1 00:00:08,520 --> 00:00:11,320 Speaker 1: Hey, Daniel, I've got a black hole question for you. 2 00:00:11,400 --> 00:00:13,680 Speaker 1: Are you still hoping to catch and raise a black 3 00:00:13,680 --> 00:00:16,080 Speaker 1: hole as a pet in your backyard? I can't confirm 4 00:00:16,200 --> 00:00:19,239 Speaker 1: or deny that, But my question is what happens to 5 00:00:19,239 --> 00:00:21,720 Speaker 1: the stuff I put into the black hole? Is this 6 00:00:21,760 --> 00:00:24,079 Speaker 1: a question you already asked the folks at pet Smart. Yeah. 7 00:00:24,079 --> 00:00:26,160 Speaker 1: You know, like, say, if I drop a banana into 8 00:00:26,239 --> 00:00:28,920 Speaker 1: a black hole, what what happens to it? Is it 9 00:00:29,160 --> 00:00:32,480 Speaker 1: gone forever? My advice is don't do it? Which part 10 00:00:32,600 --> 00:00:35,360 Speaker 1: raise a black hole or throw a banana into it? 11 00:00:36,040 --> 00:00:39,000 Speaker 1: Because I may have done both already. What's the difference? 12 00:00:39,000 --> 00:00:41,520 Speaker 1: I mean, if you feed a black hole, it will grow, 13 00:00:42,040 --> 00:00:44,280 Speaker 1: and a growing black hole will eat more, and eventually 14 00:00:44,600 --> 00:00:46,960 Speaker 1: it will eat your house and then mine. Okay, so 15 00:00:47,120 --> 00:00:49,159 Speaker 1: it's not a good idea to use a black hole 16 00:00:49,240 --> 00:01:09,039 Speaker 1: to make banana's booties. Officially, no, not a good idea. Hi, 17 00:01:09,080 --> 00:01:11,080 Speaker 1: I'm poor. Hey, I'm a cartoonist and the creator of 18 00:01:11,160 --> 00:01:14,720 Speaker 1: PhD comics. Hi, I'm Daniel. I'm a particle physicist, and 19 00:01:14,760 --> 00:01:17,679 Speaker 1: I have never created a black hole to my knowledge. 20 00:01:17,959 --> 00:01:19,880 Speaker 1: How do you know, Daniel? Maybe you do it in 21 00:01:19,880 --> 00:01:22,360 Speaker 1: your sleep by accident. Hey, I can't be responsible for 22 00:01:22,400 --> 00:01:26,000 Speaker 1: all incidental black holes I accidentally create, right, I mean, 23 00:01:26,040 --> 00:01:28,000 Speaker 1: there's got to be some legal principle there. Do you 24 00:01:28,000 --> 00:01:30,400 Speaker 1: ever take homes any work by accident, you know, like 25 00:01:30,640 --> 00:01:33,320 Speaker 1: you guys suddenly bring home some particles or some black 26 00:01:33,360 --> 00:01:35,840 Speaker 1: holes that were created at the LHC. Yeah, sometimes I 27 00:01:35,880 --> 00:01:37,920 Speaker 1: go home with a few extra protons in my pocket. 28 00:01:38,240 --> 00:01:42,600 Speaker 1: Nobody even notices that doesn't sound good. But welcome to 29 00:01:42,600 --> 00:01:45,720 Speaker 1: our podcast, Daniel and Jorge Explain the Universe, a production 30 00:01:45,880 --> 00:01:48,000 Speaker 1: of I Heart Radio, in which we tell you all 31 00:01:48,040 --> 00:01:52,360 Speaker 1: about the mysteries of the university, incredible cosmic questions that 32 00:01:52,600 --> 00:01:56,320 Speaker 1: still make scientists puzzled, the things that we all wonder 33 00:01:56,360 --> 00:01:59,560 Speaker 1: about this incredible, beautiful universe that we live in that 34 00:01:59,600 --> 00:02:02,960 Speaker 1: we all desperately like to understand. Yeah. I take home 35 00:02:03,120 --> 00:02:05,880 Speaker 1: work all the time, Daniel, because I work from home 36 00:02:06,040 --> 00:02:08,280 Speaker 1: my cartoonist. So I think you take your home to 37 00:02:08,360 --> 00:02:12,520 Speaker 1: work then, don't you You know the tomato tomato, it's 38 00:02:12,520 --> 00:02:14,840 Speaker 1: all the same thing. But that's right. This is our 39 00:02:14,880 --> 00:02:18,760 Speaker 1: podcast about the universe and all the amazing and mysterious 40 00:02:18,800 --> 00:02:21,639 Speaker 1: things that are out there for us to discover. That's right, 41 00:02:21,680 --> 00:02:25,720 Speaker 1: all those weird things floating in the cosmos doing strange, violent, 42 00:02:25,840 --> 00:02:30,359 Speaker 1: incredible stuff and our attempts as lowly humans to understand them. 43 00:02:30,639 --> 00:02:33,480 Speaker 1: Is it really possible to unravel the mysteries of the 44 00:02:33,560 --> 00:02:36,880 Speaker 1: universe and lay them out inside a human mind. We 45 00:02:36,880 --> 00:02:40,400 Speaker 1: will find out today and tomorrow and the next hundred 46 00:02:40,440 --> 00:02:43,200 Speaker 1: episodes of our podcast. Yeah, because you know, it sometimes 47 00:02:43,240 --> 00:02:45,960 Speaker 1: feels like we're building this model of the universe kind 48 00:02:45,960 --> 00:02:48,040 Speaker 1: of like we're building a whole universe kind of inside 49 00:02:48,080 --> 00:02:52,000 Speaker 1: of our heads and our physics theories, almost like a hologramma. 50 00:02:52,240 --> 00:02:55,880 Speaker 1: That's right. It's incredible to imagine that the whole external universe, 51 00:02:56,080 --> 00:03:01,240 Speaker 1: if it even exists, might be describable inside in mind, right, 52 00:03:01,320 --> 00:03:04,560 Speaker 1: Like you could represent it somehow in terms of arrangements 53 00:03:04,560 --> 00:03:06,800 Speaker 1: of neurons, right, and as I think the kind of 54 00:03:07,000 --> 00:03:10,079 Speaker 1: idea that makes people think, like maybe the entire universe 55 00:03:10,200 --> 00:03:12,440 Speaker 1: is actually just a projection of some other kind of 56 00:03:12,480 --> 00:03:15,959 Speaker 1: physical arrangement. Right. Yeah, I've always wondered like maybe our 57 00:03:16,000 --> 00:03:19,120 Speaker 1: brains just aren't equipped to like understand the universe. Do 58 00:03:19,120 --> 00:03:21,200 Speaker 1: you ever wonder about that? Oh, I'm almost certain that 59 00:03:21,240 --> 00:03:23,600 Speaker 1: we are not capable of understanding the universe at its 60 00:03:23,639 --> 00:03:27,120 Speaker 1: deepest level. So are we doomed to always not know 61 00:03:27,200 --> 00:03:30,360 Speaker 1: the universe. I think there's never going to be a 62 00:03:30,400 --> 00:03:33,799 Speaker 1: point where we're satisfied that we think we understand and 63 00:03:33,919 --> 00:03:36,360 Speaker 1: you know, imagine the kind of super intelligence that would 64 00:03:36,360 --> 00:03:39,760 Speaker 1: be necessary to like fully grasp with the universe. I 65 00:03:39,880 --> 00:03:42,640 Speaker 1: think about your dog. Your dog is intelligent, but it 66 00:03:42,720 --> 00:03:47,040 Speaker 1: certainly doesn't understand all the physics of the universe. And 67 00:03:47,120 --> 00:03:50,200 Speaker 1: so compared to some super intelligent aliens out there, we 68 00:03:50,240 --> 00:03:52,480 Speaker 1: are as small as dogs, and there's no way that 69 00:03:52,520 --> 00:03:55,040 Speaker 1: we could understand the universe at the level that they do. 70 00:03:55,640 --> 00:03:58,560 Speaker 1: And so you essentially have to be infinitely intelligent to 71 00:03:58,640 --> 00:04:02,200 Speaker 1: understand the whole university thing. And couldn't infinite intelligence exist 72 00:04:02,240 --> 00:04:04,440 Speaker 1: in the universe that that would be so that would 73 00:04:04,440 --> 00:04:07,240 Speaker 1: be a lot. It would create an intelligence black hole 74 00:04:07,320 --> 00:04:10,360 Speaker 1: inside its mind because you can't store that much information 75 00:04:10,480 --> 00:04:14,480 Speaker 1: or that much smart in a small space. Man, we've 76 00:04:14,560 --> 00:04:17,159 Speaker 1: just covered dogs and black holes and like the first 77 00:04:17,680 --> 00:04:21,479 Speaker 1: three minutes and including brains. But yeah, so we talked 78 00:04:21,480 --> 00:04:23,279 Speaker 1: about all of the mysterious things, and one of the 79 00:04:23,480 --> 00:04:26,599 Speaker 1: favorite mysterious things that we like to talk about our 80 00:04:26,800 --> 00:04:30,560 Speaker 1: black holes because they're so mysterious and it seems like, 81 00:04:30,760 --> 00:04:33,840 Speaker 1: you know, that there were these black pockets in almost 82 00:04:33,839 --> 00:04:36,240 Speaker 1: their own universes, and it seems like anything you throw 83 00:04:36,279 --> 00:04:39,120 Speaker 1: into it can never ever come out. And they're especially 84 00:04:39,160 --> 00:04:42,159 Speaker 1: wonderful and fascinating because they came out of the human 85 00:04:42,200 --> 00:04:45,240 Speaker 1: mind initially. It's not something we saw in the universe. 86 00:04:45,279 --> 00:04:47,680 Speaker 1: It's an idea we had. We said, if the laws 87 00:04:47,680 --> 00:04:50,320 Speaker 1: of physics are the way we think they are, then 88 00:04:50,360 --> 00:04:54,560 Speaker 1: these things should exist. So we like mapped something inside 89 00:04:54,560 --> 00:04:56,640 Speaker 1: our minds out into the universe and then went out 90 00:04:56,680 --> 00:04:59,800 Speaker 1: and actually found them. I mean it's incredible, right that 91 00:05:00,000 --> 00:05:03,080 Speaker 1: think that our understanding the universe could be so sophisticated 92 00:05:03,120 --> 00:05:06,559 Speaker 1: and impressive that we can predict crazy new bonker stuff 93 00:05:06,560 --> 00:05:09,000 Speaker 1: out there which turns out to be real. I think 94 00:05:09,000 --> 00:05:12,480 Speaker 1: that's really impressive. Yeah, yeah, good jobs, physicists. Even though 95 00:05:12,520 --> 00:05:17,320 Speaker 1: we are dogs compared to intelligently nothing against dogs. Of course, 96 00:05:17,360 --> 00:05:19,880 Speaker 1: dogs very smart. That's why I chose them physics example, 97 00:05:20,000 --> 00:05:23,880 Speaker 1: and not cats. Right, I think cats are smarter. They're 98 00:05:23,880 --> 00:05:26,480 Speaker 1: not smarter than dogs. Man, you cannot train a cat. 99 00:05:26,720 --> 00:05:29,360 Speaker 1: That's proof number one. That's cats are not smarter than dogs. 100 00:05:29,640 --> 00:05:33,560 Speaker 1: Maybe like cats are mathematicians and dogs are physicists. Would 101 00:05:33,560 --> 00:05:36,400 Speaker 1: you say that's a fair, fair comparison. Well, if you're 102 00:05:36,440 --> 00:05:38,359 Speaker 1: saying that dogs are smarter than cats, that I agree 103 00:05:38,400 --> 00:05:45,800 Speaker 1: with you. Masticians are just sneakier, that's right now. But 104 00:05:45,880 --> 00:05:49,479 Speaker 1: black holes are a fascinating mystery and one that began 105 00:05:49,520 --> 00:05:52,239 Speaker 1: inside the human brain, but one that we still don't 106 00:05:52,279 --> 00:05:54,440 Speaker 1: really understand. I mean, we found them, we see them 107 00:05:54,480 --> 00:05:57,760 Speaker 1: out there, but it's a continuous source of mystery and 108 00:05:57,839 --> 00:06:01,240 Speaker 1: puzzlement for people everywhere and for scientists. Yeah, and it's 109 00:06:01,240 --> 00:06:03,599 Speaker 1: amazing that we've seen it, like we've found one, Like 110 00:06:03,880 --> 00:06:06,320 Speaker 1: they took pictures of one sort of last year, and 111 00:06:06,400 --> 00:06:08,159 Speaker 1: it's like it's real, it's there, you can see it, 112 00:06:08,160 --> 00:06:10,040 Speaker 1: and it looks like what we thought they looked like. 113 00:06:10,120 --> 00:06:11,960 Speaker 1: That's right. The picture of the black hole shows you 114 00:06:12,000 --> 00:06:15,839 Speaker 1: all the incredible gas swirling around it that's trying desperately 115 00:06:16,000 --> 00:06:19,080 Speaker 1: to avoid falling into the black hole and in the 116 00:06:19,120 --> 00:06:21,640 Speaker 1: process is bouncing around against all the other gas and 117 00:06:21,680 --> 00:06:24,359 Speaker 1: emitting lots of radiations. So we're not seeing the black 118 00:06:24,360 --> 00:06:27,320 Speaker 1: hole directly, you know, although we see a black spot there, 119 00:06:27,480 --> 00:06:32,400 Speaker 1: we're seeing mostly the swirling, chaotic, crazy gas that's surrounding. Yeah. 120 00:06:32,400 --> 00:06:34,520 Speaker 1: I guess you're right, because I mean, we see the 121 00:06:34,520 --> 00:06:37,400 Speaker 1: black center, but there's nothing to see there because nothing 122 00:06:37,440 --> 00:06:39,800 Speaker 1: can come out, or at least that's the idea of 123 00:06:39,800 --> 00:06:42,520 Speaker 1: a black hole. And so the question then kind of 124 00:06:42,600 --> 00:06:45,919 Speaker 1: becomes what happens to the stuff that goes into it? 125 00:06:46,040 --> 00:06:49,960 Speaker 1: Is it gone forever or cannedy recovered? Yeah? Is that 126 00:06:50,000 --> 00:06:53,200 Speaker 1: stuff just like hanging out inside the black hole having 127 00:06:53,240 --> 00:06:55,360 Speaker 1: a great time with all the other stuff? Does it 128 00:06:55,440 --> 00:06:58,080 Speaker 1: get squeezed into some new form of matter? Is it 129 00:06:58,160 --> 00:07:00,240 Speaker 1: all in a singularity in the middle. It's of the 130 00:07:00,320 --> 00:07:03,440 Speaker 1: deepest questions in physics what's going on inside a black 131 00:07:03,480 --> 00:07:06,080 Speaker 1: hole and what happened to the stuff that fell in? 132 00:07:06,240 --> 00:07:08,560 Speaker 1: So today on the podcast we'll be asking the question 133 00:07:13,320 --> 00:07:18,040 Speaker 1: those a black hole destroy information? I guess that's an 134 00:07:18,080 --> 00:07:21,840 Speaker 1: interesting question because you know, it's kind of like asking 135 00:07:21,840 --> 00:07:23,760 Speaker 1: what happens to stuff that goes in, Like does it 136 00:07:23,800 --> 00:07:28,720 Speaker 1: get destroyed like obliterated? Does it become pure energy, unadultered, 137 00:07:29,000 --> 00:07:32,320 Speaker 1: unfiltered energy that you can't make out what it is? 138 00:07:32,560 --> 00:07:34,760 Speaker 1: Or does it you know, does a cork stay a 139 00:07:34,800 --> 00:07:37,080 Speaker 1: cork inside of the black hole? And does it still 140 00:07:37,280 --> 00:07:39,840 Speaker 1: fly around and doesn't even know it's in a black hole? Yeah? 141 00:07:39,920 --> 00:07:41,600 Speaker 1: I mean, are you wondering about what happened to that 142 00:07:41,600 --> 00:07:43,720 Speaker 1: banana you dropped into your black hole. I'm still wondering 143 00:07:43,720 --> 00:07:46,920 Speaker 1: about my banana, Daniel. I want it back. My dog 144 00:07:46,960 --> 00:07:49,120 Speaker 1: needs today. Do you like eating bananas when they're black, 145 00:07:49,120 --> 00:07:52,800 Speaker 1: because that's probably what happened to your back. You mean 146 00:07:52,880 --> 00:07:55,720 Speaker 1: it turned into a movie basically. Basically, But it's a 147 00:07:55,720 --> 00:07:58,480 Speaker 1: fascinating question, like when something goes into a black hole. 148 00:07:58,760 --> 00:08:01,440 Speaker 1: Is a black hole like a cosmic hard drive? Does 149 00:08:01,480 --> 00:08:05,040 Speaker 1: it like just compress everything into some new arrangement but 150 00:08:05,120 --> 00:08:08,000 Speaker 1: effectively keeping track of all the particles that came in, 151 00:08:08,400 --> 00:08:12,200 Speaker 1: or is it actually deleting stuff from the universe, turning 152 00:08:12,240 --> 00:08:15,760 Speaker 1: into some new configuration that doesn't have any information about 153 00:08:15,760 --> 00:08:18,400 Speaker 1: what happened before it. That's a fascinating question. Yeah, and 154 00:08:18,440 --> 00:08:20,880 Speaker 1: so we have a lot to impact here about black 155 00:08:20,880 --> 00:08:24,400 Speaker 1: holes and information. But at first we, as usually, we 156 00:08:24,400 --> 00:08:27,000 Speaker 1: were wondering how many people out there had heard of 157 00:08:27,040 --> 00:08:31,280 Speaker 1: this question of whether black holes keep or destroy information? 158 00:08:31,960 --> 00:08:34,040 Speaker 1: And so, as usual, Daniel went out there and ask 159 00:08:34,080 --> 00:08:36,160 Speaker 1: people on the internet what they thought of this question. 160 00:08:36,200 --> 00:08:38,760 Speaker 1: That's right, So thank you to everybody who have volunteered 161 00:08:38,760 --> 00:08:42,079 Speaker 1: to answer random questions. If you're willing to participate and 162 00:08:42,280 --> 00:08:45,880 Speaker 1: like to hear your uninformed speculation on the podcast right 163 00:08:45,960 --> 00:08:48,800 Speaker 1: to us two questions at Daniel and Jorge dot com 164 00:08:49,080 --> 00:08:51,960 Speaker 1: YouTube can answer these random questions. Think about it for 165 00:08:51,960 --> 00:08:54,480 Speaker 1: a second, and what do you know about information and 166 00:08:54,600 --> 00:08:57,800 Speaker 1: black holes and what goes into them? Here's what people 167 00:08:57,800 --> 00:09:00,720 Speaker 1: had to say. I think the information diss inside a 168 00:09:00,720 --> 00:09:04,880 Speaker 1: black hole. My understanding of Hawking radiation is that when 169 00:09:04,880 --> 00:09:08,000 Speaker 1: a particle interacts with the black hole, information is lost. 170 00:09:08,120 --> 00:09:13,360 Speaker 1: Therefore the black hole behaves like a garbage disposal. Ah, 171 00:09:13,400 --> 00:09:15,040 Speaker 1: so I do know a little bit about this. So 172 00:09:15,080 --> 00:09:18,080 Speaker 1: I read a book by Leonard Suskin which was talking 173 00:09:18,120 --> 00:09:21,959 Speaker 1: about the black hole wars. Stephen Hawkins believe that they 174 00:09:22,000 --> 00:09:26,800 Speaker 1: did disappear. Information did disappear, and the Suskin said it didn't. 175 00:09:27,200 --> 00:09:30,199 Speaker 1: And I think it's started to do with holographic principle 176 00:09:31,040 --> 00:09:34,640 Speaker 1: that basically all the data stays on the event arising. Yes, 177 00:09:34,720 --> 00:09:37,760 Speaker 1: information disappears from black holes because they lose mass through 178 00:09:37,800 --> 00:09:41,160 Speaker 1: Hawking radiation. They're more like garbage disposes than hard drives, 179 00:09:41,160 --> 00:09:43,640 Speaker 1: since you can't retrieve any information that's stored in them. 180 00:09:44,080 --> 00:09:46,680 Speaker 1: Um my guests would be that once an object is 181 00:09:46,679 --> 00:09:49,560 Speaker 1: sucked into a black hole. It is obliterated into its 182 00:09:49,679 --> 00:09:53,200 Speaker 1: most smallest particles that exist, and those things float around 183 00:09:53,200 --> 00:09:55,640 Speaker 1: and mess around with other particles and probably no longer 184 00:09:55,679 --> 00:09:59,319 Speaker 1: resemble whatever it is that they used to make up planets, bananas, 185 00:09:59,320 --> 00:10:02,760 Speaker 1: bunnies or whatever it is. I think they like store 186 00:10:02,800 --> 00:10:06,800 Speaker 1: information and then eventually, in like trillions and trillions and 187 00:10:06,840 --> 00:10:11,160 Speaker 1: trillions of years, there's like hawking radiation that radiates, you know, 188 00:10:11,320 --> 00:10:14,240 Speaker 1: and out in black holes go away. As far as 189 00:10:14,240 --> 00:10:18,920 Speaker 1: I understand, physics falls apart inside a black hole. I've 190 00:10:18,960 --> 00:10:25,080 Speaker 1: read that information doesn't disappear as such, and that all 191 00:10:25,160 --> 00:10:31,599 Speaker 1: the information inside the black hole would be somehow readable 192 00:10:31,800 --> 00:10:35,520 Speaker 1: on the horizon. Whatever goes in there just gets squished 193 00:10:35,559 --> 00:10:39,360 Speaker 1: into a really tiny small space. So I'd probably say 194 00:10:39,360 --> 00:10:42,120 Speaker 1: they're more like a garbage disposal. What goes in doesn't 195 00:10:42,120 --> 00:10:45,959 Speaker 1: come out, I don't think so. I think it depends 196 00:10:45,960 --> 00:10:48,120 Speaker 1: at the center of a black hole is which we 197 00:10:48,160 --> 00:10:53,760 Speaker 1: don't know. If it's an infinite density single point, then 198 00:10:53,760 --> 00:10:57,240 Speaker 1: it's probably more like a garbage disposal. But if it's not, 199 00:10:57,600 --> 00:11:00,560 Speaker 1: then I would assume information can enter it and just 200 00:11:00,600 --> 00:11:03,560 Speaker 1: gets trapped. I'm gonna equivocate on this, and so I 201 00:11:03,600 --> 00:11:08,240 Speaker 1: shall leave it to my learned colleagues Daniel Watson and 202 00:11:08,480 --> 00:11:13,720 Speaker 1: Hua Champ perhaps to answer that all so, I don't 203 00:11:13,760 --> 00:11:16,360 Speaker 1: think that information disappears into the black hole. I think 204 00:11:17,120 --> 00:11:22,120 Speaker 1: information is recorded on the edge of black hole. Information 205 00:11:22,640 --> 00:11:26,840 Speaker 1: cannot disappear, like energy cannot disappear. All right, not a 206 00:11:26,840 --> 00:11:29,440 Speaker 1: good outlook for what happens to stuff that goes into 207 00:11:29,440 --> 00:11:32,680 Speaker 1: the black hole. Nobody nobody thinks it's hanging out happily inside. 208 00:11:33,320 --> 00:11:35,840 Speaker 1: Nobody thinks that you're gonna eat that banana. I like that. 209 00:11:35,840 --> 00:11:40,120 Speaker 1: There's basically every answer here. Information disappears, information doesn't disappear, 210 00:11:40,200 --> 00:11:44,800 Speaker 1: information is radiated out, and they're basically garbage compactors. That's 211 00:11:44,920 --> 00:11:47,680 Speaker 1: a wonderful variety of answers here. Thank you to everybody 212 00:11:47,679 --> 00:11:50,920 Speaker 1: who participated, a wonderful variety of analogies here, Like is 213 00:11:51,040 --> 00:11:54,880 Speaker 1: a garbage compactor? Is it a garbage disposal? Is it 214 00:11:54,920 --> 00:12:00,160 Speaker 1: a recycling being? I don't think the universe recycles. I 215 00:12:00,200 --> 00:12:02,959 Speaker 1: don't think it's like plastic in this black hole. Please, 216 00:12:03,200 --> 00:12:05,720 Speaker 1: And you know what, if black holes are just the 217 00:12:05,760 --> 00:12:09,240 Speaker 1: universe's compost, interesting they could be right. They break stuff 218 00:12:09,280 --> 00:12:12,360 Speaker 1: down and maybe they store it for later for a 219 00:12:12,880 --> 00:12:16,160 Speaker 1: universe garden, a star garden or story for never that's 220 00:12:16,160 --> 00:12:18,800 Speaker 1: maybe the problem. Well, until the universe collapses and then 221 00:12:18,800 --> 00:12:23,000 Speaker 1: everything gets too cycled. Right, that's a very optimistic view 222 00:12:23,240 --> 00:12:25,120 Speaker 1: of what's going to happen to your banana. Well, this 223 00:12:25,240 --> 00:12:27,400 Speaker 1: is an interesting topic, and so let's jump right into it. 224 00:12:27,800 --> 00:12:30,200 Speaker 1: This might take a while because some of the things 225 00:12:30,240 --> 00:12:33,400 Speaker 1: that we need to talk about include information and quantum mechanics. 226 00:12:33,640 --> 00:12:35,439 Speaker 1: And so before we sort of get into the idea 227 00:12:35,520 --> 00:12:39,680 Speaker 1: of what happens to information that goes into a black hole, 228 00:12:40,640 --> 00:12:43,640 Speaker 1: let's talk about kind of information in general and how 229 00:12:43,720 --> 00:12:47,120 Speaker 1: that works in a quantum reality. That's right, because one 230 00:12:47,160 --> 00:12:49,319 Speaker 1: of the mysteries of black holes is what happens to 231 00:12:49,440 --> 00:12:52,360 Speaker 1: the information that goes into them. And so first we 232 00:12:52,440 --> 00:12:55,720 Speaker 1: have to understand, like what is information and what does 233 00:12:55,800 --> 00:13:00,280 Speaker 1: quantum mechanics say about that information? Right? So, information is 234 00:13:00,320 --> 00:13:02,800 Speaker 1: kind of like the arrangement of things, like the physicist. 235 00:13:02,840 --> 00:13:06,480 Speaker 1: Information is not like ones and zeros or it's not like, yeah, 236 00:13:06,600 --> 00:13:09,719 Speaker 1: you know a file or a number. It's more like 237 00:13:09,840 --> 00:13:12,040 Speaker 1: the arrangement of things, right, Yeah, And it can be 238 00:13:12,200 --> 00:13:15,079 Speaker 1: represented as ones or zeros or you know, things you 239 00:13:15,160 --> 00:13:17,520 Speaker 1: print on a piece of paper. But fundamentally, it's the 240 00:13:17,679 --> 00:13:21,200 Speaker 1: arrangement of the particles. It's really it's the quantum wave 241 00:13:21,280 --> 00:13:24,200 Speaker 1: function that tells you where the particles are or where 242 00:13:24,200 --> 00:13:26,679 Speaker 1: they are likely to be, and how they are interacting. 243 00:13:27,280 --> 00:13:31,000 Speaker 1: Remember that everything, me and you and bananas and all 244 00:13:31,040 --> 00:13:32,760 Speaker 1: that stuff are made out of particles, and we're all 245 00:13:32,800 --> 00:13:35,680 Speaker 1: made out of the same particles. So the thing that's 246 00:13:35,720 --> 00:13:39,959 Speaker 1: different between you and lava and hamsters and bananas is 247 00:13:40,000 --> 00:13:42,199 Speaker 1: not the stuff you're made out of. That's really the 248 00:13:42,280 --> 00:13:44,400 Speaker 1: same stuff that everything is made out of. It's how 249 00:13:44,520 --> 00:13:47,320 Speaker 1: that stuff is put together. It's like if you had 250 00:13:47,520 --> 00:13:49,679 Speaker 1: a book of recipes and they all had exactly the 251 00:13:49,760 --> 00:13:52,679 Speaker 1: same ingredients, just had different arrangements like where you put 252 00:13:52,760 --> 00:13:55,959 Speaker 1: the stuff. That's literally how things in the universe are built. 253 00:13:56,280 --> 00:13:58,960 Speaker 1: And so what we mean by information from a physics 254 00:13:58,960 --> 00:14:01,360 Speaker 1: point of view is just that is how the particles 255 00:14:01,400 --> 00:14:03,520 Speaker 1: are put together to make this versus that, right, And 256 00:14:03,600 --> 00:14:06,400 Speaker 1: it's also kind of the history of them a little bit, right, 257 00:14:06,440 --> 00:14:08,000 Speaker 1: Like you can make a banana cake and I can 258 00:14:08,040 --> 00:14:10,480 Speaker 1: make a banana caig, but they're going to be different 259 00:14:10,520 --> 00:14:13,679 Speaker 1: bana caggs depending on you know, what the size of 260 00:14:13,800 --> 00:14:16,280 Speaker 1: the pan I use, or whether I put in a 261 00:14:16,360 --> 00:14:17,720 Speaker 1: little bit more of this, or a little bit more 262 00:14:17,760 --> 00:14:19,520 Speaker 1: of that, or how I poured it. They're bothing that 263 00:14:19,560 --> 00:14:21,400 Speaker 1: tastes like banana aig, but they're gonna be different banana 264 00:14:21,440 --> 00:14:25,240 Speaker 1: caigs because they were arranged kind of with a different history. 265 00:14:25,360 --> 00:14:27,560 Speaker 1: And that's right. So our two banana cream pies both 266 00:14:27,600 --> 00:14:30,880 Speaker 1: have information about what happened to those bananas, how they 267 00:14:30,960 --> 00:14:34,440 Speaker 1: got there, how they originally were developed and grown and 268 00:14:34,600 --> 00:14:37,360 Speaker 1: blended up and and turned into the banana cream pies. 269 00:14:37,400 --> 00:14:40,600 Speaker 1: Because our two banana cream pies are not identical, they 270 00:14:40,680 --> 00:14:44,400 Speaker 1: contain information about how they got there. Their arrangements are 271 00:14:44,520 --> 00:14:48,000 Speaker 1: unique because only one way to create that particular banana 272 00:14:48,040 --> 00:14:51,120 Speaker 1: cream pie. And so you could run the clock backwards 273 00:14:51,280 --> 00:14:54,440 Speaker 1: and figure out where everything came from in your pie. Yeah, 274 00:14:54,720 --> 00:14:56,800 Speaker 1: So I think that kind of what you're saying is 275 00:14:56,920 --> 00:14:59,280 Speaker 1: that it's like, it's kind of like if you're playing 276 00:14:59,280 --> 00:15:01,720 Speaker 1: billiards or some thing, if you see all the balls 277 00:15:01,760 --> 00:15:03,680 Speaker 1: kind of arranged in a particular way on the table, 278 00:15:03,840 --> 00:15:06,200 Speaker 1: you can sort of backtrack how they all got to 279 00:15:06,720 --> 00:15:09,760 Speaker 1: how billiard balls usually start. That's right, And that's what 280 00:15:09,880 --> 00:15:13,000 Speaker 1: we mean when we say quantum mechanics does not destroy information. 281 00:15:13,080 --> 00:15:16,080 Speaker 1: It says that you can tell how you got to 282 00:15:16,200 --> 00:15:18,320 Speaker 1: where you are. So, just like you said in the 283 00:15:18,600 --> 00:15:22,800 Speaker 1: billiard balls example, if you see balls moving on the table, 284 00:15:23,120 --> 00:15:24,960 Speaker 1: you can tell how you got there. You said, well, 285 00:15:25,040 --> 00:15:27,680 Speaker 1: this must have happened in a certain way. You know, 286 00:15:27,800 --> 00:15:31,080 Speaker 1: Bob must have hit Alice's ball and it bounced off 287 00:15:31,120 --> 00:15:33,240 Speaker 1: this wall, etcetera, etcetera. There's only one way to get 288 00:15:33,280 --> 00:15:37,920 Speaker 1: to this exact particular arrangement. And so because information is 289 00:15:37,960 --> 00:15:41,200 Speaker 1: not destroyed, it's all the information you need to figure 290 00:15:41,240 --> 00:15:44,200 Speaker 1: out how you got here is present in this configuration. 291 00:15:44,560 --> 00:15:46,400 Speaker 1: You could run the clock backwards, you can run a 292 00:15:46,440 --> 00:15:49,440 Speaker 1: physics simulation backwards and figure out exactly how you got 293 00:15:49,520 --> 00:15:52,040 Speaker 1: to hear or run it forward. Right like that, I 294 00:15:52,120 --> 00:15:54,600 Speaker 1: think you're saying that there's no ambiguity in the universe, 295 00:15:54,720 --> 00:15:57,200 Speaker 1: Like if you you come upon a crime scene, you 296 00:15:57,280 --> 00:16:00,160 Speaker 1: can tell exactly what happened, like a physicist could. If 297 00:16:00,200 --> 00:16:02,440 Speaker 1: you sort of rewind the universe and play the laws 298 00:16:02,480 --> 00:16:05,280 Speaker 1: of physics backwards, you can sort of reconstruct what happens 299 00:16:05,560 --> 00:16:07,960 Speaker 1: every time precisely. And it's really weird that this comes 300 00:16:08,000 --> 00:16:10,600 Speaker 1: up in quantum mechanics because you might think, yeah, quantum 301 00:16:10,600 --> 00:16:12,760 Speaker 1: mechanics is not something that's going to give you certainty 302 00:16:13,040 --> 00:16:15,720 Speaker 1: that tells you you can know everything about the universe, right, 303 00:16:16,040 --> 00:16:18,440 Speaker 1: because quantum mechanics is something that feels like it has 304 00:16:18,480 --> 00:16:22,080 Speaker 1: a lot of built in uncertainty. And so what quantum 305 00:16:22,120 --> 00:16:24,600 Speaker 1: mechanics tells you is you can always know the wave function. 306 00:16:24,680 --> 00:16:26,880 Speaker 1: That's the thing that tells you where the particles are 307 00:16:26,960 --> 00:16:29,200 Speaker 1: likely to be, not that you could actually know where 308 00:16:29,280 --> 00:16:32,720 Speaker 1: the particles are. In the same way, you can backtrack 309 00:16:32,840 --> 00:16:35,240 Speaker 1: the wave function. You can say if the particles have 310 00:16:35,280 --> 00:16:37,680 Speaker 1: a certain way function that says that they're more likely 311 00:16:37,760 --> 00:16:39,200 Speaker 1: to be on the left side of the table. Now 312 00:16:39,560 --> 00:16:42,240 Speaker 1: you can backtrack that and tell where they were likely 313 00:16:42,320 --> 00:16:44,560 Speaker 1: to be in the past, not where they actually were. 314 00:16:44,760 --> 00:16:46,800 Speaker 1: It's all about the wave function. It's all about this 315 00:16:47,000 --> 00:16:50,760 Speaker 1: evolving probabilities. The way so looking back into the past 316 00:16:50,880 --> 00:16:53,840 Speaker 1: is also there's also probabilities or do you know for 317 00:16:53,960 --> 00:16:56,400 Speaker 1: sure where the party like if like if I see 318 00:16:56,400 --> 00:16:58,920 Speaker 1: an electron and I measure, you know where it is 319 00:16:59,000 --> 00:17:01,400 Speaker 1: and where it's going to the best degree that I 320 00:17:01,480 --> 00:17:03,560 Speaker 1: can can, I tell you where it was before and 321 00:17:03,600 --> 00:17:05,320 Speaker 1: how fast it was going. No, you can only know 322 00:17:05,400 --> 00:17:08,760 Speaker 1: the probabilities. You can't collapse the wave function into the 323 00:17:08,840 --> 00:17:11,399 Speaker 1: past because that would have changed where it is today. 324 00:17:12,720 --> 00:17:15,520 Speaker 1: But if you know the way function today right, then 325 00:17:15,600 --> 00:17:17,800 Speaker 1: you can backtrack it into the past and you can 326 00:17:17,840 --> 00:17:21,520 Speaker 1: propagate it into the future. Any idea is that if 327 00:17:21,560 --> 00:17:23,680 Speaker 1: you look at any configuration of matter, you should be 328 00:17:23,720 --> 00:17:26,160 Speaker 1: able to tell where it came from. That's the core 329 00:17:26,280 --> 00:17:28,200 Speaker 1: idea that you have to understand. I see. So when 330 00:17:28,200 --> 00:17:31,200 Speaker 1: you talk about information, you don't mean like where things 331 00:17:31,280 --> 00:17:33,840 Speaker 1: are and where they're going, but you also kind of 332 00:17:33,880 --> 00:17:38,040 Speaker 1: include these quantum probabilities as information, Like that's also information 333 00:17:38,160 --> 00:17:41,439 Speaker 1: to physics, Yes, that's the actual quantum information, because they 334 00:17:41,440 --> 00:17:43,960 Speaker 1: don't know where the particles are. We really just know 335 00:17:44,119 --> 00:17:46,760 Speaker 1: these probabilities. And so like when we talk about like 336 00:17:46,880 --> 00:17:51,600 Speaker 1: quantum teleportation copying things, we're talking about copying not the 337 00:17:51,640 --> 00:17:55,120 Speaker 1: where the particles actually are, but their probabilities, because that's 338 00:17:55,160 --> 00:17:57,840 Speaker 1: really what the quantum information is. It kind of feels 339 00:17:57,880 --> 00:18:01,680 Speaker 1: a little unsatisfying on physicists because I feel I feel 340 00:18:01,680 --> 00:18:05,240 Speaker 1: like you're telling me that information includes not knowing kind 341 00:18:05,280 --> 00:18:06,840 Speaker 1: of in a way, you know what I mean, Like 342 00:18:07,040 --> 00:18:11,160 Speaker 1: information includes also non information. Yeah, what's the most information 343 00:18:11,240 --> 00:18:14,359 Speaker 1: that you can have about the universe is information about 344 00:18:14,359 --> 00:18:18,159 Speaker 1: the probabilities, and that information cannot be destroyed. Like we 345 00:18:18,200 --> 00:18:20,040 Speaker 1: don't know where the electron is. It's not like there's 346 00:18:20,040 --> 00:18:22,480 Speaker 1: a fact there that's not accessible to us. It just 347 00:18:22,800 --> 00:18:25,639 Speaker 1: isn't determined. But the way function is the thing that 348 00:18:25,720 --> 00:18:28,119 Speaker 1: tells you that it's more probable to find it on 349 00:18:28,200 --> 00:18:30,880 Speaker 1: the left side or the right side. That is totally determined. 350 00:18:31,119 --> 00:18:33,280 Speaker 1: And that's the level of quantum information we can have. 351 00:18:33,520 --> 00:18:37,040 Speaker 1: That's the most information that the universe allows you to 352 00:18:37,160 --> 00:18:39,760 Speaker 1: have almost right, Like you know you can know the 353 00:18:39,840 --> 00:18:43,119 Speaker 1: position and the velocity of a particle to a perfect 354 00:18:43,160 --> 00:18:46,119 Speaker 1: degree because of the uncertainty principle, because and that's just 355 00:18:46,200 --> 00:18:47,960 Speaker 1: the rule of the universe. The universe is like, nope, 356 00:18:48,000 --> 00:18:52,040 Speaker 1: you can't know everything all of the time everywhere. That's right, 357 00:18:52,240 --> 00:18:55,280 Speaker 1: And that's why quantum information cannot be destroyed, because the 358 00:18:55,400 --> 00:18:59,240 Speaker 1: probabilities cannot be destroyed. Like if an electron is somewhere 359 00:18:59,320 --> 00:19:01,960 Speaker 1: in your box now, then it is somewhere in your 360 00:19:02,040 --> 00:19:04,040 Speaker 1: box in the future. You're like, out of all the 361 00:19:04,080 --> 00:19:06,159 Speaker 1: probabilities in the future, they still have to add up 362 00:19:06,200 --> 00:19:09,480 Speaker 1: to one. And that's why if you run the clock backwards, 363 00:19:09,520 --> 00:19:12,159 Speaker 1: you should still get probabilities adding up to one in 364 00:19:12,200 --> 00:19:14,400 Speaker 1: the past, and if you run it back even further, 365 00:19:14,480 --> 00:19:16,960 Speaker 1: you should still get probabilities added up to one because 366 00:19:17,000 --> 00:19:20,679 Speaker 1: information is not destroyed can't just disappear, because your particles 367 00:19:20,720 --> 00:19:23,520 Speaker 1: don't just disappear, you don't know where they are. But 368 00:19:23,600 --> 00:19:26,960 Speaker 1: the probabilities can't disappear. The probabilities can slash around, but 369 00:19:27,080 --> 00:19:30,000 Speaker 1: they can't just go away. And so that's why we're 370 00:19:30,000 --> 00:19:32,600 Speaker 1: so fascinated about what happens inside a black hole, because 371 00:19:32,640 --> 00:19:35,880 Speaker 1: we're wondering, like, does the information inside a black hole? 372 00:19:36,200 --> 00:19:39,360 Speaker 1: Does it get deleted or is it still stored in there, 373 00:19:39,480 --> 00:19:41,640 Speaker 1: Like it's a black hole that has a banana versus 374 00:19:41,680 --> 00:19:44,560 Speaker 1: an apple, have something different inside it that tells you 375 00:19:44,960 --> 00:19:47,000 Speaker 1: that one has a banana, one has an apple, or 376 00:19:47,119 --> 00:19:51,480 Speaker 1: the actually deleting stuff. Interesting? Interesting, Yeah, I get. The 377 00:19:51,560 --> 00:19:55,560 Speaker 1: question is if I throw a banana and one black hole, 378 00:19:56,160 --> 00:19:59,000 Speaker 1: and I throw the equivalent apple the copy of that 379 00:19:59,080 --> 00:20:01,240 Speaker 1: black hole, are the two black holes different at the 380 00:20:01,359 --> 00:20:03,560 Speaker 1: end or are they basically the same? That's kind of 381 00:20:03,560 --> 00:20:06,000 Speaker 1: the question exactly, And quantum mechanics says they have to 382 00:20:06,080 --> 00:20:09,240 Speaker 1: be different because if they're not different, then you've destroyed 383 00:20:09,280 --> 00:20:11,840 Speaker 1: the information about which one got the banana and which 384 00:20:11,920 --> 00:20:14,280 Speaker 1: one got the apple in a corner. Quantum mechanics, and 385 00:20:14,359 --> 00:20:18,560 Speaker 1: this is a very deep, very bedrock principle. Information cannot 386 00:20:18,600 --> 00:20:21,119 Speaker 1: be destroyed. Like you go to a particle theorist and 387 00:20:21,200 --> 00:20:24,280 Speaker 1: you say, what if I prove the quantum mechanics doesn't 388 00:20:24,320 --> 00:20:26,879 Speaker 1: preserve information, that you can delete information from the universe, 389 00:20:26,960 --> 00:20:29,320 Speaker 1: then basically they just throw all their books away and 390 00:20:29,400 --> 00:20:32,800 Speaker 1: we have to start everything from scratch. It's that deeply 391 00:20:33,000 --> 00:20:36,800 Speaker 1: ingrained into physics. I guess it's like comparing apple black 392 00:20:36,800 --> 00:20:40,800 Speaker 1: holes to banana black holes. All Right, I'm starting to 393 00:20:40,800 --> 00:20:42,640 Speaker 1: feel a bit a little bit like a dog here, uh, 394 00:20:42,840 --> 00:20:45,520 Speaker 1: and not fully able to grasp all this stuff. But 395 00:20:45,840 --> 00:20:48,840 Speaker 1: that's kind of the nature of quantum mechanics. So let's 396 00:20:48,920 --> 00:20:51,240 Speaker 1: get into whether or not black holes can destroy this 397 00:20:51,359 --> 00:20:54,159 Speaker 1: quantum information, and if they can, then how do we 398 00:20:54,240 --> 00:21:09,159 Speaker 1: explain it? But first let's take a quick break. All right, 399 00:21:09,200 --> 00:21:14,200 Speaker 1: we're talking about weather. Black holes can destroy quantum information. 400 00:21:14,480 --> 00:21:17,160 Speaker 1: And so Danny, you were telling me that quantum information 401 00:21:17,280 --> 00:21:21,600 Speaker 1: includes like the probability of all the particles in the universe, 402 00:21:21,760 --> 00:21:24,120 Speaker 1: or at least a bunch of particles that you're looking at, 403 00:21:24,600 --> 00:21:26,680 Speaker 1: and you're telling me that quantum mechanics says that you 404 00:21:26,840 --> 00:21:29,879 Speaker 1: can't destroy this information, Like you can't just forget about it, 405 00:21:30,119 --> 00:21:33,280 Speaker 1: Like it's always kind of encoded in how the particles 406 00:21:33,600 --> 00:21:35,880 Speaker 1: are arranged or what they're doing. That's right. It's sort 407 00:21:35,920 --> 00:21:38,159 Speaker 1: of like the central premise of that TV show Devs, 408 00:21:38,440 --> 00:21:41,640 Speaker 1: where they try to reconstruct details about what happened two 409 00:21:41,680 --> 00:21:44,720 Speaker 1: thousand years ago by getting really fine data about the 410 00:21:44,920 --> 00:21:47,840 Speaker 1: molecules in the air and the earth and just backtracking 411 00:21:47,960 --> 00:21:50,560 Speaker 1: it two thousands of years. The ideas that the evidence 412 00:21:50,600 --> 00:21:53,439 Speaker 1: for the past is still with us here in the president, 413 00:21:53,560 --> 00:21:56,560 Speaker 1: that if you had incredible computing power and enough data, 414 00:21:56,880 --> 00:22:00,600 Speaker 1: you could reconstruct any event. It's like the perfect crime novel. Wow, 415 00:22:00,800 --> 00:22:02,880 Speaker 1: and so yeah, Like can you look at a banana 416 00:22:03,080 --> 00:22:06,159 Speaker 1: and tell what the plant the griod looked like? Kind of, 417 00:22:06,200 --> 00:22:09,560 Speaker 1: that's right, the ideas that no two bananas are identical, 418 00:22:09,720 --> 00:22:12,760 Speaker 1: but somewhere in that banana there's a clue about where 419 00:22:12,800 --> 00:22:14,640 Speaker 1: it came from and what it was like and whether 420 00:22:14,680 --> 00:22:16,480 Speaker 1: it got sun on a certain day, and all that 421 00:22:16,640 --> 00:22:20,119 Speaker 1: information is somehow encoded in the banana. They're making me 422 00:22:20,160 --> 00:22:23,440 Speaker 1: feel guilty about eating a banana. You're like you're destroying 423 00:22:23,480 --> 00:22:26,600 Speaker 1: a perfect, unique gem in the univers just becomes part 424 00:22:26,640 --> 00:22:28,879 Speaker 1: of who you are. Right, if I took you apart, 425 00:22:28,880 --> 00:22:31,040 Speaker 1: I could figure out exactly how many bananas you had 426 00:22:31,160 --> 00:22:34,440 Speaker 1: last week and what happened to them, and the stars 427 00:22:34,520 --> 00:22:37,840 Speaker 1: that burn the potassium that's in that banana, Like all 428 00:22:37,920 --> 00:22:41,760 Speaker 1: that history is encoded in that banana and then in you. Well, 429 00:22:41,840 --> 00:22:43,879 Speaker 1: and also when I flushed down the toilet, technically you 430 00:22:43,920 --> 00:22:46,120 Speaker 1: would have to go down the toilet. That's a whole 431 00:22:46,160 --> 00:22:49,560 Speaker 1: different maybe podcast episode. That's a different kind of black hole. 432 00:22:49,600 --> 00:22:52,200 Speaker 1: We're not going to dive into different um. So let's 433 00:22:52,240 --> 00:22:55,000 Speaker 1: get into now. Quantum mechanics says that you can destroy 434 00:22:55,440 --> 00:22:58,320 Speaker 1: quantum information. And so what happens when you throw it 435 00:22:58,440 --> 00:23:01,080 Speaker 1: into a black hole? Like does it get destroyed or 436 00:23:01,160 --> 00:23:03,440 Speaker 1: does it stay around inside of the black hole? That's 437 00:23:03,440 --> 00:23:06,600 Speaker 1: the big question. Yeah, and so on the surface you imagine, well, 438 00:23:06,800 --> 00:23:10,120 Speaker 1: black holes suck in information. Right, you put something into 439 00:23:10,160 --> 00:23:13,120 Speaker 1: a black hole, it can never leave, So therefore it's 440 00:23:13,200 --> 00:23:16,000 Speaker 1: information is stuck inside the black hole. That doesn't mean 441 00:23:16,080 --> 00:23:18,679 Speaker 1: necessarily that it's destroyed. Right, Like you put a banana 442 00:23:18,720 --> 00:23:20,800 Speaker 1: inside a black hole, you could still be in there. 443 00:23:21,119 --> 00:23:23,680 Speaker 1: The particles that made it up could be like squished 444 00:23:23,760 --> 00:23:26,560 Speaker 1: and whatever, but they just got quantum mechanics aified into 445 00:23:26,640 --> 00:23:29,280 Speaker 1: a new arrangement. And just like when you ate the 446 00:23:29,320 --> 00:23:32,800 Speaker 1: banana or when it grew, it's information could still be preserved, 447 00:23:32,880 --> 00:23:35,359 Speaker 1: but be stuck inside the black hole, you know, like 448 00:23:35,480 --> 00:23:38,760 Speaker 1: a like a neutron star kind of breaks everything down 449 00:23:39,040 --> 00:23:41,000 Speaker 1: to the cork level, but all the courts are still 450 00:23:41,080 --> 00:23:43,720 Speaker 1: kind they're bunched together precisely, and if the information is 451 00:23:43,720 --> 00:23:46,280 Speaker 1: still in there, it's stuck inside the black hole. Right, 452 00:23:46,560 --> 00:23:49,560 Speaker 1: nothing can ever leave the black hole. But also you 453 00:23:49,680 --> 00:23:52,760 Speaker 1: can't get any information from the outside about what's in 454 00:23:52,920 --> 00:23:55,600 Speaker 1: the black hole. The only things you can know about 455 00:23:55,600 --> 00:23:59,520 Speaker 1: a black hole are its mass, whether it's spinning, and 456 00:23:59,560 --> 00:24:03,119 Speaker 1: whether as electric charge. There's this crazy theorem in physics 457 00:24:03,200 --> 00:24:06,119 Speaker 1: called the no hair theorem that says that's all you 458 00:24:06,200 --> 00:24:07,760 Speaker 1: can know about a black hole. You mean, like the 459 00:24:08,040 --> 00:24:10,560 Speaker 1: overall charge of it, Like the black hole can have 460 00:24:10,600 --> 00:24:12,080 Speaker 1: a charge to it. Yeah, if you have a black 461 00:24:12,119 --> 00:24:14,679 Speaker 1: hole with no charge, it's neutral, and you throw an 462 00:24:14,720 --> 00:24:17,000 Speaker 1: electron into it, then it has a charge and you 463 00:24:17,080 --> 00:24:20,359 Speaker 1: can measure that charge. You can know whether there are 464 00:24:20,680 --> 00:24:23,080 Speaker 1: charged particles inside a black hole. Oh, I guess you 465 00:24:23,119 --> 00:24:26,440 Speaker 1: can measure how much it pulls proton through or something 466 00:24:26,480 --> 00:24:28,760 Speaker 1: like that, just like you can measure it's mass. You 467 00:24:28,840 --> 00:24:31,199 Speaker 1: throw a banana into a black hole, it got heavier. 468 00:24:31,359 --> 00:24:33,240 Speaker 1: You should be able to measure its mass by measuring 469 00:24:33,320 --> 00:24:36,919 Speaker 1: the gravitational field around a black hole. Can also measure 470 00:24:36,960 --> 00:24:39,840 Speaker 1: whether it's spinning. But that's the extent of the information 471 00:24:39,960 --> 00:24:43,080 Speaker 1: you can have, right. You can't tell what's inside. You 472 00:24:43,160 --> 00:24:45,879 Speaker 1: can't tell the detailed history of the banana from the outside, 473 00:24:45,920 --> 00:24:49,160 Speaker 1: so you can never get that information back out, right. 474 00:24:49,240 --> 00:24:51,760 Speaker 1: So that's step number one. Is the information, if it 475 00:24:51,840 --> 00:24:55,360 Speaker 1: still exists, is inside the black hole and can never leave, right. 476 00:24:55,480 --> 00:24:57,200 Speaker 1: But that's not the same as destroying it. It's just 477 00:24:57,320 --> 00:24:59,600 Speaker 1: kind of storing it. It's like inside if somewhere I 478 00:24:59,640 --> 00:25:02,480 Speaker 1: can never that's right. And if black holes live forever, 479 00:25:02,680 --> 00:25:05,080 Speaker 1: this wouldn't really be an issue. Would be a question of, like, well, 480 00:25:05,160 --> 00:25:07,760 Speaker 1: what happens inside the black hole? It's fascinating, but we 481 00:25:07,880 --> 00:25:10,520 Speaker 1: believe that probably information is just in there, sort of 482 00:25:10,680 --> 00:25:14,119 Speaker 1: cut off from us forever, but still existing. Right, it's 483 00:25:14,119 --> 00:25:16,720 Speaker 1: still having its own little happy life inside of the 484 00:25:16,760 --> 00:25:19,840 Speaker 1: black hole. That's right. The banana party, that's where bananas 485 00:25:19,880 --> 00:25:21,600 Speaker 1: go so that you don't eat them. Right, it's the 486 00:25:21,680 --> 00:25:24,119 Speaker 1: only safe space in the universe. They don't have to 487 00:25:24,160 --> 00:25:27,200 Speaker 1: worry about training black because everything is black inside of 488 00:25:27,200 --> 00:25:31,000 Speaker 1: a black hole. That's right. But then Stephen Hawking came 489 00:25:31,040 --> 00:25:34,400 Speaker 1: along and he showed us that black holes actually they 490 00:25:34,600 --> 00:25:38,400 Speaker 1: can disappear, right, Yes, you can make it black hole disappear. 491 00:25:38,560 --> 00:25:42,000 Speaker 1: It can evaporate. Yeah, black holes they evaporate. They give 492 00:25:42,040 --> 00:25:46,160 Speaker 1: off very small amounts of radiation, little particles here there. 493 00:25:46,600 --> 00:25:49,840 Speaker 1: For very big black holes, this happens extremely slowly. But 494 00:25:50,200 --> 00:25:53,920 Speaker 1: as black holes get smaller, they evaporate more quickly, and 495 00:25:54,119 --> 00:25:56,800 Speaker 1: then they can actually disappear. They can poof out of 496 00:25:56,880 --> 00:25:59,960 Speaker 1: existence as they give away their last little bit of energy. 497 00:26:00,080 --> 00:26:04,080 Speaker 1: Even like giant black holes will eventually disappear, like once 498 00:26:04,160 --> 00:26:07,000 Speaker 1: all black holes suck everything in the universe, Eventually they 499 00:26:07,040 --> 00:26:09,879 Speaker 1: will evaporate. Right, that's right. A black hole, if you 500 00:26:09,960 --> 00:26:12,680 Speaker 1: do not feed, it will give off Hawking radiation and 501 00:26:12,760 --> 00:26:15,480 Speaker 1: get smaller. Right. It gives off its energy, and that 502 00:26:15,640 --> 00:26:18,320 Speaker 1: energy comes from its mass, and so therefore it gets smaller, 503 00:26:18,840 --> 00:26:21,879 Speaker 1: and the smaller it gets, the more radiates. So giant, 504 00:26:22,000 --> 00:26:25,440 Speaker 1: massive black holes they might have lifetimes of trillions of years. 505 00:26:25,520 --> 00:26:30,000 Speaker 1: But yes, eventually they will radiate away all of their 506 00:26:30,080 --> 00:26:33,360 Speaker 1: mass in terms of this hawking radiation and disappear, right, 507 00:26:33,440 --> 00:26:36,399 Speaker 1: And so then the question is what happened to the 508 00:26:36,480 --> 00:26:38,960 Speaker 1: information you put into it? That's right, what happened to 509 00:26:39,000 --> 00:26:41,280 Speaker 1: the information inside the black hole? Like you put this 510 00:26:41,359 --> 00:26:44,080 Speaker 1: banana inside the black hole. You trust the black hole 511 00:26:44,160 --> 00:26:46,639 Speaker 1: is going to keep your banana information safe. But then 512 00:26:46,680 --> 00:26:48,720 Speaker 1: you come back a billion years later and the black 513 00:26:48,760 --> 00:26:51,359 Speaker 1: holes gone. You're like, what what happened to my You 514 00:26:51,440 --> 00:26:54,240 Speaker 1: deleted my banana from the universe. You know you can't 515 00:26:54,280 --> 00:26:57,960 Speaker 1: do that. Quantum mechanics says that's impossible. So the question 516 00:26:58,119 --> 00:27:01,119 Speaker 1: is what happened to the information? And you might be 517 00:27:01,200 --> 00:27:03,560 Speaker 1: tempted to think, oh, well, maybe it's somehow stored in 518 00:27:03,640 --> 00:27:07,240 Speaker 1: that hawking radiation, right, because the hawking radiation came out 519 00:27:07,320 --> 00:27:10,560 Speaker 1: of the black hole. But hawking radiation is very special. 520 00:27:10,880 --> 00:27:13,399 Speaker 1: It comes from the temperature of the black hole. It 521 00:27:13,520 --> 00:27:15,760 Speaker 1: comes from treating a black hole, like everything else in 522 00:27:15,800 --> 00:27:18,000 Speaker 1: the universe, is a thing that has a non zero 523 00:27:18,040 --> 00:27:22,080 Speaker 1: temperature which glows. And what's very important to understand is 524 00:27:22,119 --> 00:27:25,320 Speaker 1: that the hawking radiation depends only on the mass of 525 00:27:25,400 --> 00:27:28,200 Speaker 1: the black hole. Like how much hawking radiation you get 526 00:27:28,440 --> 00:27:31,320 Speaker 1: and which particles you get are determined by the mass 527 00:27:31,359 --> 00:27:34,720 Speaker 1: of the black hole and literally zero else, So none 528 00:27:34,760 --> 00:27:38,480 Speaker 1: of the information that's inside the black hole can possibly 529 00:27:38,600 --> 00:27:41,239 Speaker 1: leak out in hawking radiation. Well, I guess it's kind 530 00:27:41,280 --> 00:27:43,800 Speaker 1: of like if you have a glass of water, if 531 00:27:43,840 --> 00:27:46,080 Speaker 1: you leave it out, it's gonna evaporate, but you can 532 00:27:46,200 --> 00:27:49,239 Speaker 1: sort of trace what happened to the water. You can 533 00:27:49,320 --> 00:27:51,520 Speaker 1: trace the like the vapor of what molly kills as 534 00:27:51,560 --> 00:27:54,399 Speaker 1: it least the glass of water. Like that's okay, Like 535 00:27:54,680 --> 00:27:58,160 Speaker 1: that's preserving the information. That's right. But a black hole 536 00:27:58,280 --> 00:28:01,840 Speaker 1: doesn't evaporate by having the stuff inside of it leak out. 537 00:28:02,160 --> 00:28:04,800 Speaker 1: It evaporates by almost like having the stuff at the 538 00:28:04,880 --> 00:28:07,680 Speaker 1: surface destroyed itself. Kind of that's right. And remember the 539 00:28:07,760 --> 00:28:10,320 Speaker 1: no hair theorem tells us that you can't get any 540 00:28:10,440 --> 00:28:13,040 Speaker 1: information out of a black hole. That none of the 541 00:28:13,400 --> 00:28:16,480 Speaker 1: configuration of particles inside a black hole, or the swirling 542 00:28:16,560 --> 00:28:19,600 Speaker 1: or non swirling, or the singularity or non singularity can 543 00:28:19,680 --> 00:28:22,040 Speaker 1: affect what's produced on the outside of the black hole. 544 00:28:22,440 --> 00:28:26,440 Speaker 1: So the Hawking relation cannot have any information about what's 545 00:28:26,440 --> 00:28:28,560 Speaker 1: going on inside the black hole. It's not like that 546 00:28:28,840 --> 00:28:32,080 Speaker 1: water vapor example. It's a good contrast because it doesn't 547 00:28:32,080 --> 00:28:34,560 Speaker 1: tell you anything about what happened inside the black holes. 548 00:28:34,600 --> 00:28:37,920 Speaker 1: This amazing sort of mysterious way to delete a black 549 00:28:38,000 --> 00:28:40,720 Speaker 1: hole without knowing anything about what's inside of it, right, 550 00:28:40,840 --> 00:28:42,720 Speaker 1: because the reason is not because of the theorem. The 551 00:28:42,800 --> 00:28:45,440 Speaker 1: theorem is sort of because of what's happening in the 552 00:28:45,680 --> 00:28:48,520 Speaker 1: physics of it, right, And it's yeah, the theorem describes 553 00:28:48,600 --> 00:28:51,280 Speaker 1: the physics of it right, right, And and what's happening 554 00:28:51,360 --> 00:28:53,680 Speaker 1: is that, like at the surface of a black hole, 555 00:28:53,800 --> 00:28:57,080 Speaker 1: you get this pair of particle and antiparticles kind of appearing, 556 00:28:57,160 --> 00:28:58,680 Speaker 1: and one of them goes into the black hole, the 557 00:28:58,720 --> 00:29:02,000 Speaker 1: other one goes out of the black hole, and that's 558 00:29:02,080 --> 00:29:04,480 Speaker 1: kind of how it evaporates. Happening at the surface of it. 559 00:29:04,640 --> 00:29:07,000 Speaker 1: It's not happening because of anything that's inside of the 560 00:29:07,040 --> 00:29:09,320 Speaker 1: black hole exactly, and it comes just from the mass 561 00:29:09,440 --> 00:29:13,480 Speaker 1: the black hole. As you say, virtual particles like positron 562 00:29:13,600 --> 00:29:17,640 Speaker 1: anti positron pairs are created near the black hole's edge 563 00:29:17,920 --> 00:29:21,120 Speaker 1: where there's a lot of gravitational energy, and then one 564 00:29:21,200 --> 00:29:24,080 Speaker 1: of them is given a boost from that gravitational energy 565 00:29:24,120 --> 00:29:26,720 Speaker 1: while the other one maybe gets sucked in, and because 566 00:29:26,800 --> 00:29:29,800 Speaker 1: it's given a boost from that gravitational energy, that energy 567 00:29:29,920 --> 00:29:32,360 Speaker 1: comes from the mass of the black holes. The black 568 00:29:32,440 --> 00:29:36,120 Speaker 1: hole itself is decreased a tiny little bit in mass, 569 00:29:36,720 --> 00:29:39,200 Speaker 1: and so it's stealing some of the energy from the 570 00:29:39,240 --> 00:29:43,520 Speaker 1: black hole without apparently taking any information from it. And 571 00:29:43,680 --> 00:29:46,040 Speaker 1: so that's the weird thing is that, like you put 572 00:29:46,120 --> 00:29:48,720 Speaker 1: information in a black hole, you can never get it out, 573 00:29:49,120 --> 00:29:52,160 Speaker 1: but then the black hole can disappear. So where did 574 00:29:52,240 --> 00:29:56,480 Speaker 1: the information go? Really, there's no information in that suckings radiation. 575 00:29:56,640 --> 00:30:00,240 Speaker 1: I mean, like, wouldn't it like where it happens where 576 00:30:00,320 --> 00:30:03,440 Speaker 1: there's these particles and antiparticles form and where the one 577 00:30:03,480 --> 00:30:04,920 Speaker 1: of them goes right and the other one goes left. 578 00:30:04,960 --> 00:30:09,400 Speaker 1: Wouldn't that sort of depend on exactly what's going on 579 00:30:09,480 --> 00:30:11,840 Speaker 1: inside of the black hole. Well, the where the particles 580 00:30:11,880 --> 00:30:15,000 Speaker 1: are created is just quantum randomness around the black hole, 581 00:30:15,160 --> 00:30:18,120 Speaker 1: so that happens totally randomly, not depending on what's inside 582 00:30:18,160 --> 00:30:22,120 Speaker 1: the black hole. And then they're boosted from the gravitational field, 583 00:30:22,200 --> 00:30:23,960 Speaker 1: which is the mass of the black hole. So you 584 00:30:24,120 --> 00:30:26,520 Speaker 1: can know the mass of the black hole, and that's 585 00:30:26,560 --> 00:30:29,959 Speaker 1: what determines how these particles get boosted and whether they 586 00:30:30,000 --> 00:30:32,600 Speaker 1: go in the right direction, etcetera. But that doesn't contain 587 00:30:32,720 --> 00:30:35,520 Speaker 1: all the information. Like if you threw an apple or 588 00:30:35,520 --> 00:30:38,480 Speaker 1: an equivalently masked banana into a black hole, that would 589 00:30:38,520 --> 00:30:40,240 Speaker 1: give you black holes of the same mass, so they 590 00:30:40,240 --> 00:30:43,320 Speaker 1: would affect talking radiation in exactly the same way. So 591 00:30:43,600 --> 00:30:45,080 Speaker 1: the fact that one used to be an apple and 592 00:30:45,120 --> 00:30:47,640 Speaker 1: one used to be a banana is now irrelevant, which 593 00:30:47,720 --> 00:30:52,440 Speaker 1: means quantum information has been deleted all right, which is 594 00:30:52,480 --> 00:30:55,000 Speaker 1: kind of bad news for quantum physics, because you're telling 595 00:30:55,040 --> 00:30:58,880 Speaker 1: me that this idea that you can't destroy information is 596 00:30:59,280 --> 00:31:03,880 Speaker 1: fund mental to quantum mechanics. Maybe I really quickly, can 597 00:31:03,880 --> 00:31:05,880 Speaker 1: you tell me why it's so fundamental. I mean, remember 598 00:31:05,920 --> 00:31:08,640 Speaker 1: what we talked about earlier. The reason you can't destroy 599 00:31:08,760 --> 00:31:13,720 Speaker 1: information in quantum mechanics is because particles should always exist somewhere. 600 00:31:13,880 --> 00:31:15,480 Speaker 1: I mean, if you have a particle now, as you 601 00:31:15,600 --> 00:31:19,760 Speaker 1: exist somewhere in the future, it's quantum information cannot be destroyed, 602 00:31:19,920 --> 00:31:22,640 Speaker 1: like you don't know exactly where it is, but you 603 00:31:22,720 --> 00:31:25,800 Speaker 1: know what it's probability distribution looks like, and it should 604 00:31:25,920 --> 00:31:29,840 Speaker 1: have a probability distribution in the future also, and so 605 00:31:30,400 --> 00:31:33,160 Speaker 1: that can change as the universe moves forward, but the 606 00:31:33,280 --> 00:31:36,440 Speaker 1: information about should not be deleted anywhere. Right, Well, I 607 00:31:36,520 --> 00:31:40,760 Speaker 1: guess my question is, you know why not? Like why why? 608 00:31:40,960 --> 00:31:44,800 Speaker 1: Why would we quantum mechanics breakdown if I just suddenly 609 00:31:44,880 --> 00:31:48,320 Speaker 1: took some particles and deleted their quantum information? Like why 610 00:31:48,440 --> 00:31:51,680 Speaker 1: would the universe complain or with the universe care if 611 00:31:51,720 --> 00:31:54,680 Speaker 1: I had destroyed that information? All? Right? Well, mathematically we 612 00:31:54,960 --> 00:31:57,720 Speaker 1: look at the equations that describe a wave functions. We 613 00:31:57,760 --> 00:31:59,520 Speaker 1: have a wave function that tells us where particles are 614 00:31:59,560 --> 00:32:02,120 Speaker 1: likely to be you, and that moves forward in time. 615 00:32:02,160 --> 00:32:04,720 Speaker 1: There's an equation that describes how that happens. It's called 616 00:32:04,760 --> 00:32:07,920 Speaker 1: the shrouding your equation, and the shrouding your equation says 617 00:32:08,160 --> 00:32:11,200 Speaker 1: you can move information from here to there, but it's unitary, 618 00:32:11,320 --> 00:32:16,240 Speaker 1: doesn't ever destroy information. And if information is destroyed, that 619 00:32:16,400 --> 00:32:19,680 Speaker 1: means that wave functions can disappear. And that just doesn't 620 00:32:19,720 --> 00:32:22,160 Speaker 1: happen in the shorten your equation, and so we would 621 00:32:22,160 --> 00:32:25,080 Speaker 1: have to totally rethink the way quantum mechanics works if 622 00:32:25,160 --> 00:32:27,640 Speaker 1: that was to happen. It's like a bedrock assumption that 623 00:32:27,720 --> 00:32:31,840 Speaker 1: we've built into quantum mechanics. I see, it's like I 624 00:32:31,880 --> 00:32:35,120 Speaker 1: guess in quantum mechanics and wave functions, you know, these 625 00:32:35,200 --> 00:32:37,640 Speaker 1: functions don't don't just exist in the present and in 626 00:32:37,720 --> 00:32:41,160 Speaker 1: the past. They're all sort of tied together mathematically to 627 00:32:41,240 --> 00:32:42,959 Speaker 1: where they're going to be in the future. That's right, 628 00:32:43,040 --> 00:32:45,040 Speaker 1: So like if you destroy it in the future, then 629 00:32:45,080 --> 00:32:47,760 Speaker 1: you're really destroying it through all history. You don't have 630 00:32:47,880 --> 00:32:50,040 Speaker 1: a term for that in the equation. Yeah, And the 631 00:32:50,080 --> 00:32:53,040 Speaker 1: equations work the same way forwards and backwards in time, 632 00:32:53,640 --> 00:32:56,120 Speaker 1: and so if the wave function is ever destroyed, that 633 00:32:56,240 --> 00:32:58,680 Speaker 1: means that you couldn't go from a non existent wave 634 00:32:58,720 --> 00:33:01,480 Speaker 1: function backwards in time into the wave function you have now. 635 00:33:02,160 --> 00:33:04,480 Speaker 1: So this sort of this time and variance built into 636 00:33:04,600 --> 00:33:06,880 Speaker 1: quantum mechanics. You can run the clock forward, you can 637 00:33:06,960 --> 00:33:08,920 Speaker 1: run the clock backwards. You should be able to move 638 00:33:09,000 --> 00:33:11,600 Speaker 1: backwards and forwards at all points. But if the information 639 00:33:11,720 --> 00:33:14,520 Speaker 1: is ever deleted, that means you can't move backwards and 640 00:33:14,600 --> 00:33:16,760 Speaker 1: forwards at all points. And the shrunning equation, the basic 641 00:33:16,920 --> 00:33:20,360 Speaker 1: assumptions on which it's built are totally wrong, and quantum 642 00:33:20,360 --> 00:33:22,080 Speaker 1: mechanics doesn't work, and we'd have to come up with 643 00:33:22,160 --> 00:33:24,800 Speaker 1: a new theory. It's not like the universe would puff 644 00:33:24,840 --> 00:33:28,240 Speaker 1: out of existence. Right, This is all human ideas about 645 00:33:28,280 --> 00:33:31,280 Speaker 1: how the universe might work. This is a basic assumption 646 00:33:31,360 --> 00:33:34,400 Speaker 1: we've built into quantum mechanics that we're pretty sure is right. 647 00:33:35,080 --> 00:33:37,959 Speaker 1: But black holes are telling us that they're doing something 648 00:33:38,440 --> 00:33:43,320 Speaker 1: that we thought was impossible. Man, there's such troublemakers, all right, 649 00:33:43,400 --> 00:33:45,800 Speaker 1: So we have a big unknown here. How can both 650 00:33:45,920 --> 00:33:50,400 Speaker 1: things be true? How could information never be destroyed according 651 00:33:50,440 --> 00:33:53,920 Speaker 1: to quantum mechanics and how can information be destroyed according 652 00:33:54,040 --> 00:33:57,440 Speaker 1: to black holes and hawking radiation? So let's get into 653 00:33:57,520 --> 00:34:01,520 Speaker 1: what could possibly explain this can prediction. But first let's 654 00:34:01,600 --> 00:34:14,200 Speaker 1: take a quick break, all right, Daniel, can information be 655 00:34:14,320 --> 00:34:17,640 Speaker 1: destroyed inside of a black hole? So quantum mechanics says no, 656 00:34:18,400 --> 00:34:22,280 Speaker 1: but kind of a black hole say yes. So what's 657 00:34:22,280 --> 00:34:26,160 Speaker 1: going on? Is quantum mechanics wrong or do black holes 658 00:34:26,280 --> 00:34:29,919 Speaker 1: just kind of destroy our conception of how the universe works. 659 00:34:30,160 --> 00:34:32,719 Speaker 1: This is a big puzzle in physics for a long time, 660 00:34:33,400 --> 00:34:36,080 Speaker 1: and it's such a big puzzle that like big folks 661 00:34:36,120 --> 00:34:38,759 Speaker 1: on both sides, like great brains on both sides of 662 00:34:38,760 --> 00:34:41,719 Speaker 1: the argument, had like public debates about it and even 663 00:34:41,840 --> 00:34:44,279 Speaker 1: made bets about the resolution of this. Right. Yeah, there's 664 00:34:44,280 --> 00:34:47,800 Speaker 1: a famous bed by between Hawking and Kip Thorne and 665 00:34:48,040 --> 00:34:50,920 Speaker 1: John Preskill. Right, that's right. John Prescille believed that somehow 666 00:34:51,040 --> 00:34:54,040 Speaker 1: the information was sneaking out of the black hole back 667 00:34:54,120 --> 00:34:57,719 Speaker 1: into the universe, that it was leaking out essentially where 668 00:34:57,840 --> 00:35:00,880 Speaker 1: Stephen Hawking and Kip Thorn they thought, know, the information 669 00:35:01,040 --> 00:35:03,480 Speaker 1: can't ever leave the black hole, and therefore it must 670 00:35:03,560 --> 00:35:06,239 Speaker 1: be lost from the universe, and quantum mechanics is wrong. 671 00:35:06,760 --> 00:35:08,800 Speaker 1: So they made a very public sort of bet about this. 672 00:35:08,960 --> 00:35:11,799 Speaker 1: All right, So they made this bed and did they 673 00:35:12,680 --> 00:35:14,520 Speaker 1: was one of im proven right? Well, they did come 674 00:35:14,560 --> 00:35:16,920 Speaker 1: to what they think is a resolution to this, and 675 00:35:17,080 --> 00:35:20,840 Speaker 1: so Hawking and Thorn actually capitulated on the bet in 676 00:35:20,920 --> 00:35:23,319 Speaker 1: public and said, all right, Prescott, we think you're right. 677 00:35:23,760 --> 00:35:26,239 Speaker 1: We think that the information somehow leaks out of the 678 00:35:26,320 --> 00:35:30,359 Speaker 1: black hole. So wait, physicists think that black holes don't 679 00:35:30,400 --> 00:35:33,080 Speaker 1: destroy information. That's right. So the idea now is probably 680 00:35:33,120 --> 00:35:36,719 Speaker 1: black holes don't destroy information. I mean, the general categories 681 00:35:36,760 --> 00:35:40,719 Speaker 1: of solutions are one, maybe quantum mechanics is just wrong 682 00:35:40,920 --> 00:35:43,280 Speaker 1: and we have to toss it all out and rethink 683 00:35:43,440 --> 00:35:47,200 Speaker 1: everything about our idea of the universe at the smallest scales, 684 00:35:47,320 --> 00:35:49,839 Speaker 1: like that's an option and hey, that wouldn't be so bad. 685 00:35:49,920 --> 00:35:52,959 Speaker 1: It's not like everything unravels and we all go living 686 00:35:53,000 --> 00:35:57,000 Speaker 1: in caves or something. Just a bunch of physicist careers unraveled. No, 687 00:35:57,280 --> 00:36:00,399 Speaker 1: those are the best moments for physicist careers because like, wow, 688 00:36:00,520 --> 00:36:03,200 Speaker 1: that cracks open something deep that we thought was true. 689 00:36:03,600 --> 00:36:06,040 Speaker 1: Those are the revolutions in physics we live for. That's 690 00:36:06,080 --> 00:36:09,040 Speaker 1: why we're here to figure out what in the firm 691 00:36:09,160 --> 00:36:11,120 Speaker 1: and turns out to be wrong, because those are the 692 00:36:11,560 --> 00:36:13,520 Speaker 1: times when you can get a new glimpse onto a 693 00:36:13,640 --> 00:36:16,200 Speaker 1: new insight into the universe. I mean, wow, that would 694 00:36:16,200 --> 00:36:19,440 Speaker 1: be amazing. Right, So that's one possibility maybe quantum mechanics 695 00:36:19,600 --> 00:36:23,239 Speaker 1: is wrong um, And what are other possibilities black holes 696 00:36:23,280 --> 00:36:27,080 Speaker 1: are wrong? Another one is that like black holes, you 697 00:36:27,120 --> 00:36:30,440 Speaker 1: can think of them as storing this information, but that 698 00:36:30,520 --> 00:36:33,799 Speaker 1: they're also like connected to another universe. We've talked about 699 00:36:33,800 --> 00:36:38,120 Speaker 1: how maybe black holes are like doors to wormholes that 700 00:36:38,200 --> 00:36:40,880 Speaker 1: are connected on the other side to other places in 701 00:36:40,960 --> 00:36:44,080 Speaker 1: the universe. They could also be connected to like separate 702 00:36:44,160 --> 00:36:48,239 Speaker 1: distinct universes that we don't otherwise have access to. It's 703 00:36:48,280 --> 00:36:50,400 Speaker 1: a possibility. I mean, we're it's like a what if 704 00:36:50,480 --> 00:36:52,520 Speaker 1: on top of a wood if. But the idea is 705 00:36:52,600 --> 00:36:55,960 Speaker 1: that therefore the information could be in that universe, like 706 00:36:56,080 --> 00:36:59,360 Speaker 1: maybe the banana got sucked into the black hole and 707 00:36:59,440 --> 00:37:02,040 Speaker 1: then slur belong to the wormhole and it's living off 708 00:37:02,080 --> 00:37:05,319 Speaker 1: it's banana like days in that other universe. Now, even 709 00:37:05,440 --> 00:37:09,640 Speaker 1: when our black hole disappears, I see like somehow there's 710 00:37:09,880 --> 00:37:12,759 Speaker 1: a white hole on the other side that's spewing out bananas. 711 00:37:13,200 --> 00:37:15,400 Speaker 1: That's right, a banana hole. I think it's what the 712 00:37:15,440 --> 00:37:19,000 Speaker 1: people in that universe we call it like that. I 713 00:37:19,040 --> 00:37:21,759 Speaker 1: think they call it the magic banana fountain. They're like 714 00:37:22,640 --> 00:37:26,040 Speaker 1: whole cult surrounding it about how generous this banana fountain is. 715 00:37:26,280 --> 00:37:28,560 Speaker 1: You're like a god in that universe. You're like the 716 00:37:28,640 --> 00:37:32,399 Speaker 1: giver of bananas in that universe. I'm a legend. I'm 717 00:37:32,440 --> 00:37:35,560 Speaker 1: a legend in another universe. They're like, but please stop 718 00:37:35,600 --> 00:37:37,760 Speaker 1: throwing bananas in there with a bite taken out already, 719 00:37:37,800 --> 00:37:41,080 Speaker 1: I mean please. So that's one idea, Yes, that it's 720 00:37:41,400 --> 00:37:44,640 Speaker 1: information is not disappearing, it's just going somewhere else. Yeah, 721 00:37:45,080 --> 00:37:48,040 Speaker 1: but that's hard to really understand because then you can't 722 00:37:48,040 --> 00:37:51,360 Speaker 1: still really do quantum mechanics, like the information is effectively 723 00:37:51,400 --> 00:37:54,040 Speaker 1: lost to us, and so then we can't do quantum 724 00:37:54,040 --> 00:37:57,960 Speaker 1: mechanics of our universe, so it's not really Essentially, if 725 00:37:58,000 --> 00:38:00,600 Speaker 1: it's lost to us, it's a bummer. It's a bummer 726 00:38:00,640 --> 00:38:03,759 Speaker 1: because you know, is our wave function entangled with their 727 00:38:03,800 --> 00:38:06,800 Speaker 1: wave function if they're in another universe? Then no, And 728 00:38:06,960 --> 00:38:09,800 Speaker 1: so really quantum mechanics says, you can't lose any information 729 00:38:09,920 --> 00:38:11,800 Speaker 1: from your wave functions. So if you lose it to 730 00:38:11,920 --> 00:38:17,239 Speaker 1: a totally incoherent wave function, it's effectively lost anyway. So 731 00:38:17,360 --> 00:38:20,399 Speaker 1: quantum mechanics says no to that. Very clever, I think, 732 00:38:20,760 --> 00:38:23,680 Speaker 1: awesome idea, which would be a great basis for science fiction. 733 00:38:23,800 --> 00:38:26,680 Speaker 1: Interesting like we're entangled with other universe. Yeah, but we 734 00:38:26,719 --> 00:38:29,120 Speaker 1: wouldn't actually be entangled, right, That's the problem is that 735 00:38:29,200 --> 00:38:31,520 Speaker 1: our wave function isn't connected to theirs because it goes 736 00:38:31,560 --> 00:38:34,359 Speaker 1: through the wormhole. All right, So then what's the third 737 00:38:35,160 --> 00:38:39,120 Speaker 1: The third possibility is that maybe somehow that information is 738 00:38:39,360 --> 00:38:42,920 Speaker 1: actually imprinted on the Hawking radiation. So go back, that's 739 00:38:42,960 --> 00:38:45,319 Speaker 1: what I was saying, wasn't it that you were saying? 740 00:38:45,640 --> 00:38:48,840 Speaker 1: He shot me down? But now it seems like Stephen 741 00:38:48,840 --> 00:38:51,520 Speaker 1: Hawking agrees with me. That's right. This is known as 742 00:38:51,640 --> 00:38:57,800 Speaker 1: the Hawking thorn cham theory of the universe should be. No, 743 00:38:57,920 --> 00:39:01,200 Speaker 1: you're right, and you know, our understanding before this was 744 00:39:01,280 --> 00:39:03,600 Speaker 1: that it's impossible for the information to be in the 745 00:39:03,680 --> 00:39:06,640 Speaker 1: Hawking radiation for the very reasonable arguments that I gave 746 00:39:06,680 --> 00:39:11,960 Speaker 1: you five minutes ago, which I will now undermine. It 747 00:39:12,040 --> 00:39:16,160 Speaker 1: made me feel bad, Daniel, No, nor yeah, alright, So 748 00:39:16,360 --> 00:39:18,440 Speaker 1: here's why your idea was a good one. And you know, 749 00:39:18,480 --> 00:39:20,920 Speaker 1: whenever you have an apparent contradiction, you have a string 750 00:39:21,040 --> 00:39:23,600 Speaker 1: of logical arguments that leads you to something nonsensical, you 751 00:39:23,680 --> 00:39:25,680 Speaker 1: have to go back and read examined, like well what 752 00:39:25,800 --> 00:39:27,680 Speaker 1: about this one? Is this one? Are we really sure 753 00:39:27,680 --> 00:39:29,520 Speaker 1: about this? And try to find a hole in it. 754 00:39:30,120 --> 00:39:33,840 Speaker 1: And so the idea is that maybe somehow the information 755 00:39:33,880 --> 00:39:36,400 Speaker 1: about the banana you threw in is imprinted on the 756 00:39:36,440 --> 00:39:39,840 Speaker 1: hawking radiation. Well, how could that happen because once it 757 00:39:39,920 --> 00:39:42,719 Speaker 1: goes inside the black hole, the only information we can 758 00:39:42,760 --> 00:39:44,600 Speaker 1: get about it is how much mass it has, which 759 00:39:44,680 --> 00:39:48,759 Speaker 1: is essentially destroying the banana nous of the information. So 760 00:39:49,080 --> 00:39:52,719 Speaker 1: the idea is maybe it never really goes inside the 761 00:39:52,840 --> 00:39:56,320 Speaker 1: black hole, like maybe a banana when you throw it 762 00:39:56,360 --> 00:39:59,160 Speaker 1: into a black hole, spends eternity sort of on the 763 00:39:59,360 --> 00:40:02,960 Speaker 1: surface of the black hole. One. And this is actually 764 00:40:03,000 --> 00:40:06,200 Speaker 1: what what happens when you throw something into a black hole. 765 00:40:06,520 --> 00:40:10,560 Speaker 1: You never actually see it go in because remember, when 766 00:40:10,800 --> 00:40:14,640 Speaker 1: near a black hole, there's incredible gravity, and that slows 767 00:40:14,719 --> 00:40:18,000 Speaker 1: down time. Like you threw a clock into a black 768 00:40:18,080 --> 00:40:20,759 Speaker 1: hole and you watched it with a telescope, please from 769 00:40:20,840 --> 00:40:23,960 Speaker 1: very far away, you would see that clock ticks slow 770 00:40:24,080 --> 00:40:27,960 Speaker 1: down because the presence of mass slows downtime. Right. Yeah, 771 00:40:28,560 --> 00:40:31,640 Speaker 1: So to the banana, you're seeing, the banana gets frozen 772 00:40:31,719 --> 00:40:34,000 Speaker 1: at the surface kind of. Yeah. As it gets closer 773 00:40:34,080 --> 00:40:37,799 Speaker 1: and closer to this event horizon, time slows down more 774 00:40:37,880 --> 00:40:41,279 Speaker 1: and more, to the point where it slows down essentially infinitely. 775 00:40:41,560 --> 00:40:44,319 Speaker 1: And you can watch this banana for the whole time, 776 00:40:44,400 --> 00:40:46,719 Speaker 1: the lifetime of the universe. You will never see it 777 00:40:46,880 --> 00:40:50,840 Speaker 1: cross the event horizon. Oh uh. It's not like it 778 00:40:50,960 --> 00:40:54,600 Speaker 1: goes in and then the particles the photons can come out. 779 00:40:54,680 --> 00:40:56,879 Speaker 1: It's like it never goes in. Kind of from our 780 00:40:56,960 --> 00:41:00,360 Speaker 1: point of view, From our perspective, you never see anything 781 00:41:00,440 --> 00:41:03,600 Speaker 1: actually go into a black hole. Now it gets closer 782 00:41:04,000 --> 00:41:07,440 Speaker 1: and closer, and it gets redder and redder because the 783 00:41:07,560 --> 00:41:10,080 Speaker 1: light from that banana, which can still get to you. 784 00:41:10,160 --> 00:41:12,520 Speaker 1: Because the banana is not actually in the black hole, 785 00:41:12,920 --> 00:41:15,960 Speaker 1: it gets stretched also by the gravity and gets redder 786 00:41:16,040 --> 00:41:18,800 Speaker 1: and redd or longer and longer wavelengths. So what happens 787 00:41:18,840 --> 00:41:20,959 Speaker 1: if you have trillions of years to hang out and watch, 788 00:41:21,400 --> 00:41:23,919 Speaker 1: is that banana falls in more and more slowly, gets 789 00:41:24,040 --> 00:41:27,400 Speaker 1: darker and darker, and eventually goes out past the visible spectrum. 790 00:41:27,440 --> 00:41:28,520 Speaker 1: You can't see it, and then you have to use 791 00:41:28,560 --> 00:41:32,960 Speaker 1: your infrared telescope to watch your very gently glowing banana. Right. 792 00:41:33,080 --> 00:41:37,240 Speaker 1: But I guess I thought I thought time was became 793 00:41:37,280 --> 00:41:39,839 Speaker 1: a singularity, only only at the center of the black hole. 794 00:41:39,960 --> 00:41:43,040 Speaker 1: You're saying that time actually stops at the edge of it. Yeah, 795 00:41:43,160 --> 00:41:45,640 Speaker 1: at the edge of the black hole, time slows down 796 00:41:45,760 --> 00:41:49,360 Speaker 1: essentially infinitely, like and that's for you. You're from the 797 00:41:49,480 --> 00:41:52,200 Speaker 1: outside point of view. You're watching the banana go in. 798 00:41:52,480 --> 00:41:55,160 Speaker 1: That's not the same thing as the banana experiences. Banana 799 00:41:55,520 --> 00:41:57,480 Speaker 1: can fall into a black hole, and it can totally 800 00:41:57,520 --> 00:42:00,560 Speaker 1: experience going past the event horizon, right, because time always 801 00:42:00,600 --> 00:42:03,880 Speaker 1: goes at one second per second for the person experiencing it. 802 00:42:04,440 --> 00:42:06,760 Speaker 1: We have a different story about what happens in banana 803 00:42:07,000 --> 00:42:10,319 Speaker 1: watching from the outside. So for us, the banana never 804 00:42:10,440 --> 00:42:15,120 Speaker 1: actually goes into the black hole for us. Interesting for us. Wait, 805 00:42:15,200 --> 00:42:20,040 Speaker 1: so it gets frozen at the surface forever. Yes, but 806 00:42:20,160 --> 00:42:23,040 Speaker 1: it gets stretched out right, It's not like just happy, 807 00:42:23,080 --> 00:42:24,759 Speaker 1: you can't go back and pick up your banana. It 808 00:42:24,760 --> 00:42:28,120 Speaker 1: gets stretched out and reddened and smeared over the surface 809 00:42:28,239 --> 00:42:32,440 Speaker 1: of the black hole. And essentially it distorts the event horizon. 810 00:42:32,840 --> 00:42:35,680 Speaker 1: It like changes the shape of the event horizon in 811 00:42:35,880 --> 00:42:39,480 Speaker 1: some way. And the ideas that maybe the banana changes 812 00:42:39,600 --> 00:42:42,640 Speaker 1: the shape of the event horizon differently than an apple wood, 813 00:42:42,719 --> 00:42:46,279 Speaker 1: or differently than another banana in a way that we 814 00:42:46,360 --> 00:42:48,359 Speaker 1: can see, or in a way that we will never see, 815 00:42:48,440 --> 00:42:51,880 Speaker 1: in a way that in principle preserves the quantum information 816 00:42:52,080 --> 00:42:57,320 Speaker 1: of that banana and can influence the hawking radiation produced 817 00:42:57,440 --> 00:43:00,520 Speaker 1: at that point instead of the event rise and being 818 00:43:00,560 --> 00:43:04,800 Speaker 1: a perfectly smooth sphere and now has little quantum wiggles 819 00:43:04,800 --> 00:43:07,960 Speaker 1: in it, and those quantum wiggles tell you about what's 820 00:43:08,000 --> 00:43:11,080 Speaker 1: been thrown into the black hole, meaning that you could 821 00:43:11,400 --> 00:43:14,759 Speaker 1: measure the hawking radiation and reconstruct whether you threw a 822 00:43:14,840 --> 00:43:16,879 Speaker 1: banana or an apple in exactly that the black hole. 823 00:43:16,920 --> 00:43:19,840 Speaker 1: You threw banana in would give you different hawking radiation 824 00:43:19,920 --> 00:43:22,279 Speaker 1: than the banana you threw an apple into, and that 825 00:43:22,360 --> 00:43:25,560 Speaker 1: it's encoded somehow and now in the surface of this 826 00:43:25,800 --> 00:43:29,120 Speaker 1: black hole, which contains all the information but everything that's 827 00:43:29,160 --> 00:43:31,600 Speaker 1: been thrown into the black hole. So you're not breaking 828 00:43:31,680 --> 00:43:34,960 Speaker 1: general relativity because you're not getting information but what's inside 829 00:43:35,040 --> 00:43:37,719 Speaker 1: the black hole, because in principle, all of this is 830 00:43:37,760 --> 00:43:40,560 Speaker 1: now encoded on the surface of the black hole. Right, 831 00:43:40,719 --> 00:43:45,000 Speaker 1: But the courts in the banana dude disappear or you 832 00:43:45,160 --> 00:43:47,759 Speaker 1: don't see them. You don't see them going into the 833 00:43:47,800 --> 00:43:50,960 Speaker 1: black hole. Like they're going to survive crazy experiences being 834 00:43:51,080 --> 00:43:53,480 Speaker 1: near a black hole and get torn apart and smash 835 00:43:53,560 --> 00:43:55,359 Speaker 1: and other stuff. So who knows what's going to happen, 836 00:43:55,719 --> 00:43:59,000 Speaker 1: But their quantum information should still be there. Everything that 837 00:43:59,160 --> 00:44:01,960 Speaker 1: happened to them is describable by quantum mechanics, and just 838 00:44:02,080 --> 00:44:05,120 Speaker 1: like being eaten or being turned into banana smoothie, their 839 00:44:05,280 --> 00:44:07,880 Speaker 1: history is still carried with me. And that's okay with 840 00:44:08,000 --> 00:44:11,880 Speaker 1: quantum mechanics, Like as long as the quantum history information 841 00:44:12,040 --> 00:44:15,120 Speaker 1: and information is somehow carried on, even if it's like 842 00:44:15,239 --> 00:44:18,920 Speaker 1: passed between the banana cork it passes on that information 843 00:44:19,040 --> 00:44:21,799 Speaker 1: to the hawking radiation. That's still okay, that's right. Did 844 00:44:21,800 --> 00:44:23,879 Speaker 1: you just create a new kind of cork, the banana cork. 845 00:44:24,200 --> 00:44:27,080 Speaker 1: We've got up cork, charm cork, banana cork. I thought 846 00:44:27,120 --> 00:44:31,239 Speaker 1: they already existed. No, but you're exactly right. Somehow, the 847 00:44:31,360 --> 00:44:34,080 Speaker 1: information about that cork that was inside your banana is 848 00:44:34,200 --> 00:44:37,239 Speaker 1: encoded on the surface of the black hole and influences 849 00:44:37,520 --> 00:44:41,120 Speaker 1: the hawking radiation that's produced. And therefore, if you like 850 00:44:41,560 --> 00:44:44,200 Speaker 1: gathered all the hawking radiation that came out of a 851 00:44:44,239 --> 00:44:47,319 Speaker 1: black hole, you could tell exactly what had gone into 852 00:44:47,400 --> 00:44:49,799 Speaker 1: the black hole in the whole lifetime of the black hole. 853 00:44:50,880 --> 00:44:53,719 Speaker 1: And this is weird because this is what they call 854 00:44:53,840 --> 00:44:58,120 Speaker 1: like the holographic principle, meaning like you know, you can describe, 855 00:44:58,360 --> 00:45:00,399 Speaker 1: like if the whole universe falls into a black hole, 856 00:45:00,560 --> 00:45:03,560 Speaker 1: you could at some point technically everything would be described 857 00:45:03,600 --> 00:45:05,640 Speaker 1: on the surface of the black hole, right, which is 858 00:45:05,719 --> 00:45:09,279 Speaker 1: like a two D surface. It's like a flat surface. Yeah, 859 00:45:09,320 --> 00:45:12,160 Speaker 1: it's sort of mysterious to say you can describe everything 860 00:45:12,239 --> 00:45:15,000 Speaker 1: that's happening in a three D space, like the inside 861 00:45:15,000 --> 00:45:18,000 Speaker 1: of a black hole, just by knowing information on a 862 00:45:18,160 --> 00:45:21,560 Speaker 1: two D space the surface of the black hole. So like, 863 00:45:22,000 --> 00:45:25,840 Speaker 1: how can everything inside a three D space be described 864 00:45:25,920 --> 00:45:28,440 Speaker 1: by the surface of that space. Well, that's what we 865 00:45:28,520 --> 00:45:31,360 Speaker 1: call a hologram. A hologram is a two D image 866 00:45:31,600 --> 00:45:33,680 Speaker 1: that's projected into a three D space, so it looks 867 00:45:33,760 --> 00:45:37,160 Speaker 1: three D. The entire hologram is determined actually by what's 868 00:45:37,200 --> 00:45:40,600 Speaker 1: happening on the surface. So the ideas maybe black holes, 869 00:45:40,640 --> 00:45:44,400 Speaker 1: the interiors of them are just holograms of their surfaces 870 00:45:44,840 --> 00:45:47,520 Speaker 1: that you can build a sort of a theory of 871 00:45:47,719 --> 00:45:50,800 Speaker 1: physics that works in three D. That's actually the theory 872 00:45:50,840 --> 00:45:53,279 Speaker 1: of physics in two D on a surface, like you 873 00:45:53,320 --> 00:45:56,120 Speaker 1: don't need three dimensions. Maybe you can describe everything on 874 00:45:56,280 --> 00:45:58,680 Speaker 1: on a surface exactly. And so the idea is like, well, 875 00:45:58,960 --> 00:46:02,399 Speaker 1: maybe that's also true like for our universe, Like maybe 876 00:46:02,480 --> 00:46:06,000 Speaker 1: our three D universe is just a projection, is a 877 00:46:06,080 --> 00:46:09,239 Speaker 1: two D hologram of what's happening at the edge of 878 00:46:09,320 --> 00:46:13,600 Speaker 1: our universe. We think we live in this three D 879 00:46:13,719 --> 00:46:16,680 Speaker 1: world and we're all moving around three dimensions. But if 880 00:46:16,760 --> 00:46:18,960 Speaker 1: you can print all the information of a three D 881 00:46:19,080 --> 00:46:22,400 Speaker 1: world onto a two D surface, then it's possible that 882 00:46:22,600 --> 00:46:24,800 Speaker 1: we actually live on the two D surface at the 883 00:46:25,040 --> 00:46:27,960 Speaker 1: edge of the universe somewhere and that what we experience 884 00:46:28,040 --> 00:46:29,880 Speaker 1: is that three D world is really just a two 885 00:46:30,000 --> 00:46:35,960 Speaker 1: D surface. But okay, so I guess it's like if 886 00:46:36,040 --> 00:46:38,040 Speaker 1: this can happen on a black hole, then maybe it's 887 00:46:38,040 --> 00:46:41,120 Speaker 1: happening everywhere. And maybe if we don't really need three dimensions, 888 00:46:41,239 --> 00:46:45,080 Speaker 1: maybe like we have a redundant dimensions, right, And then 889 00:46:45,120 --> 00:46:48,600 Speaker 1: there was this incredible result in string theory which backed 890 00:46:48,640 --> 00:46:51,280 Speaker 1: this up. This guy at the Institute for Advanced Science, 891 00:46:51,400 --> 00:46:54,080 Speaker 1: Jue Malda Sena, he came up with this theory that 892 00:46:54,200 --> 00:46:58,160 Speaker 1: showed that string theory in you know, three dimensions that 893 00:46:58,239 --> 00:47:02,360 Speaker 1: we experience, it can actually be described by a quantum 894 00:47:02,440 --> 00:47:05,399 Speaker 1: theory in two dimensions. So he showed how you could 895 00:47:05,520 --> 00:47:09,560 Speaker 1: reconstruct a theory of our universe in three dimensions only 896 00:47:09,640 --> 00:47:12,280 Speaker 1: on a two dimensional surface. So it sort of showed 897 00:47:12,360 --> 00:47:16,040 Speaker 1: mathematically that this might be possible. So what does that mean? 898 00:47:16,080 --> 00:47:18,800 Speaker 1: That means that we're really living an illusion, like the 899 00:47:18,880 --> 00:47:21,040 Speaker 1: three dimensions that we think we're living in are actually 900 00:47:21,960 --> 00:47:25,080 Speaker 1: just an illusion. Kind of It could be, right, Yeah, 901 00:47:25,160 --> 00:47:27,080 Speaker 1: it certainly could be. It could be that we actually 902 00:47:27,120 --> 00:47:28,920 Speaker 1: live in a two D space Like I mean, it 903 00:47:28,960 --> 00:47:31,560 Speaker 1: doesn't make any difference like feeling like you live in 904 00:47:31,600 --> 00:47:33,880 Speaker 1: three D and actually living in three D, Like what's 905 00:47:33,920 --> 00:47:38,279 Speaker 1: the difference? Uh? Nothing, But mathematically it might be that 906 00:47:38,360 --> 00:47:41,040 Speaker 1: our three D universe can be described as just a 907 00:47:41,160 --> 00:47:43,680 Speaker 1: two D surface, which is sort of fascinating because you 908 00:47:43,800 --> 00:47:47,239 Speaker 1: feel like there's too much information here, right that that 909 00:47:47,400 --> 00:47:50,000 Speaker 1: everything that's happening to us is somehow too much to 910 00:47:50,040 --> 00:47:54,240 Speaker 1: squeeze down to two dimensions. But mathematically it can be equivalent. 911 00:47:54,320 --> 00:47:56,000 Speaker 1: It could be that it's just that we don't have 912 00:47:56,120 --> 00:47:58,640 Speaker 1: the full freedom of the three dimensions, that we're just 913 00:47:58,800 --> 00:48:01,239 Speaker 1: a projection of two D spit. But I guess maybe 914 00:48:01,400 --> 00:48:03,560 Speaker 1: the way you explain it maybe is that you also 915 00:48:03,600 --> 00:48:07,479 Speaker 1: have time and maybe like somehow time is also giving 916 00:48:07,560 --> 00:48:10,759 Speaker 1: you that extra feeling of a three or third dimension. Right, Well, 917 00:48:10,800 --> 00:48:12,680 Speaker 1: here we're just talking about spatial dimensions, and so that 918 00:48:12,800 --> 00:48:15,120 Speaker 1: two D space would also have time in it, so 919 00:48:15,560 --> 00:48:18,040 Speaker 1: it's allowed to evolve that things can move on the 920 00:48:18,120 --> 00:48:21,120 Speaker 1: two D surface, and that changes what happens inside the 921 00:48:21,200 --> 00:48:23,839 Speaker 1: three D space, But we don't know right that. Yeah, 922 00:48:23,880 --> 00:48:25,680 Speaker 1: I guess that's what I mean. It's like, because you 923 00:48:25,719 --> 00:48:27,879 Speaker 1: have time, then you can maybe store more things into 924 00:48:27,920 --> 00:48:30,400 Speaker 1: that to the information than then you might think. But 925 00:48:30,520 --> 00:48:33,600 Speaker 1: you know, it's a big leap, Like we say, maybe 926 00:48:34,000 --> 00:48:36,359 Speaker 1: information is stored on the surface of black holes, which 927 00:48:36,440 --> 00:48:39,400 Speaker 1: means that maybe you can determine their interior to maybe 928 00:48:39,640 --> 00:48:42,759 Speaker 1: the whole universe is a holomeram. Like, there's a lot 929 00:48:42,840 --> 00:48:45,400 Speaker 1: of big leaps there, But again they're also fascinating there, Like, 930 00:48:45,480 --> 00:48:48,080 Speaker 1: you know, maybe trying to solve this mystery about what's 931 00:48:48,080 --> 00:48:50,359 Speaker 1: happening inside of a black hole tells us about what's 932 00:48:50,440 --> 00:48:53,640 Speaker 1: possible for ideas we could have about the universe, and 933 00:48:54,120 --> 00:48:57,280 Speaker 1: and reveals to us sort of shocking new mathematical connections 934 00:48:57,320 --> 00:49:00,239 Speaker 1: that show us that the richness of our universe might 935 00:49:00,280 --> 00:49:04,879 Speaker 1: actually be representable in terms of a smaller set of dimensions. Right, Yeah, 936 00:49:05,080 --> 00:49:07,040 Speaker 1: like maybe we're all living in a video game. Kind 937 00:49:07,080 --> 00:49:09,719 Speaker 1: of it just seems like we're in a three D world, 938 00:49:09,760 --> 00:49:13,080 Speaker 1: but really we're we're just in this kind of reconstruction 939 00:49:13,160 --> 00:49:15,080 Speaker 1: of a three D world, that's right. And if we 940 00:49:15,120 --> 00:49:16,520 Speaker 1: are living in a video game, I want to know 941 00:49:16,800 --> 00:49:20,759 Speaker 1: what are the cheat codes? How do I reset? How 942 00:49:20,800 --> 00:49:25,719 Speaker 1: do I get extra lives? Exactly? All right? Well, um, 943 00:49:26,239 --> 00:49:30,759 Speaker 1: it sounds like maybe black holes are not destroying information. 944 00:49:31,000 --> 00:49:33,280 Speaker 1: Maybe that that seems to be kind of the current 945 00:49:33,480 --> 00:49:35,960 Speaker 1: physics thinking is that maybe it is sort of recorded 946 00:49:36,000 --> 00:49:38,680 Speaker 1: on the surfaces of black holes. Yeah, and you know, 947 00:49:38,760 --> 00:49:41,040 Speaker 1: this stuff is pretty hand wavy. It's not like people 948 00:49:41,080 --> 00:49:43,520 Speaker 1: have really worked out the mathematical details of it. It's 949 00:49:43,520 --> 00:49:46,200 Speaker 1: sort of like an idea for idea we might have. 950 00:49:46,360 --> 00:49:48,880 Speaker 1: It's like a crack a way to explore it that 951 00:49:49,280 --> 00:49:52,960 Speaker 1: might be able to reveal what's happening with black holes 952 00:49:53,000 --> 00:49:55,920 Speaker 1: and information. It's not like a very totally solid worked 953 00:49:55,920 --> 00:49:58,080 Speaker 1: out idea. I see, these are just kind of like 954 00:49:58,520 --> 00:50:02,000 Speaker 1: directions in which that might have playing these things exactly exactly, 955 00:50:02,239 --> 00:50:04,919 Speaker 1: and we we we might be getting closer to knowing 956 00:50:05,000 --> 00:50:06,880 Speaker 1: the answer, right, I mean, we just took a picture 957 00:50:06,920 --> 00:50:09,319 Speaker 1: of a black hole. Maybe in the future we might 958 00:50:09,480 --> 00:50:11,840 Speaker 1: get closer to it and figure these things out. Or 959 00:50:12,080 --> 00:50:14,680 Speaker 1: is this closed off to us forever. That's a great question. 960 00:50:14,880 --> 00:50:17,000 Speaker 1: And you know, we could send somebody into a black 961 00:50:17,080 --> 00:50:18,960 Speaker 1: hole and maybe they could learn something about it. The 962 00:50:19,080 --> 00:50:22,040 Speaker 1: problem is we'd never know the answer because they couldn't 963 00:50:22,040 --> 00:50:25,920 Speaker 1: tell us. We might as well send dogs in, right, Well, 964 00:50:25,960 --> 00:50:28,120 Speaker 1: we're going to get a letter from the cat. Our 965 00:50:28,200 --> 00:50:31,399 Speaker 1: cats depending it. You know, Well, if you're a dog lover, 966 00:50:31,480 --> 00:50:33,600 Speaker 1: you can, we can send cats to we should just 967 00:50:33,680 --> 00:50:36,400 Speaker 1: send robots. And let's just send robots. No, there's no 968 00:50:36,560 --> 00:50:39,640 Speaker 1: society protecting the life of robots, right, that's right, the 969 00:50:39,760 --> 00:50:43,839 Speaker 1: dog robots, dog robots. There, that's a perfect compromise, all right. 970 00:50:43,880 --> 00:50:45,520 Speaker 1: But again, it just tells you that there's a lot 971 00:50:45,600 --> 00:50:47,680 Speaker 1: we don't know about the universe, and that even like 972 00:50:47,840 --> 00:50:50,840 Speaker 1: our experience of it, this three dimensional experience of it, 973 00:50:50,960 --> 00:50:54,399 Speaker 1: might be not real or not what we think it is. Yeah, 974 00:50:54,480 --> 00:50:56,960 Speaker 1: and that deep insights into the very nature of the 975 00:50:57,040 --> 00:50:59,719 Speaker 1: universe can come from these little odds and ends, these 976 00:50:59,760 --> 00:51:02,000 Speaker 1: things that all we thought we understood, and then there's 977 00:51:02,000 --> 00:51:04,680 Speaker 1: a little detail that doesn't quite make sense, and when 978 00:51:04,719 --> 00:51:08,400 Speaker 1: you tug on that thread, it could unravel literally everything 979 00:51:08,520 --> 00:51:11,080 Speaker 1: we think we understand about the universe. This is how 980 00:51:11,360 --> 00:51:14,960 Speaker 1: lots of great discoveries were made relativity, quantum mechanics, and 981 00:51:15,040 --> 00:51:19,160 Speaker 1: hopefully future crazy bonkers discoveries that people will have a 982 00:51:19,280 --> 00:51:22,520 Speaker 1: hard time accepting is the true nature of the anivers 983 00:51:22,880 --> 00:51:24,800 Speaker 1: Until then, I guess I'll stay to a blender to 984 00:51:24,840 --> 00:51:28,520 Speaker 1: make my fans. I think that's a good idea. All right, Well, 985 00:51:28,600 --> 00:51:31,200 Speaker 1: we hope you enjoyed that Thanks for joining us. Let's 986 00:51:31,200 --> 00:51:41,840 Speaker 1: see you next time. Thanks for listening, and remember that 987 00:51:42,000 --> 00:51:44,719 Speaker 1: Daniel and Jorge Explain the Universe is a production of 988 00:51:44,880 --> 00:51:48,200 Speaker 1: I heart Radio. For more podcast for my heart Radio, 989 00:51:48,360 --> 00:51:51,920 Speaker 1: visit the i heart Radio app, Apple Podcasts, or wherever 990 00:51:52,040 --> 00:52:02,840 Speaker 1: you listen to your favorite shows. M