1 00:00:08,600 --> 00:00:10,760 Speaker 1: Hey, Katie, are you a fan of Italian food? 2 00:00:11,119 --> 00:00:13,880 Speaker 2: Well? I live in Italy, so here we just call 3 00:00:13,920 --> 00:00:14,560 Speaker 2: it food. 4 00:00:14,880 --> 00:00:19,520 Speaker 1: But yeah, all right, Well what about Italian American food? 5 00:00:19,600 --> 00:00:23,160 Speaker 1: You know, the version made by Italian immigrants to America. 6 00:00:23,440 --> 00:00:24,400 Speaker 2: Yeah, no, I like it. 7 00:00:24,400 --> 00:00:28,360 Speaker 3: It's more meatballs and more garlic, but that's still really good. 8 00:00:28,520 --> 00:00:31,920 Speaker 1: Well what about the opposite, what about American Italian food? 9 00:00:32,200 --> 00:00:37,080 Speaker 3: So is that cuisine made by American immigrants who are 10 00:00:37,120 --> 00:00:37,760 Speaker 3: in Italy? 11 00:00:38,400 --> 00:00:38,600 Speaker 2: Yeah? 12 00:00:38,720 --> 00:00:39,559 Speaker 1: Basically you. 13 00:00:40,159 --> 00:00:44,199 Speaker 3: Well, I mean I mostly just have coffee and toast, 14 00:00:44,400 --> 00:00:46,440 Speaker 3: which would be a really short cookbook. 15 00:00:48,080 --> 00:00:50,120 Speaker 1: Maybe you should try innovating. Have you ever tried putting 16 00:00:50,120 --> 00:00:51,280 Speaker 1: a meatball in your coffee? 17 00:00:51,960 --> 00:00:55,480 Speaker 2: I know I have not tried to do that, Daniel. 18 00:00:55,960 --> 00:00:57,440 Speaker 1: Could be a cultural revolution. 19 00:00:57,680 --> 00:01:14,440 Speaker 3: Well, it would indeed be revolting. 20 00:01:15,680 --> 00:01:15,880 Speaker 2: Hi. 21 00:01:16,000 --> 00:01:19,160 Speaker 1: I'm Daniel. I'm a particle physicist and a professor at 22 00:01:19,280 --> 00:01:22,160 Speaker 1: uc Ervine, and I don't like anything in my coffee, 23 00:01:22,319 --> 00:01:23,480 Speaker 1: definitely not meatballs. 24 00:01:23,800 --> 00:01:25,399 Speaker 2: Hi. I am Katie. 25 00:01:25,560 --> 00:01:30,080 Speaker 3: I host a podcast called Creature feature on evolutionary biology, 26 00:01:30,240 --> 00:01:34,520 Speaker 3: and I like a huge amount of sugar in my coffee. 27 00:01:34,880 --> 00:01:40,440 Speaker 3: So we could see how that is with meatballs as well. Well. 28 00:01:40,440 --> 00:01:43,280 Speaker 1: That makes me wonder since you're a biologist, tell me 29 00:01:43,520 --> 00:01:46,640 Speaker 1: who are the natural consumers of coffee? Like, who out 30 00:01:46,680 --> 00:01:49,120 Speaker 1: there in the animal world is eating coffee beans off 31 00:01:49,120 --> 00:01:49,480 Speaker 1: the tree. 32 00:01:49,800 --> 00:01:54,680 Speaker 3: That's the thing is that coffee caffeine in coffee plants 33 00:01:54,760 --> 00:02:00,560 Speaker 3: is meant to be slightly toxic to insects that want 34 00:02:00,640 --> 00:02:04,080 Speaker 3: to eat it. And it's the same story for spicy foods. 35 00:02:04,120 --> 00:02:08,280 Speaker 3: It's actually defense mechanism, and so the insects that will 36 00:02:08,320 --> 00:02:13,160 Speaker 3: try to eat these plants will not farewell. But when 37 00:02:13,160 --> 00:02:16,480 Speaker 3: we have it, it's actually delicious and good. Now, there 38 00:02:16,560 --> 00:02:21,160 Speaker 3: are palm civets who will eat types of coffee plants. 39 00:02:21,800 --> 00:02:26,760 Speaker 3: They eat the berries, and there's actually a coffee drink 40 00:02:26,919 --> 00:02:31,919 Speaker 3: made out of the beans collected from the palm civet hoop. 41 00:02:32,320 --> 00:02:34,799 Speaker 2: And it's very expensive. 42 00:02:34,960 --> 00:02:35,160 Speaker 3: Wow. 43 00:02:35,200 --> 00:02:37,360 Speaker 1: I don't know what blows my mind more there the 44 00:02:37,400 --> 00:02:40,480 Speaker 1: fact that we are sipping insect poison, or the fact 45 00:02:40,520 --> 00:02:43,440 Speaker 1: that that whole strategy has backfired on the coffee tree 46 00:02:43,520 --> 00:02:46,880 Speaker 1: because it attracts us, or how quickly a biologist will 47 00:02:46,880 --> 00:02:48,480 Speaker 1: turn the conversation towards poop. 48 00:02:50,680 --> 00:02:52,639 Speaker 2: The latter is the least surprising. 49 00:02:54,440 --> 00:02:56,800 Speaker 1: That is, in the end, where we overlap the darkest 50 00:02:56,880 --> 00:03:01,120 Speaker 1: matters in the Universe and Welcome the podcast Daniel and 51 00:03:01,200 --> 00:03:05,280 Speaker 1: Jorge Explain the Universe the production of iHeartRadio, in which 52 00:03:05,280 --> 00:03:08,280 Speaker 1: we try to do just that. Explore everything that's out 53 00:03:08,320 --> 00:03:12,320 Speaker 1: there in the universe, ask our deepest, darkest questions about 54 00:03:12,360 --> 00:03:15,079 Speaker 1: who is sipping which bits of the universe and why 55 00:03:15,120 --> 00:03:18,360 Speaker 1: they exist in that way? What are the tiniest particles 56 00:03:18,480 --> 00:03:20,600 Speaker 1: that everything is made out of, What are the rules 57 00:03:20,600 --> 00:03:23,080 Speaker 1: by which they play? How do they come together to 58 00:03:23,120 --> 00:03:26,040 Speaker 1: make civets and cats and poops and coffee and biologists 59 00:03:26,080 --> 00:03:29,560 Speaker 1: who wonder about all those things combined? Is it possible 60 00:03:29,600 --> 00:03:32,760 Speaker 1: to understand and explain the universe? We're going to try. 61 00:03:33,040 --> 00:03:34,920 Speaker 3: That is the first thing I think of when I 62 00:03:34,920 --> 00:03:39,880 Speaker 3: think about civt kat poop is the tiniest of particles 63 00:03:40,560 --> 00:03:44,760 Speaker 3: that make up that coffee. But yeah, I mean, I guess, 64 00:03:44,800 --> 00:03:49,040 Speaker 3: I guess when you can go down really really tiny, 65 00:03:49,320 --> 00:03:51,960 Speaker 3: and that makes things like poop less gross because now 66 00:03:52,560 --> 00:03:56,880 Speaker 3: you're just on the atomic level and these are just atoms. 67 00:03:56,920 --> 00:03:58,840 Speaker 2: They don't smell. Atoms don't smell bad. 68 00:03:58,960 --> 00:04:01,960 Speaker 1: I don't think, well, does it make poop less gross 69 00:04:02,000 --> 00:04:04,280 Speaker 1: to think that it's made of the same basic building 70 00:04:04,280 --> 00:04:06,560 Speaker 1: blocks as everything else, or does it make everything else 71 00:04:06,800 --> 00:04:10,040 Speaker 1: more gross to know that ice cream and lava and 72 00:04:10,120 --> 00:04:12,120 Speaker 1: kittens are made out of the same stuff as poop. 73 00:04:14,560 --> 00:04:17,800 Speaker 2: Interesting question, ice cream, lava. 74 00:04:20,360 --> 00:04:22,840 Speaker 1: Let's put a pin in that. But let's dive deep 75 00:04:22,960 --> 00:04:25,800 Speaker 1: into what the universe is made out of. One of 76 00:04:25,839 --> 00:04:28,600 Speaker 1: our deepest questions in physics, and a question that humans 77 00:04:28,640 --> 00:04:31,880 Speaker 1: have been asking basically since humans have been asking questions, 78 00:04:32,400 --> 00:04:35,240 Speaker 1: is how do things work at the smallest scale? Is 79 00:04:35,279 --> 00:04:38,719 Speaker 1: it possible to zoom down on what's around us and 80 00:04:38,800 --> 00:04:41,919 Speaker 1: explain things in simpler and simpler terms, Because you know, 81 00:04:42,040 --> 00:04:44,160 Speaker 1: you start out with a huge number of things out 82 00:04:44,200 --> 00:04:47,039 Speaker 1: there in the universe blueberries and cats and ice cream 83 00:04:47,080 --> 00:04:50,920 Speaker 1: and coffee and biologists and physicists and everything in between. 84 00:04:51,200 --> 00:04:54,120 Speaker 1: It's an incredible variety. But when you dig down a 85 00:04:54,120 --> 00:04:56,599 Speaker 1: little bit, you discover, oh, everything out there is made 86 00:04:56,640 --> 00:04:59,880 Speaker 1: out of about one hundred basic building blocks the elements 87 00:05:00,160 --> 00:05:04,520 Speaker 1: periodic table. Combined in different ways, you can make essentially everything. 88 00:05:04,640 --> 00:05:07,160 Speaker 1: And even that set of one hundred building blocks is 89 00:05:07,200 --> 00:05:10,360 Speaker 1: made out of an even smaller set of stuff. Right, 90 00:05:10,400 --> 00:05:14,560 Speaker 1: Protons and neutrons and electrons make up all of those atoms, 91 00:05:15,040 --> 00:05:17,400 Speaker 1: which means that the same stuff can be used to 92 00:05:17,440 --> 00:05:20,440 Speaker 1: make lava or kittens, or ice cream or poops, or 93 00:05:20,480 --> 00:05:24,800 Speaker 1: biologists or stars. All that stuff is made out of 94 00:05:24,839 --> 00:05:25,560 Speaker 1: the same thing. 95 00:05:26,120 --> 00:05:29,560 Speaker 3: It's interesting because I do know that one of the 96 00:05:29,600 --> 00:05:33,320 Speaker 3: things that unites kittens and lava and poop is that 97 00:05:33,400 --> 00:05:38,840 Speaker 3: it all obeys the laws of physics. If you throw 98 00:05:38,880 --> 00:05:41,200 Speaker 3: a kitten in some lava, you're going to have a 99 00:05:41,279 --> 00:05:44,440 Speaker 3: predictable result because of the laws of physics. Both the 100 00:05:44,560 --> 00:05:49,039 Speaker 3: kitten and the lava are constrained by the laws of physics. 101 00:05:49,240 --> 00:05:52,800 Speaker 3: But the thing that's interesting to me, and that hurts 102 00:05:52,839 --> 00:05:55,599 Speaker 3: my brain a little bit, is that when you look 103 00:05:55,720 --> 00:06:00,520 Speaker 3: at say like a very tiny quantum part of it 104 00:06:00,560 --> 00:06:03,640 Speaker 3: does not necessarily obey the same laws of physics as 105 00:06:03,720 --> 00:06:06,920 Speaker 3: say a marble. So you know, I think of like 106 00:06:06,960 --> 00:06:11,040 Speaker 3: a marble bonking into another marble. I can somewhat understand 107 00:06:11,080 --> 00:06:14,000 Speaker 3: how that works. But then you go down small enough 108 00:06:14,400 --> 00:06:18,240 Speaker 3: and it's not just tiny atomic marbles bonking into each other. 109 00:06:18,920 --> 00:06:21,520 Speaker 3: Weird stuff happens that blows my mind. 110 00:06:21,880 --> 00:06:24,279 Speaker 1: It is incredible that the laws of physics seem to 111 00:06:24,320 --> 00:06:27,560 Speaker 1: be different at different scales, like at different distances or 112 00:06:27,640 --> 00:06:31,440 Speaker 1: different energies. It seems like different rules apply, like to 113 00:06:31,600 --> 00:06:35,640 Speaker 1: baseballs and to electrons. The rules are fundamentally different. There 114 00:06:35,640 --> 00:06:37,840 Speaker 1: are different kinds of stuff and the rules that apply 115 00:06:37,880 --> 00:06:39,800 Speaker 1: to them are different, and that does feel weird, and 116 00:06:39,800 --> 00:06:42,320 Speaker 1: it's one of the most incredible things about the universe. 117 00:06:42,400 --> 00:06:44,120 Speaker 1: But a helpful way to think about it is in 118 00:06:44,200 --> 00:06:47,919 Speaker 1: terms of phases, Like think about water. Water has a 119 00:06:47,960 --> 00:06:50,480 Speaker 1: liquid phase and a solid phase and a gas phase. 120 00:06:50,560 --> 00:06:52,120 Speaker 1: Right in the end, we think it's all made out 121 00:06:52,120 --> 00:06:54,719 Speaker 1: of the same basic stuff water molecules, but they act 122 00:06:54,920 --> 00:06:58,360 Speaker 1: very differently under different circumstances. And you wouldn't expect the 123 00:06:58,400 --> 00:07:00,720 Speaker 1: laws of an ideal gas to describe what happens when 124 00:07:00,720 --> 00:07:04,320 Speaker 1: water crystallizes, or fluid dynamics to explain how a gas 125 00:07:04,360 --> 00:07:08,599 Speaker 1: would expand different rules apply in different scenarios, different phases, 126 00:07:08,839 --> 00:07:11,360 Speaker 1: And so we imagine that the universe is organized the 127 00:07:11,400 --> 00:07:13,240 Speaker 1: same way you can think of You can think of 128 00:07:13,240 --> 00:07:15,840 Speaker 1: it as sort of different phases where different rules apply. 129 00:07:16,520 --> 00:07:19,520 Speaker 1: What we don't know is if there is an underlying 130 00:07:19,680 --> 00:07:22,960 Speaker 1: theory behind all of it, the sort of physics version 131 00:07:23,080 --> 00:07:26,520 Speaker 1: of the water molecule, the tiniest little bits who's dancing 132 00:07:26,560 --> 00:07:29,680 Speaker 1: and tuing and froing and interacting is somehow making all 133 00:07:29,760 --> 00:07:33,760 Speaker 1: this other stuff emerge, even the quantum particles, even the baseballs, 134 00:07:33,840 --> 00:07:37,440 Speaker 1: even the galaxies. Is there something at the lowest level 135 00:07:37,480 --> 00:07:41,360 Speaker 1: which is determining everything from which all of our experience emerges. 136 00:07:42,000 --> 00:07:45,440 Speaker 3: So this is an interesting and confusing question to me, 137 00:07:45,560 --> 00:07:50,720 Speaker 3: because from my understanding, if we're all in the same universe, 138 00:07:51,200 --> 00:07:55,800 Speaker 3: we would all regardless of whether we're a human or 139 00:07:56,040 --> 00:07:59,440 Speaker 3: a quark or a kitten, we'd have to play by 140 00:07:59,480 --> 00:08:01,160 Speaker 3: the same rules. 141 00:08:01,640 --> 00:08:03,480 Speaker 2: But if the rules are. 142 00:08:04,080 --> 00:08:07,480 Speaker 3: Different somehow, right, like for a quark versus a kitten 143 00:08:08,200 --> 00:08:10,360 Speaker 3: in terms of physics, even though the kitten is also 144 00:08:10,600 --> 00:08:15,080 Speaker 3: made out of quarks or atoms molecules, it's hard for 145 00:08:15,120 --> 00:08:18,560 Speaker 3: me to wrap my head around there not being a 146 00:08:19,320 --> 00:08:23,640 Speaker 3: unifying set of rules that applies to everything, given that 147 00:08:24,120 --> 00:08:26,600 Speaker 3: not only do we live in the same universe, but 148 00:08:26,640 --> 00:08:29,400 Speaker 3: we're made out of all the same stuff. 149 00:08:29,760 --> 00:08:32,839 Speaker 1: Yeah, it's a great question, and a basic assumption about 150 00:08:32,880 --> 00:08:35,360 Speaker 1: a lot of physics is that that's possible that if 151 00:08:35,400 --> 00:08:37,800 Speaker 1: you zoom down to the smallest scale, you can find 152 00:08:37,800 --> 00:08:40,000 Speaker 1: the most basic set of rules, and that then you 153 00:08:40,040 --> 00:08:43,079 Speaker 1: could somehow zoom back out with the fundamental theory of 154 00:08:43,080 --> 00:08:46,480 Speaker 1: the universe in hand, you could explain everything it might 155 00:08:46,520 --> 00:08:48,840 Speaker 1: require you to calculate, like how ten to the twenty 156 00:08:48,920 --> 00:08:51,640 Speaker 1: nine particles come together to make a baseball. But the 157 00:08:51,679 --> 00:08:55,240 Speaker 1: idea is, in principle, it's all determined by what's happening 158 00:08:55,280 --> 00:08:58,000 Speaker 1: at the smaller scale, and when you zoom out, that's 159 00:08:58,040 --> 00:09:00,600 Speaker 1: just what those laws look like. And it might be 160 00:09:00,679 --> 00:09:02,880 Speaker 1: the case, right It might be that even though we 161 00:09:02,960 --> 00:09:06,760 Speaker 1: have trouble explaining how a zillion water droplets interacting in 162 00:09:06,800 --> 00:09:09,200 Speaker 1: the atmosphere make a hurricane, we can't even do it 163 00:09:09,200 --> 00:09:12,920 Speaker 1: with our fastest supercomputers. We think that probably it is 164 00:09:13,040 --> 00:09:17,160 Speaker 1: determined by that, but that's actually a philosophical assumption, and 165 00:09:17,240 --> 00:09:20,560 Speaker 1: some philosophers of science disagree with that. It's called strong 166 00:09:20,720 --> 00:09:23,360 Speaker 1: emergence at some point to lots of things that we 167 00:09:23,440 --> 00:09:27,160 Speaker 1: can't explain using underlying details. A great example is like 168 00:09:27,559 --> 00:09:31,160 Speaker 1: why you are here your consciousness. We have completely failed 169 00:09:31,200 --> 00:09:34,280 Speaker 1: so far to explain the experience of human consciousness in 170 00:09:34,400 --> 00:09:36,960 Speaker 1: terms of like the zapping of the little neurons inside 171 00:09:37,000 --> 00:09:39,920 Speaker 1: of our brains. It might be that somehow all that 172 00:09:39,960 --> 00:09:42,680 Speaker 1: stuff comes together to explain why you are experiencing this 173 00:09:42,760 --> 00:09:45,680 Speaker 1: podcast right now. But it might also be that there 174 00:09:45,720 --> 00:09:48,920 Speaker 1: are just different rules at different levels of the universe 175 00:09:49,240 --> 00:09:52,280 Speaker 1: that aren't actually determined by the lower levels, that somehow 176 00:09:52,320 --> 00:09:56,000 Speaker 1: there are independent layers of the universe and different rules 177 00:09:56,040 --> 00:09:58,960 Speaker 1: apply at each one. It's a weird philosophy of the universe, 178 00:09:59,040 --> 00:10:01,439 Speaker 1: but it might also be our universe. 179 00:10:01,280 --> 00:10:05,280 Speaker 3: That's very hard for my conscious brain to wrap itself around. 180 00:10:05,400 --> 00:10:09,880 Speaker 3: It is very interesting, this philosophical question of consciousness because 181 00:10:10,280 --> 00:10:14,080 Speaker 3: if we apply sort of the rules of like, well, 182 00:10:14,120 --> 00:10:17,840 Speaker 3: a brain works right because you have a communication between 183 00:10:17,880 --> 00:10:21,400 Speaker 3: many parts, you have neurons that are all communicating with 184 00:10:21,480 --> 00:10:24,120 Speaker 3: each other and forming these networks. Well, there's a lot 185 00:10:24,120 --> 00:10:28,720 Speaker 3: of things that do that, from computers to ant colonies, 186 00:10:29,320 --> 00:10:33,480 Speaker 3: and so the question is, well, are those things conscious 187 00:10:33,520 --> 00:10:35,880 Speaker 3: as well? And we can't really quantify that, and we 188 00:10:35,960 --> 00:10:39,960 Speaker 3: can't know whether even though it seems like there's this 189 00:10:40,080 --> 00:10:43,960 Speaker 3: underlying rule of you know, you require these sort of 190 00:10:43,960 --> 00:10:47,559 Speaker 3: individual units that are all communicating together and forming patterns, 191 00:10:47,600 --> 00:10:50,160 Speaker 3: and that's what you need for consciousness. If you see 192 00:10:50,160 --> 00:10:54,280 Speaker 3: that repeated in other systems, whether that actually applies to say, 193 00:10:54,320 --> 00:10:59,000 Speaker 3: can you recreate a consciousness with an electronic version of 194 00:10:59,280 --> 00:11:02,679 Speaker 3: neurons or or is something like a very complex ant 195 00:11:02,720 --> 00:11:04,280 Speaker 3: colony with thousands of ants? 196 00:11:04,320 --> 00:11:08,199 Speaker 2: Does that recreate consciousness. So I guess in a way. 197 00:11:08,200 --> 00:11:12,800 Speaker 3: I could see how there could be different rules applying 198 00:11:12,840 --> 00:11:18,240 Speaker 3: to different layers, but it's just so strange and so like. Currently, 199 00:11:18,800 --> 00:11:22,680 Speaker 3: when we look at like quantum mechanics, it does not 200 00:11:22,880 --> 00:11:26,920 Speaker 3: do a good job of explaining physics on a larger scale. 201 00:11:27,240 --> 00:11:30,640 Speaker 1: Mostly we cannot connect the layers that we have. Even 202 00:11:30,679 --> 00:11:34,920 Speaker 1: though that's basically the motivation for the project to understand 203 00:11:34,920 --> 00:11:37,280 Speaker 1: everything at the smallest scale and use that to explain 204 00:11:37,360 --> 00:11:41,880 Speaker 1: everything else that's bigger, we have very rarely succeeded in 205 00:11:42,000 --> 00:11:45,959 Speaker 1: using a zoomed in microscopic approach to explain anything bigger. 206 00:11:46,040 --> 00:11:46,160 Speaker 4: You know. 207 00:11:46,240 --> 00:11:50,160 Speaker 1: One famous success story is ideal gases. Is say, okay, 208 00:11:50,160 --> 00:11:52,480 Speaker 1: we have this picture of atoms moving in a gas 209 00:11:52,559 --> 00:11:55,120 Speaker 1: as tiny little balls. Can we zoom out and think 210 00:11:55,160 --> 00:11:58,440 Speaker 1: about what happens to ten to the twenty nine balls, 211 00:11:58,440 --> 00:12:01,920 Speaker 1: and can we write equations that tell mathematical stories about 212 00:12:01,960 --> 00:12:05,040 Speaker 1: things that emerge from ten to the twenty nine tiny 213 00:12:05,080 --> 00:12:08,120 Speaker 1: little gas molecules like pressure and temperature and volume, and 214 00:12:08,240 --> 00:12:11,120 Speaker 1: we can you can actually derive, like the ideal gas 215 00:12:11,280 --> 00:12:15,280 Speaker 1: law from statistical mechanics explanations about the velocities of those 216 00:12:15,320 --> 00:12:18,199 Speaker 1: tiny little particles. That's a famous example because it's one 217 00:12:18,200 --> 00:12:21,040 Speaker 1: of the rare successes. Mostly we have failed because the 218 00:12:21,120 --> 00:12:24,680 Speaker 1: universe is kind of chaotic. It's really sensitive often to 219 00:12:24,840 --> 00:12:27,920 Speaker 1: these tiny little details. What happens to this quantum particle 220 00:12:27,920 --> 00:12:31,240 Speaker 1: affects another quantum particle, which affects another quantum particle. We 221 00:12:31,280 --> 00:12:34,040 Speaker 1: don't understand how to do that calculation. Most of the time, 222 00:12:34,160 --> 00:12:36,040 Speaker 1: we don't have the computing power, and we can't avoid 223 00:12:36,040 --> 00:12:39,000 Speaker 1: this chaos problem. So mostly we don't know how to 224 00:12:39,080 --> 00:12:41,640 Speaker 1: do that. It might be that it is determined and 225 00:12:41,679 --> 00:12:43,880 Speaker 1: it's possible to do those calculations, is just sort of 226 00:12:44,160 --> 00:12:47,200 Speaker 1: beyond our ability right now. Or it might be that 227 00:12:47,280 --> 00:12:50,360 Speaker 1: it's just not that different rules apply in different regimes, 228 00:12:50,400 --> 00:12:51,800 Speaker 1: as weird as that is. 229 00:12:52,280 --> 00:12:56,520 Speaker 3: So, I guess I'm not so familiar with quantum mechanics 230 00:12:56,600 --> 00:13:01,440 Speaker 3: and general relativity. Can we kind of just hammer down, 231 00:13:01,480 --> 00:13:04,560 Speaker 3: like what are those two things? How Like what do 232 00:13:04,600 --> 00:13:06,640 Speaker 3: they apply to and what don't they apply to? 233 00:13:07,160 --> 00:13:09,360 Speaker 1: So at the forefront of our understanding of the most 234 00:13:09,559 --> 00:13:13,320 Speaker 1: microscopic picture of how the universe works, we have two 235 00:13:13,360 --> 00:13:16,560 Speaker 1: basic theories. We have quantum mechanics, which tells us about 236 00:13:16,559 --> 00:13:19,240 Speaker 1: really tiny stuff, and general relativity, which tells us about 237 00:13:19,320 --> 00:13:23,240 Speaker 1: really big, heavy stuff, basically quantum mechanics for particles and 238 00:13:23,320 --> 00:13:26,480 Speaker 1: general relativity for gravity. One of the biggest frustrations in 239 00:13:26,480 --> 00:13:29,240 Speaker 1: physics in the last one hundred years has been our 240 00:13:29,280 --> 00:13:32,520 Speaker 1: inability to bring them together into a single story, to 241 00:13:32,640 --> 00:13:35,840 Speaker 1: weave them into a unified picture of how the universe works. 242 00:13:36,000 --> 00:13:38,200 Speaker 1: You know, this whole project of like, let's explain everything 243 00:13:38,200 --> 00:13:40,560 Speaker 1: from the tiniest particles and then zoom out. Well, we 244 00:13:40,600 --> 00:13:43,400 Speaker 1: haven't even succeeded in explaining the tinese particles yet, but 245 00:13:43,440 --> 00:13:46,360 Speaker 1: there's a vigorous program of people working on this stuff. 246 00:13:46,400 --> 00:13:48,840 Speaker 1: And in today's episode, we're going to dig into one 247 00:13:48,880 --> 00:13:52,320 Speaker 1: of the most recent and weirdest ideas about how to 248 00:13:52,360 --> 00:13:56,400 Speaker 1: bring quantum mechanics and relativity together. So on today's episode, 249 00:13:56,440 --> 00:14:05,760 Speaker 1: we're going to be answering the question, what is quantum relativity? 250 00:14:05,960 --> 00:14:11,480 Speaker 3: Hmmm, quantum relativity. So it's like quantum mechanics and general 251 00:14:11,520 --> 00:14:13,480 Speaker 3: relativity had a baby. 252 00:14:15,720 --> 00:14:18,360 Speaker 1: It also sounds like the buzzword name for a startup 253 00:14:18,360 --> 00:14:19,880 Speaker 1: where you're like, I don't even really know what it 254 00:14:20,000 --> 00:14:23,600 Speaker 1: they do, but it sounds pretty good. So before we 255 00:14:23,600 --> 00:14:25,680 Speaker 1: dig into the details of this, I checked in with 256 00:14:25,720 --> 00:14:28,720 Speaker 1: our listeners to see if they had any idea about 257 00:14:28,720 --> 00:14:32,680 Speaker 1: the theory of quantum relativity, if they had heard this before, 258 00:14:32,720 --> 00:14:34,840 Speaker 1: if they had thoughts about it. Thanks very much to 259 00:14:34,880 --> 00:14:38,840 Speaker 1: everybody who participates in this audience feedback segment of the podcast. 260 00:14:38,880 --> 00:14:41,360 Speaker 1: We really love hearing your voice and hearing your thoughts 261 00:14:41,360 --> 00:14:43,640 Speaker 1: on the question of the day. If you would like 262 00:14:43,680 --> 00:14:45,960 Speaker 1: to participate, please don't be shy. Just write to me 263 00:14:46,280 --> 00:14:50,360 Speaker 1: to Questions at Danielandjorge dot com and I'll hook you up. 264 00:14:50,920 --> 00:14:53,840 Speaker 1: So before you hear these answers, think to yourself, have 265 00:14:53,920 --> 00:14:57,760 Speaker 1: you heard of quantum relativity? What do you think that 266 00:14:57,880 --> 00:15:00,600 Speaker 1: might mean. Here's what some listeners have to say. 267 00:15:00,880 --> 00:15:02,040 Speaker 2: Quantum relativity. 268 00:15:02,800 --> 00:15:06,680 Speaker 4: I'm guessing that is the theory that brings quantum mechanics 269 00:15:06,680 --> 00:15:12,560 Speaker 4: and general relativity together. So something that the theory that 270 00:15:13,880 --> 00:15:17,560 Speaker 4: figures out how you work gravity and quantum mechanics together. 271 00:15:17,680 --> 00:15:20,640 Speaker 4: Since gravity, we're not quite sure how that works on 272 00:15:20,680 --> 00:15:22,280 Speaker 4: the smallest scales. 273 00:15:22,720 --> 00:15:25,160 Speaker 1: That is really really tiny relativity. 274 00:15:25,800 --> 00:15:29,520 Speaker 5: To me, that sounds like a parallel to general relativity. 275 00:15:29,840 --> 00:15:32,520 Speaker 5: So I bet that it has to do with how 276 00:15:32,600 --> 00:15:36,040 Speaker 5: particles interact with each other when in proximity to each 277 00:15:36,040 --> 00:15:37,720 Speaker 5: other on a quantum scale. 278 00:15:37,920 --> 00:15:42,240 Speaker 3: I love the answer really tiny relativity because it makes 279 00:15:42,280 --> 00:15:46,000 Speaker 3: me think of some ants or some mites or tartar 280 00:15:46,040 --> 00:15:49,560 Speaker 3: grades in the lab coats drawing on tiny chalkboards. 281 00:15:51,640 --> 00:15:55,480 Speaker 1: Exactly. Also, quantum just sometimes means like fancy or stinazzi, 282 00:15:55,680 --> 00:15:57,880 Speaker 1: or we're going to charge an extra ten bucks for it, 283 00:15:57,960 --> 00:16:00,560 Speaker 1: So like expensive relativity. 284 00:16:00,240 --> 00:16:05,560 Speaker 3: This is a quantum salad for twelve dollars, exactly. 285 00:16:06,400 --> 00:16:09,000 Speaker 1: I'd like to upgrade my salad, actually do a quantum salad. 286 00:16:09,720 --> 00:16:11,760 Speaker 1: Or I ordered quantum on my salad and I didn't 287 00:16:11,800 --> 00:16:12,240 Speaker 1: get enough. 288 00:16:13,720 --> 00:16:14,800 Speaker 2: Could mean anything thanks in. 289 00:16:14,800 --> 00:16:19,040 Speaker 1: A complaint anything. Well, we're going to see today. The 290 00:16:19,160 --> 00:16:22,040 Speaker 1: quantum relativity is the name of a new effort to 291 00:16:22,280 --> 00:16:25,520 Speaker 1: unify quantum mechanics and general relativity, and they really do 292 00:16:25,600 --> 00:16:28,840 Speaker 1: give it that name for a reason. But before that's 293 00:16:28,880 --> 00:16:30,400 Speaker 1: going to make any sense to us, we really have 294 00:16:30,440 --> 00:16:33,120 Speaker 1: to understand the basics of like what is quantum mechanics 295 00:16:33,120 --> 00:16:35,480 Speaker 1: in general relativity, why do we want to unify them, 296 00:16:35,840 --> 00:16:37,520 Speaker 1: and why is it so hard? 297 00:16:38,080 --> 00:16:38,400 Speaker 2: Right? 298 00:16:38,640 --> 00:16:42,680 Speaker 3: Yes, because, like you were kind of saying earlier, general 299 00:16:42,680 --> 00:16:44,520 Speaker 3: relativity is for big stuff. 300 00:16:44,600 --> 00:16:46,800 Speaker 2: Quantum mechanics is for tiny stuff. 301 00:16:47,080 --> 00:16:49,480 Speaker 3: But it's got to be a little more detailed than 302 00:16:49,480 --> 00:16:51,600 Speaker 3: that I would imagine. 303 00:16:52,040 --> 00:16:55,120 Speaker 1: No, that's basically it take quantu mechanics, generativity. It's like 304 00:16:55,160 --> 00:16:58,080 Speaker 1: all done in fifteen minutes. But listeners of the podcast 305 00:16:58,120 --> 00:17:02,120 Speaker 1: will remember that general relativity based describes space and time. 306 00:17:02,280 --> 00:17:05,600 Speaker 1: Special relativity is a theory that tells us about how 307 00:17:05,680 --> 00:17:08,760 Speaker 1: light moves and how observers always see light moving at 308 00:17:08,760 --> 00:17:12,560 Speaker 1: the same speed, and general relativity is what explains gravity. 309 00:17:13,000 --> 00:17:15,560 Speaker 1: Remember Newton had the idea that gravity was a force 310 00:17:15,840 --> 00:17:18,760 Speaker 1: that things with mass pulled on each other and that's 311 00:17:18,760 --> 00:17:21,000 Speaker 1: why the Earth goes around the Sun and you feel 312 00:17:21,040 --> 00:17:24,120 Speaker 1: like you're falling towards the Earth because he described gravity 313 00:17:24,160 --> 00:17:27,320 Speaker 1: as this force. But Einstein tells us that gravity is 314 00:17:27,400 --> 00:17:30,920 Speaker 1: not a force. A gravity is not capable of accelerating anything, 315 00:17:31,280 --> 00:17:34,280 Speaker 1: and that things are actually moving according to the invisible 316 00:17:34,440 --> 00:17:36,359 Speaker 1: curvature of space and time. 317 00:17:36,720 --> 00:17:38,919 Speaker 3: This is the thing that is so hard for me 318 00:17:39,560 --> 00:17:43,600 Speaker 3: to really visualize or hold in my head because every 319 00:17:43,720 --> 00:17:48,600 Speaker 3: kind of analogy I try to make is based in physics, 320 00:17:48,680 --> 00:17:52,399 Speaker 3: like a ball rolling down a hill or something, or 321 00:17:53,160 --> 00:17:56,200 Speaker 3: you know, I think of the fabric of space being 322 00:17:56,240 --> 00:17:58,600 Speaker 3: sort of pulled in a certain direction, and it's like 323 00:17:58,680 --> 00:18:00,719 Speaker 3: that's still physics. In the sun and so of like 324 00:18:01,320 --> 00:18:05,080 Speaker 3: you know, a fabric being pulled and something falling into it. 325 00:18:05,440 --> 00:18:09,280 Speaker 3: Whereas like the idea of gravity being sort of the 326 00:18:09,440 --> 00:18:13,800 Speaker 3: shape of the universe in a way that like makes 327 00:18:13,800 --> 00:18:16,560 Speaker 3: sense in my head is very hard to grasp. I 328 00:18:16,640 --> 00:18:19,399 Speaker 3: understand it in a certain way, but to visualize it 329 00:18:19,440 --> 00:18:20,480 Speaker 3: is so difficult. 330 00:18:20,640 --> 00:18:23,960 Speaker 1: It is very tricky because it changes your entire concept 331 00:18:24,000 --> 00:18:25,280 Speaker 1: of what space is. 332 00:18:25,960 --> 00:18:26,080 Speaker 3: Right. 333 00:18:26,119 --> 00:18:28,479 Speaker 1: We used to thinking of space as like nothingness and 334 00:18:28,640 --> 00:18:31,679 Speaker 1: stuff is there and it can move through space. But 335 00:18:31,720 --> 00:18:34,800 Speaker 1: it turns out that there is something to space, like 336 00:18:34,880 --> 00:18:39,040 Speaker 1: between two points, there's information information about how that space 337 00:18:39,160 --> 00:18:42,520 Speaker 1: is curved or bent, and that affects how stuff moves 338 00:18:42,600 --> 00:18:45,160 Speaker 1: through that space. And yeah, there's a lot of examples 339 00:18:45,160 --> 00:18:47,600 Speaker 1: out there in popular science literature. I think most of 340 00:18:47,600 --> 00:18:50,080 Speaker 1: which are very confusing. You know, the idea of like 341 00:18:50,119 --> 00:18:52,800 Speaker 1: a rubber sheet and you have a ball on the sheet, 342 00:18:53,080 --> 00:18:55,600 Speaker 1: and the rubber sheet is bent and that makes things curved. 343 00:18:55,680 --> 00:18:57,920 Speaker 1: That's very confusing because you still have to have gravity 344 00:18:57,920 --> 00:19:00,359 Speaker 1: in that example in the vertical direction. You have this 345 00:19:00,440 --> 00:19:03,480 Speaker 1: like external third dimension of gravity in your two D world. 346 00:19:03,520 --> 00:19:06,040 Speaker 1: I think that's very very misleading. I prefer to think 347 00:19:06,040 --> 00:19:08,639 Speaker 1: about it in three D. And remember that this curvature 348 00:19:08,720 --> 00:19:12,440 Speaker 1: is intrinsic. It's not external. It's not like there's somebody 349 00:19:12,520 --> 00:19:15,800 Speaker 1: else out there with a ruler in real space who's 350 00:19:15,800 --> 00:19:18,520 Speaker 1: telling us our space is bent relative to their space. 351 00:19:18,680 --> 00:19:21,720 Speaker 1: The curvature is intrinsic. There's no external ruler. It just 352 00:19:21,800 --> 00:19:25,720 Speaker 1: means that the relative distances between two points change, which 353 00:19:25,760 --> 00:19:28,920 Speaker 1: means like the shortest path from A to B might 354 00:19:28,960 --> 00:19:32,000 Speaker 1: not be a straight line that you would draw if 355 00:19:32,040 --> 00:19:34,760 Speaker 1: you ignore the curvature. Once you know what the curvature is, 356 00:19:34,800 --> 00:19:37,240 Speaker 1: there might be a shorter path between A and B, 357 00:19:37,600 --> 00:19:39,760 Speaker 1: and that's the path that light will take. Light always 358 00:19:39,800 --> 00:19:42,480 Speaker 1: takes the shortest path between two points. 359 00:19:42,960 --> 00:19:46,679 Speaker 3: So if I'm standing on my bed and I'm going 360 00:19:46,760 --> 00:19:48,679 Speaker 3: to jump off the bed, as I do every morning, 361 00:19:48,920 --> 00:19:53,199 Speaker 3: so I am subject to the gravity of Earth, and 362 00:19:53,280 --> 00:19:56,720 Speaker 3: it's not so much that it's pulling me down, but 363 00:19:56,960 --> 00:20:00,600 Speaker 3: just that I am traveling along the short this path 364 00:20:00,640 --> 00:20:03,720 Speaker 3: from point A, which is my bed, to point B, 365 00:20:04,000 --> 00:20:07,439 Speaker 3: which is the other point of space. But it's more 366 00:20:07,520 --> 00:20:09,399 Speaker 3: or less just interrupted by the floor. 367 00:20:09,800 --> 00:20:12,800 Speaker 1: Yeah, that's a great example. Let's think about it first 368 00:20:12,800 --> 00:20:15,600 Speaker 1: from the Newtonian point of view, and then let's reboot 369 00:20:15,600 --> 00:20:17,560 Speaker 1: and think about it from an Einsteinian point of view. 370 00:20:17,920 --> 00:20:20,720 Speaker 1: So Newton would say, you're standing on your bed. There's 371 00:20:20,760 --> 00:20:23,159 Speaker 1: the force of gravity pulling down on you from the Earth, 372 00:20:23,440 --> 00:20:25,560 Speaker 1: and there's the force of your bed pushing up, and 373 00:20:25,600 --> 00:20:27,880 Speaker 1: those two things are balanced, so you're not going anywhere. 374 00:20:27,960 --> 00:20:30,280 Speaker 1: Then you jump off your bed. No longer is the 375 00:20:30,320 --> 00:20:32,640 Speaker 1: bed pushing you up, and so now you're falling because 376 00:20:32,640 --> 00:20:35,040 Speaker 1: it's just the force of gravity, and that's accelerating you 377 00:20:35,080 --> 00:20:36,760 Speaker 1: down towards the center of the Earth. That's the way 378 00:20:36,760 --> 00:20:39,439 Speaker 1: people mostly learn about gravity. That's how Newton described it. 379 00:20:39,480 --> 00:20:43,800 Speaker 1: That's where we start. Einstein says something different. Einstein says, well, 380 00:20:43,800 --> 00:20:47,040 Speaker 1: when you're standing on your bed, you actually are being accelerated. 381 00:20:47,040 --> 00:20:49,879 Speaker 1: There's only one force there. There's the force of your bed. 382 00:20:50,160 --> 00:20:52,640 Speaker 1: What's it pushing you against. It's pushing you against your 383 00:20:52,720 --> 00:20:56,280 Speaker 1: natural motion, which is to fall towards the center of 384 00:20:56,320 --> 00:20:59,399 Speaker 1: the earth. So Newton says, you're accelerating when after you 385 00:20:59,480 --> 00:21:01,720 Speaker 1: jump off the bed and you're falling towards the center. 386 00:21:01,920 --> 00:21:04,440 Speaker 1: Einstein says, no, you were accelerating when you were on 387 00:21:04,480 --> 00:21:07,159 Speaker 1: your bed. It's when you jump off your bed that 388 00:21:07,240 --> 00:21:11,080 Speaker 1: you're now following the natural curvature of space. You're no 389 00:21:11,160 --> 00:21:14,719 Speaker 1: longer accelerating. The only force in this scenario is the 390 00:21:14,760 --> 00:21:17,959 Speaker 1: force of the bed on you, and that's keeping you 391 00:21:18,000 --> 00:21:20,560 Speaker 1: from naturally moving towards the center of the Earth. When 392 00:21:20,600 --> 00:21:23,360 Speaker 1: you're standing on the bed. Once you jump off, you're 393 00:21:23,440 --> 00:21:25,800 Speaker 1: the one in free fall. And you can actually measure 394 00:21:25,840 --> 00:21:28,960 Speaker 1: this because you can take an accelerometer, something which measures 395 00:21:28,960 --> 00:21:32,440 Speaker 1: your acceleration. I mean, the scale is basically a gravitometer, 396 00:21:33,000 --> 00:21:35,840 Speaker 1: and you can measure when are you feeling an acceleration. 397 00:21:36,000 --> 00:21:37,840 Speaker 1: If you jump off your bed and you're holding a scale, 398 00:21:37,920 --> 00:21:39,600 Speaker 1: you put it under your feet, what are you going 399 00:21:39,640 --> 00:21:41,639 Speaker 1: to weigh? You're going to weigh nothing because there's no 400 00:21:41,720 --> 00:21:44,479 Speaker 1: force between you and the scale. But if the scale's 401 00:21:44,480 --> 00:21:46,280 Speaker 1: on your bed and you're standing on it, then you're 402 00:21:46,320 --> 00:21:48,440 Speaker 1: going to see your weight. And that's because that's where 403 00:21:48,440 --> 00:21:50,720 Speaker 1: you're accelerating. It's when you're on your bed. 404 00:21:50,920 --> 00:21:54,439 Speaker 3: That's so interesting. Yeah, I can totally visualize that. Also, 405 00:21:54,720 --> 00:21:57,360 Speaker 3: I knew that when I sleep in, I wasn't lazy 406 00:21:57,840 --> 00:21:59,720 Speaker 3: because I've been accelerating the whole time. 407 00:22:02,520 --> 00:22:05,960 Speaker 1: So this is Einstein's picture of gravity, and it's massively successful. 408 00:22:06,040 --> 00:22:06,200 Speaker 3: Right. 409 00:22:06,240 --> 00:22:08,760 Speaker 1: It describes the motion of everything in the universe, the 410 00:22:08,840 --> 00:22:13,560 Speaker 1: expansion of the universe, incredibly high precision black holes oscillating 411 00:22:13,600 --> 00:22:16,440 Speaker 1: around each other, neutron stars getting gobbled by black holes, 412 00:22:16,520 --> 00:22:19,800 Speaker 1: gravitational waves. It's been tested in and out and up 413 00:22:19,880 --> 00:22:23,680 Speaker 1: the wazoo for decades and decades, and it's this beautiful 414 00:22:23,720 --> 00:22:26,840 Speaker 1: geometric picture of the universe that tells us gravity is 415 00:22:26,880 --> 00:22:29,200 Speaker 1: not a force. It's just the way things are flowing 416 00:22:29,240 --> 00:22:32,320 Speaker 1: through the geometry of space and time. And the things 417 00:22:32,320 --> 00:22:34,480 Speaker 1: to take away from this discussion are that it's one 418 00:22:34,880 --> 00:22:37,680 Speaker 1: deterministic right. It says that things move in a certain 419 00:22:37,680 --> 00:22:41,320 Speaker 1: way because of geometry. It's no randomness, there's no probability. 420 00:22:41,480 --> 00:22:43,080 Speaker 1: It's not like when you jump off your bed you 421 00:22:43,080 --> 00:22:45,800 Speaker 1: have a chance of landing here or there. It's determined 422 00:22:45,960 --> 00:22:48,480 Speaker 1: by exactly where you are in the shape of space. 423 00:22:48,640 --> 00:22:51,240 Speaker 1: And the other is that it mostly affects really really 424 00:22:51,280 --> 00:22:54,399 Speaker 1: big stuff because gravity is super weak. Whether it's a 425 00:22:54,440 --> 00:22:57,200 Speaker 1: force or it's the curvature of space time, it takes 426 00:22:57,280 --> 00:23:00,399 Speaker 1: a lot of mass to have any effect. You can 427 00:23:00,640 --> 00:23:03,760 Speaker 1: overcome all the gravity of the Earth or the curvature 428 00:23:03,760 --> 00:23:05,919 Speaker 1: of space and time caused by the Earth using a 429 00:23:05,960 --> 00:23:09,200 Speaker 1: simple kitchen magnet right, or your legs can overcome it. 430 00:23:09,400 --> 00:23:11,560 Speaker 1: You can leap off the surface of the Earth, which 431 00:23:11,600 --> 00:23:15,080 Speaker 1: means it applies mostly to really massive objects. So it's 432 00:23:15,080 --> 00:23:19,040 Speaker 1: deterministic and it applies to really massive stuff. That's the 433 00:23:19,080 --> 00:23:21,160 Speaker 1: important things to remember when we're going to talk about 434 00:23:21,200 --> 00:23:23,520 Speaker 1: trying to integrate it with quantum mechanics. 435 00:23:23,080 --> 00:23:27,320 Speaker 3: Because that's in the opposite direction where it is extremely 436 00:23:27,560 --> 00:23:32,919 Speaker 3: extremely tiny stuff like as a human being, gravity is 437 00:23:33,040 --> 00:23:37,719 Speaker 3: something where it's hard to you know, really visualize like 438 00:23:37,800 --> 00:23:40,840 Speaker 3: the scope of say like the size of the Sun 439 00:23:41,000 --> 00:23:43,320 Speaker 3: or this even the size of the planet. Sure you 440 00:23:43,359 --> 00:23:46,080 Speaker 3: can go on a plane and kind of see part 441 00:23:46,119 --> 00:23:49,200 Speaker 3: of it, but it's it's still hard to visualize how 442 00:23:49,440 --> 00:23:52,679 Speaker 3: big these things are, how massive it is, and then similarly, 443 00:23:53,320 --> 00:23:57,479 Speaker 3: going into quantum mechanics visualizing how tiny these things can be. 444 00:23:57,840 --> 00:24:00,480 Speaker 3: So there really as opposite as you can can get 445 00:24:00,600 --> 00:24:03,000 Speaker 3: in terms of size and scope. 446 00:24:03,520 --> 00:24:06,480 Speaker 1: They are like the ying and ying of physics. But 447 00:24:06,560 --> 00:24:10,600 Speaker 1: we hope they click together to make a holistic picture. 448 00:24:11,240 --> 00:24:14,400 Speaker 1: But let's dig into how quant mechanics explains the tiniest 449 00:24:14,400 --> 00:24:17,439 Speaker 1: stuff in the universe. But first let's take a quick break. 450 00:24:17,520 --> 00:24:20,040 Speaker 3: All right, I'm going to try to start thinking small 451 00:24:32,960 --> 00:24:37,240 Speaker 3: all right, I'm trying to think inside a very tiny box, 452 00:24:38,040 --> 00:24:39,760 Speaker 3: and hopefully that will help me. 453 00:24:41,920 --> 00:24:44,680 Speaker 1: As you mentioned already, the rules seem to be different 454 00:24:44,760 --> 00:24:49,160 Speaker 1: for things like baseball and planets than things like electrons 455 00:24:49,200 --> 00:24:52,679 Speaker 1: and photons and tiny little particles, which is really the 456 00:24:52,800 --> 00:24:56,159 Speaker 1: source of one of the biggest mysteries in modern physics, 457 00:24:56,200 --> 00:24:58,359 Speaker 1: how that all works and whether we can bring it. 458 00:24:58,240 --> 00:25:03,240 Speaker 3: Together right, Because I think I had some concept before 459 00:25:04,119 --> 00:25:07,040 Speaker 3: ever coming on this show, which is that like with 460 00:25:07,119 --> 00:25:11,560 Speaker 3: the small stuff, the really tiny quantum level stuff, there 461 00:25:11,720 --> 00:25:12,760 Speaker 3: was some sort. 462 00:25:12,560 --> 00:25:14,840 Speaker 2: Of like average you could take. 463 00:25:14,800 --> 00:25:18,920 Speaker 3: Of its behavior, and then that would be well integrated into, say, 464 00:25:19,400 --> 00:25:23,840 Speaker 3: other types of physics like general relativity, where it's like, well, 465 00:25:23,880 --> 00:25:26,560 Speaker 3: you know, you just scale up averages of the small 466 00:25:26,600 --> 00:25:29,840 Speaker 3: stuff's activity and then that would fit in some perfect 467 00:25:29,840 --> 00:25:33,680 Speaker 3: formula and represent general relativity. 468 00:25:33,720 --> 00:25:35,919 Speaker 2: But turns out it's not so simple. 469 00:25:37,040 --> 00:25:37,119 Speaker 5: No. 470 00:25:37,280 --> 00:25:39,760 Speaker 1: It turns out the rules of these two concepts are 471 00:25:39,840 --> 00:25:43,240 Speaker 1: fundamentally different and tell really different stories about the nature 472 00:25:43,320 --> 00:25:46,240 Speaker 1: of the universe we live in. About one hundred years ago, 473 00:25:46,280 --> 00:25:49,040 Speaker 1: people did experiments which showed us that when you zoom 474 00:25:49,080 --> 00:25:51,760 Speaker 1: into the tiniest level, the rules really do seem to 475 00:25:51,800 --> 00:25:54,640 Speaker 1: be different. Amazingly, it was Einstein who played a role 476 00:25:54,720 --> 00:25:57,560 Speaker 1: in both of these revolutions. He of course came up 477 00:25:57,640 --> 00:26:00,159 Speaker 1: with relativity, but he also had the idea of how 478 00:26:00,200 --> 00:26:03,280 Speaker 1: to interpret the photoelectric effect, which kicked off the entire 479 00:26:03,359 --> 00:26:07,159 Speaker 1: quantum revolution as well, So that dude was pretty central. 480 00:26:07,400 --> 00:26:09,879 Speaker 2: What's the photo reflective effect? 481 00:26:10,040 --> 00:26:12,560 Speaker 1: This is the experiment where you shine bright light at 482 00:26:12,560 --> 00:26:14,439 Speaker 1: a piece of metal and you see a bunch of 483 00:26:14,480 --> 00:26:17,720 Speaker 1: electrons boil off. And the idea is, Okay, the electrons 484 00:26:17,760 --> 00:26:20,359 Speaker 1: are absorbing the light, they're getting energy, they're boiling off. 485 00:26:20,480 --> 00:26:23,040 Speaker 1: The weird thing about the experiment was as you turn 486 00:26:23,280 --> 00:26:26,119 Speaker 1: up the brightness of the light, like the intensity of 487 00:26:26,200 --> 00:26:29,000 Speaker 1: the light, you expected to get electrons with more energy 488 00:26:29,040 --> 00:26:31,720 Speaker 1: because you're shining brighter light at it. But instead what 489 00:26:31,800 --> 00:26:35,000 Speaker 1: you got were more electrons. And this really puzzled people. 490 00:26:35,320 --> 00:26:38,160 Speaker 1: They're like, why can't the electrons get more energy? And 491 00:26:38,240 --> 00:26:40,720 Speaker 1: the answer in the end is that light is made 492 00:26:40,760 --> 00:26:43,359 Speaker 1: of these tiny little packets. It's not a continuous beam. 493 00:26:43,680 --> 00:26:46,160 Speaker 1: It's a bunch of little packets of energy, and each 494 00:26:46,200 --> 00:26:49,720 Speaker 1: electron can basically only absorb one. It's like one interaction 495 00:26:49,840 --> 00:26:52,680 Speaker 1: between a photon and n electron. So when you turn 496 00:26:52,760 --> 00:26:55,040 Speaker 1: up the brightness of the beam, which you get are 497 00:26:55,080 --> 00:26:59,520 Speaker 1: more electrons absorbing photons, not one electron absorbing more photons. 498 00:27:00,160 --> 00:27:02,399 Speaker 1: And so that was the clue that told people, oh, look, 499 00:27:02,600 --> 00:27:05,359 Speaker 1: maybe light is made of these little packets, and that 500 00:27:05,440 --> 00:27:08,119 Speaker 1: kicked off the whole quantum revolution that showed us that 501 00:27:08,160 --> 00:27:10,480 Speaker 1: everything out there is actually made of these little discrete 502 00:27:10,520 --> 00:27:12,440 Speaker 1: bits that follow very different rules. 503 00:27:12,800 --> 00:27:15,760 Speaker 3: It's like these electrons are flying ryanair and they can 504 00:27:15,800 --> 00:27:18,160 Speaker 3: only have one packet per electron. 505 00:27:19,880 --> 00:27:23,280 Speaker 1: That's right. Otherwise you get some quantum fees carry ons. 506 00:27:23,720 --> 00:27:27,879 Speaker 3: Is that a very small fee or a very big fee? 507 00:27:27,880 --> 00:27:30,919 Speaker 1: Small fees that add up to a lot because of 508 00:27:31,160 --> 00:27:32,520 Speaker 1: interference with your pocketbook? 509 00:27:32,560 --> 00:27:33,760 Speaker 2: I think? Ain't that how it is? 510 00:27:34,040 --> 00:27:36,000 Speaker 1: Anybody out there who works for the airlines, do not 511 00:27:36,119 --> 00:27:38,680 Speaker 1: take this as a creative idea for how to add fees. Okay, 512 00:27:38,760 --> 00:27:41,040 Speaker 1: I don't want to see quantum fees on my quantum fees. 513 00:27:41,119 --> 00:27:42,520 Speaker 2: That's going to be the next thing. 514 00:27:44,040 --> 00:27:46,280 Speaker 1: And what emerged from the next twenty or thirty years 515 00:27:46,280 --> 00:27:50,240 Speaker 1: of studying experiments and shining lights on things and looking 516 00:27:50,240 --> 00:27:53,040 Speaker 1: inside the atom, or a new set of rules for 517 00:27:53,240 --> 00:27:56,439 Speaker 1: how tiny stuff worked. This tiny stuff didn't follow the 518 00:27:56,520 --> 00:27:59,679 Speaker 1: rules of planets and baseballs. You couldn't make a picture 519 00:27:59,680 --> 00:28:03,200 Speaker 1: of the atom that literally had electrons orbiting the center 520 00:28:03,200 --> 00:28:05,439 Speaker 1: of the atom. That just didn't work. The physics of 521 00:28:05,480 --> 00:28:08,560 Speaker 1: it didn't make sense. Those electrons in an orbit would 522 00:28:08,680 --> 00:28:11,600 Speaker 1: radiate away all their energy and collapse into the nucleus 523 00:28:11,640 --> 00:28:14,320 Speaker 1: because anything that's moving in a circle is accelerating, and 524 00:28:14,359 --> 00:28:17,440 Speaker 1: things that accelerate have to give off radiation in order 525 00:28:17,480 --> 00:28:20,880 Speaker 1: to keep bending. But we don't see electrons collapsing into 526 00:28:20,880 --> 00:28:22,639 Speaker 1: the center of the atom and tend to the negative 527 00:28:22,680 --> 00:28:26,240 Speaker 1: thirteen seconds. I told us that the rules were fundamentally different, 528 00:28:26,240 --> 00:28:29,080 Speaker 1: and we came up with a completely new kind of mathematics, 529 00:28:29,160 --> 00:28:33,040 Speaker 1: quantum mechanics, Schrodinger's equation that described the rules of the 530 00:28:33,119 --> 00:28:36,399 Speaker 1: quantum realm, which were totally different from the rules of 531 00:28:36,480 --> 00:28:40,600 Speaker 1: baseballs and electrons. Base Balls move through space. They have 532 00:28:40,640 --> 00:28:43,440 Speaker 1: a path, like they're here and then they are there, 533 00:28:43,720 --> 00:28:46,280 Speaker 1: and so you know they went from here to there. 534 00:28:46,360 --> 00:28:48,360 Speaker 1: They have a location at every moment, and you can 535 00:28:48,400 --> 00:28:52,000 Speaker 1: string those locations together to make a smooth and continuous path. 536 00:28:52,240 --> 00:28:53,800 Speaker 1: Just sort of makes sense to you that everything has 537 00:28:53,840 --> 00:28:57,040 Speaker 1: to be somewhere at all times. But electrons don't follow 538 00:28:57,080 --> 00:28:59,920 Speaker 1: those rules. That's an intuition you developed from your experi 539 00:29:00,440 --> 00:29:03,920 Speaker 1: of baseballs and rocks and other kinds of stuff. Electrons 540 00:29:03,960 --> 00:29:05,960 Speaker 1: can be here and then they can be there, and 541 00:29:06,000 --> 00:29:09,400 Speaker 1: they don't have to go from here to there. They 542 00:29:09,400 --> 00:29:12,760 Speaker 1: don't always have to have a determined location. They can 543 00:29:12,800 --> 00:29:15,640 Speaker 1: exist in probabilistic form where they can say, well, I 544 00:29:15,720 --> 00:29:18,040 Speaker 1: might be here and I might be there. It's not 545 00:29:18,240 --> 00:29:21,960 Speaker 1: determined much more than just being not known. It's actually 546 00:29:22,080 --> 00:29:24,440 Speaker 1: not determined by the universe. 547 00:29:24,240 --> 00:29:28,160 Speaker 3: Right, Because it's hard to understand this sometimes where you 548 00:29:28,200 --> 00:29:31,800 Speaker 3: think in these kinds of thought experiments of like an 549 00:29:31,840 --> 00:29:36,000 Speaker 3: electron not knowing sort of the location of electron or 550 00:29:36,560 --> 00:29:39,680 Speaker 3: the spin of something. It's like I think sometimes I 551 00:29:39,760 --> 00:29:42,080 Speaker 3: have this concept of like, well, this is just sort 552 00:29:42,080 --> 00:29:45,680 Speaker 3: of some kind of weird math. It's not actually describing 553 00:29:45,720 --> 00:29:50,400 Speaker 3: what's actually happening. But I would assume there's like evidence 554 00:29:50,480 --> 00:29:53,520 Speaker 3: that is what's actually happening, that this is not these 555 00:29:53,560 --> 00:29:56,960 Speaker 3: positions are not have experimentally been shown to not be 556 00:29:57,120 --> 00:29:59,240 Speaker 3: like determined by the universe. 557 00:29:59,360 --> 00:30:02,400 Speaker 1: Yeah, there's a whole really fascinating set of experiments that 558 00:30:02,520 --> 00:30:05,560 Speaker 1: explore this question, like is it just something we don't 559 00:30:05,600 --> 00:30:09,000 Speaker 1: know or is it really undetermined by the universe. Is 560 00:30:09,000 --> 00:30:12,560 Speaker 1: there some like extra information the electron is carrying that 561 00:30:12,600 --> 00:30:15,080 Speaker 1: we're just not aware of that actually tells where the 562 00:30:15,120 --> 00:30:17,520 Speaker 1: universe is, like keeping track of where it really is, 563 00:30:18,000 --> 00:30:20,120 Speaker 1: and we just don't know. And it's a set of 564 00:30:20,160 --> 00:30:23,360 Speaker 1: experiments proposed by John Bell to probe a theory called 565 00:30:23,400 --> 00:30:26,400 Speaker 1: Bell's inequalities, and we have a whole set of podcasts 566 00:30:26,440 --> 00:30:29,280 Speaker 1: about those Whether quantum mechanics really is random or not. 567 00:30:29,960 --> 00:30:32,240 Speaker 1: And the upshot is that it seems like it really 568 00:30:32,320 --> 00:30:35,080 Speaker 1: is random. There are some loopholes there, how you might 569 00:30:35,120 --> 00:30:37,520 Speaker 1: have like some sort of like non local pilot wave 570 00:30:37,560 --> 00:30:41,360 Speaker 1: that's controlling the whole universe. But the most mainstream interpretation 571 00:30:41,480 --> 00:30:44,200 Speaker 1: is that it really is random. There really is some 572 00:30:44,560 --> 00:30:48,000 Speaker 1: non determinism to the universe that you could do the 573 00:30:48,040 --> 00:30:52,240 Speaker 1: same experiment twice, exactly the same setup and get different answers. 574 00:30:52,560 --> 00:30:55,200 Speaker 1: Like you're shoot an electron into an experiment with exactly 575 00:30:55,280 --> 00:30:58,240 Speaker 1: the same conditions twice and it'll end up going left 576 00:30:58,320 --> 00:31:00,600 Speaker 1: once and it'll end up going right on another time. 577 00:31:00,760 --> 00:31:03,200 Speaker 1: There's like a die being thrown by the universe to 578 00:31:03,240 --> 00:31:06,800 Speaker 1: determine where an electron goes. It's crazy, it's bonkers, but 579 00:31:06,920 --> 00:31:08,239 Speaker 1: that's the universe we live in. 580 00:31:08,520 --> 00:31:11,120 Speaker 3: So it'd be like if you like, you know, there's 581 00:31:11,160 --> 00:31:14,320 Speaker 3: the classic thing that even babies. This is so interesting 582 00:31:14,360 --> 00:31:18,400 Speaker 3: about human cognition is that babies have a sort of 583 00:31:18,480 --> 00:31:22,080 Speaker 3: baseline understanding of physics. It seems like if they see 584 00:31:22,240 --> 00:31:25,440 Speaker 3: a little marble hit a big marble, they don't expect 585 00:31:25,440 --> 00:31:27,280 Speaker 3: the big marble to go flying off. 586 00:31:27,480 --> 00:31:28,800 Speaker 2: And if you show them that, they. 587 00:31:28,800 --> 00:31:31,400 Speaker 3: Look they kind of stare at it because it's surprising 588 00:31:31,440 --> 00:31:34,000 Speaker 3: to them. But you know, because we kind of have 589 00:31:34,120 --> 00:31:37,040 Speaker 3: this this innate understanding that if a little thing hits 590 00:31:37,040 --> 00:31:38,720 Speaker 3: a big thing, the big thing isn't going to go 591 00:31:38,760 --> 00:31:41,600 Speaker 3: shooting off, whereas if the big thing hits the little thing, 592 00:31:41,600 --> 00:31:44,320 Speaker 3: it's going to go shooting off. And like, if we 593 00:31:44,400 --> 00:31:47,440 Speaker 3: hit things at a certain angle, it's gonna, you know, 594 00:31:47,840 --> 00:31:51,120 Speaker 3: go at a certain direction, just like I guess that's 595 00:31:51,120 --> 00:31:53,880 Speaker 3: how people can be good at pool, not me, but 596 00:31:54,000 --> 00:31:58,080 Speaker 3: other people. And so it would be shocking though, if 597 00:31:58,080 --> 00:32:00,640 Speaker 3: you're if you're good at pool and you something at 598 00:32:00,680 --> 00:32:04,960 Speaker 3: a certain angle and it's just completely random about of 599 00:32:05,360 --> 00:32:08,360 Speaker 3: whether it goes left or right, or forward or backwards 600 00:32:08,480 --> 00:32:09,280 Speaker 3: or up or down. 601 00:32:09,880 --> 00:32:11,960 Speaker 1: It is a really weird way to think about the universe. 602 00:32:12,080 --> 00:32:13,920 Speaker 1: I was recently trying to explain this stuff to my 603 00:32:14,000 --> 00:32:16,880 Speaker 1: sixteen year old who's taking chemistry and was learning about 604 00:32:16,920 --> 00:32:20,840 Speaker 1: the atomic structure and all this stuff and photons and probabilities, 605 00:32:21,200 --> 00:32:23,000 Speaker 1: and it was pretty bewildering. But it was a fun 606 00:32:23,040 --> 00:32:25,520 Speaker 1: experience to try to download into his mind this new 607 00:32:25,560 --> 00:32:28,040 Speaker 1: way of thinking about the universe. But it really is 608 00:32:28,120 --> 00:32:31,280 Speaker 1: counterintuitive because you don't ever experience it. And that's one 609 00:32:31,320 --> 00:32:34,040 Speaker 1: of the big mysteries of quantum mechanics, is why not. 610 00:32:34,400 --> 00:32:37,680 Speaker 1: Because when we interact with quantum stuff, it tends to collapse. 611 00:32:38,040 --> 00:32:39,840 Speaker 1: It says, Oh, I have a bunch of possibilities, but 612 00:32:39,880 --> 00:32:42,240 Speaker 1: I'm just going to pick one now. When a photon 613 00:32:42,320 --> 00:32:44,800 Speaker 1: hits your eyeball, it decides, Oh, I'm here or I'm there. 614 00:32:44,960 --> 00:32:47,960 Speaker 1: When a electron hits the screen, the universe decides. For 615 00:32:48,000 --> 00:32:51,080 Speaker 1: some reason, the universe has this distinction between tiny little 616 00:32:51,120 --> 00:32:55,120 Speaker 1: stuff that can exist with uncertainty and bigger stuff which can't. 617 00:32:55,320 --> 00:32:58,040 Speaker 1: People sometimes describe this as acting like a particle or 618 00:32:58,040 --> 00:33:02,280 Speaker 1: acting like a wave. Really is between classical physics like 619 00:33:02,400 --> 00:33:06,320 Speaker 1: general relativity that's talking about stuff having specific locations and 620 00:33:06,400 --> 00:33:08,360 Speaker 1: quantum physics, where stuff can still have. 621 00:33:08,440 --> 00:33:13,080 Speaker 3: Uncertainty, So quantum physics would be the particle, and general 622 00:33:13,080 --> 00:33:15,400 Speaker 3: relativity would be the wave, or vice versa. 623 00:33:15,520 --> 00:33:18,480 Speaker 1: So quantu physics is about tiny little stuff, but it's 624 00:33:18,520 --> 00:33:21,240 Speaker 1: the wave like behavior of that stuff that's really weird 625 00:33:21,480 --> 00:33:24,720 Speaker 1: because the wave appears in the Shortener equation, and people 626 00:33:24,720 --> 00:33:27,440 Speaker 1: tend to think about particles as having like a definite location, 627 00:33:27,560 --> 00:33:30,200 Speaker 1: like you've seen this particle on the screen. So general 628 00:33:30,240 --> 00:33:33,280 Speaker 1: relativity and classical physics more broadly thinks about stuff as 629 00:33:33,280 --> 00:33:36,600 Speaker 1: having definitive locations. It is here, it is there, it 630 00:33:36,800 --> 00:33:40,040 Speaker 1: was here, And quantum mechanics says that there can be uncertainty. 631 00:33:40,280 --> 00:33:43,600 Speaker 1: So quantum is the more wavy stuff, and in this case, 632 00:33:43,640 --> 00:33:47,240 Speaker 1: the classical theory is more like definitive locations, which people 633 00:33:47,280 --> 00:33:49,760 Speaker 1: sometimes describe as acting like a particle. 634 00:33:50,120 --> 00:33:53,320 Speaker 3: So quantum mechanics is kind of whibbly wobbly. 635 00:33:53,600 --> 00:33:57,280 Speaker 1: Yeah, that's exactly right. So these are two very different 636 00:33:57,320 --> 00:34:01,040 Speaker 1: pictures of the world. Right, things moving along classical pass 637 00:34:01,040 --> 00:34:03,720 Speaker 1: where they always have a definitive location at every time, 638 00:34:04,200 --> 00:34:07,640 Speaker 1: or things being wibbly wobbling, being undetermined. And you might think, well, 639 00:34:07,680 --> 00:34:09,960 Speaker 1: it should be pretty easy to figure out which is right, 640 00:34:10,040 --> 00:34:13,480 Speaker 1: can't we do experiments to tell us which one is 641 00:34:13,520 --> 00:34:16,360 Speaker 1: predicting things correctly. Right, Often you have two theories, you 642 00:34:16,480 --> 00:34:18,399 Speaker 1: just do an experiment, you say, well, which one is right, 643 00:34:19,000 --> 00:34:21,400 Speaker 1: And the problem is that it's so hard to do 644 00:34:21,480 --> 00:34:24,759 Speaker 1: an experiment where both of them have something to say. 645 00:34:25,120 --> 00:34:27,680 Speaker 1: Most of the universe is divided up into stuff where 646 00:34:27,760 --> 00:34:31,040 Speaker 1: general relativity is important and quantum mechanics can be ignored, 647 00:34:31,360 --> 00:34:35,280 Speaker 1: like the motion of planets, or stuff where quantum mechanics 648 00:34:35,360 --> 00:34:38,759 Speaker 1: is important and general relativity can be ignored, like two 649 00:34:38,760 --> 00:34:40,480 Speaker 1: electrons bouncing off of each other. 650 00:34:41,080 --> 00:34:45,239 Speaker 3: Right, Like you could do a physics experiment on a baseball, 651 00:34:45,840 --> 00:34:49,240 Speaker 3: But then to do a physics experiment and a quantum 652 00:34:49,360 --> 00:34:52,600 Speaker 3: level experiment on the baseball's electrons at the same time 653 00:34:52,760 --> 00:34:55,920 Speaker 3: in a way that makes sense seems very difficult. 654 00:34:56,040 --> 00:34:58,480 Speaker 1: Exactly when you do an experiment with baseballs, you can 655 00:34:58,520 --> 00:35:00,960 Speaker 1: pretty much ignore the fact that it's made from ten 656 00:35:01,080 --> 00:35:04,239 Speaker 1: to twenty nine tiny buzzing particles, and you can just 657 00:35:04,360 --> 00:35:07,279 Speaker 1: use Newton's laws F equals MA to describe its path 658 00:35:07,440 --> 00:35:10,239 Speaker 1: very very accurately. That's because the quantum effects tend to 659 00:35:10,280 --> 00:35:12,960 Speaker 1: average out for reasons. Again, we don't really know how 660 00:35:13,000 --> 00:35:15,120 Speaker 1: that works or why that works. But it does, so 661 00:35:15,200 --> 00:35:18,560 Speaker 1: quantum effects tend to disappear when you zoom out far enough. 662 00:35:18,680 --> 00:35:21,000 Speaker 1: On the other hand, when you zoom in far enough, 663 00:35:21,320 --> 00:35:24,040 Speaker 1: gravity is so weak that it becomes irrelevant. Like we 664 00:35:24,080 --> 00:35:26,200 Speaker 1: do collisions between protons all the time at the Large 665 00:35:26,239 --> 00:35:30,319 Speaker 1: Hadron Collider, but we always ignore their gravity, Like there 666 00:35:30,520 --> 00:35:34,200 Speaker 1: is a gravitational attraction we think between the protons, but 667 00:35:34,239 --> 00:35:37,600 Speaker 1: protons have such tiny masses that we can essentially ignore 668 00:35:37,680 --> 00:35:40,280 Speaker 1: their gravity when we do those calculations. 669 00:35:40,520 --> 00:35:43,520 Speaker 3: I mean that makes sense because even though technically, even 670 00:35:43,560 --> 00:35:46,520 Speaker 3: as people, we have gravity, it's not like we can 671 00:35:46,600 --> 00:35:50,480 Speaker 3: suck things into ourselves. I know that's not how gravity works, 672 00:35:50,520 --> 00:35:54,080 Speaker 3: but still we're not. We are not generating enough of 673 00:35:54,120 --> 00:35:59,440 Speaker 3: a gravitational effect that things, you know, fall into our bodies. 674 00:35:59,560 --> 00:36:01,640 Speaker 2: And so what chance does a proton have? 675 00:36:02,320 --> 00:36:05,080 Speaker 1: Exactly, you can't blame gravity for the reason you ate 676 00:36:05,080 --> 00:36:07,040 Speaker 1: that pint of ice cream. It didn't just like fall 677 00:36:07,080 --> 00:36:07,920 Speaker 1: into your body. 678 00:36:08,040 --> 00:36:09,000 Speaker 2: That was my alibi. 679 00:36:10,719 --> 00:36:13,520 Speaker 1: But that's exactly right. We could hardly even measure the 680 00:36:13,600 --> 00:36:17,240 Speaker 1: gravity between things that are like a kilogram. The smallest 681 00:36:17,280 --> 00:36:20,640 Speaker 1: thing we've ever measured gravity for is just about a kilogram, 682 00:36:20,640 --> 00:36:24,879 Speaker 1: and protons are a tiny, tiny fraction of that. We're 683 00:36:24,960 --> 00:36:27,440 Speaker 1: like thirty orders of magnitude away from being able to 684 00:36:27,480 --> 00:36:30,480 Speaker 1: measure the gravity of a proton. And more than that, 685 00:36:30,560 --> 00:36:33,160 Speaker 1: we don't even understand what the gravity of a proton 686 00:36:33,239 --> 00:36:35,600 Speaker 1: would look like. You know, say you have a particle 687 00:36:35,719 --> 00:36:38,720 Speaker 1: with uncertainty to it. Maybe it's here, maybe it's there, 688 00:36:38,920 --> 00:36:40,920 Speaker 1: maybe it's in this third location you don't know. The 689 00:36:41,000 --> 00:36:44,359 Speaker 1: universe says, that's cool, the particle can be uncertain, all right, 690 00:36:44,440 --> 00:36:48,280 Speaker 1: But then what is the gravity of an uncertain particle? 691 00:36:48,440 --> 00:36:50,359 Speaker 1: Does it have a little bit of curvature over here 692 00:36:50,400 --> 00:36:51,920 Speaker 1: because it might be over there, and a little bit 693 00:36:51,920 --> 00:36:54,239 Speaker 1: of curvature over there because it might be over there. 694 00:36:54,640 --> 00:36:58,440 Speaker 1: Is the curvature of space itself uncertain? We don't know 695 00:36:58,480 --> 00:37:01,440 Speaker 1: how to unify these two ideas of quantum mechanics and 696 00:37:01,640 --> 00:37:04,800 Speaker 1: of gravity. Nobody really knows how that can be done. 697 00:37:04,960 --> 00:37:10,359 Speaker 3: That's so interesting and uncomfortable from a sort of biology perspective, 698 00:37:10,520 --> 00:37:15,560 Speaker 3: because when you look at biology, big stuff is made 699 00:37:15,560 --> 00:37:19,160 Speaker 3: out of small stuff, and so that tracks. But when 700 00:37:19,160 --> 00:37:23,160 Speaker 3: you look at biological processes, like you look at a cell, 701 00:37:23,840 --> 00:37:27,759 Speaker 3: and it's interesting because, of course, on a certain level, 702 00:37:27,840 --> 00:37:32,640 Speaker 3: each cell's activity does not necessarily explain everything about a 703 00:37:32,719 --> 00:37:36,600 Speaker 3: human being or a cat or a dog their behavior. 704 00:37:36,880 --> 00:37:42,120 Speaker 3: But you can generally track how the small stuff creates 705 00:37:42,200 --> 00:37:45,480 Speaker 3: the big stuff. And there's generally some like the rules 706 00:37:45,520 --> 00:37:49,600 Speaker 3: that govern the small stuff, these biological processes that govern 707 00:37:49,719 --> 00:37:53,080 Speaker 3: the small stuff. You can track how that is impacting 708 00:37:53,200 --> 00:37:56,040 Speaker 3: the big stuff. Like you chug a bunch of soy sauce, 709 00:37:56,160 --> 00:37:59,919 Speaker 3: and those salt ions are you know, messing up your 710 00:38:00,080 --> 00:38:03,640 Speaker 3: or your ion channels in your brain, and then that's 711 00:38:03,680 --> 00:38:07,279 Speaker 3: why you're in a coma. So it's you know, it's 712 00:38:07,520 --> 00:38:11,280 Speaker 3: very uncomfortable, this idea that you couldn't track, like, okay, 713 00:38:11,360 --> 00:38:14,480 Speaker 3: so this proton is acting in a certain way, and 714 00:38:14,560 --> 00:38:18,040 Speaker 3: then we can scale up to you know, an item 715 00:38:18,200 --> 00:38:22,080 Speaker 3: like a watermelon, because it has a bunch of protons 716 00:38:22,080 --> 00:38:22,400 Speaker 3: in it. 717 00:38:23,040 --> 00:38:26,080 Speaker 2: We know how that the behavior. 718 00:38:25,640 --> 00:38:28,680 Speaker 3: Of those protons would somehow affect the behavior of the 719 00:38:28,719 --> 00:38:30,400 Speaker 3: watermelon exactly. 720 00:38:30,440 --> 00:38:32,759 Speaker 1: And we'd love to do an experiment where we could 721 00:38:32,800 --> 00:38:36,200 Speaker 1: study that right, where we could take something where quantum 722 00:38:36,239 --> 00:38:39,960 Speaker 1: mechanics was relevant and also gravity was relevant, Like if 723 00:38:40,000 --> 00:38:43,040 Speaker 1: we could take enough protons and squeeze them together and 724 00:38:43,120 --> 00:38:46,040 Speaker 1: keep them in a small enough space so they're still 725 00:38:46,080 --> 00:38:49,400 Speaker 1: being quantum mechanical, but we had enough protons where we 726 00:38:49,400 --> 00:38:53,040 Speaker 1: could also measure its gravity. That way we could understand, 727 00:38:53,080 --> 00:38:55,640 Speaker 1: like how the small stuff is affecting the big stuff. 728 00:38:55,760 --> 00:38:58,320 Speaker 1: So in order to keep the quantum mechanical effects relevant, 729 00:38:58,440 --> 00:39:01,279 Speaker 1: you've got to keep it like really really small. And 730 00:39:01,360 --> 00:39:03,040 Speaker 1: so what happens when you try to do that, when 731 00:39:03,080 --> 00:39:06,439 Speaker 1: you add enough stuff together so that it stays quantum 732 00:39:06,480 --> 00:39:09,480 Speaker 1: mechanical and gravity starts to get relevant, you get a 733 00:39:09,520 --> 00:39:12,600 Speaker 1: black hole. That's what a black hole is is a 734 00:39:12,680 --> 00:39:16,520 Speaker 1: huge amount of mass in a tiny little space. And so, 735 00:39:16,719 --> 00:39:19,640 Speaker 1: on one hand, that's exciting, Wow, the answer is inside 736 00:39:19,640 --> 00:39:22,640 Speaker 1: a black hole. On the other hand, all that's really frustrating. 737 00:39:22,719 --> 00:39:26,160 Speaker 1: The answer is hidden inside a black hole. We can't 738 00:39:26,200 --> 00:39:28,560 Speaker 1: see it. We think that probably inside a black hole 739 00:39:28,920 --> 00:39:31,600 Speaker 1: is evidence that would point us in the direction of 740 00:39:31,640 --> 00:39:34,240 Speaker 1: how to bring these two theories together, how to explain 741 00:39:34,280 --> 00:39:36,960 Speaker 1: what happens when you have a bunch of quantum stuff 742 00:39:37,040 --> 00:39:39,920 Speaker 1: that has enough gravity that you can't ignore it anymore. 743 00:39:40,400 --> 00:39:42,880 Speaker 3: It feels like a sick joke, right to put all 744 00:39:42,920 --> 00:39:47,000 Speaker 3: the answers inside a thing that we can't see inside, 745 00:39:47,440 --> 00:39:50,640 Speaker 3: and if we tried to get someone in there, it 746 00:39:50,680 --> 00:39:51,879 Speaker 3: would destroy them. 747 00:39:53,320 --> 00:39:56,520 Speaker 1: Exactly, and they might actually survive going inside the black 748 00:39:56,520 --> 00:39:58,680 Speaker 1: hole and seeing the answer, But then they could never 749 00:39:58,800 --> 00:40:02,239 Speaker 1: tell us even come collect their Nobel prize. We'd have 750 00:40:02,280 --> 00:40:05,040 Speaker 1: to send in the Nobel Prize after them, assuming that 751 00:40:05,040 --> 00:40:06,000 Speaker 1: they'd figured it out. 752 00:40:06,280 --> 00:40:08,600 Speaker 3: Like I feel like, if someone dives into a black hole, 753 00:40:08,640 --> 00:40:11,799 Speaker 3: they just deserve a Nobel Prize, whether they discover. 754 00:40:11,560 --> 00:40:12,200 Speaker 2: Anything or not. 755 00:40:13,120 --> 00:40:16,600 Speaker 3: But we can study black holes, we just can't like 756 00:40:16,760 --> 00:40:21,240 Speaker 3: see inside them. So is there any way to study 757 00:40:21,239 --> 00:40:24,720 Speaker 3: a black hole such that it gives us any clues 758 00:40:24,760 --> 00:40:25,319 Speaker 3: about this? 759 00:40:25,760 --> 00:40:29,080 Speaker 1: Well, there is one possible crack in the veneer of 760 00:40:29,080 --> 00:40:32,560 Speaker 1: black holes, which is their hawking radiation. Black holes are 761 00:40:32,600 --> 00:40:36,120 Speaker 1: not totally black. They do emit some radiation. It's even 762 00:40:36,160 --> 00:40:38,759 Speaker 1: talking to the calculation a few decades ago, and he 763 00:40:38,800 --> 00:40:42,279 Speaker 1: didn't have a theory for what is the gravity of particles, 764 00:40:42,320 --> 00:40:45,240 Speaker 1: but he did some sort of like clever handwavey approximations, 765 00:40:45,640 --> 00:40:48,400 Speaker 1: and he showed that if you have a quantum field 766 00:40:48,800 --> 00:40:51,799 Speaker 1: near something with an event horizon, then there has to 767 00:40:51,840 --> 00:40:55,240 Speaker 1: be radiation leaving the event horizon. So now we interpret 768 00:40:55,239 --> 00:40:57,719 Speaker 1: this as like the black hole is evaporating, it's like 769 00:40:57,760 --> 00:40:59,920 Speaker 1: giving up some of its energy. The idea is that 770 00:41:00,160 --> 00:41:03,880 Speaker 1: maybe in that radiation, maybe as particles are being generated 771 00:41:03,920 --> 00:41:06,560 Speaker 1: by the event horizon, there might be clues as to 772 00:41:06,640 --> 00:41:09,920 Speaker 1: what's inside the black hole. It's sort of very speculative, 773 00:41:09,960 --> 00:41:13,799 Speaker 1: cutting edge research, but it's possible that if we did 774 00:41:13,840 --> 00:41:17,400 Speaker 1: see hawking radiation, we could maybe infer from it something 775 00:41:17,440 --> 00:41:20,759 Speaker 1: about what's inside the black hole. But hawking radiation would 776 00:41:20,760 --> 00:41:23,759 Speaker 1: be very very faint, and black holes are very very 777 00:41:23,800 --> 00:41:26,680 Speaker 1: far away and hidden by all sorts of other, very 778 00:41:26,719 --> 00:41:30,120 Speaker 1: noisy stuff like hot gases emitting all sorts of radiation. 779 00:41:30,520 --> 00:41:33,239 Speaker 1: So we've never seen hawking radiation, and frankly, we don't 780 00:41:33,320 --> 00:41:36,719 Speaker 1: seem very likely to anytime in the near future. So 781 00:41:36,800 --> 00:41:40,040 Speaker 1: until then, the only frontier really is mental. Can we 782 00:41:40,120 --> 00:41:42,839 Speaker 1: come up with a new theory that brings these two 783 00:41:42,840 --> 00:41:46,480 Speaker 1: things together that reconciles the uncertainty of quantum mechanics and 784 00:41:46,520 --> 00:41:48,680 Speaker 1: the determinism of relativity. 785 00:41:49,000 --> 00:41:52,080 Speaker 2: Well, give me like three minutes while ads play, and 786 00:41:52,160 --> 00:41:53,680 Speaker 2: I'll try to come up with something. 787 00:41:54,840 --> 00:41:56,839 Speaker 1: All right, The Katie Golden tries to win the Nobel 788 00:41:56,840 --> 00:41:58,080 Speaker 1: Prize in three minutes challenge. 789 00:41:58,400 --> 00:42:13,040 Speaker 2: Go all right, I think I've got it, Daniel. 790 00:42:13,280 --> 00:42:15,319 Speaker 1: Oh wow, I'm so desperate to hear what you came 791 00:42:15,400 --> 00:42:15,640 Speaker 1: up with. 792 00:42:15,760 --> 00:42:21,560 Speaker 3: Did you guys remember to carry the one. 793 00:42:20,880 --> 00:42:23,040 Speaker 1: Hold on a second? Did we miss a minus science? 794 00:42:23,400 --> 00:42:26,720 Speaker 1: Is that the whole problem? Oh my gosh, Katie, pause 795 00:42:26,800 --> 00:42:29,360 Speaker 1: this recording right now to rush off to Sweden to 796 00:42:29,400 --> 00:42:30,560 Speaker 1: collecting about rice. 797 00:42:31,680 --> 00:42:35,720 Speaker 3: Well you're very welcome, but yes, let's talk about how 798 00:42:35,840 --> 00:42:41,400 Speaker 3: to go from like our observational science to bringing it 799 00:42:41,560 --> 00:42:46,040 Speaker 3: into the brain. How could we possibly do science from 800 00:42:46,400 --> 00:42:47,640 Speaker 3: inside our own heads? 801 00:42:49,080 --> 00:42:51,560 Speaker 1: Well, sometimes it comes down to just being creative. You 802 00:42:51,560 --> 00:42:55,239 Speaker 1: know a lot of big advances in human history have 803 00:42:55,320 --> 00:42:58,000 Speaker 1: come from just people sitting in their dank study thinking 804 00:42:58,000 --> 00:43:01,040 Speaker 1: about the nature of the universe and pulling ideas together. 805 00:43:01,400 --> 00:43:05,040 Speaker 1: You know, Einstein's revolution with a photoelectric effect. He didn't 806 00:43:05,040 --> 00:43:07,440 Speaker 1: do that experiment. He didn't have a piece of metal 807 00:43:07,520 --> 00:43:09,960 Speaker 1: and a bright light in his laboratory. Guy didn't have 808 00:43:10,040 --> 00:43:13,200 Speaker 1: a laboratory. He read a paper or somebody else did 809 00:43:13,239 --> 00:43:15,600 Speaker 1: this experiment, and he just thought about it and had 810 00:43:15,600 --> 00:43:18,800 Speaker 1: this idea for how to explain it and combined it 811 00:43:18,840 --> 00:43:21,520 Speaker 1: with something he heard from Max Plank about how to 812 00:43:21,560 --> 00:43:25,120 Speaker 1: explain how stuff glows and the temperature at which things glow. 813 00:43:25,320 --> 00:43:29,640 Speaker 1: And decades earlier, Maxwell brought together electricity and magnetism just 814 00:43:29,680 --> 00:43:32,080 Speaker 1: by writing them down nicely on a sheet of paper 815 00:43:32,120 --> 00:43:34,759 Speaker 1: and noticing that there were symmetries between them. So we 816 00:43:34,800 --> 00:43:37,080 Speaker 1: can make a lot of progress in physics just by 817 00:43:37,120 --> 00:43:38,319 Speaker 1: having new ideas. 818 00:43:38,800 --> 00:43:44,439 Speaker 3: So are there people in dank rooms I imagine them 819 00:43:44,440 --> 00:43:47,480 Speaker 3: with like maybe one light bulb lighting the entire room, 820 00:43:47,560 --> 00:43:50,000 Speaker 3: hard at work trying to figure this out. Has there 821 00:43:50,040 --> 00:43:52,960 Speaker 3: been any progress made on trying to come up with 822 00:43:53,120 --> 00:43:55,919 Speaker 3: a philosophical or mathematical explanation. 823 00:43:56,239 --> 00:43:58,440 Speaker 1: So people have been working on this for a long time, 824 00:43:58,680 --> 00:44:02,040 Speaker 1: and it's very challenging. Mathematically. It's hard to see how 825 00:44:02,120 --> 00:44:05,360 Speaker 1: you can get this sort of uncertainty of quantum mechanics 826 00:44:05,920 --> 00:44:10,239 Speaker 1: and the rigor and determination of general relativity to play 827 00:44:10,360 --> 00:44:13,040 Speaker 1: nicely together. There's been a lot of attempts, and a 828 00:44:13,080 --> 00:44:14,839 Speaker 1: lot of them have failed. But there is a new 829 00:44:14,880 --> 00:44:18,640 Speaker 1: idea out there, and that's quantum relativity what we're talking 830 00:44:18,640 --> 00:44:21,920 Speaker 1: about today, and the idea is instead of taking general 831 00:44:21,960 --> 00:44:25,240 Speaker 1: relativity and trying to change it so that it's like uncertain, 832 00:44:25,480 --> 00:44:28,480 Speaker 1: rather than saying maybe the curvature or space time is 833 00:44:28,560 --> 00:44:31,120 Speaker 1: uncertain in the way we're talking about earlier, it's wondering 834 00:44:31,200 --> 00:44:35,680 Speaker 1: can we actually see how quantum mechanics comes naturally from relativity, 835 00:44:36,000 --> 00:44:40,160 Speaker 1: Like maybe the weirdness of quantum mechanics just emerges from 836 00:44:40,320 --> 00:44:44,319 Speaker 1: relativity itself, the way the ideal gas law emerges from 837 00:44:44,360 --> 00:44:48,560 Speaker 1: the motion of particles, or hurricanes emerge from the swirling 838 00:44:48,600 --> 00:44:51,800 Speaker 1: of droplets in the atmosphere. Is it possible to find 839 00:44:51,880 --> 00:44:55,839 Speaker 1: hints in relativity from which we could build the weirdness 840 00:44:55,880 --> 00:45:00,240 Speaker 1: of quantum mechanics directly. That's why it's called quantum relativity. 841 00:45:00,520 --> 00:45:03,240 Speaker 1: Take relativity and find a way to build quantum mechanics 842 00:45:03,320 --> 00:45:06,160 Speaker 1: on top of it, rather than like jamming quantum uncertainty 843 00:45:06,200 --> 00:45:07,960 Speaker 1: directly into relativity. 844 00:45:08,440 --> 00:45:11,719 Speaker 3: That's interesting because I think of when I think of 845 00:45:11,800 --> 00:45:15,160 Speaker 3: sort of the direction of causality, I think of, like 846 00:45:15,800 --> 00:45:18,960 Speaker 3: the small things cause the big things to happen, right, 847 00:45:19,040 --> 00:45:23,399 Speaker 3: the little particles there's some causality of like the small 848 00:45:23,480 --> 00:45:26,040 Speaker 3: particles that make up the big things, you know, cause 849 00:45:26,120 --> 00:45:29,320 Speaker 3: some effect, so that I would always kind of intuitively 850 00:45:29,360 --> 00:45:31,719 Speaker 3: think like, well, we have to figure out how the 851 00:45:31,760 --> 00:45:35,080 Speaker 3: small things behavior explains the big things. But it seems 852 00:45:35,120 --> 00:45:38,480 Speaker 3: like this is more like you're taking the kind of 853 00:45:38,520 --> 00:45:43,080 Speaker 3: behavior of big things with general relativity and seeing how 854 00:45:43,120 --> 00:45:49,040 Speaker 3: that could either explain or how you could see quantum 855 00:45:49,040 --> 00:45:50,799 Speaker 3: mechanics grow out of that. 856 00:45:51,200 --> 00:45:53,520 Speaker 1: Yeah, exactly, and so let's drill in on some of 857 00:45:53,560 --> 00:45:56,080 Speaker 1: the details to make this a little bit more concrete. 858 00:45:56,520 --> 00:45:56,719 Speaker 2: You know. 859 00:45:56,800 --> 00:45:59,719 Speaker 1: One of the crucial things we have in quantum mechanics 860 00:45:59,719 --> 00:46:03,040 Speaker 1: that we don't have in relativity is this uncertainty, this 861 00:46:03,160 --> 00:46:07,240 Speaker 1: possibility for things to be in two locations. Right, a particle, 862 00:46:07,280 --> 00:46:09,360 Speaker 1: for example, we say maybe it does this and maybe 863 00:46:09,360 --> 00:46:11,799 Speaker 1: it does that, and we said, that's uncertain It has 864 00:46:11,880 --> 00:46:15,920 Speaker 1: both possibilities, whereas in relativity we have a lot of determination. 865 00:46:16,080 --> 00:46:18,200 Speaker 1: Like you shoot a particle, even if it's near the 866 00:46:18,239 --> 00:46:20,480 Speaker 1: speed of light, it's going in some direction, you know 867 00:46:20,520 --> 00:46:22,640 Speaker 1: what it's going to do. You can calculate it. One 868 00:46:22,680 --> 00:46:25,400 Speaker 1: of the core conflicts between these two theories is just that. 869 00:46:25,680 --> 00:46:28,959 Speaker 1: So the authors of this theory quantum relativity have found 870 00:46:29,000 --> 00:46:33,560 Speaker 1: a way to try to find multiple possibilities in relativity. 871 00:46:33,800 --> 00:46:37,600 Speaker 1: They say, hmm, maybe there's some overlooked mathematics that shows 872 00:46:37,640 --> 00:46:43,000 Speaker 1: us how relativity actually can have like multiple solutions simultaneously. 873 00:46:43,440 --> 00:46:45,719 Speaker 1: One of the founding principles of relativity is that light 874 00:46:45,760 --> 00:46:48,640 Speaker 1: always moves at the speed of light. Right, all observers 875 00:46:48,719 --> 00:46:50,879 Speaker 1: see light moving at the speed of light, no matter 876 00:46:50,960 --> 00:46:53,680 Speaker 1: how fast you're going. So you're moving in half the 877 00:46:53,680 --> 00:46:55,960 Speaker 1: speed of light relative to the Earth. You turn on 878 00:46:56,000 --> 00:46:58,320 Speaker 1: a flashlight, you're going to see that light being moving 879 00:46:58,640 --> 00:47:01,520 Speaker 1: at the speed of light relative you. Somebody on the 880 00:47:01,560 --> 00:47:04,440 Speaker 1: ground who sees you moving at half the speed of 881 00:47:04,520 --> 00:47:06,600 Speaker 1: light and turning on your flashlight, they look at that 882 00:47:06,680 --> 00:47:09,200 Speaker 1: light beam, they also see it moving at the speed 883 00:47:09,239 --> 00:47:11,080 Speaker 1: of light. They don't see it moving at the speed 884 00:47:11,120 --> 00:47:13,759 Speaker 1: of light plus half the speed of light. It's one 885 00:47:13,760 --> 00:47:16,279 Speaker 1: of the really weird things about special relativity. 886 00:47:16,680 --> 00:47:20,879 Speaker 3: Right, so light there is a constant speed of light 887 00:47:21,160 --> 00:47:24,640 Speaker 3: that can't really be slowed down or sped up exactly. 888 00:47:24,680 --> 00:47:27,239 Speaker 1: And this is the founding assumption of special relativity, at 889 00:47:27,320 --> 00:47:29,279 Speaker 1: least to a whole bunch of mathematics. It tells us 890 00:47:29,520 --> 00:47:32,360 Speaker 1: how to see things from different perspectives. Tells us like, 891 00:47:32,800 --> 00:47:35,440 Speaker 1: how is it possible to see light moving at this 892 00:47:35,520 --> 00:47:37,560 Speaker 1: speed for this observer and seeing it move at the 893 00:47:37,560 --> 00:47:39,880 Speaker 1: same speed for that observer. It helps us tie it 894 00:47:39,920 --> 00:47:43,000 Speaker 1: all together, tells a different story for how the universe works, 895 00:47:43,040 --> 00:47:46,319 Speaker 1: and time goes weird sometimes and things get short, and 896 00:47:46,360 --> 00:47:48,880 Speaker 1: we have podcasts digging into all those details. But it 897 00:47:48,880 --> 00:47:51,279 Speaker 1: gives us this picture of like how different people can 898 00:47:51,320 --> 00:47:54,160 Speaker 1: see the universe from different velocities, and this is called 899 00:47:54,200 --> 00:47:57,280 Speaker 1: the Lorentz transforms. It tells you how to transform between 900 00:47:57,280 --> 00:47:59,880 Speaker 1: one observer and another observer. Because it turns out to 901 00:48:00,200 --> 00:48:01,600 Speaker 1: not as simple as we thought. 902 00:48:01,800 --> 00:48:04,640 Speaker 3: Yeah, I'm looking at this formula and doesn't look super 903 00:48:04,680 --> 00:48:05,239 Speaker 3: simple to me. 904 00:48:06,200 --> 00:48:08,239 Speaker 1: No, it's not simple, and it's nonlinear, and it's got 905 00:48:08,239 --> 00:48:10,279 Speaker 1: square roots in it, and it gets really wonky, which 906 00:48:10,320 --> 00:48:13,320 Speaker 1: is why relativity is so weird and time flows strangely 907 00:48:13,360 --> 00:48:15,520 Speaker 1: and you have the twin paradox and all that stuff. Now, 908 00:48:15,560 --> 00:48:19,360 Speaker 1: that's fine, But it turns out there's actually a second solution. 909 00:48:19,840 --> 00:48:23,840 Speaker 1: There's another way you could describe the transformation how people 910 00:48:23,880 --> 00:48:28,120 Speaker 1: see things in different velocities. That also satisfies this requirement 911 00:48:28,440 --> 00:48:30,680 Speaker 1: that the speed of light is the same for everybody, 912 00:48:30,840 --> 00:48:33,239 Speaker 1: sort of like a second solution to an equation. You know, 913 00:48:33,280 --> 00:48:36,920 Speaker 1: if you have like X squared equals nine, one solution is, oh, 914 00:48:37,080 --> 00:48:40,360 Speaker 1: X equals three. Another solution is what if X equals 915 00:48:40,360 --> 00:48:42,480 Speaker 1: minus three. This is the kind of thing that crops 916 00:48:42,560 --> 00:48:45,920 Speaker 1: up all the time in mathematics and sometimes in physics, 917 00:48:45,920 --> 00:48:48,279 Speaker 1: we like, well, minus three doesn't make sense. We'll just 918 00:48:48,320 --> 00:48:51,160 Speaker 1: ignore that. We'll just drop the unphysical solution. 919 00:48:51,360 --> 00:48:55,200 Speaker 3: Yeah, you can't have negative three apples, missus Birch. 920 00:48:56,320 --> 00:48:58,480 Speaker 1: You can actually go into debt for apples, and you 921 00:48:58,480 --> 00:49:01,440 Speaker 1: can be an apple or prison. So yeah, thanks financial 922 00:49:01,440 --> 00:49:03,240 Speaker 1: engineers for inventing negative money. 923 00:49:03,440 --> 00:49:07,600 Speaker 3: I forgot that our currency was based on the Apple standard. 924 00:49:09,560 --> 00:49:12,719 Speaker 1: Exactly. So in this scenario, there's one solution to these 925 00:49:12,760 --> 00:49:15,799 Speaker 1: transformations to tell you, like how different observers see the 926 00:49:15,880 --> 00:49:18,880 Speaker 1: universe different velocities, And that's the one that assumes that 927 00:49:18,960 --> 00:49:21,759 Speaker 1: everything travels at the speed of light or less. It's 928 00:49:21,800 --> 00:49:25,080 Speaker 1: actually a second solution, a second way to transform between 929 00:49:25,120 --> 00:49:29,040 Speaker 1: these frames that holds for velocities greater than the speed 930 00:49:29,080 --> 00:49:31,800 Speaker 1: of light. And that's like, what, hold on a second, 931 00:49:31,840 --> 00:49:34,839 Speaker 1: I thought the whole assumption of special relativity was that 932 00:49:34,880 --> 00:49:38,439 Speaker 1: you can only move slower than the speed of light, right, 933 00:49:38,640 --> 00:49:42,320 Speaker 1: That is one way to interpret these transformations. There's another 934 00:49:42,360 --> 00:49:45,840 Speaker 1: way to interpret them for velocities greater than the speed 935 00:49:45,840 --> 00:49:49,719 Speaker 1: of light. So these would mean particles moving faster than 936 00:49:49,760 --> 00:49:50,640 Speaker 1: the speed of light. 937 00:49:51,080 --> 00:49:53,239 Speaker 2: What kind of particles are these? Do we know? 938 00:49:53,760 --> 00:49:56,160 Speaker 1: So there's a theory about particles moving faster than the 939 00:49:56,160 --> 00:50:00,200 Speaker 1: speed of light. They're called tachyons, and they do satisfy 940 00:50:00,239 --> 00:50:03,719 Speaker 1: the mathematics of relativity, though nobody's ever seen one. One 941 00:50:03,719 --> 00:50:06,480 Speaker 1: problem with anything moving faster than the speed of light 942 00:50:06,640 --> 00:50:09,440 Speaker 1: is that you can end up with tricky paradoxes about 943 00:50:09,440 --> 00:50:12,759 Speaker 1: the order of things and causality, because remember that observers 944 00:50:12,840 --> 00:50:16,240 Speaker 1: moving at high speeds can see stuff happening at different times. 945 00:50:16,440 --> 00:50:19,040 Speaker 1: Like if I see event A happening before event B, 946 00:50:19,520 --> 00:50:21,839 Speaker 1: you might see the opposite order of stuff because you're 947 00:50:21,840 --> 00:50:24,279 Speaker 1: flying by me at a high speed. That's one of 948 00:50:24,320 --> 00:50:28,560 Speaker 1: the consequences of special relativity that you're not guaranteed simultaneity 949 00:50:28,640 --> 00:50:31,560 Speaker 1: for all frames. That different observers can see the order 950 00:50:31,560 --> 00:50:34,120 Speaker 1: of events differently, and that's usually fine, it's not a 951 00:50:34,120 --> 00:50:36,719 Speaker 1: big deal. But if you can move faster than the 952 00:50:36,719 --> 00:50:38,880 Speaker 1: speed of light, then you start to see things that 953 00:50:38,920 --> 00:50:42,440 Speaker 1: are causally linked be reversed. Like, for example, if I 954 00:50:42,600 --> 00:50:45,960 Speaker 1: fire an arrow, then somebody moving past me is faster 955 00:50:46,000 --> 00:50:48,160 Speaker 1: than the speed of light could see the arrow hit 956 00:50:48,200 --> 00:50:51,120 Speaker 1: the apple before I even fire it. That seems sort 957 00:50:51,120 --> 00:50:53,320 Speaker 1: of problematic, and people are like, yeah, let's just cross 958 00:50:53,360 --> 00:50:56,200 Speaker 1: that off and say that doesn't happen, but actually opens 959 00:50:56,239 --> 00:50:58,759 Speaker 1: the door and exactly the way we might need to 960 00:50:58,960 --> 00:51:02,960 Speaker 1: link relativity with quantum mechanics, because now we have like 961 00:51:03,040 --> 00:51:06,200 Speaker 1: two explanations for those events, like does Daniel fire the 962 00:51:06,280 --> 00:51:08,520 Speaker 1: arrow before it hits the apple or does it hit 963 00:51:08,560 --> 00:51:11,880 Speaker 1: the apple before I fire the arrow? So the idea 964 00:51:11,920 --> 00:51:14,719 Speaker 1: of quantum relativity is to say, well, what if you 965 00:51:14,760 --> 00:51:16,759 Speaker 1: look at these things both from the less than the 966 00:51:16,760 --> 00:51:20,200 Speaker 1: speed of light perspective and the greater than the speed 967 00:51:20,200 --> 00:51:23,040 Speaker 1: of life perspective, Like if you allow both views of it, 968 00:51:23,320 --> 00:51:26,120 Speaker 1: then you have sort of like two different ideas for 969 00:51:26,200 --> 00:51:29,600 Speaker 1: what might be happening here, and there isn't a deterministic 970 00:51:29,680 --> 00:51:32,120 Speaker 1: explanation for which is the right one. 971 00:51:32,239 --> 00:51:34,839 Speaker 3: I mean, you had mentioned earlier that this was kind 972 00:51:34,880 --> 00:51:38,040 Speaker 3: of dismissed, right, because like the idea is that you 973 00:51:38,120 --> 00:51:43,200 Speaker 3: can't observe causally linked events in reverse. What is the 974 00:51:43,280 --> 00:51:46,239 Speaker 3: assumption behind that that says that you can't do that? 975 00:51:46,520 --> 00:51:47,440 Speaker 2: Because like, I. 976 00:51:47,360 --> 00:51:49,480 Speaker 3: Know, it sounds obvious, right, like, of course you can't. 977 00:51:49,719 --> 00:51:52,480 Speaker 3: I would assume there's actually some kind of law in 978 00:51:52,520 --> 00:51:55,920 Speaker 3: physics that does link to that, because you know what 979 00:51:56,000 --> 00:51:58,080 Speaker 3: we know about like assumptions, like we have all sorts 980 00:51:58,120 --> 00:52:00,480 Speaker 3: of assumptions about the world works because that's how we 981 00:52:00,520 --> 00:52:04,280 Speaker 3: observe it. We as humans never observe things in reverse. 982 00:52:04,760 --> 00:52:08,200 Speaker 3: But is there an actual law in either physics or 983 00:52:08,280 --> 00:52:13,000 Speaker 3: general relativity that would prohibit that observation from coming before 984 00:52:13,080 --> 00:52:13,480 Speaker 3: the event? 985 00:52:13,880 --> 00:52:16,799 Speaker 1: Yeah, that's a great question. Why do we assume that 986 00:52:16,840 --> 00:52:19,840 Speaker 1: there's causality in the universe, that things have to be linked? 987 00:52:19,920 --> 00:52:21,520 Speaker 1: And it's just sort of like part of how we 988 00:52:21,600 --> 00:52:24,799 Speaker 1: think about physics. It's a core assumption we make. We 989 00:52:24,880 --> 00:52:26,960 Speaker 1: don't know that it's true, but it sort of makes 990 00:52:27,080 --> 00:52:29,120 Speaker 1: sense to us, and so we try to hold on 991 00:52:29,160 --> 00:52:31,799 Speaker 1: to it as long as possible, build theories on that 992 00:52:31,880 --> 00:52:34,520 Speaker 1: assumption and see if they work. But it might be 993 00:52:34,640 --> 00:52:36,839 Speaker 1: that we have to give it up. There are other 994 00:52:36,920 --> 00:52:39,640 Speaker 1: hints in other theories of physics, sort of the cutting edge, 995 00:52:39,760 --> 00:52:43,160 Speaker 1: that maybe causality isn't the fundamental aspect of the universe. 996 00:52:43,360 --> 00:52:45,960 Speaker 1: It might be something we are trying to impose on it. 997 00:52:46,400 --> 00:52:48,840 Speaker 1: You know, think about the way that we explain the universe. 998 00:52:48,920 --> 00:52:53,000 Speaker 1: We tend to tell stories. Stories are like little causal links. 999 00:52:53,400 --> 00:52:55,640 Speaker 1: I did this, and then she did that, and then 1000 00:52:55,680 --> 00:52:58,520 Speaker 1: this happened. It's like A, then B and C, then D. 1001 00:52:58,760 --> 00:53:01,200 Speaker 1: It's sort of embedded deeply in how we think. It 1002 00:53:01,239 --> 00:53:04,160 Speaker 1: doesn't mean it has to be embedded deeply into the universe. 1003 00:53:04,719 --> 00:53:06,520 Speaker 1: And so this is sort of like giving up that 1004 00:53:06,560 --> 00:53:10,080 Speaker 1: causal chain and saying, well, maybe A cause B, but 1005 00:53:10,200 --> 00:53:13,200 Speaker 1: maybe B caused A. And that's where you get your 1006 00:53:13,239 --> 00:53:17,120 Speaker 1: crack indeterminism In relativity, it says, maybe there are two 1007 00:53:17,120 --> 00:53:22,360 Speaker 1: ways to view these events. One subliminal, sorry, one subluminal, 1008 00:53:22,600 --> 00:53:25,320 Speaker 1: not subliminal as in slower than the speed. 1009 00:53:25,160 --> 00:53:30,520 Speaker 3: Of lfemptoms about the superliminal messaging, yeah. 1010 00:53:30,200 --> 00:53:33,600 Speaker 1: And one super illuminal, like a view from an observer 1011 00:53:33,760 --> 00:53:35,920 Speaker 1: moving fast than the speed of light that sees an 1012 00:53:35,920 --> 00:53:39,640 Speaker 1: opposite order of events. And this is basically the crack 1013 00:53:39,760 --> 00:53:42,719 Speaker 1: that this whole theory of quantum relativity is built on. 1014 00:53:42,800 --> 00:53:47,560 Speaker 1: It says, within relativity, maybe you can have nondeterminism, because 1015 00:53:47,600 --> 00:53:51,399 Speaker 1: maybe the superluminal view of the universe is different from 1016 00:53:51,440 --> 00:53:55,040 Speaker 1: the subluminal view, that the order of events can be different. 1017 00:53:55,200 --> 00:53:58,680 Speaker 1: From within relativity, we now see a little bit of uncertainty, 1018 00:53:59,000 --> 00:54:02,440 Speaker 1: a loss of de herminism, and that's basically the starting 1019 00:54:02,480 --> 00:54:04,160 Speaker 1: place for quantum relativity. 1020 00:54:04,480 --> 00:54:07,680 Speaker 3: I think we have to remind ourselves that physicists are 1021 00:54:07,760 --> 00:54:13,919 Speaker 3: human beings and they have the same kind of mental fallacies, 1022 00:54:14,239 --> 00:54:17,640 Speaker 3: or not necessarily fallacies, but just habits the routine that 1023 00:54:18,080 --> 00:54:23,399 Speaker 3: all humans have, which is viewing things in terms of 1024 00:54:23,560 --> 00:54:28,520 Speaker 3: what we have adapted to as human beings or earlier 1025 00:54:28,560 --> 00:54:32,440 Speaker 3: as primates, and it's such a strong thing. There have 1026 00:54:32,440 --> 00:54:36,359 Speaker 3: been studies on people's behavior where when you look at 1027 00:54:36,440 --> 00:54:40,440 Speaker 3: like a screen that has like randomly moving dots on 1028 00:54:40,520 --> 00:54:44,480 Speaker 3: a screen or something like, people will try to impose 1029 00:54:44,520 --> 00:54:47,800 Speaker 3: some kind of like rules on this or like volition 1030 00:54:48,080 --> 00:54:51,319 Speaker 3: to these things, like that these feel alive because they're 1031 00:54:51,360 --> 00:54:54,560 Speaker 3: moving randomly, and so you think, well, then there must 1032 00:54:54,560 --> 00:54:57,880 Speaker 3: be some kind of autonomy of these things, like some 1033 00:54:58,080 --> 00:55:01,200 Speaker 3: reason that it's doing is so like this causality link, 1034 00:55:01,320 --> 00:55:05,120 Speaker 3: like I mentioned earlier. It's even found in like babies, 1035 00:55:05,160 --> 00:55:08,480 Speaker 3: where you'll see, like if they see something that defies 1036 00:55:08,640 --> 00:55:11,480 Speaker 3: the laws of very simple physics of like a ball 1037 00:55:11,600 --> 00:55:14,680 Speaker 3: hitting a ball and that ball kind of moving, they 1038 00:55:15,320 --> 00:55:16,640 Speaker 3: stare at that because. 1039 00:55:16,360 --> 00:55:17,600 Speaker 2: That's not what they're expecting. 1040 00:55:17,680 --> 00:55:22,120 Speaker 3: So it seems like a huge challenge to overcome our 1041 00:55:22,320 --> 00:55:27,080 Speaker 3: humanness when we're also trying to answer these questions about 1042 00:55:27,120 --> 00:55:31,680 Speaker 3: the universe that do not necessarily play by the same 1043 00:55:31,760 --> 00:55:36,080 Speaker 3: rules as say, like a primate that has somehow gotten 1044 00:55:36,080 --> 00:55:38,320 Speaker 3: smart enough to start writing down numbers. 1045 00:55:39,480 --> 00:55:43,040 Speaker 1: Yeah, and we've often seen the appearance of autonomy and 1046 00:55:43,239 --> 00:55:47,040 Speaker 1: action in the universe, you know, explaining whether in terms 1047 00:55:47,040 --> 00:55:49,839 Speaker 1: of some big guy in the sky throwing thunderbolts, et cetera, 1048 00:55:49,840 --> 00:55:52,000 Speaker 1: et cetera. And so we do have to be careful 1049 00:55:52,040 --> 00:55:55,520 Speaker 1: and question our assumptions. And sometimes when we are failing 1050 00:55:55,560 --> 00:55:58,360 Speaker 1: to describe the universe that we see, we need to 1051 00:55:58,480 --> 00:56:00,960 Speaker 1: circle back and say, well, maybe there's something wrong in 1052 00:56:01,000 --> 00:56:04,160 Speaker 1: the foundations of our science itself. Maybe we need to 1053 00:56:04,200 --> 00:56:07,160 Speaker 1: be asking questions about whether all of these assumptions really 1054 00:56:07,200 --> 00:56:10,239 Speaker 1: hold and what breaks if we get rid of them, 1055 00:56:10,440 --> 00:56:12,640 Speaker 1: or what breakthroughs we might be able to make. 1056 00:56:12,920 --> 00:56:16,799 Speaker 3: So, once we get rid of this assumption that there 1057 00:56:16,960 --> 00:56:20,600 Speaker 3: has to be this causality, has there been any breakthroughs 1058 00:56:20,640 --> 00:56:23,920 Speaker 3: in terms of then connecting this potential new model of 1059 00:56:24,320 --> 00:56:29,160 Speaker 3: general relativity to quantum mechanics, Like, have there been successful 1060 00:56:29,239 --> 00:56:33,640 Speaker 3: sort of developments in quantum relativity beyond? Just like maybe 1061 00:56:33,719 --> 00:56:35,800 Speaker 3: we can issue the causality. 1062 00:56:36,280 --> 00:56:39,040 Speaker 1: Not yet. It's sort of like a promising direction for 1063 00:56:39,120 --> 00:56:41,400 Speaker 1: people to build on. What it has generated is a 1064 00:56:41,400 --> 00:56:44,319 Speaker 1: whole series of papers arguing about it. So a bunch 1065 00:56:44,320 --> 00:56:46,239 Speaker 1: of physicis are like, hey, you can't do that. This 1066 00:56:46,280 --> 00:56:49,440 Speaker 1: doesn't make sense, and other people be like, no, actually, 1067 00:56:49,440 --> 00:56:52,520 Speaker 1: maybe it does. And so, you know, it's a healthy conversation. 1068 00:56:52,960 --> 00:56:56,160 Speaker 1: So far hasn't led anywhere concrete yet, but you know, 1069 00:56:56,200 --> 00:56:58,319 Speaker 1: it might be that we look back in one hundred 1070 00:56:58,400 --> 00:57:01,200 Speaker 1: years and tell stories about this moment where people are like, 1071 00:57:01,239 --> 00:57:04,759 Speaker 1: wait a second, what about this basic assumption, or this 1072 00:57:04,800 --> 00:57:08,240 Speaker 1: could just end up on the very very deep trash 1073 00:57:08,320 --> 00:57:11,400 Speaker 1: can of the theories that have attempted to unify general 1074 00:57:11,400 --> 00:57:13,520 Speaker 1: relativity and quantum mechanics and failed. 1075 00:57:14,080 --> 00:57:17,320 Speaker 3: I mean, you need to fill a few trash cans 1076 00:57:17,320 --> 00:57:20,600 Speaker 3: full of crumpled up sheets to make a physics aline, 1077 00:57:20,760 --> 00:57:22,120 Speaker 3: as I understand it. 1078 00:57:23,880 --> 00:57:26,960 Speaker 1: Exactly. But it's fun to examine all these assumptions to 1079 00:57:26,960 --> 00:57:29,720 Speaker 1: try to explain our universe in terms of the tiniest 1080 00:57:29,720 --> 00:57:32,640 Speaker 1: little particles, and to try to unify those theories, the 1081 00:57:32,640 --> 00:57:35,360 Speaker 1: ones that describe the really big, heavy stuff and the 1082 00:57:35,360 --> 00:57:39,120 Speaker 1: ones that describe the tiniest little particles flitting around inside 1083 00:57:39,200 --> 00:57:42,480 Speaker 1: our atoms. Maybe one day we'll figure it out. Until then, 1084 00:57:42,520 --> 00:57:45,160 Speaker 1: thanks very much Kinnie for joining me on this journey 1085 00:57:45,200 --> 00:57:47,840 Speaker 1: to our lack of understanding about the universe. 1086 00:57:48,000 --> 00:57:50,760 Speaker 3: Thanks for having me, and really do check on whether 1087 00:57:50,800 --> 00:57:53,280 Speaker 3: you guys just forgot to carry the one, because you know, 1088 00:57:53,760 --> 00:57:54,840 Speaker 3: we all make mistakes. 1089 00:57:55,880 --> 00:57:57,640 Speaker 1: I'm on it, and if it turns out you were right, 1090 00:57:57,840 --> 00:58:01,200 Speaker 1: we'll definitely cite you. Thanks everyone for listening, See you 1091 00:58:01,240 --> 00:58:08,680 Speaker 1: next time. For more science and curiosity, come find us 1092 00:58:08,680 --> 00:58:12,120 Speaker 1: on social media, where we answer questions and post videos. 1093 00:58:12,360 --> 00:58:16,040 Speaker 1: We're on Twitter, disc Org, Insta, and now TikTok. Thanks 1094 00:58:16,080 --> 00:58:18,720 Speaker 1: for listening and remember that Daniel and Jorge Explain the 1095 00:58:18,760 --> 00:58:23,560 Speaker 1: Universe is a production of iHeartRadio. For more podcasts from iHeartRadio, 1096 00:58:23,680 --> 00:58:27,880 Speaker 1: visit the iHeartRadio app, Apple Podcasts, or wherever you listen 1097 00:58:27,920 --> 00:58:29,120 Speaker 1: to your favorite shows.