatures,
- 00:16:05so if I come back to here,
- 00:16:09so the fact that they're individually curving the space,
- 00:16:12they're not affecting each other,
- 00:16:14so they're not being pulled together anymore
- 00:16:16by this sort of what we would call
- 00:16:20the gravitational attraction, the force,
- 00:16:22but it is really down to the curvature
- 00:16:24around each of these galaxies.
- 00:16:26So they're really very far apart.
- 00:16:28And what you'd find if you looked at these galaxies,
- 00:16:31is if they started a mega parsec apart,
- 00:16:34one second later,
- 00:16:36they would be one mega parsec plus 70 kilometers apart.
- 00:16:41So they're actually moving away from each other.
- 00:16:44So that's really weird, actually.
- 00:16:48It's really hard to explain.
- 00:16:50Like, how do you explain that using a gravitational force?
- 00:16:53These objects are normal galaxies,
- 00:16:55they have positive mass and matter in them,
- 00:16:58and so they should, if anything, attract each other.
- 00:17:02Or, you know, if they're so far apart,
- 00:17:03they should just kind of stay where they are,
- 00:17:05they should just stay a certain distance apart in time.
- 00:17:09But what Pablo showed is that in fact,
- 00:17:11they are moving apart in this way.
- 00:17:14And the reason that they're moving apart
- 00:17:16is because the universe is curved in the time direction.
- 00:17:21So we never say this,
- 00:17:23we always say the universe is expanding.
- 00:17:25I would like people to say,
- 00:17:26"The universe is curved in the time direction,"
- 00:17:28but it's not really caught on.
- 00:17:31So the point is that if you see it in this way,
- 00:17:35suddenly things make a bit more sense.
- 00:17:37So the interesting thing which you'll notice immediately,
- 00:17:40is somehow, the universe as a whole
- 00:17:42is curved in the opposite way
- 00:17:44to how it's curved kind of locally around objects.
- 00:17:48So this is completely consistent with Einstein's theory.
- 00:17:51It can happen this way.
- 00:17:54But the universe is somehow curved such that,
- 00:17:57you know, it's like it being curved up instead of down,
- 00:18:00so instead of things sort of moving together,
- 00:18:02they move apart over time.
- 00:18:04But it's still curvature in the time direction.
- 00:18:07But as I say, if you think of it in this way,
- 00:18:09it's really nice because a lot of the questions
- 00:18:12that people often have about cosmology
- 00:18:13and about the universe, you start to think of them
- 00:18:16in what I think is kind of more the right way.
- 00:18:20You start to ask the right kind of questions.
- 00:18:23So for example, one question that people always ask
- 00:18:26is what is the universe expanding into?
- 00:18:29You know, if the universe is expanding,
- 00:18:31what is it expanding into?
- 00:18:34But this is like asking,
- 00:18:36what's the Earth's surface expanding into?
- 00:18:39Or, you know, would you describe the Earth's surface
- 00:18:41as somehow expanding as you move north?
- 00:18:45I mean, you kind of could describe it in this way,
- 00:18:48you know, somehow, the Earth kind of gets bigger
- 00:18:50as you get north, but it's not really expanding,
- 00:18:54it's like it's...
- 00:18:55You know, it's already there
- 00:18:56and we are just moving on this curved surface.
- 00:18:58So this is in a way,
- 00:18:59how you should think about our universe,
- 00:19:01that it's just this kind of curved surface.
- 00:19:03So a more interesting question is to ask something about,
- 00:19:06you know, can I go round the universe, right?
- 00:19:08Like, I can go round the Earth,
- 00:19:11can I sort of fly to the outages of the universe
- 00:19:14and go back on myself and come round again?
- 00:19:19Then another question that people always ask is,
- 00:19:21what came before the start of time?
- 00:19:25And this is like asking
- 00:19:26what is further south than the South Pole, right?
- 00:19:30So if I rewind time in my picture
- 00:19:32of the sort of curved Earth, that's equivalent to saying,
- 00:19:37you know, what happens when you get back to the South Pole?
- 00:19:41And you know that on the Earth,
- 00:19:42you know, all people would come to the South Pole,
- 00:19:44there'd be nowhere else for them to go, right?
- 00:19:46You can't go any further south than the South Pole.
- 00:19:49So of course, you can start asking questions about,
- 00:19:51well, somehow then you need to go off the surface
- 00:19:54of the Earth, right?
- 00:19:55You need to go into a higher dimension.
- 00:19:57So then, you know, that makes string theorists very happy,
- 00:19:59you know, they think about higher dimensions
- 00:20:01and things like that.
- 00:20:02But, you know, maybe that's the right question
- 00:20:03to be asking, right?
- 00:20:04You know, did this come from some higher dimension?
- 00:20:07The two dimensional surface of the Earth
- 00:20:09is somehow embedded in sort of three dimensional space.
- 00:20:15Okay, so let me get on to black holes,
- 00:20:20wormholes, and warp drives.
- 00:20:23So, starting with black holes.
- 00:20:25So I think the really interesting question
- 00:20:28to ask yourself...
- 00:20:28So I hope actually, everyone knows what a black hole is.
- 00:20:31I kind of assume that if people sign up to talks like this,
- 00:20:33they've at least watched one science fiction film
- 00:20:35where there's a black hole in it.
- 00:20:38But maybe I shouldn't assume knowledge.
- 00:20:40Sorry?
- 00:20:41"Star Trek"?
- 00:20:43As long as people have watched "Star Trek,"
- 00:20:45you're definitely okay.
- 00:20:47You're gonna really enjoy the end of the talk.
- 00:20:50So black holes, how do I make a black hole?
- 00:20:53So yeah, a black hole, as I say,
- 00:20:55the sort of definition of a black hole
- 00:20:57is a region of space and time
- 00:20:59that somehow separated from the rest of the universe.
- 00:21:03So the idea is that you can't get out of a black hole.
- 00:21:06So there's some surface that once you've crossed it,
- 00:21:09you would need to travel faster than the speed of light
- 00:21:11to escape from it, and therefore,
- 00:21:14you know, since as far as we know,
- 00:21:16nothing can travel faster than the speed of light,
- 00:21:19everything gets trapped in a black hole.
- 00:21:22But the interesting question that I want to ask today
- 00:21:25is how do I make a black hole?
- 00:21:27Because that's really a question about,
- 00:21:29you know, can one of these things really exist?
- 00:21:31How real is it?
- 00:21:32And so, you know,
- 00:21:34I can now use again my little demonstration.
- 00:21:37What I wanna do is I wanna make this deeper, right?
- 00:21:41So if I want things to get trapped in it,
- 00:21:43somehow I want this to make it go down.
- 00:21:46So I can put my heavier object,
- 00:21:50and you see it, it's getting deeper, right?
- 00:21:52So it becomes more difficult for something to escape if I...
- 00:21:56Ooh!
- 00:21:57This is why I said
- 00:21:58I shouldn't be trusted with a demonstration.
- 00:22:01Ooh. It's really quite addictive.
- 00:22:03So they said that they will leave it outside
- 00:22:05once we've finished the lecture
- 00:22:06and everyone can play with it.
- 00:22:07And I tell you, it is massively addictive.
- 00:22:10But I need something more, right?
- 00:22:12So, here we go.
- 00:22:15What have I got here?
- 00:22:18Oh!
- 00:22:21They said two hands, two hands.
- 00:22:23Bend your knees.
- 00:22:26Okay.
- 00:22:27So what I'm doing, right,
- 00:22:29what I'm doing is putting more and more stuff
- 00:22:33into one place.
- 00:22:34So it's not enough...
- 00:22:36So if you think about it,
- 00:22:37it's not enough just to make the ball bigger.
- 00:22:39So obviously, making it bigger
- 00:22:41isn't gonna sort of give me this kind of tube
- 00:22:44that I'm really looking for.
- 00:22:46I need to somehow contract this stuff into a small space,
- 00:22:49so I need something that's very dense.
- 00:22:51So this ball is very dense.
- 00:22:52So having a ball of the same size but a lower weight,
- 00:22:56wouldn't work, right?
- 00:22:58So this is the thing we have to do.
- 00:23:02So actually, what we have to do
- 00:23:04is we have to get all the mass that's in the sun,
- 00:23:07so all the matter that makes up our sun,
- 00:23:10and we have to sort of squash it into a region
- 00:23:13that's only a kilometer across, right?
- 00:23:16So kilometer is like, I don't know,
- 00:23:18here to Green Park Station.
- 00:23:19If it's not, it's a bit further.
- 00:23:23No, okay, I've got no sense of distance.
- 00:23:26So, yeah, what I need to do is sort of compact the sun
- 00:23:33into a region that's very small.
- 00:23:35And so on the face of it,
- 00:23:36initially people thought black holes sounded crazy
- 00:23:38because they said, well, you know, how did that happen?
- 00:23:42That seems like it would be really hard to do, right?
- 00:23:44Like, how do you get the sun and squash it?
- 00:23:46So initially, people thought that black holes
- 00:23:49were just a mathematical curiosity.
- 00:23:53So yeah, as I said, they have...
- 00:23:55So actually, the point I wanted to bake,
- 00:23:59I was gonna do it with slides as well,
- 00:24:00but then they made me do it with this.
- 00:24:03So what I wanted to say is that actually,
- 00:24:05technically speaking, black holes are this event horizon.
- 00:24:10So it's quite interesting,
- 00:24:11we don't actually describe black holes
- 00:24:14by what they're made of.
- 00:24:15So if you think all the other things
- 00:24:16that we have in astrophysics, like a star or a planet,
- 00:24:19we generally describe them by what they're made of.
- 00:24:22But with black holes, we actually don't do that,
- 00:24:24we actually define them as just being this surface
- 00:24:28beyond which nothing can escape.
- 00:24:30And one of the reasons that we do this
- 00:24:32is because we really can't know what's in them.
- 00:24:36So there's actually no way, if I fly up to a black hole,
- 00:24:40for me to tell what it's made of.
- 00:24:42So was it made of stars? Was it made of bowling balls?
- 00:24:46Was it made of televisions that got thrown in?
- 00:24:49You know, whatever I throw into a black hole
- 00:24:51and make this black hole,
- 00:24:52once it's formed this event horizon,
- 00:24:54somehow I can't tell anymore what it's made of.
- 00:24:57So it doesn't really make sense to define a black hole
- 00:25:00as what it's made of.
- 00:25:05But you might really wanna know,
- 00:25:06you know, what is this object?
- 00:25:07So there has to be something in there, right?
- 00:25:09Like there has to have been something that fell in
- 00:25:11that curved the spacetime that causes the black hole,
- 00:25:14the spacetime to be so curved.
- 00:25:17And so we would really like to know,
- 00:25:19you know, what is this object that's curving the black hole?
- 00:25:23So at this point, usually, people sort of...
- 00:25:26Well, naively, people sort of think,
- 00:25:27"Well, couldn't you somehow fly into the black hole
- 00:25:32and then look at what's in the black hole, and then..?"
- 00:25:36You know?
- 00:25:37But then, no, you can't, right?
- 00:25:38So there's actually so many reasons
- 00:25:40that flying into a black hole is a bad idea.
- 00:25:44It's actually, you know...
- 00:25:45Always when I give this talk at schools and stuff,
- 00:25:47all children want to fly into black holes.
- 00:25:49They're like, "I could fly into the black hole."
- 00:25:50I'm like, "No, don't fly into black holes."
- 00:25:53Like, fortunately they don't have any way to do it,
- 00:25:55so it's okay, but I'm always telling them like, "No."
- 00:25:57So obviously, firstly, once you go in,
- 00:26:00you can't get out again.
- 00:26:02So it's pointless, right?
- 00:26:03Like even if you went in and you looked
- 00:26:05and you found that the black hole was made of stars,
- 00:26:08you couldn't go out again and tell anyone, right?
- 00:26:11So somehow, that knowledge is trapped
- 00:26:13in the black hole with you.
- 00:26:16Then in addition, it's deadly to fly into a black hole.
- 00:26:20So at some point...
- 00:26:22So because it's very curved,
- 00:26:24so it's actually quite nice in this picture,
- 00:26:26the part of you that's closer to the black hole
- 00:26:29will be kind of falling into the black hole
- 00:26:32much faster than the part further away.
- 00:26:34So somehow, the gravitational force on it is different
- 00:26:37on the part of you that's closer to the black hole
- 00:26:39than further away from the black hole,
- 00:26:41and so it ends up stretching you.
- 00:26:43And this tidal stretching force
- 00:26:45will actually kill you at some point.
- 00:26:48So it doesn't actually necessarily happen
- 00:26:50as you cross the event horizon.
- 00:26:52A lot of people think
- 00:26:53it's like a property of the event horizon.
- 00:26:55So some very super massive black holes,
- 00:26:58you could still cross the horizon
- 00:27:00without being torn apart by tidal forces.
- 00:27:03But eventually, as you got closer and closer
- 00:27:05to the center of the black hole, you would die.
- 00:27:08So as I say, it's really not a good idea.
- 00:27:12And the final reason why it's really not a good idea
- 00:27:14to fly into a black hole, or even very close to one,
- 00:27:18is this point about time that I mentioned earlier,
- 00:27:22that time changes.
- 00:27:24So if you go very close to a black hole
- 00:27:27and then you fly back to your planet,
- 00:27:29what you'll find is that time hasn't passed as much for you
- 00:27:34as it has for everyone else on your planet,
- 00:27:36who is a long way from the black hole.
- 00:27:38And so actually, when you get back home,
- 00:27:41you know, it's a bit sad, everyone you ever knew is gone,
- 00:27:43and, you know, maybe, I dunno,
- 00:27:45your planet's not even theirs, being taken over by aliens.
- 00:27:48So as I say, don't fly into a black hole, not a good idea.
- 00:27:53But of course, black holes do exist,
- 00:27:56I've told you they do exist in nature.
- 00:27:58So how do they form? How are they made?
- 00:28:00How do we crush something the size of the sun
- 00:28:03into something a kilometer across?
- 00:28:06Well, it turns out that actually, nature does it for us.
- 00:28:09So this was first realized by Chandrasekhar.
- 00:28:13So Chandrasekhar actually gave a talk
- 00:28:16just down the road from here,
- 00:28:17at the Royal Astronomical Society,
- 00:28:20roughly a hundred years ago.
- 00:28:22And he gave this really fantastic and interesting talk
- 00:28:25on some research he'd been doing about massive stars.
- 00:28:29So what he'd realized
- 00:28:31is that if you have a very massive star,
- 00:28:33when it comes to the end of its life
- 00:28:35and it's burnt all of its fuel, it will start to collapse.
- 00:28:40And people had said,
- 00:28:41"Well, even though it starts to collapse at some point,
- 00:28:44it will be supported again by electrons
- 00:28:47in the matter of the start moving around very fast."
- 00:28:51But what Chandrasekhar realized is
- 00:28:54that's actually at some point, not enough.
- 00:28:56So the electrons would start to have to move
- 00:28:59faster than the speed of light
- 00:29:00to be able to support the star against further collapse.
- 00:29:04And since we know that things can't move faster
- 00:29:06than the speed of light, he concluded that therefore,
- 00:29:08it must continue to collapse.
- 00:29:10And actually, this would end up creating something
- 00:29:13that was compact enough to form a black hole.
- 00:29:16And so he said, "A star of large mass
- 00:29:18cannot pass into the white dwarf stage,
- 00:29:21and one is left speculating about other possibilities."
- 00:29:24So he realized this was quite controversial,
- 00:29:26and so he put it in this slightly polite way,
- 00:29:29you know, "speculating about other possibilities,"
- 00:29:31but he understood what he was saying.
- 00:29:35So unfortunately for Chandrasekhar,
- 00:29:37the next person to take the stage was Arthur Eddington.
- 00:29:41And Eddington...
- 00:29:42So Eddington was an expert in general relativity.
- 00:29:46So actually, Eddington was the person who proved
- 00:29:48that Einstein was correct about general relativity
- 00:29:51by measuring the bending of light around the sun.
- 00:29:55But he really didn't like this idea.
- 00:29:57He said, "I think there should be a law of nature
- 00:30:00to stop a star behaving in this absurd way."
- 00:30:03But notice the language he uses, right?
- 00:30:05"I think there should be a law."
- 00:30:09But there isn't one, right?
- 00:30:10So he was actually wrong and it was just his idea
- 00:30:14that this should not happen, that this was a crazy idea,
- 00:30:16this couldn't possibly be true,
- 00:30:18that led him to completely discount
- 00:30:20the perfectly valid scientific result
- 00:30:23that had been presented to him by Chandrasekhar.
- 00:30:27And it was really unfortunate because actually,
- 00:30:30of course Chandrasekhar was right,
- 00:30:32but because Eddington was so well known and influential
- 00:30:36and considered so clever, everyone listened to him,
- 00:30:38and so the whole scientific community
- 00:30:40just rejected this idea that Chandrasekhar had.
- 00:30:43And it was 40 years later, 40 years,
- 00:30:47before this idea was kind of revived
- 00:30:49and shown to be correct.
- 00:30:50So it was a kind of a big setback for science.
- 00:30:54And of course, you know, you can actually speculate a bit
- 00:30:57about the fact that Chandrasekhar being an Indian,
- 00:31:02you know, was there an element of racism
- 00:31:04in this dismissal of his idea?
- 00:31:06I think that's certainly a possibility,
- 00:31:08and it was certainly something that he felt was the case,
- 00:31:12which is why he left the UK and went to the US.
- 00:31:16But it was definitely a prejudice against how we think
- 00:31:19that our universe should work, right?
- 00:31:21We have these very strong prejudices about,
- 00:31:23this is how our universe is and it can't behave another way.
- 00:31:26And this led, as I say, to this idea being sadly discounted.
- 00:31:33So even with this idea
- 00:31:35about stars having to collapse inevitably into black holes
- 00:31:39at the end of their life,
- 00:31:41the real proof that a black hole is not a crazy idea
- 00:31:45is experiment, right?
- 00:31:47Is observation.
- 00:31:48Like, ultimately, the real test is, do we see them?
- 00:31:51Do they exist in our universe?
- 00:31:54And so, yes,
- 00:31:57so there's been some really exciting developments recently,
- 00:32:00in black hole observations.
- 00:32:03So this is one of them.
- 00:32:04There's actually been a photo taken of the black hole
- 00:32:08at the center of our galaxy.
- 00:32:10This is the photo.
- 00:32:11And so this is completely consistent
- 00:32:14with what we expect a black hole to look like.
- 00:32:16So obviously, we're not really seeing the black hole,
- 00:32:18so in a way it's a bit of a cheat to say
- 00:32:20it's a picture of a black hole.
- 00:32:22We are really seeing the sort of hot gas and dust
- 00:32:25around the black hole, that's falling into the black hole.
- 00:32:29But what we see is that there's this dark patch
- 00:32:32at the center, right?
- 00:32:33So this dark patch is a part
- 00:32:35where there is gas and dust falling in,
- 00:32:37but somehow the light from it can't escape anymore
- 00:32:40because it's gone past the event horizon.
- 00:32:43So this image is, you know, in a sense,
- 00:32:45the most direct proof we have that black holes exist.
- 00:32:50So unfortunately for the people
- 00:32:51at the event horizon telescope
- 00:32:53who made this very nice image,
- 00:32:54which was obviously a very massive scientific achievement,
- 00:32:59Hollywood made one before,
- 00:33:01and actually only a few years before.
- 00:33:03So I felt really sorry for the people
- 00:33:05at the event horizon telescope
- 00:33:06because when they unveiled their image,
- 00:33:08I think everyone was expecting this,
- 00:33:11and then it was like, you know,
- 00:33:12it was this.
- 00:33:14And so it was a bit of like, "Oh, that's nice."
- 00:33:20Okay, you can't beat Hollywood, right?
- 00:33:22But, you know, this is a Hollywood image,
- 00:33:25so it's from the movie "Interstellar,"
- 00:33:26has anyone seen the movie "Interstellar,"?
- 00:33:28Yeah, of course. Someone said, "Of course."
- 00:33:30I take nothing for granted.
- 00:33:32So, yeah, this is the super massive black hole
- 00:33:37that appears in the movie, "Interstellar."
- 00:33:39And it was really impressive because they actually did
- 00:33:43a scientifically accurate representation
- 00:33:45of what the black hole would look like.
- 00:33:47So this, maybe, I don't know if you can see the reference,
- 00:33:51but it's from a journal, "Classical & Quantum Gravity,"
- 00:33:54so it was actually published as a scientific result
- 00:33:56because no one had done such accurate simulations
- 00:33:59of what this would look like before.
- 00:34:01And, you know, it looks kind of fantastic,
- 00:34:03and indeed, it kind of matches what we actually see.
- 00:34:10So the second really exciting advance in black holes,
- 00:34:15in observations of black holes,
- 00:34:18is this one, is gravitational waves from black holes.
- 00:34:21So this was in 2015,
- 00:34:23we had the first observation of gravitational waves
- 00:34:27coming from binary black holes.
- 00:34:29So it turns out that binary...
- 00:34:31So black holes can exist in pairs, in binaries,
- 00:34:34where they orbit each other over time.
- 00:34:37And because they're omitting these gravitational waves,
- 00:34:39they lose energy.
- 00:34:41So very much like my ball going around here,
- 00:34:44you know, eventually, it will spiral in and they will merge.
- 00:34:49And so when they merge, it's a hugely energetic event
- 00:34:52and there is this ripples in space and time,
- 00:34:55these gravitational waves that are given off,
- 00:34:57and they reach us here on the Earth,
- 00:34:59and we were able to measure them in 2015.
- 00:35:02So this is the image of the wave that was seen.
- 00:35:07This is the signal that was detected.
- 00:35:10And so for me,
- 00:35:11this is quite a kind of personally exciting image.
- 00:35:16So 2015, so I actually started my PhD in 2013,
- 00:35:20so I was two years into my PhD when this discovery was made.
- 00:35:24And my sort of job, my day job certainly during my PhD,
- 00:35:28was to generate these signals, to do computer simulations
- 00:35:32that predicted what these signals would look like.
- 00:35:36And so I was spending all day generating signals like this
- 00:35:39and then suddenly, you know, wow, here they were in reality.
- 00:35:43And we all got called into the seminar room
- 00:35:45and we were sitting and watching the broadcast,
- 00:35:48and it was just such a...
- 00:35:50You know, it was quite emotional
- 00:35:52to see that this had really been detected on Earth.
- 00:35:58But as I say, yeah, this is the ultimate proof, right?
- 00:36:01So black holes are real science,
- 00:36:04they're not science fiction,
- 00:36:06and the reasons are that they don't violate
- 00:36:09any fundamental principles.
- 00:36:11In addition, they really are inevitably,
- 00:36:13the endpoint of super massive stars.
- 00:36:16And then of course, finally,
- 00:36:18the proof is that they've been observed.
- 00:36:23Wormholes.
- 00:36:25Okay, maybe Dan can take away the...
- 00:36:29I can't make a wormhole demonstration.
- 00:36:31So this is why I said I can't do a demonstration,
- 00:36:33because how do you make a wormhole?
- 00:36:35Well, I guess we could.
- 00:36:36So I hope you all know what wormholes are.
- 00:36:40Again, if you've watched enough science fiction,
- 00:36:43you'll probably know.
- 00:36:44We had a "Star Trek" fan, right?
- 00:36:47Good.
- 00:36:48Yeah, so this is an image from "Deep Space Nine,"
- 00:36:52which is in my view, one of the finest "Star Trek" series.
- 00:36:57But I have to say that... Thanks, Dan.
- 00:36:59I have to say that that picture of a wormhole,
- 00:37:02I'm not actually so keen on.
- 00:37:04It's a bit...
- 00:37:05It's not quite right.
- 00:37:07So you can see it looks like a tunnel.
- 00:37:09So as I say,
- 00:37:11again, I kind of assume people know what wormholes are.
- 00:37:14So wormholes are somehow like tunnels
- 00:37:16that take you from one part of the universe to another,
- 00:37:19quickly, you know, a shortcut that stops you having to go
- 00:37:22the long way round through space.
- 00:37:23So in "Deep Space Nine,"
- 00:37:24it takes you from the alpha quadrant to the delta quadrant
- 00:37:27It's very useful.
- 00:37:29So this one is sort of shown like this tunnel,
- 00:37:33it sort of opens up like, "Whew!"
- 00:37:35And then you fly into the tunnel
- 00:37:36and it's got like an entranceway.
- 00:37:39And certainly, they were influenced
- 00:37:40by this picture of wormhole.
- 00:37:43So again, this is one of these two dimensional pictures
- 00:37:46of four dimensional spacetime.
- 00:37:49So this is quite a bad picture because the rocket
- 00:37:53is like not on the surface.
- 00:37:55So in these two dimensional pictures,
- 00:37:57you're supposed to stay on the surface, right?
- 00:37:59You can't go into the higher dimension,
- 00:38:01you're supposed to roll along the surface like a marble
- 00:38:04and then go through this tunnel and come out the other side.
- 00:38:07So this is the kind of two dimensional picture
- 00:38:10of the four dimensional wormhole in space and time.
- 00:38:15And fortunately for us, "Interstellar" made another picture
- 00:38:20that was much better, of an intra-universe wormhole,
- 00:38:25so one that's going from one point to another.
- 00:38:27So this is the image they made,
- 00:38:28and again, it's scientifically accurate in some ways.
- 00:38:32So what a wormhole would look like is this,
- 00:38:34it would look like some kind of soap bubble.
- 00:38:37You know, it doesn't have an entrance, right?
- 00:38:39Like, you can fly around this bubble
- 00:38:42and you can go into it from any direction,
- 00:38:44and once you go in, you'll go through this tunnel
- 00:38:46and you'll come out the other side.
- 00:38:47Or in principle, that's how it works.
- 00:38:50And what you're seeing through the wormhole,
- 00:38:52these things that make it look shiny,
- 00:38:55that's the light from the galaxies and the stars
- 00:38:58on the other side of the wormhole,
- 00:38:59coming through the wormhole to you.
- 00:39:02So this is how it would really look in space.
- 00:39:08Okay, so let's play the game
- 00:39:10like we played with the black hole.
- 00:39:12How do I make a wormhole?
- 00:39:15So this is when we start to immediately have problems.
- 00:39:18So I want a wormhole, but I don't want...
- 00:39:21I want to be able to go through it.
- 00:39:23So a traversable wormhole is one...
- 00:39:26So you might have noticed it kind of looks like
- 00:39:28two black holes stuck together,
- 00:39:31but I don't want it to be two black holes stuck together
- 00:39:34because if it's two black holes stuck together,
- 00:39:36I'll get stuck once I get to their event horizon.
- 00:39:39So you can have it so that, you know,
- 00:39:41if you went through the event horizon,
- 00:39:43you'd end up stuck in this...
- 00:39:45Let me go back to this image.
- 00:39:46You'd get stuck in the middle of this throat
- 00:39:49and you couldn't go out either end,
- 00:39:51and that would obviously not be a useful wormhole.
- 00:39:53I want one that I can go all the way through.
- 00:39:56And I also don't wanna be pulled apart by these tidal forces
- 00:39:59that you get when you get sort of into a black hole.
- 00:40:04So if I want those things,
- 00:40:07then I need exotic matter in order to support the wormhole.
- 00:40:12So what is exotic matter?
- 00:40:13So just broadly speaking,
- 00:40:16exotic matter is something that has negative energy.
- 00:40:21So you could ask, what's negative energy?
- 00:40:24That's a very good question.
- 00:40:26So everything that we know of in our universe
- 00:40:28has positive energy.
- 00:40:30So you, me, stars, planets,
- 00:40:32everything is a positive energy object, right?
- 00:40:36So even things in cosmology
- 00:40:38that we don't understand very well,
- 00:40:40dark matter and dark energy,
- 00:40:42these components of our universe
- 00:40:43that we actually don't understand,
- 00:40:45they also have positive energy,
- 00:40:47and so they're not something that we can build
- 00:40:49a wormhole with.
- 00:40:51But, okay, if we just assume
- 00:40:53that somehow we do get some negative energy from somewhere,
- 00:40:58then can I somehow stuff this negative energy density
- 00:41:02into one place, and punch a hole through spacetime,
- 00:41:07and then have it form a wormhole?
- 00:41:11No, is the short answer.
- 00:41:15So it turns out that that is just forbidden
- 00:41:18by the laws of physics as we know them.
- 00:41:22So the really difficult thing is this punching a hole.
- 00:41:24So if I wanna go from the image on the left
- 00:41:27to the image on the right,
- 00:41:28I wanna go from this sheet to this wormhole thing,
- 00:41:31what I need to do is fold it over,
- 00:41:33and that's okay,
- 00:41:35but then I need to somehow punch a hole, as I said,
- 00:41:38in the top and bottom, and then stick them back together.
- 00:41:41And it's this punching a hole and sticking back together
- 00:41:44that seems to not be possible.
- 00:41:46So forming a wormhole in this way,
- 00:41:49so building one from scratch, is somehow not allowed.
- 00:41:53However, if one already happened to exist in the universe,
- 00:41:58if say during the big bang,
- 00:42:01the universe formed with lots of connections
- 00:42:03between different points in spacetime,
- 00:42:06then maybe I could get hold of one of these
- 00:42:09and like, you know,
- 00:42:10reinforce it with some additional exotic matter,
- 00:42:13and then use it to go through.
- 00:42:15So this is mining wormholes.
- 00:42:18So we want to mine wormholes,
- 00:42:19we don't want to build them from scratch.
- 00:42:23So Matt Visser compares this to a recipe for dragon stew.
- 00:42:27First find a dragon, right?
- 00:42:30Like, you know, it kind of seems...
- 00:42:32So it's not like black holes, right?
- 00:42:34So with black holes, we have a sort of a natural way
- 00:42:37for them to form in our universe,
- 00:42:39whereas with worm holes, we kind of have to say
- 00:42:41that they're already there.
- 00:42:46The thing that really sort of does it I think,
- 00:42:48for wormholes, is that they allow time travel.
- 00:42:51So has everyone seen "Back to the Future,"?
- 00:42:55I don't know, because I showed this
- 00:42:56to one of my younger collaborators the other day
- 00:42:59and they were like, "What's 'Back to the Future'?"
- 00:43:01And I was like, "No, this is not possible.
- 00:43:03You must know what 'Back to the Future' is," right?
- 00:43:05Okay, anyway, so for young people who are, you know,
- 00:43:08it's not on TikTok, so don't know,
- 00:43:12"Back to the Future," Marty uses a flux capacitor...
- 00:43:16Okay, it's not real science.
- 00:43:18Uses a flux capacitor to go back in time,
- 00:43:21and accidentally prevents his parents from getting together,
- 00:43:25thereby, you know, stopping himself from existing,
- 00:43:28and so he has to fix it before he goes back home.
- 00:43:30So already you see, there are lots of problems, right?
- 00:43:33When you you start to have time travel,
- 00:43:35we've all watched films with time travel in,
- 00:43:38and it's always a mess, and it's always unsatisfactory,
- 00:43:40because somehow it doesn't all join up correctly.
- 00:43:43So really, this is what in physics,
- 00:43:47we call this concept of causality, right?
- 00:43:50So causality is really at the sort of the base
- 00:43:53of every physical theory.
- 00:43:55And it's this idea that somehow,
- 00:43:57you know, things have an ordering,
- 00:43:59and so if I have a fire and that fire spreads over time,
- 00:44:04and then it sets some factory on fire,
- 00:44:07then there's an explosion at that factory.
- 00:44:10That explosion cannot have started the fire, right?
- 00:44:13Oh, so I can't have a loop in time, right?
- 00:44:18I can't have the thing that happens in the future,
- 00:44:21causing the thing in the past.
- 00:44:22And this seems so obvious that it's like,
- 00:44:24you know, we hardly ever say it.
- 00:44:26It's always like a, you know,
- 00:44:28zeroth more minus one law of physics,
- 00:44:30that there should be this idea of causality.
- 00:44:35And wormholes, as I say, wormholes potentially break that.
- 00:44:39So in order to make
- 00:44:41these closed time-like curves from wormholes,
- 00:44:44you have to take the two wormholes
- 00:44:46and you have to make them move relatively to each other
- 00:44:48so that the two mouths of the wormhole,
- 00:44:52you have to move them relative to each other,
- 00:44:54and then you have to kind of bring them together.
- 00:44:57And at some point when they get close enough,
- 00:44:59they will form one of these closed time-like curves,
- 00:45:01these loops in time,
- 00:45:03and allow you to travel backwards into the past.
- 00:45:08So obviously, people really don't like this,
- 00:45:10like this is really bad.
- 00:45:12So there are some solutions,
- 00:45:14saying that they're solutions is probably a bit strong.
- 00:45:18I don't think they've really solved the problem,
- 00:45:20they are all conjectures.
- 00:45:22So how could I have wormholes
- 00:45:25and still have things be okay for time travel?
- 00:45:30So most of these are from science fiction
- 00:45:32so I don't really need to explain them,
- 00:45:33but there's multiple universe timelines, right?
- 00:45:36So when Marty goes backwards in time
- 00:45:38and he stops his parents getting together,
- 00:45:40the idea would be here, that he doesn't affect his timeline,
- 00:45:45there's somehow a branching of a new universe that comes off
- 00:45:49in which his parents don't get together and he's never born.
- 00:45:52So he can still exist
- 00:45:53because he comes from this other timeline.
- 00:45:55But, you know, there are then multiple universes
- 00:45:58kind of branching off
- 00:45:59every time someone does one of these time traveling events.
- 00:46:02And so the problem with this is,
- 00:46:03you know, we have no known mechanism
- 00:46:05for branching the universe into many different time paths.
- 00:46:09As I say, that's still science fiction, sadly.
- 00:46:14The Novikov consistency conjecture.
- 00:46:17This is a very like,
- 00:46:18sort of formal sounding name for something that again,
- 00:46:21you probably know from science fiction films, where...
- 00:46:25So what happens here is this is like where I go back in time
- 00:46:29to try and stop my friend being killed,
- 00:46:31but then somehow accidentally,
- 00:46:33I become the person that kills her, you know?
- 00:46:36So somehow what has happened must always happen.
- 00:46:39So despite the fact that I go back in time,
- 00:46:41I can't change things,
- 00:46:42you know, history is set in stone and by going back in time,
- 00:46:46I will only propagate that loop as it has always been.
- 00:46:51And so this is very unsatisfactory
- 00:46:53for the same kind of reasons
- 00:46:54that the films that include it are very unsatisfactory
- 00:46:57because it's somehow very contrived, right?
- 00:47:01Like, it means that we don't have control over what we do
- 00:47:05and it makes things that are very unlikely somehow certain.
- 00:47:08So like, you know, I go back in time
- 00:47:10to try and kill someone,
- 00:47:11it means that the gun must jam at the last minute,
- 00:47:14which would be a very unlikely event,
- 00:47:17but that somehow has to happen
- 00:47:18because I can't be allowed to kill this person.
- 00:47:22So this one, as I say, I find a bit unsatisfactory.
- 00:47:25There's also the "chronology protection" conjecture.
- 00:47:29So this one is, if you think of the wormholes,
- 00:47:31I had to sort of bring them somehow together
- 00:47:34to form this closed time-like loop.
- 00:47:37And so this one sort of says something,
- 00:47:41sort of maybe quantum physics, quantum gravity,
- 00:47:44you know, waving my hands here,
- 00:47:46something stops me from moving them close enough together
- 00:47:49to form this time-like loop.
- 00:47:50So somehow they will repel each other
- 00:47:52in a way that prevents me from ever forming
- 00:47:55this closed time-like loop.
- 00:47:59And of course, the final one,
- 00:48:02and probably sadly, the most likely one
- 00:48:04is the "boring physics" conjecture,
- 00:48:05which just tells you that wormholes sadly don't exist.
- 00:48:11Okay. Warp drives.
- 00:48:15So, okay, warp drives.
- 00:48:17Warp drives, again, if you're a "Star Trek" fan,
- 00:48:19warp drives are everyday stuff.
- 00:48:21So the idea of the warp drive
- 00:48:23is actually very inspired by cosmology,
- 00:48:25by this idea of our universe expanding.
- 00:48:29So the space in front of my warp ship
- 00:48:33is contracting over time,
- 00:48:36and the space behind is expanding over time.
- 00:48:39And so this somehow drives me forward through space.
- 00:48:43So for me, I just feel like I'm kind of sitting there
- 00:48:45in this bubble, but for someone outside the bubble,
- 00:48:48I'm traveling potentially faster than the speed of light.
- 00:48:52So you don't have to travel faster than the speed of light
- 00:48:54in a warp ship, it could be one that traveled slower
- 00:48:56than the speed of light.
- 00:48:58But, you know, somehow you're being powered forward
- 00:49:00by this contraction and expansion of space time
- 00:49:04behind and in front of the ship.
- 00:49:08So the bad news,
- 00:49:10warp drives, like wormholes, require exotic matter.
- 00:49:15So we have all of the problems
- 00:49:16associated with needing to find some
- 00:49:19sort of negative energy material.
- 00:49:22They also violate causality.
- 00:49:24You can also create these kind of paradoxes
- 00:49:27where you generate time travel.
- 00:49:29And so again, they're slightly unlikeable for that reason.
- 00:49:35A really practical point about warp drives
- 00:49:38is how do you steer one?
- 00:49:40So it turns out that if you are in this bubble
- 00:49:42and you want to send a signal to the front of the bubble,
- 00:49:46you can't, right?
- 00:49:47You actually can't get a message to the front of the bubble,
- 00:49:50and that means you can't turn it off.
- 00:49:52So once you are in the warp drive,
- 00:49:55you just kind of have to keep going, right?
- 00:49:57So that's not, again, very useful
- 00:50:00if you really want to use it as a warp drive
- 00:50:02for traveling through spacetime.
- 00:50:04But okay, let's just set these aside
- 00:50:08and see if we could make gravitational waves with one.
- 00:50:11So this is...
- 00:50:13I have to emphasize, this is a bit of a hobby of mine.
- 00:50:18So I'm very aware that most of the people in the audience
- 00:50:20are probably British taxpayers and you do pay my salary,
- 00:50:25so I want to assure you that I do actually do
- 00:50:28other more useful stuff in my main research.
- 00:50:33Well, you can judge that for yourself. I also do teaching.
- 00:50:37So in my spare time, my hobby is to simulate warp drives.
- 00:50:44So as I say, you know, these objects,
- 00:50:46although they're science fiction,
- 00:50:47they actually have quite good descriptions in physics.
- 00:50:50And so I can actually build one in my computer simulation
- 00:50:55and I can actually see whether I can generate
- 00:50:57gravitational waves from it,
- 00:50:58that maybe could be observed here on Earth.
- 00:51:02So it's an international collaboration.
- 00:51:06So Tim "Jim T." Dietrich is the captain,
- 00:51:11so he's actually an expert in neutron star physics
- 00:51:14from Potsdam University.
- 00:51:17I also have Sebastian "Wrath of" Khan
- 00:51:21who is an expert in gravitational wave data science
- 00:51:24and data analysis from Cardiff University.
- 00:51:27And then there's me,
- 00:51:29and I'm very much like Scotty in the original "Star Trek"
- 00:51:31in that I do all the work
- 00:51:34and these guys literally do nothing.
- 00:51:36So Tim just writes me emails saying,
- 00:51:38"Have you done the simulations yet?"
- 00:51:40And I'm like, "You know, I have a day job
- 00:51:42so there's things I have to do."
- 00:51:45And Sebastian just sends us all "Star Trek" memes
- 00:51:48all the time,
- 00:51:49and episodes of "Star Trek" that he's been watching,
- 00:51:51thinking about warp drives.
- 00:51:53So as I say, I am the one who does all the work.
- 00:51:57And so we've actually done some calculations,
- 00:51:58so this is to prove that we have calculations,
- 00:52:00we have simulations, we even wrote a code to do this.
- 00:52:04So this is our computer, it's available on GitHub,
- 00:52:07so for anyone who wants to download,
- 00:52:08it's publicly available, a warp drive code.
- 00:52:11And I will now share with you our results.
- 00:52:15So in this slightly poor looking movie,
- 00:52:20you can see that there's a blue patch and a red patch.
- 00:52:23And so the blue patch is the part of the spacetime
- 00:52:26that's expanding behind the warp ship,
- 00:52:29and the red part is the part that's...
- 00:52:32Sorry, yeah, the part that's expanding,
- 00:52:34and the red part's the part that's contracting
- 00:52:36in front of the warp ship.
- 00:52:37So like in my previous picture.
- 00:52:39And so the premise for this simulation is
- 00:52:42the containment field for the warp drive has broken down,
- 00:52:46and so the warp drive is gonna...
- 00:52:47The warp bubble is gonna collapse
- 00:52:50and give off gravitational waves.
- 00:52:52Okay, so are you ready? Are you watching the bubble?
- 00:52:54Okay.
- 00:52:56(dramatic music)
- 00:52:59So the thing that took me the longest
- 00:53:00was actually attaching the soundtrack to this movie.
- 00:53:04Doing the simulation was easy,
- 00:53:05but then I couldn't work out how to do the thing.
- 00:53:08So I'll show it to you again 'cause I'm so proud of it.
- 00:53:11(audience laughing)
- 00:53:12I have to go back.
- 00:53:13(dramatic music)
- 00:53:17Thank you. Thank you.
- 00:53:18(audience applauding)
- 00:53:23So what you might have seen is that it's actually very bad
- 00:53:26for the people in the warp bubble.
- 00:53:28So you probably noticed
- 00:53:29that everything kind of collapses inwards
- 00:53:31before it goes out again,
- 00:53:33so actually they would be completely torn apart
- 00:53:35by this like, stretching of spacetime,
- 00:53:38and they would sadly, unfortunately, die.
- 00:53:41But you can also see that there are waves being given off.
- 00:53:44So now we have these gravitational wave signals
- 00:53:47that we've generated,
- 00:53:49we can actually go and look in the data
- 00:53:51from the Ligo gravitational wave detector,
- 00:53:54and maybe in the future,
- 00:53:56you may see this news article saying
- 00:53:59that Einstein's gravitational waves have been seen
- 00:54:02from warp drives.
- 00:54:03Or sadly, maybe not.
- 00:54:08Okay, so that's all I wanted to tell you about black holes,
- 00:54:13wormholes, and warp drives.
- 00:54:15So, you know, I had this...
- 00:54:16"What's the Difference Between a Crazy Idea
- 00:54:18and a Brilliant One?"
- 00:54:19So that was the premise of my talk.
- 00:54:21So when I started writing this talk,
- 00:54:23I actually thought it would be quite easy to say,
- 00:54:27"No, this is where the line is drawn.
- 00:54:29Don't worry guys, we've got it all under control.
- 00:54:31We know what's real and what's not real."
- 00:54:34But actually, some of the issues were quite subtle,
- 00:54:36you know, these questions that I raised about exotic matter.
- 00:54:40You know, there are cases where you have quantum effects
- 00:54:43where you can generate
- 00:54:44small amounts of negative energy density,
- 00:54:47not enough to power a warp ship.
- 00:54:49But, you know, in principle,
- 00:54:50there are aspects of physics that we don't understand well,
- 00:54:53particularly this quantum realm
- 00:54:56where you have very small scale physics
- 00:54:58that interacts with gravity.
- 00:54:59We just don't understand that well.
- 00:55:01So, you know, sometimes,
- 00:55:03I can think, you know, maybe,
- 00:55:06maybe somewhere in the universe,
- 00:55:08someone has figured this out
- 00:55:10and they've figured it out in a way that they can use it
- 00:55:12to power warp drives, for example.
- 00:55:15I think unfortunately, it's probably not the case.
- 00:55:19It's the "boring physics" conjecture is gonna win out.
- 00:55:22But, you know, we should always remember the story
- 00:55:25of Chandrasekhar and Eddington
- 00:55:27and remember to keep an open mind to these kind of ideas.
- 00:55:32And so I will stop there,
- 00:55:34and with fear and trepidation, ask for questions.
- 00:55:38(audience laughing and applauding)
- Astrophysics
- Spacetime
- Gravity
- Black Holes
- Wormholes
- Warp Drives
- Exotic Matter
- Hubble Expansion
- Einstein
- Mathematics