WEBVTT - Staring into a Black Hole

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<v Speaker 1>Pushkin from Pushkin Industries. This is Deep Background, the show

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<v Speaker 1>where we explored the stories behind the stories in the news.

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<v Speaker 1>I'm Noah Feldman. The world has recently been gripped by

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<v Speaker 1>the extraordinary and extraordinarily beautiful image of a black hole,

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<v Speaker 1>a thing which we know allows no information or light

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<v Speaker 1>to escape, and of which we therefore, strictly speaking, shouldn't

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<v Speaker 1>have an image at all to make sense of this.

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<v Speaker 1>At the level of logic, at the level of physics,

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<v Speaker 1>and at the level of deeper meaning, we're thrilled to

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<v Speaker 1>have with us today. Andy Strominger one of the leading

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<v Speaker 1>theoretical physicists in the world who's made fundamental contributions to

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<v Speaker 1>quantum gravity theory, to string theory, and has also worked

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<v Speaker 1>extensively on black holes. Don't take my word for it

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<v Speaker 1>that and he's the right person to talk to. He's

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<v Speaker 1>one of every prize there is to win in the

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<v Speaker 1>space of theoretical physics. And Andy is also a director

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<v Speaker 1>of the Center for Fundamental Laws of Nature at Harvard.

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<v Speaker 1>On top of that, he's also one of the co

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<v Speaker 1>directors of the black Hole Initiative here at Harvard University

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<v Speaker 1>where I'm speaking to Andy today. Andy, thank you so

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<v Speaker 1>much for coming and joining great to be here. Ah. So, Andy,

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<v Speaker 1>let's just start with the image, which is a great

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<v Speaker 1>headline grabber and something that is extraordinarily beautiful, but which

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<v Speaker 1>strictly speaking, isn't a classic photographic image, whatever the world

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<v Speaker 1>may imagine. So say a word, if you will, about

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<v Speaker 1>what we are seeing, what it is, and then from

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<v Speaker 1>there we can move on to what it tells us. Okay, well,

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<v Speaker 1>I'd like to back up a little bit. It was

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<v Speaker 1>a hundred years ago that Einstein predicted with his equations

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<v Speaker 1>that there would be black holes, and people have been

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<v Speaker 1>arguing about them for most of the time, not believing

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<v Speaker 1>that they exist. Einstein wrote a paper nineteen thirty eight

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<v Speaker 1>saying black holes don't exist. Most people thought they didn't

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<v Speaker 1>exist until probably the seventies. And how they behave, what's

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<v Speaker 1>inside them, why they're there, has been a central debate

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<v Speaker 1>in physics for the last one hundred years. I have

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<v Speaker 1>spent the majority of my scientific career thinking about them,

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<v Speaker 1>trying to understand them, along with hundreds of other people,

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<v Speaker 1>and then all of a sudden to see it, to

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<v Speaker 1>see a picture of it, like Wow, that thing is real,

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<v Speaker 1>it's really it's really it's not. We're not the only

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<v Speaker 1>ones who have that. You could be the deepest specialist

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<v Speaker 1>and you're moved by it. I promise you that we

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<v Speaker 1>have a bunch bore. It rocked our worlds to like

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<v Speaker 1>see this thing that we've been talking about our whole lives.

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<v Speaker 1>So there it is, you know, even though you knew

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<v Speaker 1>it was there. We knew it was there. But there

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<v Speaker 1>is a big difference between knowing something's there and seeing it.

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<v Speaker 1>You know, maybe there was still that tidy bagging about

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<v Speaker 1>I don't know, but it really is great to see it.

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<v Speaker 1>It's a great thing actually to hear that from a physicist,

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<v Speaker 1>because when non physicists like me, mere lay people, we

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<v Speaker 1>instinctively have the feeling if we don't see something, maybe

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<v Speaker 1>it's not there. And then the physicists tell us it's

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<v Speaker 1>all equations, it's all logic, there are experiments that validate

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<v Speaker 1>these things. Take it on faith, you know, like you'll

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<v Speaker 1>never fully understand those things, but we know. And so

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<v Speaker 1>to hear that you too, or even you like to

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<v Speaker 1>actually see stuff as a kind of I don't know,

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<v Speaker 1>there's like some epistemological relief to me. And hearing that, yeah, yeah,

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<v Speaker 1>so what is it that we are in fact seeing

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<v Speaker 1>a black hole, by definition, is a region of space

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<v Speaker 1>and time from which no light escapes. So we're not

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<v Speaker 1>seeing light from the black hole. What we're really seeing

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<v Speaker 1>is light emitted by gases swirling around the black hole,

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<v Speaker 1>things that we don't understand very well. And we're seeing

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<v Speaker 1>the shadow of the black hole. So that dark spot

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<v Speaker 1>in the middle of that picture, the absence in the

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<v Speaker 1>middle of the breast, the absence in the middle of

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<v Speaker 1>the picture is where the black hole is. One of

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<v Speaker 1>the ways that was central too, or the main thing

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<v Speaker 1>that was central to making this telescope able to see

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<v Speaker 1>something so extraordinarily far away, was to turn the whole

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<v Speaker 1>Earth into a telescope. How does that work? We get

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<v Speaker 1>to the size of the Earth because we take about

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<v Speaker 1>eight different telescopes located at different points around the Earth

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<v Speaker 1>and we synchronize them and so it's of course not

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<v Speaker 1>a complete lens covering the entire Earth, but it's still

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<v Speaker 1>gives you a lot of resolving power if you can

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<v Speaker 1>just grab the light at those separate points. And as

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<v Speaker 1>an accomplishment, the creation of the image with all of

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<v Speaker 1>its coolness is scientifically significant. Why for several reasons. First

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<v Speaker 1>of all, it is in and of itself a spectacular

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<v Speaker 1>technical accomplishment, one that would not have been possible ten

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<v Speaker 1>years ago. It required many things. It required amazing improvements

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<v Speaker 1>in the accuracy of atomic clocks, um, it required uh,

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<v Speaker 1>bigger hard drives, bigger data processing capabilities, it recovered. I

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<v Speaker 1>read at one point that the data was so much

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<v Speaker 1>that it actually had to be flown from one place. Yeah,

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<v Speaker 1>because the Internet couldn't accommodated. Right at Sheep himself, I

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<v Speaker 1>saw lugging around these you know, discs with the you know,

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<v Speaker 1>he would go down to Mexico, go up to the

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<v Speaker 1>top of the mountain and lug lug it back. Of course,

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<v Speaker 1>the whole team was working on it. But Shep is

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<v Speaker 1>the director of is the direct and your your co

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<v Speaker 1>director at the black the director of this event Horizon

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<v Speaker 1>project at a great great scientist and uh, and the

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<v Speaker 1>algorithm has also gotten some attention and deserves some attention.

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<v Speaker 1>I take it produced by Katie Bowman, a recent post doc. Right, Yes,

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<v Speaker 1>there were of course, the whole there's there's a big

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<v Speaker 1>team of one hundred to two hundred people, and you know,

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<v Speaker 1>all this kind of big science is done in a

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<v Speaker 1>big teams and big teams now and it's it's the

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<v Speaker 1>only way it could can be done. But number one

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<v Speaker 1>of the big technical accomplishment. Number Two, there is the

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<v Speaker 1>importance of having seen these objects you know, that should

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<v Speaker 1>be shouldn't be underestimated. Number three, it's only the beginning. Um.

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<v Speaker 1>One of the things that struck me when I saw

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<v Speaker 1>the papers was, which I was not privy too before

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<v Speaker 1>the the general release, was how little actual observing time

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<v Speaker 1>they had when I first met Chapter ten fifteen years ago.

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<v Speaker 1>This project was you know, it was it was a

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<v Speaker 1>dark horse. It was it was not, you know, the

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<v Speaker 1>center of astronomical efforts. Um. And it was a funny idea,

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<v Speaker 1>but one that the more you thought about it, the

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<v Speaker 1>more since it made Why was it Why was that

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<v Speaker 1>just panenthetically? Why why wasn't it at the centerpiece of

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<v Speaker 1>as you say, black hole so crucial, so important and

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<v Speaker 1>seeing it would be a big deal, you know, because

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<v Speaker 1>it wasn't. There many ways it could have failed, right,

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<v Speaker 1>They had to increase their observational precision by many orders

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<v Speaker 1>of magnitude over whatever what anybody had ever seen. What

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<v Speaker 1>they did. It's like standing in Boston and reading the

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<v Speaker 1>data on a quarter in Los Angeles. That is, that

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<v Speaker 1>is the precision that they had to have to image

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<v Speaker 1>this black hole. The general public tends to forget, I

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<v Speaker 1>tend to forget that the funding of scientific projects is

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<v Speaker 1>always a kind of a bet or a gamble. It's

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<v Speaker 1>a beat, and when the odds of the success are

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<v Speaker 1>relatively low, the funders are skeptical about putting too much

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<v Speaker 1>money on that gamble. When people thought about it ten

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<v Speaker 1>or fifteen years ago, did they think, well, if we

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<v Speaker 1>get enough computing power, this is one of the things

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<v Speaker 1>will fix. And it's a question of whether we'll ever

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<v Speaker 1>get enough computing power, or was it rather a question

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<v Speaker 1>of other aspects of the technical difficulty of doing it.

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<v Speaker 1>He wasn't dismissed, and the thing was funded in it

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<v Speaker 1>and it did happen, but it was not obvious. It

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<v Speaker 1>was not obvious. You know, the Earth is just barely

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<v Speaker 1>big enough to image this thing. It's also very important

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<v Speaker 1>that the wavelength that they could access with this large

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<v Speaker 1>collator array is one in which there isn't a lot

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<v Speaker 1>of absorption between us and the black hole. You know

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<v Speaker 1>that there isn't a lot of dust that blocks the

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<v Speaker 1>light at that that wavelength. Right, So there were some

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<v Speaker 1>coincidence that you know, Luck smiled on the project. It

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<v Speaker 1>might not have been possible. I don't I doubt if

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<v Speaker 1>you get cheppy, you could ask him, but I doubt

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<v Speaker 1>he would have been certain you ten fifteen years go

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<v Speaker 1>that it would work. But I was going on to say,

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<v Speaker 1>they didn't get all that much observing time. Now clearly

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<v Speaker 1>they'll get more, right, there will be better resolution, more

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<v Speaker 1>observing time, they'll set one up out in space. So

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<v Speaker 1>there we are entering an era. So this is the

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<v Speaker 1>opening of that era of precision black hole astronomy. So

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<v Speaker 1>let's talk about now what we can see and what

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<v Speaker 1>we will see when we get more time, more observations,

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<v Speaker 1>and the emergence of what you described as a new

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<v Speaker 1>a new science really of precision black hole astronomy. You

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<v Speaker 1>with some collaborators have been actually making predictions the way

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<v Speaker 1>theoretical physicists like to do. You know, a theoretical physicist

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<v Speaker 1>makes predictions and sometimes they can be tested in his

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<v Speaker 1>or her lifetime. Sometimes it takes generations. In this instance,

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<v Speaker 1>you've made a series of observational predictions the things that

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<v Speaker 1>you expect can be picked up, and now that will

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<v Speaker 1>turn to whether they will in fact be be picked up,

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<v Speaker 1>which is dramatic and exciting. What kinds of predictions have

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<v Speaker 1>you already been making and when can we expect to

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<v Speaker 1>see results. I've been working with Alex Sasa, Delilah Gates,

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<v Speaker 1>and Dan Coppetts, and we are very interested in what

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<v Speaker 1>happens very near the horizon of of the black hole,

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<v Speaker 1>right at the edge of that inner shadow, and remind people,

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<v Speaker 1>just because it's never bad, to redefine it the event horizon. Yeah.

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<v Speaker 1>So the event horizon is the boundary of the region

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<v Speaker 1>of space time from which light rays connects escape. So

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<v Speaker 1>in practical terms, it's the edge of that you're inside

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<v Speaker 1>the event horizon, you're in the black holiness of the

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<v Speaker 1>black hole. Yeah. Once you go inside the event horizon,

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<v Speaker 1>you can never come out, and so your predictions relate

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<v Speaker 1>to what's happening at that edge, right. And one of

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<v Speaker 1>the things that we are very interesting in is that

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<v Speaker 1>black holes can spin around like a top and it's

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<v Speaker 1>believed that the M eighty seven, the black hole that

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<v Speaker 1>we've just seen, is spinning at light speed or very

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<v Speaker 1>near light speed. So there has been claims of this

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<v Speaker 1>from other kinds of measurements in the literature, and a

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<v Speaker 1>black hole which spins at light speed does some incredibly

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<v Speaker 1>peculiar things. Is you get near the edge of the

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<v Speaker 1>black hole, a long sort of funnel or wormhole forms.

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<v Speaker 1>It's kind of like a tornado with a long spout.

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<v Speaker 1>And as the black hole spins faster and faster, that's spout.

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<v Speaker 1>It sounds like I'm talking about sub sides fiction stuff.

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<v Speaker 1>But everything with respected black holes though, so go on

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<v Speaker 1>sounds like I'm talking about sizes fiction stuff. But we

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<v Speaker 1>maybe seeing this kind of black hole. Now the spout

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<v Speaker 1>or the wormhole that goes to the horizon, the black

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<v Speaker 1>hole actually becomes an infinitely long tube protruding out of

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<v Speaker 1>the out of space doot, and that will lead to

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<v Speaker 1>about to ask you where where the wormhole leads. But

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<v Speaker 1>if it's infinitely long, the answer is, yeah, it leads

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<v Speaker 1>to infinity. It goes, it leads to infinity. But before

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<v Speaker 1>it gets infinitely long where the wormhole leads it goes

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<v Speaker 1>into the rise of black hole, and once it crosses there,

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<v Speaker 1>we don't know. We don't know what's inside a black hole.

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<v Speaker 1>So the part of the wormhole is in the very

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<v Speaker 1>edge of the wormhole is at the event horizon, right

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<v Speaker 1>as it were, and then it extends infinitely away from

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<v Speaker 1>the black hole and connects on to the space time

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<v Speaker 1>that you and I live in, and that so we're

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<v Speaker 1>seeing into what does sound like science fiction. It does

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<v Speaker 1>sound like science fiction, but we're seeing it, you know,

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<v Speaker 1>And how would that be seen? I mean, what would

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<v Speaker 1>that as it were look like? We in our paper

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<v Speaker 1>gave some very specific predictions about what the polarization of

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<v Speaker 1>the light coming out will be. It's known that it's polarized.

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<v Speaker 1>Not that's coming from the black hole, but the lights, sorry,

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<v Speaker 1>the light and the halo. Yes, it's known that it's

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<v Speaker 1>polar polarized, but the distribution hasn't been extracted from the

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<v Speaker 1>data yet. I think they've already seen it. They have

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<v Speaker 1>these mountains of hard drives the data they need to process,

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<v Speaker 1>and they haven't extracted from that what the polarization is.

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<v Speaker 1>Luck will have to shine on us for Are there

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<v Speaker 1>measurements to be sufficient to prove what you've predicted? Yeah? Right,

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<v Speaker 1>because they weren't there looking for what you predicted. Well,

0:14:23.636 --> 0:14:28.316
<v Speaker 1>that's right, and also might not be this round might

0:14:28.396 --> 0:14:32.076
<v Speaker 1>not be a precise enough measurement for our prediction to

0:14:32.196 --> 0:14:38.196
<v Speaker 1>be verified or not. But I'd stress that our prediction

0:14:38.956 --> 0:14:42.636
<v Speaker 1>is a prediction of the Einstein equation. It's just the

0:14:42.716 --> 0:14:48.596
<v Speaker 1>Einstein equation in a very unusual circumstance, not like the

0:14:48.596 --> 0:14:52.276
<v Speaker 1>predictions that Einstein made, where the effects of general relativity

0:14:52.396 --> 0:14:55.356
<v Speaker 1>on the bending of light or in the Solar system

0:14:55.596 --> 0:14:59.556
<v Speaker 1>they were small effects. Yes here, it's huge effect. Here

0:14:59.556 --> 0:15:04.556
<v Speaker 1>it changes dramatically the nature of space and time, everything

0:15:04.556 --> 0:15:07.356
<v Speaker 1>that we really have to to somebody even reimagine what

0:15:07.436 --> 0:15:09.996
<v Speaker 1>we are, what we mean in ordinary language term. Yeah.

0:15:10.556 --> 0:15:14.636
<v Speaker 1>So we think that if you were to go in

0:15:14.676 --> 0:15:17.756
<v Speaker 1>a spaceship to near the horizon of M eighty seven,

0:15:18.356 --> 0:15:22.956
<v Speaker 1>you would be forced to whirl around it. You couldn't

0:15:22.996 --> 0:15:25.516
<v Speaker 1>just approach it straight on. There would be a force

0:15:25.636 --> 0:15:28.036
<v Speaker 1>by the warping of space time that would drag you

0:15:28.116 --> 0:15:32.756
<v Speaker 1>around like a tornado and pull you down this down

0:15:32.796 --> 0:15:36.076
<v Speaker 1>the drain into the down drain at the speed of

0:15:36.156 --> 0:15:40.556
<v Speaker 1>light through the wormhole. Yeah, bow the wormhole to the Yeah,

0:15:40.796 --> 0:15:42.636
<v Speaker 1>and it would grab you well before you got to

0:15:42.636 --> 0:15:45.916
<v Speaker 1>the event horizon. So, in practical terms, though it's outside

0:15:45.916 --> 0:15:48.436
<v Speaker 1>the event horizon, you're descent into the black hole would

0:15:48.436 --> 0:15:50.956
<v Speaker 1>begin a lot sooner than it. Otherwise it would be

0:15:51.876 --> 0:15:53.996
<v Speaker 1>if it were really spitting all the way at the

0:15:54.036 --> 0:15:56.596
<v Speaker 1>speed of light, it would grab you when you were

0:15:56.756 --> 0:16:00.156
<v Speaker 1>infinitely far away from the event horizon, but suck you

0:16:00.276 --> 0:16:04.356
<v Speaker 1>there in a finite amount of time by pulling you

0:16:04.436 --> 0:16:07.556
<v Speaker 1>up to the speed of light. But when you say

0:16:07.636 --> 0:16:09.116
<v Speaker 1>we grab you when so I'm just trying to get

0:16:09.156 --> 0:16:11.236
<v Speaker 1>my mind around this and not so much succeeding when

0:16:11.276 --> 0:16:14.596
<v Speaker 1>you say would grab you the reason you're infinitely far

0:16:14.636 --> 0:16:17.476
<v Speaker 1>away is that sounds as though, well, we're infinitely we're

0:16:17.476 --> 0:16:20.036
<v Speaker 1>at some distance less than infinitely far away from M

0:16:20.116 --> 0:16:21.876
<v Speaker 1>eighty seven right now. Why doesn't it grab up? Oh,

0:16:21.916 --> 0:16:25.636
<v Speaker 1>we don't know that, because we're not infinitely far away

0:16:26.396 --> 0:16:30.156
<v Speaker 1>from the edge of the wormhole, and the wormhole could

0:16:30.196 --> 0:16:33.476
<v Speaker 1>be infinitely long. I don't think it is. You'd have

0:16:33.516 --> 0:16:35.516
<v Speaker 1>to be going absolutely at the speed of light for

0:16:35.556 --> 0:16:37.396
<v Speaker 1>it to be infinitely long. But it could be very

0:16:37.476 --> 0:16:40.876
<v Speaker 1>very long, and so we could be much farther away

0:16:40.916 --> 0:16:44.356
<v Speaker 1>than it seems. I mean, the rest of the universe exists.

0:16:44.716 --> 0:16:47.356
<v Speaker 1>The rest of the universe is not presently I take

0:16:47.396 --> 0:16:53.276
<v Speaker 1>it currently captured by the wormhole right and spinning at

0:16:53.276 --> 0:16:56.196
<v Speaker 1>some very rapid speed around the black hole, and on

0:16:56.276 --> 0:16:58.756
<v Speaker 1>the way to the event horizon, we're not headed all

0:16:58.836 --> 0:17:01.436
<v Speaker 1>headed that way, I take it right. So my question

0:17:01.516 --> 0:17:07.036
<v Speaker 1>is why, Well, because we're far away week, but when

0:17:07.076 --> 0:17:10.676
<v Speaker 1>you get to some critical point instance, all of a

0:17:10.716 --> 0:17:17.316
<v Speaker 1>sudden it's a spinning black hole is surrounded by a

0:17:17.476 --> 0:17:21.716
<v Speaker 1>science fiction region which was discovered in the sixties called

0:17:21.716 --> 0:17:26.396
<v Speaker 1>the ergosphere. And life inside the ergosphere is very different

0:17:26.436 --> 0:17:30.276
<v Speaker 1>than life in this room, and existence rather than life,

0:17:30.276 --> 0:17:34.476
<v Speaker 1>because nothing's living once you get into the ergosphere. Anyone

0:17:34.516 --> 0:17:37.836
<v Speaker 1>who enters the ergosphere, which is still outside the black holes,

0:17:38.636 --> 0:17:42.876
<v Speaker 1>you you are forced to spin around in the in

0:17:42.916 --> 0:17:48.116
<v Speaker 1>the tornado vortex outside the black hole, and the wormhole

0:17:48.196 --> 0:17:51.316
<v Speaker 1>is a big extension of that. The wormhole is the

0:17:51.676 --> 0:17:54.276
<v Speaker 1>is the vortex going Yeah, it is the vortex going

0:17:54.316 --> 0:17:57.236
<v Speaker 1>down to the black hole. So we what we know

0:17:57.396 --> 0:18:00.036
<v Speaker 1>really is our distance from the mouth of the wormhole,

0:18:00.396 --> 0:18:04.916
<v Speaker 1>not how long the wormhole is. Now nobody thinks it's

0:18:04.916 --> 0:18:08.796
<v Speaker 1>infinitely long, but it could be long enough to be

0:18:08.836 --> 0:18:13.956
<v Speaker 1>in testing and long enough to make a signal. And

0:18:14.156 --> 0:18:17.956
<v Speaker 1>how how will the observation of the polarization of the

0:18:18.076 --> 0:18:21.436
<v Speaker 1>light that presently is visible at the edge of the

0:18:21.436 --> 0:18:24.556
<v Speaker 1>black hole get you to some better understanding of the

0:18:25.076 --> 0:18:28.516
<v Speaker 1>of the wormhole. Well, the worm it will verify the

0:18:28.556 --> 0:18:32.436
<v Speaker 1>existence of of the wormhole, I say. And the polarization

0:18:32.556 --> 0:18:34.996
<v Speaker 1>is not the only thing um. There are other things

0:18:34.996 --> 0:18:39.676
<v Speaker 1>that you might try to to to measure. Now I

0:18:39.796 --> 0:18:44.156
<v Speaker 1>stress it there. We're just one of and not even

0:18:44.196 --> 0:18:47.556
<v Speaker 1>the most important, what of many groups who are in

0:18:47.596 --> 0:18:51.076
<v Speaker 1>the vent Horizon telescope themselves are making predictions. Of course,

0:18:51.076 --> 0:18:54.876
<v Speaker 1>they had to compare their their theory to the theoretical

0:18:54.876 --> 0:18:59.396
<v Speaker 1>predictions to their observation to get their estimate that they

0:18:59.436 --> 0:19:03.836
<v Speaker 1>published of the mass. We are especially interested in some

0:19:03.916 --> 0:19:09.076
<v Speaker 1>of these novel aspects because first of all, because they're

0:19:09.316 --> 0:19:12.436
<v Speaker 1>weird and interesting and they're there and we're seeing them,

0:19:12.476 --> 0:19:17.916
<v Speaker 1>and also because they tie in with ideas about the

0:19:17.996 --> 0:19:21.236
<v Speaker 1>quantum structure of black holes and what's inside a black

0:19:21.276 --> 0:19:24.396
<v Speaker 1>hole in a very intricate way. And that question of

0:19:24.396 --> 0:19:29.916
<v Speaker 1>what's inside is hugely controversial and fascinating. So the question

0:19:29.956 --> 0:19:33.956
<v Speaker 1>of what's inside also philosophical, if I yeah, I venture

0:19:33.956 --> 0:19:37.756
<v Speaker 1>to use that word. There are philosophical aspects to it,

0:19:38.636 --> 0:19:42.596
<v Speaker 1>but there is a very sharp meaning to it because,

0:19:43.316 --> 0:19:48.556
<v Speaker 1>as Stephen Hawking showed, if you wait long enough and

0:19:48.756 --> 0:19:52.796
<v Speaker 1>even the you know, event Horizon team won't have this

0:19:52.956 --> 0:19:55.436
<v Speaker 1>much patience. I'd be like a very very long time,

0:19:56.796 --> 0:20:05.876
<v Speaker 1>the black hole will evaporate and what's inside using quantum

0:20:05.916 --> 0:20:10.556
<v Speaker 1>effects will come out. And then the question is would

0:20:10.596 --> 0:20:12.476
<v Speaker 1>the thing that came out, would what was inside to

0:20:12.516 --> 0:20:15.076
<v Speaker 1>come out and have some information? And then there is

0:20:15.116 --> 0:20:18.836
<v Speaker 1>an inside that we would ultimately see if we could

0:20:18.836 --> 0:20:24.436
<v Speaker 1>wait long enough, which I think, yeah, more than billions

0:20:24.676 --> 0:20:28.116
<v Speaker 1>moves it from philosophy to physics because there would because

0:20:28.116 --> 0:20:32.276
<v Speaker 1>it's not an unanswerable question. Well, it's a question people

0:20:32.276 --> 0:20:34.916
<v Speaker 1>could argue about. That's a separate, interesting question. What makes

0:20:34.916 --> 0:20:37.156
<v Speaker 1>something a physics question as opposed to philosopher ques I

0:20:37.236 --> 0:20:40.516
<v Speaker 1>was using a shorthand of imagining that physicists only like

0:20:40.636 --> 0:20:44.436
<v Speaker 1>questions that, in principle could be answered. It's a question

0:20:44.476 --> 0:20:47.516
<v Speaker 1>which can be answered with a goadoncan experiment when you're

0:20:47.516 --> 0:20:49.596
<v Speaker 1>do in your mind? Yes, I thought, you can't get

0:20:49.596 --> 0:20:52.836
<v Speaker 1>the funding to do it? Okay, right, So some people

0:20:52.836 --> 0:20:55.556
<v Speaker 1>would say infinite time, Well, you don't have infinite time.

0:20:55.876 --> 0:20:59.516
<v Speaker 1>Some people would say that physics is the study of

0:20:59.636 --> 0:21:03.156
<v Speaker 1>questions you could answer with real experiments that could be funded.

0:21:04.476 --> 0:21:07.396
<v Speaker 1>That's a pretty cramp though, view if it wouldn't cover

0:21:07.436 --> 0:21:10.356
<v Speaker 1>a lot of your your earlier work, wouldn't cover wouldn't

0:21:10.356 --> 0:21:11.956
<v Speaker 1>cover a lot of my work, right, And I think,

0:21:12.116 --> 0:21:13.676
<v Speaker 1>to be fair, I don't think that's what most non

0:21:13.716 --> 0:21:16.236
<v Speaker 1>physicists think. I think it's that would be a very

0:21:16.356 --> 0:21:19.596
<v Speaker 1>hard nosed, predictive, pragmatist view, and it's not physics if

0:21:19.596 --> 0:21:21.436
<v Speaker 1>I can't test it, you know, and get funding to

0:21:21.436 --> 0:21:24.076
<v Speaker 1>test it. Yea. The laws of nature presumably should be

0:21:24.636 --> 0:21:27.756
<v Speaker 1>resistant to being cabined by what we can fund. But

0:21:27.876 --> 0:21:31.156
<v Speaker 1>what's exciting to me here is that this observation is

0:21:31.236 --> 0:21:36.116
<v Speaker 1>touching the edge, possibly touching the edge of the things

0:21:36.156 --> 0:21:41.276
<v Speaker 1>that bearing on the issues of people that people think

0:21:41.316 --> 0:21:44.196
<v Speaker 1>about who want to understand what's really inside a black hole.

0:21:44.276 --> 0:21:48.116
<v Speaker 1>So you mentioned your friend Stephen Hawking, also your collaborator

0:21:48.916 --> 0:21:51.116
<v Speaker 1>who died not so long ago and with whom you

0:21:51.156 --> 0:21:52.796
<v Speaker 1>did a lot of work over the years, but most

0:21:52.836 --> 0:21:55.956
<v Speaker 1>recently you had been working on some pretty major projects

0:21:55.996 --> 0:21:58.556
<v Speaker 1>with him, also connected to black holes. Yeah, tell us

0:21:58.556 --> 0:22:02.876
<v Speaker 1>a little bit about that. Yes, Stephen, in his most

0:22:03.316 --> 0:22:08.876
<v Speaker 1>famous work in the Seven Daies, showed that with an

0:22:09.156 --> 0:22:13.156
<v Speaker 1>argument that is so simple and elegant that it has

0:22:13.236 --> 0:22:19.676
<v Speaker 1>never been seriously questioned that when you include quantum effects,

0:22:20.596 --> 0:22:26.796
<v Speaker 1>black holes are not completely black. That quantum effects allow

0:22:26.876 --> 0:22:31.156
<v Speaker 1>a sort of the uncertainty principle about where the horizon

0:22:31.196 --> 0:22:35.956
<v Speaker 1>of the black hole is allows a small amount of

0:22:36.036 --> 0:22:40.196
<v Speaker 1>light and matter to slowly trickle out of the of

0:22:40.196 --> 0:22:44.276
<v Speaker 1>a black hole a very slow rate. So those are

0:22:44.276 --> 0:22:46.796
<v Speaker 1>big things, and let me try a very very lay

0:22:46.836 --> 0:22:51.316
<v Speaker 1>person's attempt to make sense of that. If we imagined

0:22:52.196 --> 0:22:56.756
<v Speaker 1>determinative locations and laws of physics, then nothing escapes the

0:22:56.796 --> 0:22:59.116
<v Speaker 1>black hole. That's what makes it a black hole. But

0:23:00.036 --> 0:23:03.756
<v Speaker 1>one of the key points of quantum theory is it

0:23:03.916 --> 0:23:09.076
<v Speaker 1>precisely you can't pin down the exact location of every

0:23:09.276 --> 0:23:12.836
<v Speaker 1>quantum phenomenon. And since you can't pin it down exactly,

0:23:13.196 --> 0:23:16.676
<v Speaker 1>that puts enough wiggle room, if you will, into the

0:23:16.796 --> 0:23:19.876
<v Speaker 1>equation that there is some information in the black hole

0:23:19.916 --> 0:23:22.636
<v Speaker 1>that might be capable of being discovered. How's that for

0:23:22.676 --> 0:23:25.796
<v Speaker 1>a first order? That's right. So quantum mechanics says that

0:23:25.916 --> 0:23:31.396
<v Speaker 1>the horizon and the black hole must fluctuate around a

0:23:31.436 --> 0:23:34.756
<v Speaker 1>little bit, according must be slightly uncertain, and so that

0:23:36.316 --> 0:23:40.116
<v Speaker 1>gives just enough wiggle room for a few quantum particles

0:23:40.156 --> 0:23:44.636
<v Speaker 1>to escape from inside the black hole at a slow rate,

0:23:45.036 --> 0:23:49.596
<v Speaker 1>so that you began with describing Hawking's famous nineteen seventies

0:23:49.916 --> 0:23:52.796
<v Speaker 1>that was forty years ago, yep. And he gave an

0:23:52.876 --> 0:23:59.996
<v Speaker 1>argument that the information about how the black hole was

0:24:00.116 --> 0:24:05.636
<v Speaker 1>made would not escape, would not come out with this

0:24:05.796 --> 0:24:09.596
<v Speaker 1>leak of energy and particles and so on. Things would

0:24:09.636 --> 0:24:11.916
<v Speaker 1>come out, but not the information about how the black

0:24:11.916 --> 0:24:16.876
<v Speaker 1>black hole came to be made. He claimed, the present

0:24:17.236 --> 0:24:21.876
<v Speaker 1>does not determine the future and cannot, even in principle,

0:24:22.036 --> 0:24:25.716
<v Speaker 1>be used to reconstruct the past. Bad news for historians,

0:24:26.356 --> 0:24:28.636
<v Speaker 1>bad news for hystories for people who like free will

0:24:28.636 --> 0:24:33.396
<v Speaker 1>in the future maybe, but bad news for physicists because

0:24:33.636 --> 0:24:37.196
<v Speaker 1>it's equivalent to saying there aren't absolute laws of physics,

0:24:37.596 --> 0:24:40.996
<v Speaker 1>because a law of physics is supposed to predict the

0:24:41.036 --> 0:24:44.436
<v Speaker 1>future from the present. It was a very simple argument,

0:24:45.516 --> 0:24:49.716
<v Speaker 1>and people didn't like the conclusion. It had been questioned

0:24:49.756 --> 0:24:54.436
<v Speaker 1>in many different ways, but none of the ways in

0:24:54.476 --> 0:24:58.876
<v Speaker 1>which it was questioned really stuck. So a few years

0:24:58.876 --> 0:25:05.636
<v Speaker 1>ago I found, while investigating other problems in physics, I

0:25:05.796 --> 0:25:10.836
<v Speaker 1>came across what seemed to be an error in the

0:25:10.876 --> 0:25:18.596
<v Speaker 1>original flawed assumption in his original reasoning. Moreover, the nature

0:25:19.116 --> 0:25:24.556
<v Speaker 1>of the flaw suggested a research program for understanding what

0:25:24.876 --> 0:25:32.916
<v Speaker 1>really did happen. And I explained this to Stephen and

0:25:33.276 --> 0:25:36.196
<v Speaker 1>he was very excited about it, and I just say,

0:25:36.276 --> 0:25:38.756
<v Speaker 1>this is also it's a great model of what scientific

0:25:38.756 --> 0:25:43.156
<v Speaker 1>collaboration can be and isn't always You find a flaw

0:25:43.276 --> 0:25:47.396
<v Speaker 1>in an important claim by another famous physicist and you

0:25:47.476 --> 0:25:51.356
<v Speaker 1>call him up and you say, hey, there's a problem,

0:25:51.516 --> 0:25:54.436
<v Speaker 1>and that's collegial of you, and then he responds positively,

0:25:54.436 --> 0:25:56.236
<v Speaker 1>and that's collegial of him. This is the way it's

0:25:56.236 --> 0:25:59.876
<v Speaker 1>supposed to work in the textbooks. Yeah, and it really

0:25:59.916 --> 0:26:03.076
<v Speaker 1>does work this way for the for the most part. Yeah,

0:26:03.156 --> 0:26:05.676
<v Speaker 1>it's heartwarming. It's not like this in my end of

0:26:05.716 --> 0:26:08.276
<v Speaker 1>the academy. I promise you that. Well, it may be

0:26:08.396 --> 0:26:10.316
<v Speaker 1>related to the fact that there's no money in my

0:26:10.436 --> 0:26:14.036
<v Speaker 1>branch of science. I know there's a there's a there's

0:26:14.036 --> 0:26:18.996
<v Speaker 1>a money in those prizes. But go on. So he

0:26:19.116 --> 0:26:23.436
<v Speaker 1>and I and his colleague Malcolm Perry, he had some

0:26:23.476 --> 0:26:25.996
<v Speaker 1>ideas about how to proceed on this and to make

0:26:26.036 --> 0:26:29.676
<v Speaker 1>sense of it, and so we began a very active

0:26:29.756 --> 0:26:33.796
<v Speaker 1>and productive collaboration which went on for the last three

0:26:33.876 --> 0:26:38.516
<v Speaker 1>years with life and we're pushing forward in that direction.

0:26:38.556 --> 0:26:43.636
<v Speaker 1>It's looking promising, but we haven't delivered the goods, right.

0:26:43.756 --> 0:26:48.756
<v Speaker 1>We don't know yet that there isn't some reason this

0:26:48.876 --> 0:26:54.236
<v Speaker 1>is a technical issue rather than the fundamental right. When

0:26:54.276 --> 0:26:57.636
<v Speaker 1>you were describing how you came up with the original

0:26:57.676 --> 0:27:00.756
<v Speaker 1>thought that led to this collaboration, my reaction was you

0:27:00.796 --> 0:27:03.196
<v Speaker 1>were describing how you were thinking about something else in physics,

0:27:03.276 --> 0:27:06.996
<v Speaker 1>and then you hit upon reason to think that one

0:27:06.996 --> 0:27:09.556
<v Speaker 1>of Hawking's original assumptions was inaccurate. And it's struck me

0:27:09.716 --> 0:27:12.716
<v Speaker 1>that's a very andy way to go about things. One

0:27:12.716 --> 0:27:17.436
<v Speaker 1>of the key features of your contributions across the whole

0:27:17.516 --> 0:27:20.716
<v Speaker 1>range of areas where you've worked is that you find

0:27:20.836 --> 0:27:25.876
<v Speaker 1>and see correspondences between different areas of thought physics, math

0:27:26.396 --> 0:27:29.916
<v Speaker 1>that other people have never hit upon before. That's like

0:27:29.996 --> 0:27:32.756
<v Speaker 1>the Andy move, as it were, and it's quite a move.

0:27:33.156 --> 0:27:35.636
<v Speaker 1>So well, I don't think I have a pattern on

0:27:35.676 --> 0:27:37.996
<v Speaker 1>this move. But it's the structure of the field the

0:27:38.036 --> 0:27:44.956
<v Speaker 1>physics is. You know, there's many It's interconnected in surprising ways,

0:27:45.436 --> 0:27:49.916
<v Speaker 1>and it often happens. Maybe I'm lucky enough that it

0:27:49.996 --> 0:27:53.836
<v Speaker 1>happens to enough times that I'm not sure it looks

0:27:53.876 --> 0:27:56.756
<v Speaker 1>like a coincidence, but maybe coincidental in nature, but it's

0:27:56.796 --> 0:28:00.516
<v Speaker 1>not coincidental in you. But anyway, go on, and you know,

0:28:00.676 --> 0:28:04.596
<v Speaker 1>maybe one could say, you know, our creator didn't have

0:28:04.676 --> 0:28:08.756
<v Speaker 1>so many ideas that he kept using the same one

0:28:08.836 --> 0:28:12.836
<v Speaker 1>over overget and you solve a problem in one area

0:28:12.956 --> 0:28:17.516
<v Speaker 1>and it has a translation into another area. So that

0:28:17.636 --> 0:28:20.276
<v Speaker 1>hints at a kind of set of structures of unity.

0:28:20.276 --> 0:28:22.476
<v Speaker 1>I mean, you're sort of kidding about reusing the same idea.

0:28:22.676 --> 0:28:25.196
<v Speaker 1>What you really mean is that there is an underlying

0:28:25.276 --> 0:28:29.236
<v Speaker 1>unity and we are describing different parts of reality in

0:28:29.276 --> 0:28:31.996
<v Speaker 1>different ways. We've got these mathematical tools or these physics

0:28:32.036 --> 0:28:35.716
<v Speaker 1>tools to describe something, but we're actually describing a more

0:28:35.876 --> 0:28:41.996
<v Speaker 1>unified underlying phenomenon. Yeah, we have many ideas and we

0:28:42.076 --> 0:28:45.316
<v Speaker 1>often don't realize that they're the same idea. And is

0:28:45.356 --> 0:28:50.076
<v Speaker 1>it your belief that there is some directionality here? I mean,

0:28:50.636 --> 0:28:53.436
<v Speaker 1>now I'm aiming for something bigger, as it were, even

0:28:53.476 --> 0:28:57.196
<v Speaker 1>bigger than you know, than the wormhole and the black hole?

0:28:57.956 --> 0:29:02.116
<v Speaker 1>Are you a believer in direction in physics towards more

0:29:02.156 --> 0:29:05.876
<v Speaker 1>and more unification of our theoretical knowledge? Sometimes people talk

0:29:05.876 --> 0:29:08.596
<v Speaker 1>about a grand unified theory string theory, to which you've

0:29:08.596 --> 0:29:11.916
<v Speaker 1>made fundamental contributions. Is sometimes described as a step in

0:29:11.956 --> 0:29:13.996
<v Speaker 1>the direction of a grand unified theory or an aspiration

0:29:13.996 --> 0:29:16.356
<v Speaker 1>in that direction. I'm asking you to put it along

0:29:16.356 --> 0:29:21.996
<v Speaker 1>the line here. You know, the honest answer to that

0:29:22.116 --> 0:29:27.796
<v Speaker 1>question is, I don't know. People work in different ways.

0:29:28.836 --> 0:29:34.676
<v Speaker 1>Some people have beliefs that they think that that is

0:29:35.156 --> 0:29:42.196
<v Speaker 1>how nature works, and they relentlessly pursue demonstrating the physical

0:29:42.276 --> 0:29:49.436
<v Speaker 1>reality of their beliefs. Others just take the mathematical equations

0:29:49.436 --> 0:29:54.156
<v Speaker 1>and follow them and see where they lead. And you

0:29:54.196 --> 0:29:58.996
<v Speaker 1>see yourself in the latter camp. I'm somewhere in between.

0:29:59.196 --> 0:30:03.196
<v Speaker 1>I have things I believe in, but I pride myself

0:30:04.156 --> 0:30:08.076
<v Speaker 1>in being ready to drop my beliefs when they don't

0:30:08.116 --> 0:30:11.796
<v Speaker 1>measure up to the equation. The equations are the final arbiters.

0:30:11.836 --> 0:30:14.516
<v Speaker 1>The equations and the experiments are the final arbiters of

0:30:14.556 --> 0:30:21.796
<v Speaker 1>truth in our field, and many people have, including you

0:30:21.836 --> 0:30:27.796
<v Speaker 1>know Einstein. Einstein had very strong beliefs about how things

0:30:28.316 --> 0:30:35.156
<v Speaker 1>should be should be, and that got him through special relativity,

0:30:35.276 --> 0:30:40.316
<v Speaker 1>general relativity, and the beginnings of quantum mechanics. But then

0:30:40.396 --> 0:30:43.876
<v Speaker 1>he had beliefs about the way the world should be

0:30:44.636 --> 0:30:47.876
<v Speaker 1>that were being countermanded that we're being own by his

0:30:47.956 --> 0:30:51.756
<v Speaker 1>own equations, and then the experiments that were validating those equations,

0:30:51.796 --> 0:30:56.276
<v Speaker 1>and that reduced his his his productivity. M He did

0:30:56.316 --> 0:30:59.196
<v Speaker 1>pretty well, He did pretty well. Then he did pretty well.

0:30:59.236 --> 0:31:01.596
<v Speaker 1>But at some point he believed things that weren't true.

0:31:01.756 --> 0:31:05.196
<v Speaker 1>He believed that quantum mechanics was wrong. He believed their

0:31:05.196 --> 0:31:08.276
<v Speaker 1>word black holes, he believed their word gravity weight. You know,

0:31:08.316 --> 0:31:11.836
<v Speaker 1>he had some raw beef, wrong beliefs that he got

0:31:11.836 --> 0:31:14.556
<v Speaker 1>stuck on. So it interfered with his being able to

0:31:14.596 --> 0:31:16.636
<v Speaker 1>move on to make the next set of He might

0:31:16.676 --> 0:31:18.796
<v Speaker 1>have come up with even more fundamental things if he

0:31:18.796 --> 0:31:21.196
<v Speaker 1>had been able to keep on pushing. That's right, that's right.

0:31:21.316 --> 0:31:24.196
<v Speaker 1>So that's an argument that you may need some beliefs

0:31:24.196 --> 0:31:26.516
<v Speaker 1>to get you started. Yeah, but there needs to be

0:31:26.556 --> 0:31:28.756
<v Speaker 1>some kind of a reflective equilibrium where at some point

0:31:28.796 --> 0:31:32.316
<v Speaker 1>you have to start believing your equations. Yeah, you know,

0:31:32.596 --> 0:31:39.196
<v Speaker 1>it's always a conflict between sticking with what you believe

0:31:39.236 --> 0:31:44.756
<v Speaker 1>in and not giving up, and being too stubborn and

0:31:44.876 --> 0:31:47.916
<v Speaker 1>not being flexible enough. The real truth is it takes

0:31:47.956 --> 0:31:51.516
<v Speaker 1>all types. You know, there's some people who have an

0:31:51.556 --> 0:31:58.996
<v Speaker 1>idea and pursue it in the face of unreasonable hardship

0:31:59.036 --> 0:32:02.556
<v Speaker 1>and difficulty, and everybody's saying no, and everybody's saying no,

0:32:03.196 --> 0:32:04.956
<v Speaker 1>and some of those people turn out to be right.

0:32:04.996 --> 0:32:07.476
<v Speaker 1>Now people turn out to be right, but most of

0:32:07.476 --> 0:32:10.916
<v Speaker 1>them fall by the way side. Yeah, you need some

0:32:10.996 --> 0:32:14.436
<v Speaker 1>of You need people with unreasonable beliefs. You need people

0:32:14.596 --> 0:32:16.836
<v Speaker 1>who are ready to drop their beliefs. You know, it

0:32:16.836 --> 0:32:19.956
<v Speaker 1>takes a village. Let me ask a final question about

0:32:20.636 --> 0:32:24.436
<v Speaker 1>how these different pathways to understanding the world are going

0:32:24.436 --> 0:32:27.836
<v Speaker 1>to play out in the black hole context. Yea. When

0:32:27.836 --> 0:32:31.076
<v Speaker 1>you started working on black holes, as you said, there

0:32:31.196 --> 0:32:33.156
<v Speaker 1>was still a view among lots of people that there

0:32:33.196 --> 0:32:36.196
<v Speaker 1>were no such things right, and now we're in a

0:32:36.356 --> 0:32:40.196
<v Speaker 1>very different place. We've seen one. Yeah, does that take

0:32:40.596 --> 0:32:43.516
<v Speaker 1>some of the thrill out of it? Does it seem

0:32:44.316 --> 0:32:47.116
<v Speaker 1>you know? I mean, it's nice to be right, But

0:32:47.316 --> 0:32:50.156
<v Speaker 1>there seems like there's a stage of, as you said,

0:32:50.836 --> 0:32:54.916
<v Speaker 1>great observational astronomy in the space of black holes, which

0:32:54.956 --> 0:32:58.236
<v Speaker 1>is important and will expand our knowledge and maybe give

0:32:58.316 --> 0:33:01.836
<v Speaker 1>us radically new ideas about the world. But somehow seems

0:33:01.876 --> 0:33:04.836
<v Speaker 1>to be confirmatory of what you and others predicted and

0:33:05.036 --> 0:33:07.876
<v Speaker 1>what is actually now believed to be true. Is there

0:33:07.916 --> 0:33:11.596
<v Speaker 1>some it takes. I mean it's thrilling now, but ten

0:33:11.676 --> 0:33:13.476
<v Speaker 1>years from now, will some of the thrill will be

0:33:13.556 --> 0:33:18.476
<v Speaker 1>gone in working on something which everyone acknowledges exists. No,

0:33:20.436 --> 0:33:23.516
<v Speaker 1>I think it's only getting more interesting. We can think

0:33:23.596 --> 0:33:27.876
<v Speaker 1>of this. The last few years, or this observation even

0:33:28.396 --> 0:33:31.316
<v Speaker 1>is kind of a historical marker. You know, a hundred

0:33:31.356 --> 0:33:37.236
<v Speaker 1>years ago the existence of black holes was predicted. Now

0:33:37.316 --> 0:33:42.116
<v Speaker 1>they've been seen in the most straightforward way. So going

0:33:42.196 --> 0:33:46.596
<v Speaker 1>forward there will be better and better observations. But we

0:33:46.716 --> 0:33:53.116
<v Speaker 1>still have this huge puzzle. Yeah, the godon Can experient.

0:33:53.236 --> 0:33:56.436
<v Speaker 1>What is the result of the Godonkan experiment? What's coming

0:33:56.436 --> 0:34:00.196
<v Speaker 1>out of the black hole? Or equivalently, what is inside

0:34:00.196 --> 0:34:04.676
<v Speaker 1>the black hole? Then you know there's a fundamental contradiction

0:34:04.756 --> 0:34:08.396
<v Speaker 1>in the laws of physics as we currently understand them.

0:34:08.436 --> 0:34:10.836
<v Speaker 1>So that's what makes it so exciting. Something has to give.

0:34:10.956 --> 0:34:14.116
<v Speaker 1>It's that the thought experiment poses a contradiction between different

0:34:14.116 --> 0:34:17.716
<v Speaker 1>things that we're we are committed to. All the things

0:34:17.836 --> 0:34:21.836
<v Speaker 1>that we believe to be true. Can't all be true.

0:34:22.356 --> 0:34:26.236
<v Speaker 1>Something which we are completely at this moment unwilling to

0:34:26.276 --> 0:34:32.156
<v Speaker 1>give up as a truth about the universe must actually

0:34:32.196 --> 0:34:36.796
<v Speaker 1>be wrong, and the fact that that contradictions was recognized

0:34:36.916 --> 0:34:40.356
<v Speaker 1>forty years ago by Hawking and has sat there. As

0:34:40.356 --> 0:34:43.076
<v Speaker 1>the years have gone by, the longer it's sat there,

0:34:43.436 --> 0:34:47.476
<v Speaker 1>the more that we've realized what central importance it is.

0:34:48.196 --> 0:34:54.996
<v Speaker 1>So somehow the observational astronomy world and the theoretical physics

0:34:54.996 --> 0:35:00.876
<v Speaker 1>worlds have converged on black holes as the most interesting

0:35:00.916 --> 0:35:07.796
<v Speaker 1>and things around and it is. I'm pretty confident that well,

0:35:07.796 --> 0:35:11.036
<v Speaker 1>first of all, I there's no reason we can't ultimately

0:35:11.076 --> 0:35:14.876
<v Speaker 1>solve this problem. And the fact that it has sat

0:35:14.956 --> 0:35:19.596
<v Speaker 1>there for so long, I think there is a consensus

0:35:19.636 --> 0:35:24.956
<v Speaker 1>in the community that we can't solve the problem without

0:35:24.996 --> 0:35:29.716
<v Speaker 1>a fundamental new insight into the structure of the universe

0:35:30.276 --> 0:35:36.836
<v Speaker 1>at the same revolutionary level as quantum mechanics or relativity.

0:35:36.876 --> 0:35:39.556
<v Speaker 1>That it's not a technical problem that we missed a

0:35:39.636 --> 0:35:42.476
<v Speaker 1>factor of two somewhere. So that's the holy grail. That

0:35:42.916 --> 0:35:48.556
<v Speaker 1>is the holy grail. It's an exciting thing that black

0:35:48.596 --> 0:35:53.276
<v Speaker 1>holes have become come to center stage and observational astronomy

0:35:53.556 --> 0:35:57.396
<v Speaker 1>at the same time as in theoretical physics. We don't

0:35:57.516 --> 0:36:00.276
<v Speaker 1>have a roadmap how we're going to talk to each

0:36:00.276 --> 0:36:05.276
<v Speaker 1>other and close that gap. But we're thinking here on

0:36:05.276 --> 0:36:07.556
<v Speaker 1>a hundred year time scale, we might not even have

0:36:07.596 --> 0:36:10.396
<v Speaker 1>found the city where the whole grail is hidden, but

0:36:10.436 --> 0:36:13.036
<v Speaker 1>we've maybe found the continent, and now we're gonna have

0:36:13.036 --> 0:36:15.836
<v Speaker 1>to keep exploring. But it's a pretty big deal to

0:36:15.916 --> 0:36:18.396
<v Speaker 1>have found the continent. That's a big deal to have

0:36:18.396 --> 0:36:20.876
<v Speaker 1>found the kind we know where we're looking and now.

0:36:21.036 --> 0:36:23.076
<v Speaker 1>And I think you know, Although I'm loath to draw

0:36:23.156 --> 0:36:28.036
<v Speaker 1>too many non physics metaphoric conclusion from physics, the idea

0:36:28.076 --> 0:36:31.316
<v Speaker 1>that sometimes we're in the grips of contradictory views and

0:36:31.396 --> 0:36:34.676
<v Speaker 1>something's got to give, we need some new account to

0:36:34.716 --> 0:36:36.916
<v Speaker 1>make it work out is about as good a lesson

0:36:37.236 --> 0:36:40.876
<v Speaker 1>to take away from black Holes as I can imagine. Andy,

0:36:40.916 --> 0:36:43.596
<v Speaker 1>thank you so so much for your for your brilliant

0:36:43.596 --> 0:36:51.436
<v Speaker 1>thoughts in your time. Thank you Eddie, thank you Noah.

0:36:51.796 --> 0:36:53.916
<v Speaker 1>When I see an image like the image of the

0:36:53.956 --> 0:36:58.516
<v Speaker 1>black hole, I'm filled with wonderment. The mere accomplishment of

0:36:58.596 --> 0:37:01.116
<v Speaker 1>human beings, to be able to see something so far away,

0:37:01.476 --> 0:37:03.956
<v Speaker 1>to conceive of it, to make sense of it. That's

0:37:03.956 --> 0:37:05.876
<v Speaker 1>the kind of thing that really hits me where I live.

0:37:05.996 --> 0:37:09.796
<v Speaker 1>It makes me believe that being human is actually worth something.

0:37:09.876 --> 0:37:13.556
<v Speaker 1>After all, we can actually know things and achieve connection.

0:37:14.396 --> 0:37:16.956
<v Speaker 1>But you know what, when I listen to Andy, somebody

0:37:16.956 --> 0:37:19.676
<v Speaker 1>who actually understands at the most profound level what these

0:37:19.676 --> 0:37:23.116
<v Speaker 1>discoveries are, I'm even more struck by the wonderment that

0:37:23.276 --> 0:37:26.636
<v Speaker 1>he feels than the wonderment that I feel. He's not

0:37:26.756 --> 0:37:30.516
<v Speaker 1>jaded at all. He spent a lifetime working on black holes,

0:37:30.636 --> 0:37:33.276
<v Speaker 1>and to him, where at the crossroads of excitement where

0:37:33.316 --> 0:37:37.036
<v Speaker 1>things are only going to keep on getting better. That's

0:37:37.116 --> 0:37:42.996
<v Speaker 1>genuine scientific exploration. That's genuine scientific collegiality and collaboration like

0:37:43.036 --> 0:37:46.036
<v Speaker 1>the kind that Andy has done with Stephen Hawking. And

0:37:46.116 --> 0:37:48.156
<v Speaker 1>it makes you think not just that the universe is

0:37:48.156 --> 0:37:52.396
<v Speaker 1>an amazing place, but maybe we at our best when

0:37:52.396 --> 0:37:55.116
<v Speaker 1>we're not fighting and we're searching for the truth. Are

0:37:55.116 --> 0:38:03.396
<v Speaker 1>in such bad people? After all? Deep Background is brought

0:38:03.396 --> 0:38:06.596
<v Speaker 1>to you by Pushkin Industries. Our producer is Lydia Geane Coott,

0:38:06.676 --> 0:38:10.796
<v Speaker 1>with engineering by Jason Gambrell and Jasonstkowski. Our showrunner is

0:38:10.796 --> 0:38:13.836
<v Speaker 1>Sophie mckibbon. Our theme music is composed by Luis GERA

0:38:14.396 --> 0:38:17.876
<v Speaker 1>special thanks to the Pushkin Brass Malcolm Gladwell, Jacob Weisberg

0:38:17.876 --> 0:38:20.676
<v Speaker 1>and Mia Lobel. I'm Noah Feldman. You can follow me

0:38:20.716 --> 0:38:24.316
<v Speaker 1>on Twitter at Noah R. Feldman. This is deep background