What happens to event horizons when black holes collide?

Published Jun 30, 2022, 5:00 AM

Daniel and Jorge take you step by step through the process of black hole mergers .

https://www.youtube.com/watch?v=Y1M-AbWIlVQ&t=47s

See omnystudio.com/listener for privacy information.

If you love iPhone, you'll love Apple Card. It's the credit card designed for iPhone. It gives you unlimited daily cash back that can earn four point four zero percent annual percentage yield. When you open a high Yield savings account through Apple Card, apply for Applecard in the wallet app subject to credit approval. Savings is available to Apple Card owners subject to eligibility. Apple Card and Savings by Goldman Sachs Bank USA, Salt Lake City Branch Member FDIC terms and more at applecard dot com. When you pop a piece of cheese into your mouth, you're probably not thinking about the environmental impact. But the people in the dairy industry are. That's why they're working hard every day to find new ways to reduce waste, conserve natural resources, and drive down greenhouse gas emissions. How is US Dairy tackling greenhouse gases? Many farms use anaerobic digesters to turn the methane from manure into renewable energy that can power farms, towns, and electric cars. Visit us Dairy dot COM's Last Sustainability to learn more.

Here's a little secret. Most smartphone deals aren't that exciting. To be honest, they're barely worth mentioning. But then there's AT and T and their best deals. Those are quite exciting. They're the kind of deals that are really worth talking about, like their deal in the new Samsung Galaxy Z flip six. With this deal, you can trade in your eligible smartphone, any year, any condition for a new Samsung Galaxy Z flip six. It's so good, in fact, it will have you shouting from the rooftops. So get yourself down a street level and learn how to snag the new Samsung Galaxy Z flip six on AT and T and maybe grab a ladder on the way home. AT and T connecting changes everything requires trade in a Galaxy s Note or Z series smartphone. Limited time offer two hundred and fifty six gigabytes for zero dollars. Additional fees, terms and restrictions apply. See att dot com, slash Samsung or visit an AT and T store for details.

As a United Explorer Card member, you can earn fifty thousand bonus miles plus look forward to extraordinary travel rewards, including a free checked bag, two times the miles on United purchases and two times the miles on dining and at hotels. Become an explorer and seek out unforgettable places while enjoying rewards everywhere you travel. Cards issued by JP Morgan Chase Bank NA Member FDIC subject to credit approval Offer, subject to change terms apply.

Hey Daniel, I have a question about smashing things together.

Oh well, yeah, came to the right place.

I know you're a professional smasher. I guess I'm actually wondering if it's the right way to study things.

I don't know, I mean, what could go wrong?

I mean, does it work for everything? Like let's say you're trying out a new restaurant. It's smashing two plates together really the best way to test it?

I mean, I would read that restaurant review, wouldn't you?

Or what about movies? Like you would smash Blu Ray disc together.

Maybe that's how they came up with awesome crossover events.

Maybe that's the origin of the Marvel multiverse.

Somebody had a stack of DVDs on their coffee table and.

Eureka, somebody smashed two comic books together, or a comic book with a Blu Ray. There you go, that's what happened.

Smash two Hollywood actors together.

Hi, I am Horhanry. Cartoonists and the co author of Frequently Asked Questions about the Universe.

Hi, I'm Daniel. I'm a particle physicist and a professor at UC Irvine, and I'm the other co author of Frequently Asked Questions about the Universe.

What what a coincidence? What are the chances that we would collide on a podcast like this?

What happens when you smash two co authors together? Do you get one big author?

You can?

Do?

You get a voltron author? Maybe? Can I be like left.

Foot jokes aside? You get a really fun book that neither of us could have written on our own, filled with amazing physics insides, deep revelations about the nature of the universe, and hilarious cartoons.

Yeah, tagles, really amazing and frequent questions about the universe, like why we can't get to other stars? Or is there an afterlife possible in this universe?

Or why Daniel doesn't believe in time travel?

Wait?

You don't believe in time travel?

Didn't you read the book?

Man, I'm gonna have to go back in time and read it.

It's too late. You're out of time.

I ran out of time, that's why. But anyways, welcome to our podcast. Daniel and Jorge Explain the Universe, a production of iHeartRadio in which.

We smash up the two most amazing things in the universe, your brain and the entire universe. We try to take everything that's out there, all the craziness, the insanity, the frothing quantum mess that is our reality, and squeeze all of it into your brain because we believe in you. We believe that your beautiful brain, even though it's a tiny part of the universe, can contain within it a whole idea of the universe that we can look out into the depths of space and actually understand what's going on out there. On the podcast, we talk about everything that's happening out there and explain all of it to you.

That's right. We smash together scientific ideas and discoveries and collide them with bad puns and a lot of conversation here in order to pick up the pieces and hopefully make sense of this amazing and wonderful cosmos that we live in.

And you give me a hard time for it sometimes, but I really do think that smashing stuff together is really the best way to understand it. I mean, like, who hasn't tried a sample of their neighbor's plate at the table right and mixed it with their own dinner to create something new.

Wow, do you ask for their permission for us? Though? At least?

I mean usually it's somebody in my family. So yes, I'm reaching over to my wife's plate to try a French fry and dip it in whatever sauce is on my plate. And you never know that could have been a culinary invention that rocked the world.

It just seems a little, you know, sort of a destructive way of studying the universe. You know, I'm more of an engineering type. I like to take things apart, not smash it together.

That's because you care about putting them back together. I just want to know what's going on inside.

Well, I mean, doesn't it seem a little destructive in a way, Like you know, it's sort of like a little kid who smashes things out of anger.

It is destructive, absolutely, but you know, sometimes that's all you can do. Joking aside, if you have a toaster, yes, you can take it apart carefully, piece by piece and catalog what's inside it. And that probably is a better way to understand how a toaster works. Than taking two toasters and making a toaster collider. But sometimes the forces that hold these things together are so strong and that the only way to break it up, to understand what's going on inside is to smash it up. And that's the case, for example, with protons.

Have you actually look, maybe there's a screwdriver for protons. You need to get the right one with the right you know shape.

Yeah, the screwdriver for protons is another proton. I guess it's more like a hammer than a screwdriver.

But then, what is that screwdriver made out of Danny Exactly?

That's the only tool you have. If everything in the universe is a proton, then basically you're just smashing protons together.

Wait, doesn't everything eventually fall apart or break apart? Can you just wait for things to break open?

I mean, I have grand deadlines, and you know, I got to get stuff done. I can't just wait till the heat death of the universe when everything collapses.

I see, it's a lack of patience, not a lack of better methods.

You're encouraging procrastination to the heat death of the universe. Right, that's really on brand for you.

That there you go and in the meantime, the grant could support you right while you wait.

That's right, I'm going to write a grant for waiting for ten to the fourteen years until the universe does its experiments for me. We'll see how that goes. I'll cut you in if it gets funded.

Yeah. Yeah, as long as it's for ten to the fourteen dollars, I'm totally in now. But a smashing things together does seem to be the preferred way Physicists like to explore things at the smallest levels because there is no screwdriver for opening things like protons or even quarts.

There is no screwdriver, there are no tweezers, and it's something that we can actually do. We can manipulate protons, we can tune in their energy, we can smash them together to see what's going on inside. And the same thing is true for even bigger stuff. We can't take stars apart. We don't have the machinery to understand what's inside a planet, so the best way to learn about it is to watch collisions of enormous astronomical objects to see what's going on inside.

Yeah, I guess sometimes it's hard to take things apart, Like you said, right, like it's hard to take a star apart. That would be pretty difficult.

It's pretty hard to take a star apart. It's even hard to look inside a star. We had the Parker Solar Probe recently, which came super close to the Sun and almost freed itself but not quite. And it gives us a picture of what's going on in the surface and helps map a little bit of the insides. But you know, we have questions about what's going on deep deep in the heart of our Sun that we could only really answer by smashing it into another star.

Yeah, I guess sometimes it's hard to look inside of the things, so you kind of have to break them apart because they don't open up so easily, and to be honest in the engineering, and we do sometimes things together until they break. Just trust test them.

Now, don't worry. I don't know how to build a star collider, so I'm not going to shoot Proxima Centauri at our star anytime soon. That's a grand proposal that will never be funded. But we don't have to build these colliders ourselves. We don't have to construct cosmic colliders to smash planets together. Because the universe is doing it for us. We just have to look out there into the skies and find the experiment already underway.

Yeah, because it is a pretty big universe, and even though it's huge and empty, it's pretty big and pretty full stuff, And so there's always something going on in the universe, and some things that going on is a big collusion.

We have seen comets slam into planets. We have seen binary stars collapse into each other. We've seen all sorts of crazy stuff smash into itself and learned an incredible amount in the process.

Yeah, we've seen galaxy smash together, right, that's sort of how dark matter was confirmed.

Yeah, we can see galaxies merging in the middle of this process of swirling around each other and their stars forming one new elliptic galaxy. And you're right, we've even seen galaxy clusters collide. The Bullet cluster is two big groups of galaxies, enormous piles of galaxies smashing into each other, dark matter coming out on either side, which tells us, as you said, dark matter is its own thing and not just some weird twist on gravity.

Yeah. I guess smashing things together is a good way to explore things, especially if they're sort of mysterious and kind of hard to know that they're there or what's going on inside of them. Right, Like smashing things with dark matter in them, so it helps you see the dark matter.

Yeah, it helps you separate the dark matter from the rest of the stuff because different things smash differently. Right, The gas and the dust in those galaxies smashed into each other, making huge explosions and bright flashes of light, but the dark matter passed right through. So that tells you that dark matter really is different from normal kind of matter. So yeah, absolutely, smashing stuff together great way to figure out what's going on.

Great way to support physicists. We like to smash things as little kids.

Yeah, but you know, don't like smash your kids together if you're not sure what they're up to. There is a limit to this idea.

I see, Well, I think they usually smash themselves pretty good without your help or direction.

All right, But in no way am I endorsing kids smashing on the podcast.

I don't even know why you would bring it up. I guess you don't. I guess kids are mysterious. Also, they're hard to understand.

Yes, absolutely, kids are hard to understand. But there are better ways to understand what's going on inside your children than smashing them together.

All right, I guess you could talk to them.

I guess you could just make references to them on the podcast and hope they listen.

Yeah, maybe, like twenty years from now, when they're in therapy, they'll be like, what did my father think of me?

Oh?

It's right here on this podcast. What But anyways, there is something mysterious out there in the universe that we would like to know more about it. We would like to know what's going on inside of them, but so far they are one of the hardest things to look at and figure out.

And a lot of people write to me and ask what happens when these two mysterious objects in the universe come together? Is it just like other collisions or are some of the fundamental rules of the universe broken?

So today on the podcast, we'll be tackling the question what happens when black holes collide? This is a very sensation of this question. I feel what happens when black holes collie.

It's sort of like shark versus shark, Like which shark eats the other one? You know? On black holes sucking in the other one, the sucking each other. What does that even mean? Man?

Yeah, I know, it's like can a hole fall into another hole? Like, you know, Holy moly, that's a complicated question. That is a whole lot of holes there in that theory.

We need a holistic understanding of how this works.

But this is sort of part of our I guess a recent theme we've had going on in the podcast. We can almost call it like Smash month or smash week exactly.

We've got smashing on the brain over here at the podcast headquarters.

Hopefully will be a smashing success. But we have been smashing things together, photons together last time and we smashed what else did we smash?

We did a whole listener episode's question about smashing stuff together. That was the theme annihilation questions.

And then we smashed light together, which turns out you can't smash together. And now we're smashing black holes. What's next, Daniel smashing universes?

Oh wow, universe collisions. Actually, there is a theory about different bubbles in the multiverse and bumping into each other and leaving an imprint on the cosmic microwave background radiation.

I just read about this theory. Yeah, oh you're big bounce.

Yeah, there was a theory by Roger Penrose and he claimed to see evidence for it in the cosmic microwave background radiation, but nobody could confirm it. So it's definitely not something we've seen, but a pretty awesome idea. Yeah.

Also, it's called the Big Bounce, not the Big smash, so we can't talk about it.

This episode sponsored by a Smashburger by smash Now. But I remember the first time I heard about black holes being collided and I thought, Wow, that's incredible, like two things that we definitely do not understand. And I thought to myself, I want to see what happens, what comes out, what's revealed in the shards of that collision, Like, show me the answer, universe.

Yeah, what are the shards of the two sharks when they collide?

And it's sort of amazing you know that it happens out there in the universe and that we can see it. So to me, it feels like we are peeking under the rug of nature, really understanding something deep about the nature of space and time by looking for these extreme collisions when nature has to tell us how things work.

Yeah, because black holes are pretty extreme in the universe, right, there are some of the most extreme conditions imaginable. Maybe they're breaking the laws of physics inside, or at least the laws that we know, and so you can't imagine amazing things are going to happen when you smash two of them together.

Yeah, they're probably going to smash the laws of physics.

And I guess maybe a more philosophical question is, is Daniel two holes actually collide? Like, what's actually hitting each other? Nothing's going to hit each other. Is there just two holes?

You could think of them as like merging, right, if you and a friend are both digging holes in the ground, you just keep digging, then eventually you just get one big hole, right, so those two holes can sort of merge.

Hmmm, so it's more of a black hole merger.

It is, But actually the math doesn't quite work that way because the black hole that comes out is a little bit smaller than the sum of the two black holes that went in, which is pretty weird.

Wait, what, well you just spoiled it, you said, another hole comes out. I guess the two holes don't cancel each other.

Yeah, they do an amazing dance of relativity to form something new that comes out.

Well, then, as you said, this kind of thing happens all the time in the years, and we get too observe it.

Right, we certainly do, and we learn a lot about the nature of space and time in the process.

All right, Well, as usual, we were curious how many people out there had heard of black holes colliding and what maybe they think happens when they do.

So thank you to everybody who participates in these segments for our podcast. We hope you have a good time answering random questions without any chance to prepare. If you like to participate and hear your speculator on the podcast for everybody else to enjoy, please don't be shy. Write to us two questions at Danielandhorge dot com.

So think about it for a second. What do you think happens when two black holes collide? Here's what people had to say. Yeah, I think we know this right.

So if two black holes collide, a they make a bigger black hole. But be I think some people have discovered that they make gravitational waves. But that seems like too simple announswer.

So I read black Hole Blues by Jan eleven, and my best guess is when black holes collide, they circle around each other faster and faster, and as they get closer to each other, they're circling almost at the speed of light at the very last split second, and when they collide, the force has enough energy to overpower the energy that an entire galaxy might put out, and that's why we can sense the gravitational waves galaxies away here on Earth with the the new instruments we have.

In general, I don't think there is a direct collision of a black hole, but rather they orbit each other closer and closer and closer, with probably the stronger one feeding off of the weaker one. Ultimately, after all the fireworks are done, I would assume that the smaller one would be eventually absorbed into the larger one, and you have one substantially larger black hole.

When two black holes collide, I think they just merge into a larger one. We can observe gravitational waves happening while this occurs, but other than that, I think they just merge.

When black holes collide, gravity waves make their way to our clever listening devices here on Earth, and I think probably there's a lot of energy released and they become one black hole.

When black holes collide, I mean you have very very heavy, heavily dent, and very strong gravity coming from these things. So when they collide, it's got it kind of one win's out, which everyone is a more dense and be strongly have stronger gravitational forces, and then it kind of absorbs.

They make a lot of gravity waves and then they make one big black hole.

All right, A lot of fun answers here. I like the one that said when they collide they eat each other kind of like sharks.

But who is eating who? Man, that doesn't really answer.

But if one shark starts eating the tail of the other shark, and then the other sharks starts eating the tail of the other shark, what's going to happen?

It's like a Yin yang shark somehow, Yeah, a ying shark. Yeah, maybe the shark ends up eating itself.

When you get a shark nado because they're spinning around so fast.

That's probably how that crossover event happened. Right, A Shark DVD and a Tornado DVD. Boom, that's right.

Yeah, one bad idea smashed another bad idea.

Yeah, why not?

Right?

Who knows what happens when you collide the craziest things in the universe. So I love the creativity there, thank you.

Yeah, why not? Maybe that should be the die of the podcast.

Why not, let's get smashing.

Well, let's break it down for people here, Daniel. Maybe let's start with the basics. What is a black hole?

Black hole, as you said, is a hole in space and time. But it's a really strange hole, you know. Really, what it is is a location where there's so much mass and energy in one spot that it's dense enough that particles that are near it are doomed to fall in. You know, mass and energy tells space how to bend, and then space tells particles and mass and other things how to move. So the more mass and energy you have somewhere, the more space curve, which is why, for example, satellites orbit the Earth instead of just flying away. You could think of all of gravity in fact, as the invisible curvature of space rather than like a Newtonian tugging. And so black holes are where space is curved so much that there are particles that can never escape.

So there's sort of holes in space, and there are sort of holes caused by gravity, right, Like that's another way to do sort of think about it, right, It's like there's so much stuff and energy in them that it just sucks everything in, and it sucks them so much they can never get out.

Yeah. Mostly you can think about gravity in two different ways. You can think about it like a force something is pulling on you, and like the Earth is tugging on you. That's sort of Newton's idea of gravity. But black holes come out of general relativity, which encourage you to think about gravity in a very different way. It says that gravity isn't a force, it's just that space is curved. But you can't see that curvature. The only thing you can see is the effect of that curvature on the motion of objects. So you shine a flashlight, for example, through curved space, then it seems to you to bend, But that bending is just because it's moving in a straight line through curved space you can't see. So when you apply that to black holes, you don't get like a really strong force of gravity. You get a place where space is bent so much that now it's just one directional. Things inside the event of horizon of a black hole always end up at the singularity. According to general relativity, because that's the only direction left in space.

Right. Yeah, but general relativity might be wrong too, right, Like there's this possibility that maybe gravity is a force and there are force gravity particles in everything. Right.

General relativity almost certainly wrong at some level, not in the sense that it's making mistakes about GPS or that we're getting the numbers wrong, but it can't really be the true description of nature, as you said, because, for example, it predicts singularities at the hearts of black hole, and you know that's not as much a physical prediction, like general relativity doesn't say there is a point of infinite density as much as it's a breakdown of the theory. It says, well, here's what I predict, and that seems sort of nonsense. So at this point, replace me with a better theory. So we don't know what's going on at the heart of black holes. It could be that the right picture of gravity is as a sort of quantum field, the way we have all the other forces. You can think about gravity as the exchange of gravitons. So yeah, you're right, general relativity almost certainly wrong. On the other hand, it predicts black holes and we see them so it's right about a lot of stuff.

Well, black holes are really strange and there are a couple of really strange things about them, like first of all, like can't escape, so they just look like a giant whole aud in space. But it also does interesting things like slow down time.

Yeah, there are two different kinds of time dilation in our universe from relativity. One is much more commonly talked about, which is velocity based time dilation. If you see somebody moving fast through the universe relative to you, you see their clocks slowing down, and that kind of time dilation is relative because if they look back at you, they see your clocks slowing down, so you too, disagree about whose clock is slowing down, which is really weird and confusing makes you doubt like you know truth and the existence of reality. But the kind of time dilation that happens to near a black hole is different. The more space is curved where you are, the more your clock will slow down. And that's not a relative effect, it's absolute. So if your friend gets near a black hole where space is curved more, you will see their clocks slow down because they're in more curved space. They will see your clock going faster. Right, it's the opposite of the relative time dilation that happens due to velocity. Here is absolute because everybody agrees. So if you are falling near a black hole, your friend will see you slow down and you will see them sped up.

Yeah, it's a pretty cool effect. And you will literally see them moving slow motion, right, and they will literally see the entire rest of the universe moving in fast forward.

Yeah. And so if you see somebody falling towards a black hole, the closer they get, the more their time slows down. And so it actually takes an infinite amount of time for the last thing to fall into a black hole. Like you toss a banana into a black hole, you don't actually see it enter the black hole past the event horizon until time equals infinity.

Right. We've had I think whole podcast about this because it's sort of a little bit mind bending because you do sort of see black holes growing over time, right, and at some point they're going to overtake the banana. Right.

Yeah, that seems confusing because it suggests that black holes could never grow because nothing could actually fall into them. That's why I said it's only true for the last thing to fall into a black hole, because as the banana falls towards the black hole, the event horizon actually grows before the banana crosses over. A black hole isn't like a pet where you need to put something in it for it to get bigger. It does not have to like eat the banana. Besides, the event horizon reflects the total gravitational energy of the system, so as the banana falls into the black hole, the event horizon actually grows out to meet it. And then if you throw something else like an apple after the banana, that also pulls out the event horizon, so it will come and encompass the banana. So that's how we see black holes actually grow out there in the universe. There's a continuous stream of stuff falling into it and pulling out the event horizon.

Right.

Right, You don't have to feed them, but it's nice to feed them, right. You don't want a black hole to starve.

I don't know. It depends where the black hole lives. If it lives in your basement, I don't think it's a good idea to feed it.

I think if it lives in your basement, it's game over for you. For your house.

You know, there is some size of a black hole where it's radiating away energy, and you could feed it at the same rate. So you could have a stable black hole that you keep as a pet.

You can have a pet. Then you just contradict it yourself. Just don't pet it. I guess, don't touch it.

I wouldn't recommend it. But theoretically it's possible to keep a black hole stable.

I see. And so something else that's interesting about a black hole is that there are only a few things we can know about them, right, I mean, there are a black hole. Stuff falls in and we never see it again, but there are a few things that you can tell about them.

Yeah, everything that falls into the event horizon is lost to us and what happens to it. We cannot know information about what's inside the event horizon. Can't escape. But that doesn't mean we can't measure things about the global black hole. Like a black hole has mass, it tugs on you even though you're out side the event horizon. So you can use that to measure how much stuff is inside the event horizon. How much mass does this black hole have? So there are a few things you can measure from outside the event horizon, and that's the mass of the black hole. Also the electric charge of the black hole, because charge is conserved in the universe. You drop an electron into a black hole, that changes its charge and its electric field. The same thing for its spin. Black holes can spin. So there's this theorem called the no hair theorem that says those are the only three things you can know about a stable black hole, mass, spin, and charge.

Wait, why is it called the no hair theorem? How does hair fall fit into this?

I think it's a joke that says that you can't know whether black holes are hairy, Like, you can't know what's going on inside the black hole. Does it have blonde hair? Does that have a mohawk? It's like, you know, just an example of something you can't know about a black hole. It could have been called the no tattoos theorem. Also, yeah, that makes no sense to me.

But that's all right. Well that's a black hole. And so now the big question is what happens if I take two black holes and I smushed them or smashed them or merged them together. Apparently a lot of things happen, So let's get into that. But first, let's take a quick break.

With big wireless providers, what you see is never what you get. Somewhere between the store and your first month's bill, the price, your thoughts you were paying magically skyrockets. With mint Mobile, You'll never have to worry about gotcha's ever again. When Mint Mobile says fifteen dollars a month for a three month plan, they really mean it. I've used mint Mobile and the call quality is always so crisp and so clear. I can recommend it to you, So say bye bye to your overpriced wireless plans, jaw dropping monthly bills and unexpected overages. You can use your own phone with any mint Mobile plan and bring your phone number along with your existing contacts. So dit your overpriced wireless with mint Mobiles deal and get three months a premium wireless service for fifteen bucks a month. To get this new customer offer and your new three month premium wireless plan for just fifteen bucks a month, go to mintmobile dot com slash universe. That's mintmobile dot com slash universe. Cut your wireless build a fifteen bucks a month at mintmobile dot com slash universe. Forty five dollars upfront payment required equivalent to fifteen dollars per month new customers on first three month plan only speeds slower about forty gigabytes on unlimited plan. Additional taxi spees and restrictions apply. See mint Mobile for details.

AI might be the most important new computer technology ever. It's storming every industry and literally billions of dollars are being invested, so buckle up. The problem is that AI needs a lot of speed and processing power, So how do you compete without cost spiraling out of control. It's time to upgrade to the next generation of the cloud. Oracle Cloud Infrastructure or OCI. OCI is a single platform for your infrastructure, database, application development, and AI needs. OCI has forty eight times the bandwidth of other clouds, offers one consistent price instead of variable regional pricing, and of course nobody does data better than Oracle. So now you can train your AI models at twice the speed and less than half the cost of other clouds. If you want to do more and spend less, like Uber eight by eight and Data Bricks Mosaic, take a free test drive of OCI at Oracle dot com slash strategic. That's Oracle dot com slash Strategic, Oracle dot Com slash strategic.

If you love iPhone, you'll love Apple Card. It's the credit card designed for iPhone. It gives you unlimited daily cash back that can earn four point four zero percent annual percentage yield. When you open a high yield savings account through Applecard, apply for Applecard in the wallet app, subject to credit approval. Savings is available to Applecard owners subject to eligibility. Apple Card and Savings by Goldman Sachs Bank USA, Salt Lake City Branch Member FDIC terms and more at applecard dot com. When you pop a piece of cheese into your mouth or enjoy a rich spoonful of Greek yogurt, you're probably not thinking about the environmental impact of each and every bite. But the people in the dairy industry are US. Dairy has set themselves some ambitious sustainability goals, including being greenhouse gas neutral by twenty to fifty. That's why they're working hard every day to find new ways to reduce waste, conserve natural resources, and drive down greenhouse gas emissions. Take water, for example, most dairy farms reuse water up to four times the same water cools the milk, cleans equipment, washes the barn, and irrigates the crops. How is US Dairy tackling greenhouse gases? Many farms use anaerobic digestors that turn the methane from maneure into renewable energy that can power farms, towns, and electric cars. So the next time you grab a slice of pizza or lick an ice cream cone, know that dairy farmers and processors around the country are using the latest practices and innovations to provide the nutrient dense dairy products we love with less of an impact. Visit usdairy dot com slash sustainability to learn more.

All Right, we're talking about smashing black holes together, and this happens all the time, right, Like, we've recently been able to listen to black holes colliding and a lot of the they happened more often than we thought.

Yeah, black hole collisions were first observed in twenty fifteen, but it was a very very long search for black holes. People started decades and decades before that trying to invent systems that were sensitive enough to the radiation emitted from black hole collisions so that we could see it here on Earth. This is something predicted by Albert Einstein, though he thought we could never actually observe it. This is a cool effect. Too bad, it's too tiny for us to ever see.

Oh I see, so before we could listen to them with gravitational waves. People were trying to see them, but they never found any right, Yeah.

People were trying to listen to them with gravitational waves for a long time. That was Einstein's prediction that they would create from gravitational waves, but that would be impossible for us to see these gravitational waves, to observe them. And you know, I'm in the company who agreed with Einstein for a long time. When I was thinking about grad school, I had a few different choices, and one was going to university that was deep into LEGO, that was developing the technology and trying to observe gravitational waves. And I remember thinking, that's cool, but they're never going to make that happen, and so I'm going to go do particle physics instead.

Yeah. Yeah, I'm in the company of Einstein as well. I have crazy hair as well.

But Einstein was wrong and so was I. Because they did see gravitational waves. They did see this crazy pattern of radiation emitted from the collisions of black.

Holes Yeah, I think what I was asking is, like, could you see two black holes merging together? I mean, we can sort of see black holes out there in the universe, and we can definitely see their effect on the stars or the galaxy around them. Could you ever hope to detect the black hole collision without the gravitational waves detection? Like, could you ever see two black holes actually colliding?

You can't actually see them, but you're right, you don't see the black holes themselves colliding. Black holes are surrounded by accretion disks, all sorts of matter. They're sort of on deck for falling into the black holes, and so sometimes when two black holes collide, their accretion discs also collide and create light. They've seen this a couple of times where they've seen flashes of bright light at the same time and in the same direction as they've observed gravitational waves. So they have seen in a couple of occasions bright flashes of light emitted from black hole collisions.

Right, but before twenty fifteen, like, maybe you would see the bright flash of light, but you wouldn't be able to know if it was a black hole collision.

Yeah, exactly. It just seemed like a flash of light, and there's lots of weird flashes of light in the universe, and you can't necessarily tell that one is from a black hole or from something else, or just from two stars colliding or two blobs of gas colliding. So really the unique signature, the thing that told us that black holes were colliding were these patterns of gravitational waves, which are like ripples in space and time itself.

And so far since twenty fifteen, we've seen a whole bunch or have heard, but a whole bunch of these black hole collisions, like maybe like ten a year or something.

Right, it's incredible, we have like fifty examples now. Preciate how amazing that is realized that we didn't know how often black holes collided. When Lego turned on, it was like a new kind of instrument, and we're listening to something new in the universe, or a new kind of eyeball. We're looking for things in the universe. It's all just an analogy, because gravitational radiation is not something you can see or hear. We're just trying to translate it into sort of human experience. But we didn't know if this kind of thing happened once in a century, once in a millennium, or like ten times a second. So when they turned this thing on, it could have been that they were waiting for years to hear the first one, or that they came fast and hard and amazingly. We were lucky, and they're pretty common. And they saw a gravitational wave in the first test run, Like they turned this thing on and they were just like doing calibration runs just to make sure everything was working, and boom, they saw a signal in the first calibration run. So they were like off to the races, writing a paper and week two.

Yeah, it's pretty amazing, pretty cool. And they happened pretty often, maybe like once a month, once every month and a half. And do they happen here in our galaxy or are we listening to these collisions from all over the universe.

They happen all over the universe, and we can see these things really far away, like billions of light years. Now, the further you are away from these things, of course, the fainter they are. And so if they're closer, it's easier for us to see them. They're further away, then that need to be more dramatic, more powerful for us to observe them. But we've detected these collisions from black holes that are billions of light years away, But.

Are they happening here in our milk away galaxy?

We see black hole collisions fairly commonly, but we can see them from really really far away, and they don't happen actually that often in any individual galaxy, So we haven't actually seen one happen yet in the Milky Way. Remember that black holes are not that common. We have really big ones in the center of the galaxy. Then you have black holes created from stellar collapse. But to get two black holes to collide, you really need like two black holes in a binary.

System, because I guess fifty seems like a lot of black holes colliding. But it's a big universe, right, There are trillions of galaxies out there, So the fact that we're only seeing, you know, maybe one year, it means that maybe they're not that common.

Yeah, they're not that common sort of per galaxy, but they happen often enough for us to have a pretty nice data sample, which means that we can really study these things. It's not just like we saw one and then we're wondering if that was typical or not. We have like dozens of these things, so we can start to ask statistical questions about what's likely and what's common. We can see which ones are weird, which ones are normal. It's really an awesome moment when you can start to do like population science on black hole collisions.

M Yeah, like statistical you know, surveys. All right, Well, maybe step us through here. What happens? What's like, step by step, what's going on when two black holes collide? Because you know, I think one thing that a lot of people might not know is that black holes can move, right, Like it's weird to think of a hole moving, like a hole in the ground doesn't move, But black holes can move, and they can sort of like fly through space and run into other black holes.

Yeah, black holes have mass just like everything else, and so they have inertia and they can have momentum. Black hole can move. You can move past a black hole. Remember that velocity is just relative in our universe. So if you're flying past a black hole from its point of view, then from your point of view, the black hole is flying past you, right, And so these things definitely can move, and a lot of people probably think about black hole collisions is like two black holes just flying through space and bumping into each other like two dogs in the park smashing into each other or something, because they weren't looking where they were going. Instead, these two things have sort of been faded to collide since their birth. Remember that a lot of stars are born as binary systems. They were made near each other and gravitationally bound from the beginning, orbiting each other in a long dance. And that's how most black hole collisions happen. They start as a binary star system, then each one collapses into a black hole. Then you get black holes orbiting each other. So they've always been neighbors. It's not like they're just two strangers that smash into each other, and they're orbiting each other and they're slowly losing that energy, radiating away their orbital energy until eventually they collide.

WHOA yeah, because I guess most black holes come from stars. And so if you have a binary system and both stars turn into a black hole, then you have a binary black hole system. Right. But isn't that sort of rare? I mean, it's a little rare for a start to turn into a black hole, But now you need to have both of them in the binary star system turned into black holes exactly.

And so those are the conditions you need, and we're still understanding in black hole formation, but it depends on how much mass there was in each individual star. If it's massive enough, then eventually it will collapse into a black hole. There's like no way to avoid it once it burns up its fuel. And the thing I think as interesting is understanding why these things are inevitable, Like why can't two black holes just orbit each other happily forever until the end of the universe. Why do they have to fall into each other?

Right? Like in our Solar system, you know, the planets are orbiting the Sun pretty stably.

Pretty stably, that's true.

We're not falling to the Sun yet.

Not today and not tomorrow. But you know, these orbits are not technically stable because every time you're in orbit around something, you're accelerating, and anything that's accelerating in our universe, it's changing its velocity, is generating gravitational waves. You know what is a gravitational wave. It's just when your gravitational field changes. If you have an object in space, it has a gravitational field, it's changing the shape the curvature of space. Is that object accelerates, then the curvature of space changes, but it doesn't change instantaneously. Just like if the Sun disappeared, we wouldn't notice for eight minutes or whatever. It would take time for that gravitational information to propagate. And so when something accelerates, it's changing the curvature of space. And that's what's happening. When the Earth is going around the Sun. It's accelerating and so that radiates away some energy in terms of the information about updating the.

Curvature, right, right, So we're slowly losing a little bit of energy in our orbit, and so eventually I guess in the very very very very far future, the Earth is going to fall into the Sun.

That's right, although other things will happen and before the Earth falls into the Sun due to radiating gravitational energy, because the Earth is not that massive, but if you have two black holes that are really really massive, they're going to radiate a lot more gravitational energy, and so as they lose energy, they fall into each other.

Right.

They can't maintain their orbit if they don't have that energy, so they're very orbit. The thing that's accelerating them around each other, is shaking the curvature of space around them, creating these gravitational waves and forcing them to get closer and closer and faster and faster. So it's more like a swirl in than a collision.

Right. It's sort of like if you have a still lake or a still body of water and you take two fingers and you sort of rotate them or spin them around each other, they're going to be generating waves on the water. That's sort of how people see two black holes kind of radiating out energy as waves exactly.

And it's a deep concept that's really applicable to lots of different physical phenomena, right, Like how do you generate radio transmissions? You take electrons which have an electric field, and you accelerate them up and now you shake them, and that wiggles the electric field. That wiggle in the electric field is nothing more than a photon. It's passing of information and energy through that field. So you take a mass, now it has a curvature in space. You wiggle that mass, you accelerate it. That wiggling of space time is gravitational radiation. It carries away energy, all.

Right, So they're not sort of you know, aimed at each other. They're more like swirling together. But then at some point they lose energy and they swirl faster and faster and closter and closer, and at some point they start to touch, I guess right, or collide.

Yeah, they start to touch. And to think about that, you have to think about what you mean by two black holes touching, right, Like, what is the edge of a black hole? What's the surface of it? Often we talk about it in terms of the event horizon. We talk about the event horizon as if it's like something physical, you know, like a surface or a boundary or something. It's really just sort of like a location past which you can never escaped the black hole. But it's not like there's anything there at the event horizon. There's no physical surface. It's just like past this point you will never escape.

It's like the edge of a hole is not really a barrier. It's just where you fall in.

Yeah, it's just where you fall in. The subtle point also is that you can't measure the event horizon technically. To calculate where the event horizon is, you need to know, like what happens to every particle that comes near it. Then you find sort of like the surface in which if a particle passed through it, nothing ever escaped, So you sort of need to know the fate of every particle to figure out exactly where the event horizon is.

Wait, wait, what what do you mean we can't tell where it is? Like? Can we can? We just take a picture of a black hole recently? Doesn't that give us a pretty good idea, by the way that the light bends around it where the event horizon is.

We did take a picture of black hole, and that does give us clues about the size of the event horizon, because actually what we're seeing there is the shadow of the black hole, which is larger than the event horizon because you know, some light, for example, near it and get bent around it, so the shadow actually looks a little bit bigger than the event horizon. But check out our whole episode about the black hole image for details about that. But in principle, even that picture doesn't tell you exactly where the event horizon is. Like it could be that there's a particle that could pass a little bit closer to the black hole that we're seeing in that picture and then escape. You don't know for sure. Now we can calculate it, right. General relativity lets you calculate the size of the event horizon. So we have this short styled radius. But it's not like something you can locally measure. You can't say I'm in or I'm out at any given moment in the universe. It's not like some device you could build that could tell you I'm inside a black hole or I'm outside of black hole. You can either calculate it from general relativity, or you can shoot a bunch of particles at it and wait till the end of the universe and see which ones escaped and which ones didn't.

So it's sort of a fuzzy boundary, I think, is what you're saying exactly.

And we're going to have to keep that definition in mind as we think about what happens when the event horizons get close to each other.

All right, yeah, so what happened? So I have a one black hole and I have another black hole each of my hands, and I'm swirling them and I'm bringing them together, and they're swirling and swirling, and at some point where the event horizon would be, or where we think it is, or fuzzly where it should be, they start to overlap.

They start to overlap. And when people write to me about this, something they're confused about is like a black hole. The event horizon is a sphere, right, it's like centered around the singularity. Now you have two black holes, both of rich are spheres. What happens when they touch? Do you suddenly get a sphere at the center of the two? You know? Does that mean the event horizon is like shrinking a little bit? What happens there? And so the answer is you can't have like discontinuities with the event horizon is in one place and then one instant later it's totally different. It's a smooth transformation from having two blobs to one blob and a little bit surprisingly, that means that the event horizon is not always spherical, and the transition between two black holes and one black hole that results it's a weird sort of peanut shape.

Yeah, I'm imagining. I guess. You know, like if you take two ink plots, like two blobs of ink, and you sort of bring them together, they're going to sort of like touch maybe at the boundary, and then sort of merge, but just a little bit first, and then the blob sort of merges together, the two blobs become a peanut shaped and then they sort of blob blob together. Is that sort of what happens.

That's sort of what happens. And to figure out exactly what the shape of the event horizon is, people do these numerical relativity calculations where basically they shoot a bunch of particles near these two masses and they figure out where the no go zones are, where if a particle passed through it, it ends up in the singularity no matter what. They have to calculate the event horizon in this way to figure out where the no go zones are, and they do these incredible simulations and you can find these images online if you want to look for the video. We'll put a link into the show notes. And what happens is you have like two blobs and as they get closer to each other, there's like a filament that forms between them. Now the event horizon looks sort of like a dumbbell. It's like two big blobs with a very thin line between them. Then as they get closer closer, that line grows and grows and grows. Eventually you have like a peanut and then a tic tac and finally a sphere.

Away we skip past the peanut minm are of a whole bunch of other candies. All right, well, let's get into what actually is happening with that event horizon and where do all the gravitational waves come from.

But first, let's take another quick break. When you pop a piece of cheese into your mouth, or enjoy a rich spoonful of greeky yogurt, you're probably not thinking about the environmental impact of each and every bite. But the people in the dairy industry are. US dairy has set themselves some ambitious sustainability goals, including being greenhouse gas neutral by twenty to fifty. That's why they're working hard every day to find new ways to reduce waste, conserve natural resources, and drive down greenhouse gas emissions. Take water, for example, most dairy farms reuse water up to four times. The same water cools the milk, cleans equipment, washes the barn, and ears the crops. How is US dairy tackling greenhouse gases? Many farms use anaerobic digestors that turn the methane from maneuver into renewable energy that can power farms towns and electric cars. So the next time you grab a slice of pizza or lick an ice cream cone, know that dairy farmers and processors around the country are using the latest practices and innovations to provide the nutrient dens dairy products we love with less of an impact. Visit us dairy dot com slash sustainability to learn more.

There are children, friends, and families walking, riding on paths and roads every day. Remember they're real people with loved ones who need them to get home safely. Protect our cyclists and pedestrians because they're people too. Go safely California from the California Office of Traffic Safety and Caltrans.

Every day, when you log into chumbucasino dot com, the ultimate online social casino, you get a free daily bonus. Imagine if you got daily bonuses in other parts of your life.

I chose French fries, overloaded French Fries.

I asked Stuart from accounting about his weekend even though.

I don't care. I updated my operating system with out having to call tech support.

Collect your free daily bonus at jumbacasino dot com. Now jump and live the Jumba life where necessary For we're phiited by bock the term conditions eating plus.

I've been struggling with my gut health for years and years. I tried everything, I mean everything without luck. But then I stumbled upon the solution. I've been looking for coffee enemas. Yep, coffee inemas from Happy bumco. And you know what the best part is, It's all natural and I can do it at home. When my friends started to notice something was different, they were shocked. When I told them I was literally glowing from the inside out. I had tons of energy, my skin cleared, and my gut issues were gone. Now they are all hooked. Coffee inemas are my new wellness tool. Thank goodness, Happy Bomb has made it so easy. After my naturopathic doctor recommended them, I wasn't sure where to start. Happy Bomb has everything you need to begin your coffee inema detox journey. Their products are safe, organic and all natural. Trust me, it's a game changer. If you are ready to transform your health, visit happybumcode dot com and use code glow for fifteen percent off your first bundle. Trust me, you'll feel the difference. That's happybumcode dot com. I promise you won't regret it.

All right, we're talking about smashing two black holes together, and the scenario we're picturing is two black holes that came from a set of binary stars and each start became a black hole. Now the black holes are swirling around each other, getting closer and closer and closer, and just as they're about to touch, they actually sort of reach out and touch each other kind of in a way. Right, Yeah, they.

Become regions in space between the two black holes that are now effectively inside their event horizon, their combined event horizon. Because if you're in that place, you will not escape. So you could have been outside the event horizon just before, but now this filament has formed where if you were right between them, you no longer have any chance to escape black hole. And to me, it's really fascinating this moment when the event horizon is no longer a sphere, because it's an opportunity to learn something, to know something about the history of the black hole, what's going on inside, even from the outside.

What do you mean, what can you learn and what could you hope to learn?

Well, if you come along a black hole and it's a perfect sphere, you have no idea what's inside? Is it bananas? Is it apples? Is it the result of a star collapsing or two stars collapsing. You have no idea about like the merger history of that black hole. But if you come along at the moment when the black holes are still merging, then you know this must have come from two mergers. You know that there are two singularities inside that event horizon, or you know something about the history of it, more so than if you just come along to a sphere. Right, so you know a little bit about what's going on inside the event horizon.

I see you're saying. It tells you a little bit about what happens when you change a black hole, right, because a non changing black hole is sort of mysterious and impenetrable. But uh, black holes that's changing. Maybe you can tell something about whether you know all the stuff inside of it is concentrated in the middle or spread out evenly, things like that.

Yeah, it's fascinating to me because black holes are like the most identical thing in the universe. Remember this, in theory, only three things to know about a black hole. There only three numbers that totally determine it, and two black holes that had the same mass, spin and charge are totally equivalent. There's no way you could do experiments to tell them apart, except unless and this is the crack in the no hair theorem. If you have a black hole with that mass and that's spin in that charge, but it's still finishing its last merger, you can know one little clue about that black hole. You can know that it came from this merger. And that must mean that the innerds of the black hole haven't quite settled down yet. They haven't like formed the singularity or the quantum fuzz of all or whatever is going on inside, because the event horizon has a different shape. It's the same mass, the same spin, and the same charge, but a different shape. Event horizon hasn't yet collapsed into a sphere.

Oh, I see, you're saying, we can learn about the resulting black holes, but we don't really would know anything about the holes the two holes that went into it, right Like, those would still be a mystery.

Those would be a little bit of a mystery, but you could know something about their relative masses. For example, if two black holes that are equal in mass merge, and as they're e merging, they look different than a black hole where one was like ninety nine percent of the final mass and the other one was one percent, because it's more asymmetric, So you know something about what went into the black hole from the shape of the sort of peanut before it collapses into a sphere. I just think that's fascinating because it's a tiny little crack, and any crack to say like I know something about what's going on past the event horizing. That's tantalizing, because I mean, it was so little about what's inside.

I see you're saying, like a regular black hole by itself, it's inscrutable, but if you see what two of them joining together, you're like, hey, I know a little bit about what happens in these extreme conditions.

Yeah, you know a little bit about the history of this black hole, whereas for another normal black hole, you know literally zi except for the mass, spin and the charge. And here you have like a little bit more information. Plus you get to describe these things in terms of a diagram the physicists call a pair of pants diagram, which is a lot of fun.

I guess if you google pants and black holes, you'll get a whole bunch of interesting images. I haven't tried it to me. Maybe we should have the adults in the audience check that first.

The idea is that you have two patches of space time, which is sort of like the legs of the pants, and then they're merging and they form like the waste eventually. So if you draw that out with like tubes of space time connecting each other, you start with two, you end with one. It's sort of like a pair of pants.

Yeah, I think it's gonna be hard to paint that picture, but I think the main point is that when the two black holes get together, they sort of reach out in the middle they start merging. That's sort of I guess where your en scene would be in the pants, and then they blop together, right, Is that sort of what happens?

Like?

Is that what this? At least that's what the simulations say, that they just block together and become one big hole.

Yeah, they block together and become one big hole and in the process released an incredible amount of gravitational radiation. We can learn something about that process from looking at the details of the wiggles of that radiation.

Right, And a lot of this energy comes from the angular momentum, right, like maybe they're spinning around each other slowly when they're far apart, But then when as the two black holes get together, they have to preserve the same angular momentum as so by the time they get really really close to each other, they're spinning at incredible speeds, right, which makes for huge accelerations, which make for huge gravitational waves.

And that's why probably every black hole out there is spinning. The simplest idea we have of a black hole, the short style black hole of a sphere, is in the event that the mass is not spinning, it's just sitting there. But because things fall into a black hole, and they will always swirl around before they fall in, because otherwise they'd have to fall in directly to the center, like perfectly online with the singularity from that, they're going to fall in with a little bit of angular velocity and so with momentum, and so they're going to end up spinning. So the final black hole has to be spinning. Every black hole out there in the universe is almost certainly spinning for that reason. And two black holes spinning around each other, you're absolutely right, how a lot of angular momentum, and they're going to generate a lot of gravitational radiation.

But the end result, what ends up happening at the end is they emerge into one bigger black hole that's bigger than the two individual black holes, but maybe like not as big as if you just added the mass of the two black holes exactly.

They lose some of that mass, right, What happens when you lose energy as a black hole, you lose mass. Just like if a black hole is radiating hawking radiation, it's shooting out particles, it's losing mass, and so if therefore it's shrinking, right, So black holes can evaporate. They can lose their mass through hawking radiation and get smaller and smaller. If they also lose energy by gravitational radiation, they are also getting smaller. And so there's so much energy released in these collisions that sometimes they can lose a lot of mass, like as much mass as our sun.

Right, And this energy goes out as gravitational ways. But also I imagine a whole bunch of light too, right, like quasars have all that gas that was around each of them is going through these extreme velocities and smashing against each other. A lot of them must go out as basically light as.

Well, most of the energy is radiated as gravitational radiation. It can be like five percent of the mass of the system is lost due to gravitational radiation. There can also be light emitted, and this is sort of an open question. People have only seen a couple examples where they have seen flashes of light perfectly coincident with black hole collisions, and so something they're excited to study. This is an era of multi messenger astronomy where you can see the same thing you know, electromagnetic radiation light as you can in gravitational radiation, and so you can study it much more deeply. It's not something we've seen many ex samples of, so it's not something that's very well understood yet.

All right, So stay tuned as we get more samples of these collisions. But I guess one big question. It kind of goes back to what you were saying before, which is that you know, time slows down near a black hole. So if you're if I'm near a black hole, my time is frozen basically or super slow motion. So how do these But now if you get a black hole next to the other, one isn't one of them slowing time down for the other one. And wouldn't they just look to us like they're frozen in time?

Yeah, you might wonder, like, why do black holes ever collide? Don't they slow each other's time down so much that they basically just get frozen before they merge? Right, Remember that a black hole is not a single point in space, So really what we're talking about is the merger of their event horizons. And so while the two singularities may orbit each other for a long time, slowing down because of the time dilation, their event horizons can merge before the singularities come together.

Right, but still, like the time should be slowing down almost to a standstill near the edge of each black hole, so as they start to merge, when things kind of freeze in time.

So things sort of do freeze in time in the sense that they get slowed down. Like, what are we seeing when we see black holes merge? We see a pattern of gravitational radiation that comes from the black hole. We see it speed up and go faster and faster and faster. Now, when you look at that, you might wonder like, why isn't that slowed down? Why isn't it get like spread out and slowed down. Why don't we see the gravitational radiation get slower and slower. The answer is that we are. We are seeing the effects of that time dilation already. Like if there wasn't time dilation, then that gravitational radiation just bore the collision would be going insanely fast. So we are seeing the effects of time dilation already sort of build in. When we see black holes collide, it would look different without the time dilation.

Oh, I see, you're saying, like things are so extreme. Things are moving so fast around these collisions, and gravitational waves are being emitted so quickly and so intensely that even with almost freezing time, they still come out and they seem at a sort of a certain frequency for us exactly.

That's built into those calculations, and when we do the numerical relativity to figure out like what's happening and where is the event horizon, how much gravitational radiation is emitted, that's of course taken into account. And so we're seeing just what we expect, time dilated, slowed down collision, but still generating these gravitational waves. So it's not slowed down to zero.

I see. So if you were like near one of these black holes as an observer, like, it would be like insane, right, It would just like happen in a flash.

Yes, exactly, would happen much more quickly. If you were very close to the event horizons of these black holes as they were happening, so you had sort of the same clock as they would, you would see something very different. Just the same way if you see somebody fall into a black hole from far away, you see their time getting slowed down. But they don't see that, right, they experienced time normally. They just fall in and end up hitting the singularity. Very very different if you were in the neighborhood of the black hole.

So that's pretty convenient, right, Like usually when you want to observe something colliding really fast, you have to use a high speed camera or you have to somehow slow down on time or sample it's super fast, you get a good picture of what's going on. This one has sort of like a built in slow mo setting.

Exactly when the most interesting thing happens in the universe, it automatically goes slow mo, just like in special effects in the movies, right, just.

Like in Marvel movies where like the bad guy shoots at the good guy and it's like time slows down so they can dodge it.

Yeah, exactly, just like in the matrix, they can make those crazy bends and dodge those bullets.

All right, Well, I guess then that's what happens when you collide to black holes. They sort of slowly reach out to each other they start to merge. You get a peanut shaped black hole, I guess, and then that eventually blots into a bigger black hole.

And some folks write and ask questions like is it possible for particles to escape the black hole during the merger, because they've heard that black holes shrink a little bit they radiate this energy away, and so like maybe when the black holes are combining, something can like sneak out the back right, which is a fun idea, but unfortunately no, black holes do not leak out any of this information when they merge. And the key thing to understand is that even though the mass of the two black holes is smaller than there's some the volume of a black hole grows very quickly with its mass. So even though the final mass is not just the sum of the incoming mass, the final volume can be like eight times the original black hole volume. So the event horizon is smaller than it would have been if it hadn't radiated gravitational radiation, but it's still bigger than either of the two black holes combined.

But you're saying, I think some things do sort of escape, right, Some information escapes, right, like even if it's a different form, in the form of gravitational waves. I think you were saying earlier that you know, you can learn a little bit of its history as stuff escapes, right, that's information, right.

Yeah, the gravitational waves contain information about the mass of the black hole and its location and its velocity. It doesn't tell you anything about what's going on inside. But you're right, from the shape of the event horizon, you can tell a little bit about the history of this black hole. And you're right, that's also encoded in the gravitational waves.

What if something was just like at the edge of the black hole as it was merging, could somehow, you know, get lucky and somehow, you know, as these things are merging, it maybe pools on the event horizon in such a way that somehow it gives you a little bit of a window for like one particle to like shoot out.

No, unfortunately not. That's what the event horizon means. The event horizon is not a physical surface. It's just like the location past which no information ever actually gets out, So you can't ask, like, is it possible for something to get out? Well, that's like, by definition, that's what the event horizon is. It's the point where nothing ever escapes, no information leaks out. That's how we figure out where the event horizon is for these things at any given moment. We look into the future history of these black holes in our simulation and say, where's the point past which nothing ever escapes?

Right? Right? I guess I'm thinking, like, you know, like if you're accelerating the black hole really fast, isn't it possible for something to escape? You know, like if I accelerate it the Earth really fast, the things on one side would be squished against the Earth, but maybe the things on the other side of the Earth might fly off and get left behind.

It's certainly true that if you did that to the Earth you would cause incredible damage. And I like the way you're thinking about really destructive experiments just to learn about the nature of the universe. Kudo's there, you really becoming a physicist. But if you did that to a black hole, would nothing would leak out of the event horizon. That black hole is enough curvature that even photons moving at the speed of light can't escape, and by accelerating the black hole can't make anything travel faster than the speed of life.

All right, seems like it's plausible. Well, but I think the main question is what happens when two black holes collide? And they sort of don't collide, right, They sort of smush together. I guess it's the simple answer, and they.

Sort of grow to meet each other, and for a few moments there you have a black hole that doesn't have a spherical event horizon, which is kind of an incredible revealing moment for the black hole.

Yeah, you get a peanut, I guess, peanut black hole. All right, Well, I think this really kind of points to some of the amazing things that can happen out there in the universe. You know, the situations with that are not just extreme, but it's like you take two extreme situations and you smash them together, you get like extra extreme.

The thing that amazes me is that we can do these calculations. People perform these simulations using numerical relativity tools. They describe these incredible, bonkers things that's happening, and then we can actually look out there in the universe and we see them. It really happens, and that makes you wonder, like, is this what's really going on out there? If I could fly out to the black hole and like watch it with my eyeballs, is this what I would see? You know? And I hope that one day eventually we can travel the universe and we don't have to just see these black holes from billions of light years away. We could see the these collisions close up.

Yeah, just make sure you bring some peanuts to snack on while you watch.

And smash your peanuts together with a chocolate bar and boom, you invented chocolate m and ms.

That's too extreme, Daniel.

Extreme snacking with Daniel and Jorge.

All right, Well, we hope you enjoyed that, And think about all the amazing things that are happening right now in the universe. Whose echoes we're hearing right now, that are washing through you right now and maybe telling you about what happened in that collision.

Think about all the things that are happening in the universe and sending us information that we don't even know about. That we're ignoring that future generations of scientists will discover and will use to learn incredible things about the universe.

Yeah, I mean there must have been hundreds or thousands or hundreds or thousands of black hole collisions, whose crash, whose mush sounds washed over humanity, but we never even knew.

We see a tiny, tiny fraction of the universe and we understand even less of it.

Thanks for joining us, See you next time.

Thanks for listening, and remember that Daniel and Jorge Explain the Universe is a production of iHeartRadio. For more podcasts from iHeartRadio, visit the iHeartRadio app, Apple Podcasts, or wherever you listen to your favorite shows. When you pop a piece of cheese into your mouth, you're probably not thinking about the environmental impact. But the people in the dairy industry are. That's why they're working hard every day to find new ways to reduce waste, conserve natural resources, and drive down greenhouse gas emissions. House US dairy tackling greenhouse gases, Many farms use anaerobic digestors to turn the methane from manure into renewable energy that can power farms, towns, and electric cars. Visit us Dairy dot COM's Last Sustainability to learn more.

There are children, friends, and families walking, riding on passing the roads every day. Remember they're real people with loved ones who need them.

To get home safely.

Protect our cyclists and pedestrians because they're people too. Go safely, California from the California Office of Traffic Safety and Caltrans.

Ryan Seacrest here.

When you have a busy schedule, it's important to maximize your downtime. One of the best ways to do that is by going to Chumbuckcasino dot com. Chumpbuck Casino has all your favorite social casino games like spin, slots, bingo, and Solitaire that you can play for free for a chance to redeem some serious prizes.

So hop on to Chumbuckcasino dot.

Com now and live the Chumba life sponsored by Chumpa Casino.

No purchase necessary.

VGW group void.

We're prohibited by Law eighteen plus.

Terms and conditions apply.

Daniel and Jorge Explain the Universe

A fun-filled discussion of the big, mind-blowing, unanswered questions about the Universe. In each e 
Social links
Follow podcast
Recent clips
Browse 637 clip(s)