1 00:00:08,480 --> 00:00:12,040 Speaker 1: Hey, Daniel, do you read science articles in the popular press? 2 00:00:12,200 --> 00:00:14,960 Speaker 1: You know, I can't help myself because I love hearing 3 00:00:15,000 --> 00:00:18,239 Speaker 1: about new science discoveries, but I always read them with 4 00:00:18,320 --> 00:00:21,080 Speaker 1: a big grain of salt. You don't trust him well? 5 00:00:21,079 --> 00:00:23,360 Speaker 1: You know, Sometimes I read an article where I actually 6 00:00:23,520 --> 00:00:27,040 Speaker 1: know the science really well, and often I strongly disagree 7 00:00:27,080 --> 00:00:31,680 Speaker 1: with how it's presented. And by often you mean always know. 8 00:00:31,840 --> 00:00:35,479 Speaker 1: There are some great science journalists out there, but I 9 00:00:35,520 --> 00:00:37,239 Speaker 1: guess I mean general you don't have a lot of 10 00:00:37,280 --> 00:00:40,159 Speaker 1: confidence in science journalists. I mean sometimes you read these 11 00:00:40,200 --> 00:00:44,519 Speaker 1: popular science articles that are just totally bonkers, like the 12 00:00:44,520 --> 00:00:48,760 Speaker 1: headline scientists discover the universe is filled with invisible dark matter. Okay, 13 00:00:49,080 --> 00:00:51,959 Speaker 1: that one's actually pretty good. Or physics discovers a new 14 00:00:52,040 --> 00:00:54,920 Speaker 1: forced tearing the universe apart. All right. It sounds like 15 00:00:54,960 --> 00:00:57,520 Speaker 1: clickbait but also true. Oh man, then how do I 16 00:00:57,520 --> 00:01:00,240 Speaker 1: tell the difference? I guess you have to email us 17 00:01:00,280 --> 00:01:02,560 Speaker 1: and we'll break it down for you on the podcast. 18 00:01:02,640 --> 00:01:20,840 Speaker 1: Like they I am or Hey, I'm a cartoonist and 19 00:01:20,880 --> 00:01:24,080 Speaker 1: the creator of PhD comics. Hi, I'm Daniel. I'm a 20 00:01:24,120 --> 00:01:27,080 Speaker 1: particle physicist, and I'll admit to gritting my teeth while 21 00:01:27,160 --> 00:01:29,800 Speaker 1: reading popular science article excitement. You just read it and 22 00:01:29,800 --> 00:01:32,759 Speaker 1: you're so excited you clench your draw No, not always 23 00:01:32,760 --> 00:01:35,200 Speaker 1: out of excitement. Sometimes I see a headline and I think, 24 00:01:35,280 --> 00:01:38,360 Speaker 1: oh my gosh, how could they even write that? What 25 00:01:38,480 --> 00:01:40,960 Speaker 1: if it's something you don't know, are not familiar with. Well, 26 00:01:41,000 --> 00:01:43,240 Speaker 1: then you know, I have to extrapolate, and I say, well, 27 00:01:43,480 --> 00:01:45,560 Speaker 1: if I know that it's bonkers half the time, then 28 00:01:45,560 --> 00:01:48,120 Speaker 1: there's a good chance that this is a bonker's article. 29 00:01:48,720 --> 00:01:50,560 Speaker 1: And so I had to write to a friend of 30 00:01:50,600 --> 00:01:52,400 Speaker 1: mine who is an expert in that area and say, 31 00:01:52,560 --> 00:01:56,440 Speaker 1: how bonkers is this? I see it's bonkers until proven otherwise. 32 00:01:57,440 --> 00:02:02,240 Speaker 1: That's my general philosophy. That's our general podcast. Welcome to 33 00:02:02,840 --> 00:02:05,680 Speaker 1: Daniel and Jorge Explained the Universe, a production of I 34 00:02:05,760 --> 00:02:09,000 Speaker 1: Heart Radio, in which we explore the bonkers nature of 35 00:02:09,040 --> 00:02:11,840 Speaker 1: the universe, some of it true, some of it clickbait, 36 00:02:12,040 --> 00:02:14,320 Speaker 1: and we break it down for you. We want you 37 00:02:14,360 --> 00:02:19,320 Speaker 1: to understand the truth about our crazy, amazing, wonderful, beautiful 38 00:02:19,440 --> 00:02:24,040 Speaker 1: universe without resorting to silly science journalism. Well, I guess 39 00:02:24,080 --> 00:02:26,919 Speaker 1: it's tricky, because you know, sometimes the universe is kind 40 00:02:26,919 --> 00:02:30,640 Speaker 1: of bonkers, right, So I guess the question it's more about, 41 00:02:30,680 --> 00:02:33,760 Speaker 1: you know, telling the difference between things that are maybe 42 00:02:33,800 --> 00:02:37,600 Speaker 1: overblown and what scientists actually discover. Yeah, and as a 43 00:02:37,639 --> 00:02:39,799 Speaker 1: lay person, how can you tell the difference, Because there 44 00:02:39,840 --> 00:02:42,440 Speaker 1: really are things that science has discovered that are hard 45 00:02:42,480 --> 00:02:45,480 Speaker 1: to understand, that are hard to take seriously. I mean, 46 00:02:45,520 --> 00:02:48,040 Speaker 1: the universe is billions of years old and began with 47 00:02:48,080 --> 00:02:51,840 Speaker 1: a huge explosion. I mean, it's ridiculous. There are pockets 48 00:02:51,840 --> 00:02:55,000 Speaker 1: of space out there that light cannot even escape and 49 00:02:55,040 --> 00:02:57,320 Speaker 1: can eat any kind of matter. I mean it sounds 50 00:02:57,600 --> 00:02:59,840 Speaker 1: absurd and made up, but some of it is true. 51 00:03:00,360 --> 00:03:03,120 Speaker 1: Sometimes we pay people to sit around and drink coffee 52 00:03:03,120 --> 00:03:07,160 Speaker 1: and smash particles together. That's that's bonkers as well. Now 53 00:03:07,200 --> 00:03:10,840 Speaker 1: you're being ridiculous. Come on, I heard it happens in Geneva. 54 00:03:11,639 --> 00:03:15,520 Speaker 1: That's not a job. Come on, I guess it's like 55 00:03:15,560 --> 00:03:21,040 Speaker 1: podcasting to miss No. I feel very fortunate to be 56 00:03:21,120 --> 00:03:23,400 Speaker 1: able to smash particles together to try to reveal the 57 00:03:23,480 --> 00:03:26,280 Speaker 1: secrets of the universe, and we take our responsibility very 58 00:03:26,280 --> 00:03:29,160 Speaker 1: seriously on this podcast to explain the science to you 59 00:03:29,200 --> 00:03:32,239 Speaker 1: in a way that actually makes sense and doesn't overhype 60 00:03:32,440 --> 00:03:35,680 Speaker 1: the already amazing discoveries of science. Yeah, So to be 61 00:03:35,720 --> 00:03:38,440 Speaker 1: on the program, we'll be discussing a recent article in 62 00:03:38,520 --> 00:03:43,160 Speaker 1: the popular press that has some apparently pretty bonkers results 63 00:03:43,360 --> 00:03:46,840 Speaker 1: from none other than NASA. That's right. And this is 64 00:03:46,880 --> 00:03:49,600 Speaker 1: an article that went all around the Internet and readers 65 00:03:49,600 --> 00:03:52,200 Speaker 1: from all over the world asked us what is this real? 66 00:03:52,480 --> 00:03:54,760 Speaker 1: Made a lot of noise on Twitter and on the 67 00:03:54,760 --> 00:03:56,680 Speaker 1: rest of the internets, and so we thought to be 68 00:03:56,760 --> 00:03:58,640 Speaker 1: useful to break it down for you, to tell you 69 00:03:58,800 --> 00:04:02,560 Speaker 1: what actually happened, why it really is fascinating scientifically, but 70 00:04:02,800 --> 00:04:05,280 Speaker 1: why the clickbait headlines may have gone a step too far. 71 00:04:05,760 --> 00:04:07,480 Speaker 1: What does a lot of noise and Twitter sound like? 72 00:04:07,680 --> 00:04:11,280 Speaker 1: Is it like click click, click, chirp, chirp, chirp, chirp, 73 00:04:11,520 --> 00:04:16,280 Speaker 1: chirp chirp, unlike unlike like like retweet retweeting. There's not 74 00:04:16,320 --> 00:04:19,080 Speaker 1: a hate button is there on Twitter? There's I think 75 00:04:19,080 --> 00:04:22,320 Speaker 1: there's enough hate on Twitter already. I don't think you 76 00:04:22,440 --> 00:04:26,760 Speaker 1: need the extra buttons there. But yes, today we'll be 77 00:04:26,839 --> 00:04:29,560 Speaker 1: talking about an article that came out in several outlets. 78 00:04:30,000 --> 00:04:33,000 Speaker 1: For example, in New Scientists magazine, there was a headline 79 00:04:33,279 --> 00:04:40,000 Speaker 1: we may have spotted a parallel universe going backwards in time. Boom, Wow, 80 00:04:40,120 --> 00:04:42,520 Speaker 1: that's a lot of um, that's a lot of words 81 00:04:42,560 --> 00:04:45,640 Speaker 1: in one sentence that makes you think, what, Yeah, yeah, 82 00:04:45,720 --> 00:04:48,920 Speaker 1: I know, whow apparel universe could exist? What it goes 83 00:04:48,960 --> 00:04:51,760 Speaker 1: backwards in time backwards? And what we spotted it? Oh 84 00:04:51,880 --> 00:04:55,920 Speaker 1: my gosh, there's so much there, right, It's incredible. Yeah. 85 00:04:56,360 --> 00:05:00,839 Speaker 1: And the Daily Star, the newspaper, says, a parallel universe 86 00:05:01,000 --> 00:05:03,320 Speaker 1: right next to ours where all the rules of physics 87 00:05:03,520 --> 00:05:06,839 Speaker 1: seemed to be operating in reverse, and now it's next 88 00:05:06,880 --> 00:05:09,440 Speaker 1: to us, apparently right next to ours. It could be 89 00:05:09,560 --> 00:05:12,240 Speaker 1: like in your pocket or you know, sitting at that 90 00:05:12,320 --> 00:05:15,799 Speaker 1: next table in the cafe or something. It's adjacent, it's nearby, 91 00:05:16,040 --> 00:05:19,480 Speaker 1: it's im right beyond your reach. And I don't know 92 00:05:19,560 --> 00:05:21,560 Speaker 1: what happened on the internet that day, but this just 93 00:05:21,760 --> 00:05:24,360 Speaker 1: really took off. It got zillions of likes, It was 94 00:05:24,360 --> 00:05:28,760 Speaker 1: retweeted by everybody, and then newspaper after newspaper reported this claim, 95 00:05:28,839 --> 00:05:31,080 Speaker 1: and so it's spread everywhere and a lot of people 96 00:05:31,160 --> 00:05:33,720 Speaker 1: heard about it. Yeah, and so a lot of readers 97 00:05:33,800 --> 00:05:36,720 Speaker 1: asked us to break this down. And so today on 98 00:05:36,839 --> 00:05:44,960 Speaker 1: the podcast, we'll be asking the question, didn't NASA discover 99 00:05:45,400 --> 00:05:48,560 Speaker 1: a parallel universe? Maybe in a parallel universe they did. 100 00:05:49,480 --> 00:05:53,400 Speaker 1: Maybe a parallel universe discovered us. Maybe, yeah, there you go. 101 00:05:53,640 --> 00:05:57,240 Speaker 1: Maybe we're the evil twins. Daniel, how's your gotee growing up? 102 00:05:58,960 --> 00:06:01,360 Speaker 1: I guess it's sort of like alien question, like would 103 00:06:01,400 --> 00:06:04,240 Speaker 1: you rather a parallel universe discover us, which means they're 104 00:06:04,240 --> 00:06:06,720 Speaker 1: probably better at science than we are, or that we 105 00:06:06,920 --> 00:06:09,400 Speaker 1: discover them? What do you think you're the one trying 106 00:06:09,440 --> 00:06:12,560 Speaker 1: to discover these parallel universes? Well, I love they discovered 107 00:06:12,680 --> 00:06:15,280 Speaker 1: us because we're not capable of discovering them. On the 108 00:06:15,360 --> 00:06:18,840 Speaker 1: other hand, the people getting discovered don't usually fare very 109 00:06:18,920 --> 00:06:22,240 Speaker 1: well in these scenarios, So I'd love to be discovered 110 00:06:22,320 --> 00:06:26,120 Speaker 1: by an intelligent, benevolent parallel universe. You'd rather be the 111 00:06:26,440 --> 00:06:34,600 Speaker 1: conquist the physicist than the confiscated. No, I do not 112 00:06:34,760 --> 00:06:38,000 Speaker 1: want to be officially aligned with conquistadors on this program. No, 113 00:06:38,320 --> 00:06:40,760 Speaker 1: thank you. Well, So a lot of people wrote to 114 00:06:40,920 --> 00:06:43,839 Speaker 1: us asking us to break this down and talk about 115 00:06:43,880 --> 00:06:46,440 Speaker 1: it and see what's real and not real about it. 116 00:06:46,640 --> 00:06:48,560 Speaker 1: So before we dug into it, I went out into 117 00:06:48,640 --> 00:06:50,960 Speaker 1: the Internet and asked random people if they had heard 118 00:06:50,960 --> 00:06:53,200 Speaker 1: about this article and what they thought about it. So, 119 00:06:53,240 --> 00:06:54,920 Speaker 1: before you listen, to these answers. Think about it for 120 00:06:54,960 --> 00:06:58,200 Speaker 1: a second. Have you heard of NASA discovering a parallel universe? 121 00:06:59,000 --> 00:07:02,400 Speaker 1: Here's what people had to say. I have been stuck 122 00:07:03,000 --> 00:07:06,279 Speaker 1: inside due to the coronavirus, so I have been reading 123 00:07:06,320 --> 00:07:09,800 Speaker 1: that much news. Um So, honestly, I don't know the 124 00:07:09,880 --> 00:07:12,360 Speaker 1: answer to that one. I have not heard if if 125 00:07:12,400 --> 00:07:14,960 Speaker 1: they did, that would be amazing. I'm going to say 126 00:07:15,040 --> 00:07:17,960 Speaker 1: no because I think this would be all over the 127 00:07:18,040 --> 00:07:20,960 Speaker 1: news if it happened. And I also don't think we 128 00:07:21,080 --> 00:07:27,440 Speaker 1: have any way to probe another universe. I have no idea. 129 00:07:28,200 --> 00:07:30,920 Speaker 1: What that's a reference to you? I have no idea. 130 00:07:31,320 --> 00:07:35,520 Speaker 1: I sort of doubt it. I have not heard that. Well, no, 131 00:07:38,240 --> 00:07:43,960 Speaker 1: how would you discover a parallel universe? I don't think so. 132 00:07:44,200 --> 00:07:47,640 Speaker 1: I really I really don't think they did, But I'd 133 00:07:47,680 --> 00:07:50,520 Speaker 1: like I hope that they did, because I would really 134 00:07:50,640 --> 00:07:55,720 Speaker 1: love it. From my understanding of multiverse theories, there's nothing 135 00:07:55,840 --> 00:08:00,880 Speaker 1: preventing there from being other universes. It might even be probable. However, 136 00:08:01,000 --> 00:08:04,760 Speaker 1: we don't have a way currently to do an experiment 137 00:08:05,480 --> 00:08:08,080 Speaker 1: to prove it. All right, it seems that not a 138 00:08:08,120 --> 00:08:09,800 Speaker 1: lot of people are on Twitter. Maybe a lot of 139 00:08:09,840 --> 00:08:12,360 Speaker 1: these people were not on Twitter or the Internet, or 140 00:08:12,520 --> 00:08:16,080 Speaker 1: maybe our listeners just read better sources of science news 141 00:08:16,240 --> 00:08:20,440 Speaker 1: than the New Scientists and the Daily Star. Yeah, it 142 00:08:20,520 --> 00:08:25,560 Speaker 1: aren't those like the tabloids of science writing. You know, 143 00:08:25,640 --> 00:08:28,040 Speaker 1: we've talked about the New Scientists in the past. They 144 00:08:28,080 --> 00:08:31,880 Speaker 1: have an article promoting the e M Drive the Impossible Drive, 145 00:08:32,160 --> 00:08:34,719 Speaker 1: which also in that case hyped up the claims of 146 00:08:35,080 --> 00:08:39,040 Speaker 1: some scientists associated with NASA, and I think probably created 147 00:08:39,200 --> 00:08:41,800 Speaker 1: a lot of misunderstanding. So we've been a little harder 148 00:08:41,880 --> 00:08:44,120 Speaker 1: than in the past. They have some great articles. We've 149 00:08:44,240 --> 00:08:46,240 Speaker 1: even been to their show. Remember we did n S 150 00:08:46,320 --> 00:08:48,720 Speaker 1: Live in the UK a couple of years ago. They 151 00:08:48,760 --> 00:08:51,640 Speaker 1: did a lot of great work promoting science, but sometimes 152 00:08:51,720 --> 00:08:53,839 Speaker 1: you know, they need to rein it in. Well. So 153 00:08:54,240 --> 00:08:58,040 Speaker 1: there's this apparently this experiment that is organized and run 154 00:08:58,160 --> 00:09:01,200 Speaker 1: by NASA that apparently did this. There were some interesting things, 155 00:09:01,360 --> 00:09:03,920 Speaker 1: or at least saw some promising things that are related 156 00:09:03,960 --> 00:09:07,559 Speaker 1: to neutrinos. That's right. There really is a super fascinating 157 00:09:07,720 --> 00:09:10,719 Speaker 1: discovery by an experiment on the South Pole that we 158 00:09:10,920 --> 00:09:14,599 Speaker 1: cannot currently explain. And so that's a wonderful opportunity in 159 00:09:14,640 --> 00:09:17,599 Speaker 1: physics to learn something new, and it makes some big discovery, 160 00:09:18,120 --> 00:09:21,319 Speaker 1: and so it's totally worth digging into and understanding how 161 00:09:21,400 --> 00:09:23,920 Speaker 1: it works, what they saw, and what it really could 162 00:09:24,040 --> 00:09:27,440 Speaker 1: mean for physics, whether or not you believe in parallel universes. 163 00:09:27,520 --> 00:09:29,480 Speaker 1: All right, so let's break it down, Daniel. So this 164 00:09:29,600 --> 00:09:32,520 Speaker 1: is a real experiment that's happening in the South Pole 165 00:09:32,679 --> 00:09:36,199 Speaker 1: in an Antarctica, and it's called ANITA, or at least 166 00:09:36,280 --> 00:09:39,319 Speaker 1: the acronym for it is ANITA. Yeah, it's called ANITA. 167 00:09:39,720 --> 00:09:41,680 Speaker 1: And the awesome thing is that it's not actually happening 168 00:09:41,920 --> 00:09:44,800 Speaker 1: in the South Pole, is happening above the South Pole. 169 00:09:45,240 --> 00:09:48,719 Speaker 1: It's a balloon experiment. What you can't be above the 170 00:09:48,800 --> 00:09:52,160 Speaker 1: South Pole, you can only be below the South Pole, Daniel. Okay, 171 00:09:52,679 --> 00:09:55,960 Speaker 1: right right, that's your Northern hemisphere biased speaking right there. Man. 172 00:09:56,320 --> 00:09:59,079 Speaker 1: I'm I'm an upright ist. Yeah. But what does it 173 00:09:59,160 --> 00:10:01,680 Speaker 1: stand for? ANITA A N I T A. I'm gonna 174 00:10:01,720 --> 00:10:10,480 Speaker 1: guess amazing neutrino interferometer trans supporting anions. That's not terrible. 175 00:10:10,559 --> 00:10:16,920 Speaker 1: Actually it stands for Antarctic impulsive transient antend. Oh no, 176 00:10:17,360 --> 00:10:20,440 Speaker 1: did they really cheat on the acronym And the end 177 00:10:20,559 --> 00:10:24,800 Speaker 1: is actually part of Antarctic. I would have gone for 178 00:10:24,880 --> 00:10:27,480 Speaker 1: Aida too. That's a pretty good name. That sounds like 179 00:10:27,559 --> 00:10:29,680 Speaker 1: an opera. Yeah, well this is sort of a science 180 00:10:29,679 --> 00:10:33,079 Speaker 1: opera here going on here because they did discover something 181 00:10:33,080 --> 00:10:35,800 Speaker 1: because they were looking for neutrinos. Yeah, and it's an 182 00:10:35,840 --> 00:10:39,439 Speaker 1: amazing experiment because it hovers above the South Pole's not 183 00:10:39,600 --> 00:10:42,800 Speaker 1: something they built like in a facility at the South Pole. 184 00:10:43,120 --> 00:10:46,920 Speaker 1: It flies on a balloon like forty kilometers above the 185 00:10:47,000 --> 00:10:50,200 Speaker 1: South Pole. Like imagine you're a graduate student. You developed 186 00:10:50,240 --> 00:10:53,640 Speaker 1: this complicated, expensive, delicate piece of electronics and then you 187 00:10:53,720 --> 00:10:55,800 Speaker 1: attach it to a balloon and just send it up 188 00:10:55,840 --> 00:10:59,320 Speaker 1: into the sky. Well again, I should correct, it's floating 189 00:10:59,559 --> 00:11:03,719 Speaker 1: below a southpool. Thank you for keeping me honest. I 190 00:11:03,840 --> 00:11:07,839 Speaker 1: really appreciate the fact checking me straight here. And and 191 00:11:08,080 --> 00:11:10,199 Speaker 1: also science on a balloon, I mean, how fun is that? 192 00:11:10,440 --> 00:11:12,160 Speaker 1: It's pretty cool. Yeah, but you know, if you're a 193 00:11:12,240 --> 00:11:14,360 Speaker 1: graduate student and you spend years building this thing and 194 00:11:14,400 --> 00:11:17,240 Speaker 1: then it just crashes, like you're out of luck. So 195 00:11:17,480 --> 00:11:20,520 Speaker 1: it's pretty risky. But it's an awesome experiment. And this 196 00:11:20,720 --> 00:11:23,120 Speaker 1: is an experiment that's trying to understand one of the 197 00:11:23,280 --> 00:11:27,120 Speaker 1: big mysteries of astro particle physics, which is basically like 198 00:11:27,640 --> 00:11:32,160 Speaker 1: who is shooting crazy high energy particles at us from space. Right. 199 00:11:32,200 --> 00:11:34,920 Speaker 1: We've covered this before in our podcast, And the Earth 200 00:11:35,040 --> 00:11:38,360 Speaker 1: is getting pelted by cosmic super high energy costmic grace 201 00:11:38,400 --> 00:11:40,240 Speaker 1: and we don't know where they're coming from. They're too 202 00:11:40,679 --> 00:11:42,560 Speaker 1: high energy to be coming from the Sun. That's right, 203 00:11:42,600 --> 00:11:45,120 Speaker 1: they're definitely not coming from the Sun. We don't see 204 00:11:45,160 --> 00:11:47,200 Speaker 1: any point source in the sky. We can look around 205 00:11:47,240 --> 00:11:49,240 Speaker 1: to see where they're coming from, and we don't see 206 00:11:49,280 --> 00:11:53,160 Speaker 1: them coming from just one spot. And they're ridiculously high energy. 207 00:11:53,559 --> 00:11:55,959 Speaker 1: Nothing we know of in the universe is capable of 208 00:11:56,080 --> 00:11:59,040 Speaker 1: making particles of this high energy, and yet we see them. 209 00:11:59,120 --> 00:12:02,319 Speaker 1: So it's all really a great opportunity to learn something new. 210 00:12:03,080 --> 00:12:05,480 Speaker 1: And the interesting thing is like where are they coming from? 211 00:12:06,040 --> 00:12:09,080 Speaker 1: And these particles can be protons, that can be iron, 212 00:12:09,200 --> 00:12:12,120 Speaker 1: nuclear actially, all sorts of crazy things. But one really 213 00:12:12,200 --> 00:12:15,719 Speaker 1: cool idea is to look for really high energy neutrinos. 214 00:12:16,120 --> 00:12:19,439 Speaker 1: There's Neutrinos are these really weird, little whispy particles that 215 00:12:19,520 --> 00:12:22,840 Speaker 1: have no electric charge and hardly interact, and they're really 216 00:12:22,880 --> 00:12:25,160 Speaker 1: good for doing this kind of physics because it means 217 00:12:25,200 --> 00:12:27,400 Speaker 1: they point right back to what made them. They don't 218 00:12:27,480 --> 00:12:30,439 Speaker 1: bend at all in magnetic fields, and so neutrinos are 219 00:12:30,640 --> 00:12:32,760 Speaker 1: part of the cosmic rays that are hitting us. It's 220 00:12:32,800 --> 00:12:36,040 Speaker 1: not just like protons and and course and stuff being 221 00:12:36,200 --> 00:12:39,280 Speaker 1: sent as is whatever it's making these is also sathing neutrinos. Well, 222 00:12:39,320 --> 00:12:42,320 Speaker 1: that's the question, is are we seeing also super high 223 00:12:42,480 --> 00:12:45,920 Speaker 1: energy neutrinos. If so, that might give us another clue 224 00:12:46,040 --> 00:12:48,120 Speaker 1: to tell us, like what could be out there creating 225 00:12:48,160 --> 00:12:52,079 Speaker 1: these things? Is there an alien particle physics factory pumping 226 00:12:52,120 --> 00:12:55,360 Speaker 1: out high energy particles? Are the only making protons? Gives 227 00:12:55,400 --> 00:12:58,480 Speaker 1: a sunburned or something? We would be their motivation? Well, 228 00:12:58,520 --> 00:13:01,320 Speaker 1: who knows what I do understand aliens? I certainly don't. 229 00:13:01,640 --> 00:13:03,360 Speaker 1: But every time you look at the sky, you want 230 00:13:03,400 --> 00:13:05,439 Speaker 1: to look at it in lots of different spectrum. You 231 00:13:05,480 --> 00:13:06,920 Speaker 1: want to see what are the X ray, what is 232 00:13:06,960 --> 00:13:09,520 Speaker 1: the visible light, what is the infrared? So this is 233 00:13:09,520 --> 00:13:11,800 Speaker 1: in the same category. It says, let's look at the 234 00:13:11,880 --> 00:13:15,439 Speaker 1: cosmic ray sky using neutrinos because they don't bend, and 235 00:13:15,520 --> 00:13:17,079 Speaker 1: it's like another way to look at But I guess 236 00:13:17,120 --> 00:13:19,360 Speaker 1: we're also getting showered by neutrinos from the sun, Like 237 00:13:19,440 --> 00:13:21,640 Speaker 1: the Sun produces a lot of neutrinos and we're getting 238 00:13:21,840 --> 00:13:23,880 Speaker 1: hit by a ton of them here. We're looking for 239 00:13:23,920 --> 00:13:26,200 Speaker 1: them coming from a different direction or something. That's right. 240 00:13:26,280 --> 00:13:29,160 Speaker 1: The Sun pumps out huge numbers of neutrinos, like you're 241 00:13:29,240 --> 00:13:33,280 Speaker 1: hit with a hundred billion neutrinos per square centimeter per 242 00:13:33,440 --> 00:13:37,000 Speaker 1: second all the time. So it's an incredible number. But 243 00:13:37,160 --> 00:13:39,079 Speaker 1: those come from the Sun, and we can tell the 244 00:13:39,200 --> 00:13:42,200 Speaker 1: direction of these particles. So we're looking like out into 245 00:13:42,240 --> 00:13:44,599 Speaker 1: space to see if they're coming from anywhere else. And 246 00:13:44,840 --> 00:13:47,040 Speaker 1: the ones from the Sun are not nearly as high 247 00:13:47,160 --> 00:13:49,280 Speaker 1: energy as the one that we're looking for. We're looking 248 00:13:49,360 --> 00:13:53,320 Speaker 1: for super duper high energy neutrinos, not just the ones 249 00:13:53,400 --> 00:13:55,160 Speaker 1: coming from the Sun. Oh I see. So that it 250 00:13:55,360 --> 00:13:58,360 Speaker 1: is that if something is making high energy particles and 251 00:13:58,440 --> 00:14:02,600 Speaker 1: shooting them at us, there maybe probably also shooting neutrinos 252 00:14:02,600 --> 00:14:05,240 Speaker 1: along the way, and if so, they would have the 253 00:14:05,360 --> 00:14:08,200 Speaker 1: same sort of high energy and also maybe would preserve 254 00:14:08,240 --> 00:14:10,760 Speaker 1: the direction. That's right, And that's the question. Whatever is 255 00:14:10,800 --> 00:14:13,840 Speaker 1: this mysterious source of cosmic rays? Is it also making 256 00:14:13,960 --> 00:14:19,560 Speaker 1: super high energy neutrinos? Let's look and and you never know. Right, Wow, 257 00:14:19,960 --> 00:14:22,000 Speaker 1: that's a big question. It is a big question. Yeah, 258 00:14:22,800 --> 00:14:25,200 Speaker 1: it seems like a small question for which you would 259 00:14:25,240 --> 00:14:27,880 Speaker 1: need a lot of the quiment to measure. And you know, 260 00:14:27,920 --> 00:14:30,440 Speaker 1: there's a history of discovery there, like when people first 261 00:14:30,520 --> 00:14:33,200 Speaker 1: looked at the sky in the X ray, they found 262 00:14:33,240 --> 00:14:35,400 Speaker 1: all sorts of things that were really bright in X 263 00:14:35,520 --> 00:14:39,080 Speaker 1: rays but dark invisible light, Like the first black hole 264 00:14:39,200 --> 00:14:41,000 Speaker 1: was spotted that way. We should do a whole podcast 265 00:14:41,000 --> 00:14:43,520 Speaker 1: episode on that. So you might see in the sky 266 00:14:43,680 --> 00:14:46,440 Speaker 1: in neutrinos really bright sources that don't line up with 267 00:14:46,560 --> 00:14:48,480 Speaker 1: anything else, and that could be a clue. So like, oh, 268 00:14:48,560 --> 00:14:51,040 Speaker 1: there's a new thing in the universe. So it's always 269 00:14:51,080 --> 00:14:53,560 Speaker 1: exciting to look out in the universe using a new 270 00:14:53,680 --> 00:14:55,840 Speaker 1: set of eyeballs, all right, So then this they set 271 00:14:55,920 --> 00:14:58,960 Speaker 1: up this experiment in Antarctica that uses a balloon and 272 00:14:59,040 --> 00:15:02,320 Speaker 1: it uses the eye from Antarctica. Right, that's why you 273 00:15:02,360 --> 00:15:03,920 Speaker 1: need the balloon to sort of look at all the ice. 274 00:15:04,040 --> 00:15:06,640 Speaker 1: That's right, because neutrinos are really hard to spot, right, 275 00:15:06,680 --> 00:15:09,360 Speaker 1: They fly through a lot of material and don't interact, 276 00:15:09,920 --> 00:15:12,520 Speaker 1: and so essentially we use the whole earth and the 277 00:15:12,640 --> 00:15:16,000 Speaker 1: ice in Antarctica as our detector. And one thing that's 278 00:15:16,000 --> 00:15:18,200 Speaker 1: really important to understand is you may have heard of 279 00:15:18,280 --> 00:15:20,840 Speaker 1: neutrinos flying through like a light year of lead and 280 00:15:20,920 --> 00:15:24,720 Speaker 1: not interacting. That's true for neutrinos from the Sun at 281 00:15:24,720 --> 00:15:27,200 Speaker 1: a certain energy, but as neutrinos get the higher and 282 00:15:27,320 --> 00:15:30,280 Speaker 1: higher energy, they tend to interact more. And we can 283 00:15:30,360 --> 00:15:32,840 Speaker 1: dig into why that is a little bit later. But 284 00:15:32,960 --> 00:15:36,160 Speaker 1: what these things are looking for is neutrinos flying through 285 00:15:36,280 --> 00:15:40,400 Speaker 1: the Earth, so upwards through the Earth. I guess downwards, right, 286 00:15:40,440 --> 00:15:42,600 Speaker 1: since we're on the North Pole. I am so upside 287 00:15:42,600 --> 00:15:44,960 Speaker 1: down here. But they're they're coming from the Sun through 288 00:15:44,960 --> 00:15:47,480 Speaker 1: the Earth, and they're popping out of Antarctica. They're not 289 00:15:47,600 --> 00:15:49,840 Speaker 1: coming from the Sun. They're coming from somewhere else, somewhere 290 00:15:50,040 --> 00:15:52,920 Speaker 1: in space. They go through the Earth and they go 291 00:15:53,120 --> 00:15:55,720 Speaker 1: through the ice and Antarctica, and when they go through 292 00:15:55,760 --> 00:15:58,040 Speaker 1: the ice, which is like one or two kilometers thick, 293 00:15:58,320 --> 00:16:02,480 Speaker 1: they make a chirp in radio frequency electromagnetic waves because 294 00:16:02,520 --> 00:16:06,000 Speaker 1: they hit something and then they split up. That's right, 295 00:16:06,200 --> 00:16:08,840 Speaker 1: they hit something, they interact with the nucleus and then 296 00:16:08,920 --> 00:16:12,320 Speaker 1: it causes this cascade of electrons and positrons which make 297 00:16:12,400 --> 00:16:16,040 Speaker 1: this a little brief, essentially chirp in the radio frequency spectrum. 298 00:16:16,360 --> 00:16:18,360 Speaker 1: And the reason that ice is important is that ice 299 00:16:18,520 --> 00:16:20,880 Speaker 1: is transparent, Like if you make this chirp in the ice, 300 00:16:21,240 --> 00:16:23,560 Speaker 1: it will propagate through the ice and then you can 301 00:16:23,640 --> 00:16:26,560 Speaker 1: see it above the ice. If it makes this chirp 302 00:16:26,680 --> 00:16:29,520 Speaker 1: like in deep rock, then it just gets absorbed. So 303 00:16:29,640 --> 00:16:32,080 Speaker 1: you needed a big slab of something which will make 304 00:16:32,120 --> 00:16:36,840 Speaker 1: it chirp and also propagate those chirps. So you thought Antarctica, 305 00:16:37,400 --> 00:16:39,560 Speaker 1: there's a lot of ice there, better use it before 306 00:16:39,560 --> 00:16:42,120 Speaker 1: it goes away. Yeah, exactly, Like where else can you 307 00:16:42,240 --> 00:16:46,680 Speaker 1: get a one mile thick sheet of ice. It's pretty incredible. 308 00:16:47,280 --> 00:16:49,880 Speaker 1: And so then they look for these chirps. But you know, 309 00:16:49,880 --> 00:16:51,480 Speaker 1: if you just put a detector on the surface and 310 00:16:51,560 --> 00:16:53,560 Speaker 1: look down, you can only see a tiny little bit 311 00:16:53,640 --> 00:16:56,640 Speaker 1: of ice. So the higher you are, the more ice 312 00:16:56,760 --> 00:16:59,280 Speaker 1: you can visualize. So that's why they put this thing 313 00:16:59,360 --> 00:17:03,240 Speaker 1: on a balloon and fly like forts above the ice 314 00:17:03,840 --> 00:17:06,479 Speaker 1: looking for these signals coming out of the ice from 315 00:17:06,520 --> 00:17:09,600 Speaker 1: neutrinos that are flying through the earth and coming out 316 00:17:09,840 --> 00:17:12,440 Speaker 1: through the end. Okay, so then really what's on the 317 00:17:12,440 --> 00:17:14,320 Speaker 1: balloon is just kind of a camera, So it's just 318 00:17:14,400 --> 00:17:17,440 Speaker 1: taking pictures of the ice looking for these neutrino collisions. 319 00:17:17,480 --> 00:17:19,720 Speaker 1: That's right, And it's a special kind of camera. You know, 320 00:17:19,800 --> 00:17:23,040 Speaker 1: there really are radio frequency antennas, and that's why the 321 00:17:23,119 --> 00:17:27,080 Speaker 1: experiment is called transient antenna. Transient because it's not up 322 00:17:27,080 --> 00:17:30,040 Speaker 1: there all the time, and they're looking also transient because 323 00:17:30,080 --> 00:17:32,760 Speaker 1: the signals are transient, and because they're using an antenna 324 00:17:32,840 --> 00:17:34,200 Speaker 1: as a form of a camera. You know, they have 325 00:17:34,240 --> 00:17:36,199 Speaker 1: a bunch of these antennas, so they can essentially take 326 00:17:36,240 --> 00:17:40,639 Speaker 1: a picture of the ice in this radio frequency spectrum. Cool. 327 00:17:40,760 --> 00:17:43,440 Speaker 1: All right, Well let's get a little bit into what 328 00:17:43,800 --> 00:17:46,720 Speaker 1: the experiment is actually looking for and how it's looking 329 00:17:46,800 --> 00:17:50,480 Speaker 1: for it, and whether or not they discovered a parallel universe. 330 00:17:50,840 --> 00:18:05,760 Speaker 1: But first let's take a quick break. All right, Daniel, 331 00:18:05,800 --> 00:18:08,879 Speaker 1: we're talking about whether NASA discovered a parallel universe, is 332 00:18:08,960 --> 00:18:13,720 Speaker 1: headlines recently seemed to say out loud, And so it 333 00:18:13,880 --> 00:18:16,240 Speaker 1: just has to do with the experiment called Anita. That's 334 00:18:16,280 --> 00:18:19,480 Speaker 1: a balloon floating above the Antarctic taking pictures of the 335 00:18:19,640 --> 00:18:23,760 Speaker 1: ice looking for neutrinos hi, not just neutrinos, high energy 336 00:18:23,800 --> 00:18:26,639 Speaker 1: neutrina that's right. And they've been running this thing for 337 00:18:27,080 --> 00:18:29,879 Speaker 1: almost a couple of decades now. Like they build it, 338 00:18:30,160 --> 00:18:32,639 Speaker 1: they launch it, it flies up there for like thirty 339 00:18:32,720 --> 00:18:35,880 Speaker 1: to forty days essentially until it runs out of helium 340 00:18:36,359 --> 00:18:38,560 Speaker 1: and then it comes back down. Really, it's been going 341 00:18:38,640 --> 00:18:40,680 Speaker 1: for several decades. Yeah, well they have that, you know, 342 00:18:40,760 --> 00:18:43,199 Speaker 1: they need to rebuild it every time. So they had 343 00:18:43,240 --> 00:18:44,760 Speaker 1: a run in two thousand and six, and then had 344 00:18:44,760 --> 00:18:47,080 Speaker 1: another run in two thousand nine, and they did one 345 00:18:47,080 --> 00:18:49,520 Speaker 1: in two thousand fourteen. What do you what do you 346 00:18:49,560 --> 00:18:51,399 Speaker 1: mean the balloon doesn't last? No, you can't have a 347 00:18:51,440 --> 00:18:53,840 Speaker 1: balloon up there forever. Eventually the helium leaks out and 348 00:18:53,840 --> 00:18:56,760 Speaker 1: the thing comes back down to Earth. But eventually the 349 00:18:56,800 --> 00:18:59,520 Speaker 1: balloon comes down and it runs for a long time. 350 00:18:59,560 --> 00:19:02,080 Speaker 1: It runs on solar power. That hangs up there for 351 00:19:02,160 --> 00:19:05,520 Speaker 1: like thirty or forty days collecting data. All Right, they're 352 00:19:05,560 --> 00:19:07,320 Speaker 1: up there. They're taking pictures of the ice and they're 353 00:19:07,320 --> 00:19:11,040 Speaker 1: looking for high energy neutrino collisions. So I guess, let's 354 00:19:11,080 --> 00:19:13,760 Speaker 1: maybe dig a little bit into the signs. And so, 355 00:19:14,000 --> 00:19:16,760 Speaker 1: why are neutrinos more likely to hit things if they're 356 00:19:16,760 --> 00:19:19,720 Speaker 1: going faster. It seems like it should be the opposite. Yeah, 357 00:19:19,800 --> 00:19:22,800 Speaker 1: So what they're looking for a really high energy neutrinos, right, 358 00:19:23,119 --> 00:19:25,080 Speaker 1: And they saw something really weird is that they saw 359 00:19:25,320 --> 00:19:28,159 Speaker 1: neutrinos that are super duper high energy. And these are 360 00:19:28,280 --> 00:19:31,639 Speaker 1: fascinating because, as you say, they're actually more likely to 361 00:19:31,760 --> 00:19:35,920 Speaker 1: stop and being into something than slower neutrinos. And the 362 00:19:36,000 --> 00:19:40,280 Speaker 1: reason is special relativity. Like remember that when you move quickly, 363 00:19:40,640 --> 00:19:43,760 Speaker 1: things in your view tend to look shorter. Like if 364 00:19:43,800 --> 00:19:46,880 Speaker 1: you're running past your house and nearly the speed of light, 365 00:19:47,240 --> 00:19:51,520 Speaker 1: there's length contraction. Your house seems to get shorter. What wait, 366 00:19:51,680 --> 00:19:56,200 Speaker 1: so to to the neutrino, the universe sort of contracts. 367 00:19:56,400 --> 00:19:59,640 Speaker 1: Everything feels smaller, yes, or like closer. That's right, because 368 00:19:59,760 --> 00:20:03,239 Speaker 1: for very fast moving neutrino, the universe is rushing by 369 00:20:03,280 --> 00:20:06,720 Speaker 1: at a fast speed, so the universe contracts and effectively 370 00:20:06,800 --> 00:20:10,399 Speaker 1: gets denser. So it's like the neutrino sees more of 371 00:20:10,480 --> 00:20:13,600 Speaker 1: the universe or more of the material it's passing through 372 00:20:13,720 --> 00:20:16,320 Speaker 1: at any given moment, which means it has like more 373 00:20:16,520 --> 00:20:22,320 Speaker 1: chances to interact with some Oh man, that makes no sense, 374 00:20:22,400 --> 00:20:25,960 Speaker 1: Daniel to us. Then neutrino, it's just moving fast, you 375 00:20:26,040 --> 00:20:27,840 Speaker 1: know what I mean, Like it's not actually going through 376 00:20:27,880 --> 00:20:30,359 Speaker 1: more stuff, that's right, But we're talking about the range 377 00:20:30,400 --> 00:20:33,720 Speaker 1: of its potential interaction. Remember going through stuff and banging 378 00:20:33,800 --> 00:20:36,800 Speaker 1: into it. Really, we're not talking about like physically stuff 379 00:20:36,840 --> 00:20:40,479 Speaker 1: connecting and hitting. We're talking about things interacting. It's all 380 00:20:40,480 --> 00:20:43,600 Speaker 1: about the power of your forces. Are you being influenced 381 00:20:43,840 --> 00:20:46,359 Speaker 1: by the gravity of the Sun. Yes. Are you being 382 00:20:46,400 --> 00:20:49,840 Speaker 1: influenced by the gravity of Alpha Centauri? Probably not a 383 00:20:49,920 --> 00:20:52,520 Speaker 1: little bit. But if you were moving really really fast, 384 00:20:52,880 --> 00:20:55,359 Speaker 1: then you would be influenced by things even further away 385 00:20:55,400 --> 00:20:58,280 Speaker 1: because it would be effectively contracted to be closer to you. 386 00:20:58,520 --> 00:21:00,520 Speaker 1: What if I was moving to or it's the Sun, 387 00:21:00,560 --> 00:21:03,400 Speaker 1: I would feel it's gravity more. Yes, absolutely, because space 388 00:21:03,440 --> 00:21:07,119 Speaker 1: would be contracted between you and the Sun. All right, 389 00:21:07,160 --> 00:21:09,960 Speaker 1: I don't I don't recommend it. I kind of have 390 00:21:10,000 --> 00:21:12,239 Speaker 1: to take your word for a Daniel. It seems kind 391 00:21:12,280 --> 00:21:14,920 Speaker 1: of bonkers, But you're it's going really fast, so it 392 00:21:15,040 --> 00:21:18,560 Speaker 1: seemed more of the universe. The universe seems denser, and 393 00:21:18,680 --> 00:21:21,439 Speaker 1: so it's interacting more. It's more likely to interact, that's right. 394 00:21:21,480 --> 00:21:23,920 Speaker 1: And so a slow moving neutrino like when that comes 395 00:21:23,960 --> 00:21:26,000 Speaker 1: from the Sun will pass through the Earth and have 396 00:21:26,280 --> 00:21:30,000 Speaker 1: almost no chance of interacting. But a faster moving neutrino, 397 00:21:30,160 --> 00:21:33,840 Speaker 1: like a really really high energy neutrino, is very unlikely 398 00:21:33,960 --> 00:21:36,280 Speaker 1: to make it all the way through the Earth. So 399 00:21:36,359 --> 00:21:39,200 Speaker 1: if neutrino comes to the Earth and hits the North Pole, 400 00:21:39,480 --> 00:21:42,800 Speaker 1: then start traveling through the very very high energies, it's 401 00:21:42,840 --> 00:21:44,399 Speaker 1: unlikely to make it all the way through. It's going 402 00:21:44,440 --> 00:21:46,320 Speaker 1: to bang into something and the core of the Earth 403 00:21:46,560 --> 00:21:49,520 Speaker 1: and get absorbed and stop. Most of them will probably 404 00:21:49,520 --> 00:21:51,440 Speaker 1: get absorbed by the Earth, but some of them will 405 00:21:51,480 --> 00:21:54,239 Speaker 1: make it through and hit the ice in Antarctica. That's right. 406 00:21:54,280 --> 00:21:56,200 Speaker 1: And so what this experiment was designed to look for 407 00:21:56,400 --> 00:21:58,600 Speaker 1: is actually not neutrino is going all the way through 408 00:21:58,640 --> 00:22:01,199 Speaker 1: the Earth, but just sort of skimming it a little bit. 409 00:22:01,520 --> 00:22:04,280 Speaker 1: They knew that they couldn't see neutrinos a very high 410 00:22:04,400 --> 00:22:06,040 Speaker 1: energy to go all the way through the Earth because 411 00:22:06,040 --> 00:22:08,520 Speaker 1: they shouldn't make it through the Earth. So they're expecting 412 00:22:08,560 --> 00:22:10,760 Speaker 1: to sort of skim the horizon and see neutrinos that 413 00:22:10,840 --> 00:22:12,600 Speaker 1: just sort of like dip into the Earth a little 414 00:22:12,640 --> 00:22:14,760 Speaker 1: bit and then come up through the ice. That was 415 00:22:14,840 --> 00:22:17,240 Speaker 1: their goal. Oh, that just kind of hit the edge 416 00:22:17,280 --> 00:22:19,879 Speaker 1: of the Earth at the north pole. Yeah, precisely at 417 00:22:19,920 --> 00:22:22,399 Speaker 1: the South pole, and that makes the ice, I mean thicker, right, 418 00:22:22,400 --> 00:22:24,400 Speaker 1: because it's like if you hit the sheet of ice sideways, 419 00:22:24,440 --> 00:22:26,480 Speaker 1: it's it's a lot thicker, you've got a longer view 420 00:22:26,520 --> 00:22:28,639 Speaker 1: of the ice. So they were that's what they were 421 00:22:28,680 --> 00:22:30,640 Speaker 1: expecting to see. That's what they were hoping to see. 422 00:22:30,880 --> 00:22:33,600 Speaker 1: That's what they were designed to see. And weirdly, they 423 00:22:33,680 --> 00:22:36,119 Speaker 1: don't see any of those. Like they've been running for 424 00:22:36,200 --> 00:22:39,680 Speaker 1: a long time, they've never seen a single high energy 425 00:22:39,760 --> 00:22:43,560 Speaker 1: neutrino passing near the horizon. They're like just coming up 426 00:22:43,600 --> 00:22:45,520 Speaker 1: through the Earth in the way they would expect to 427 00:22:45,600 --> 00:22:48,480 Speaker 1: see them if there were these very high energy neutrinos 428 00:22:48,600 --> 00:22:50,800 Speaker 1: flying through space. Right, So I'm trying to picture it. 429 00:22:50,880 --> 00:22:54,200 Speaker 1: The ne trino's coming kind of at an angle. It's 430 00:22:54,200 --> 00:22:56,880 Speaker 1: skimming the Earth. It hits the ice, it cream makes 431 00:22:56,920 --> 00:23:00,720 Speaker 1: an interaction and it's braced some other stuff in all directions, 432 00:23:00,880 --> 00:23:04,760 Speaker 1: make an interaction, and its sprays radio frequency light. Essentially, 433 00:23:04,880 --> 00:23:08,240 Speaker 1: the sprays a little burst of radio frequency noise out 434 00:23:08,280 --> 00:23:10,600 Speaker 1: through the ice, which is then picked up in the 435 00:23:10,760 --> 00:23:14,360 Speaker 1: air by the ANITA antenna like it creates photons. Yeah, 436 00:23:14,480 --> 00:23:18,720 Speaker 1: radio waves are photons, that's right, and then it explodes 437 00:23:18,760 --> 00:23:21,160 Speaker 1: like it they come off in all directions. Now, because 438 00:23:21,200 --> 00:23:24,320 Speaker 1: the neutrino is moving really fast, it's actually collimated, so 439 00:23:24,359 --> 00:23:26,920 Speaker 1: it's a very narrow tube. And so you can tell 440 00:23:27,000 --> 00:23:30,399 Speaker 1: the direction of the neutrino by seeing where this arrived 441 00:23:30,440 --> 00:23:33,520 Speaker 1: and exactly when. And Anita has like lots of different antennas, 442 00:23:33,560 --> 00:23:36,760 Speaker 1: and so by the different arrival times on different parts 443 00:23:36,800 --> 00:23:39,679 Speaker 1: of Anita, they can tell the direction that this pulse 444 00:23:40,000 --> 00:23:42,920 Speaker 1: of radio waves from the neutrino came from. Okay, so 445 00:23:43,080 --> 00:23:45,560 Speaker 1: then that's how you would see them, But they didn't 446 00:23:45,560 --> 00:23:47,879 Speaker 1: see them for years and years and years. Yeah, that's right. 447 00:23:48,160 --> 00:23:50,280 Speaker 1: They look at the horizon, they look for these neutrinos 448 00:23:50,320 --> 00:23:53,200 Speaker 1: skimming the horizon, and they see nothing, not a zilch 449 00:23:53,320 --> 00:23:57,280 Speaker 1: in all of their runs. But they did see something 450 00:23:57,400 --> 00:24:00,920 Speaker 1: really weird that they didn't expect to see. Okay, recently 451 00:24:01,080 --> 00:24:03,080 Speaker 1: or was this a way back in its early runs, 452 00:24:03,160 --> 00:24:05,240 Speaker 1: So in two thousand and six and then again in 453 00:24:05,320 --> 00:24:08,560 Speaker 1: two thousand fourteen, so now twice in the total runs 454 00:24:08,600 --> 00:24:11,399 Speaker 1: of this experiment, they saw neutrinos or what looks like 455 00:24:11,520 --> 00:24:15,680 Speaker 1: neutrinos coming straight up through the Earth. So something that 456 00:24:15,720 --> 00:24:18,239 Speaker 1: shouldn't happen, because neutrinos shouldn't make it all the way 457 00:24:18,280 --> 00:24:21,640 Speaker 1: through the Earth. But they see these pulses that look 458 00:24:21,760 --> 00:24:26,080 Speaker 1: like very very fast moving neutrino, ridiculously high energy neutrino, 459 00:24:26,320 --> 00:24:29,040 Speaker 1: but coming straight up out of the ice. Wow, So 460 00:24:29,119 --> 00:24:32,320 Speaker 1: it's sort of coming from the Earth or through the Earth. Well, 461 00:24:32,400 --> 00:24:35,240 Speaker 1: we don't know, right if it's a neutrino, it's hard 462 00:24:35,280 --> 00:24:38,600 Speaker 1: to understand how it could be coming through the Earth, right, Like, 463 00:24:38,960 --> 00:24:41,880 Speaker 1: because neutrinos at that high energy, and we're talking about 464 00:24:42,000 --> 00:24:45,440 Speaker 1: energies much much higher than like the particles at the 465 00:24:45,520 --> 00:24:48,680 Speaker 1: Large Hadron Collider, right We're talking about seventy or a 466 00:24:48,800 --> 00:24:52,600 Speaker 1: hundred thousand times more energy. These are really really high 467 00:24:52,680 --> 00:24:54,920 Speaker 1: energy particles. But they shouldn't make it through the Earth. 468 00:24:55,000 --> 00:24:58,360 Speaker 1: So maybe they're created inside the Earth, or maybe there's 469 00:24:58,400 --> 00:25:01,080 Speaker 1: something else, some other weird kind of particle that turns 470 00:25:01,119 --> 00:25:03,359 Speaker 1: into neutrinos. And we can dig into all of that. 471 00:25:03,520 --> 00:25:05,760 Speaker 1: But I guess maybe couldn't it just be a neutrino 472 00:25:05,840 --> 00:25:08,720 Speaker 1: that got lucky, you know, Like, couldn't it just be 473 00:25:09,080 --> 00:25:11,760 Speaker 1: um one that did somehow make it through the Earth. Yeah, 474 00:25:11,800 --> 00:25:15,600 Speaker 1: it could certainly be. Like one explanation is there's some 475 00:25:15,880 --> 00:25:19,199 Speaker 1: source of very high energy new trinos and it's shooting 476 00:25:19,240 --> 00:25:21,040 Speaker 1: it right in that direction, and you have a lot 477 00:25:21,119 --> 00:25:23,640 Speaker 1: of them, and so even if the chances are low, 478 00:25:23,840 --> 00:25:26,119 Speaker 1: maybe one of them leaked through or two of them 479 00:25:26,280 --> 00:25:28,800 Speaker 1: leaked through and then hit the ice right and then 480 00:25:28,920 --> 00:25:31,280 Speaker 1: hit the ice. And so we have other detectors out 481 00:25:31,280 --> 00:25:33,959 Speaker 1: the South Pole that do similar things, like this one 482 00:25:34,040 --> 00:25:39,760 Speaker 1: called ice cube, which actually seriously like the wrapper, did 483 00:25:39,840 --> 00:25:42,399 Speaker 1: he sign off on this um? I have not been 484 00:25:42,400 --> 00:25:45,199 Speaker 1: in touch with these people, but ice cube, I think 485 00:25:45,240 --> 00:25:49,400 Speaker 1: it's a general phrase. And they've drilled into the ice 486 00:25:49,440 --> 00:25:52,240 Speaker 1: and they dropped cameras into the ice. They've like instrumented 487 00:25:52,320 --> 00:25:55,400 Speaker 1: the ice itself to look for particles coming through the ice. 488 00:25:55,800 --> 00:25:59,040 Speaker 1: So they have sort of similar capabilities, and they didn't 489 00:25:59,040 --> 00:26:01,399 Speaker 1: see these things. So you would expect if there was 490 00:26:01,440 --> 00:26:04,800 Speaker 1: like a really high energy source of neutrinos pointed at 491 00:26:04,840 --> 00:26:07,359 Speaker 1: the Earth that happened to be going all the way through, 492 00:26:07,880 --> 00:26:10,399 Speaker 1: that this other experiment, ice Cube, would have seen them. 493 00:26:10,440 --> 00:26:13,080 Speaker 1: But it doesn't really. I mean, I mean two over 494 00:26:13,200 --> 00:26:15,560 Speaker 1: like twenty years, it seems like these are pretty rare, 495 00:26:15,760 --> 00:26:17,800 Speaker 1: So it could still it could maybe still be that 496 00:26:17,960 --> 00:26:19,960 Speaker 1: it's just super rare. The other ones that haven't seen it, 497 00:26:20,040 --> 00:26:22,240 Speaker 1: it could still be. I mean, cosmic ray physics is 498 00:26:22,240 --> 00:26:25,240 Speaker 1: all about small numbers, like These things are very rare 499 00:26:25,400 --> 00:26:28,200 Speaker 1: and very weird, but that's what makes them fascinating. And 500 00:26:28,280 --> 00:26:30,720 Speaker 1: if you've only ever seen one, you'd be pretty skeptical. 501 00:26:30,840 --> 00:26:33,480 Speaker 1: But seeing two man that tells you this something real there. 502 00:26:33,640 --> 00:26:36,879 Speaker 1: You know, it's like seeing two big Foot or big feet. 503 00:26:36,920 --> 00:26:40,399 Speaker 1: I guess that's you believe it a lot more easily 504 00:26:40,480 --> 00:26:43,119 Speaker 1: than just seeing one. All right, it's like two people. 505 00:26:43,240 --> 00:26:47,240 Speaker 1: It's like seeing Bigfoot twice, like taking two photographs of 506 00:26:47,480 --> 00:26:50,560 Speaker 1: her over like twenty years. Yeah, except you know, you 507 00:26:50,600 --> 00:26:52,720 Speaker 1: were out there looking for something else. You were trying 508 00:26:52,760 --> 00:26:55,320 Speaker 1: to take pictures of chimpanzees, and you saw Bigfoot twice, 509 00:26:55,440 --> 00:26:58,320 Speaker 1: so you're like, what what's going on here? Isn't even 510 00:26:58,400 --> 00:27:01,640 Speaker 1: what could be something? All right? Well, that's what they found. 511 00:27:01,680 --> 00:27:04,040 Speaker 1: They found these two. So it's just two nutrinos that 512 00:27:04,119 --> 00:27:06,760 Speaker 1: they found. It's just these two chirps from the ice 513 00:27:06,880 --> 00:27:09,520 Speaker 1: that they think are neutrinos. They look like neutrinos and 514 00:27:09,560 --> 00:27:12,520 Speaker 1: they're coming up straight up from the ice. And that's 515 00:27:12,560 --> 00:27:15,199 Speaker 1: the data. That's what they've seen, and they can't explain 516 00:27:15,280 --> 00:27:18,239 Speaker 1: it using current physics. Captured by a balloon, captured by 517 00:27:18,280 --> 00:27:21,680 Speaker 1: a balloon. That's that seems like the was a bonkers 518 00:27:21,720 --> 00:27:24,119 Speaker 1: part of it. It's sort of Victorian, right. I imagine, 519 00:27:24,160 --> 00:27:27,679 Speaker 1: like you know, steam pumping and mechanical knobs and valves 520 00:27:27,720 --> 00:27:30,000 Speaker 1: and stuff. Some woman with a big hat and a 521 00:27:30,119 --> 00:27:33,639 Speaker 1: guy with a big mustache up there taking nutrito measurements. 522 00:27:33,680 --> 00:27:36,000 Speaker 1: Hope they packed a picnic. Yeah, all right, Well, let's 523 00:27:36,040 --> 00:27:39,320 Speaker 1: get into whether or not they actually discovered a parallel 524 00:27:39,520 --> 00:27:42,680 Speaker 1: universe and what makes them think that they did. But 525 00:27:42,880 --> 00:27:59,680 Speaker 1: first let's take at another quick break. All right, dinnel, 526 00:27:59,840 --> 00:28:03,320 Speaker 1: we're talking about the Anita experiment, which found two over 527 00:28:03,440 --> 00:28:07,040 Speaker 1: twenty years, they found two neutrinos, and so help me 528 00:28:07,119 --> 00:28:09,920 Speaker 1: make the connection here. How do these two neutrinos tell 529 00:28:10,000 --> 00:28:13,160 Speaker 1: me there's a whole parallel universe out there? All right, Well, 530 00:28:13,280 --> 00:28:17,080 Speaker 1: it's a very long walk from two neutrinos to there's 531 00:28:17,080 --> 00:28:20,480 Speaker 1: a parallel universe right next to you. All right, yeah, 532 00:28:20,600 --> 00:28:24,440 Speaker 1: I know. So how much time do we have? Ten minutes? Alright? Go, 533 00:28:24,720 --> 00:28:28,040 Speaker 1: it's complicated. But the short version of it is, if 534 00:28:28,080 --> 00:28:31,639 Speaker 1: there's a parallel universe, then there might be some heavy 535 00:28:31,800 --> 00:28:35,440 Speaker 1: kind of neutrino gathered collected in the center of the Earth, 536 00:28:35,760 --> 00:28:39,360 Speaker 1: which is decaying and producing these neutrinos and shooting them 537 00:28:39,400 --> 00:28:42,200 Speaker 1: out from the center of the Earth. What that's the 538 00:28:42,280 --> 00:28:45,160 Speaker 1: short version. Wait, there's what's at the center of Neutrinos 539 00:28:45,200 --> 00:28:46,960 Speaker 1: are hanging out in the center of the Earth. Yeah. 540 00:28:47,000 --> 00:28:49,800 Speaker 1: The idea is we have neutrinos, and there's lots of 541 00:28:49,840 --> 00:28:53,120 Speaker 1: mysteries about neutrinos, like we don't know if neutrinos have 542 00:28:53,240 --> 00:28:57,560 Speaker 1: their own antiparticle, if there are other really heavy neutrinos 543 00:28:57,640 --> 00:28:59,600 Speaker 1: we've never seen before. And we had a whole episode 544 00:28:59,600 --> 00:29:02,640 Speaker 1: about that kind of mystery. And they're connected to other 545 00:29:02,920 --> 00:29:05,840 Speaker 1: really deep mysteries in physics, like why do we have 546 00:29:06,080 --> 00:29:10,000 Speaker 1: matter and not antimatter? Why does time flow forward and 547 00:29:10,120 --> 00:29:12,880 Speaker 1: not backwards? You know, every time in physics we see 548 00:29:13,000 --> 00:29:16,160 Speaker 1: something which isn't balanced, which is in symmetric, we ask why, 549 00:29:16,760 --> 00:29:20,040 Speaker 1: you know, the way we blame Adrina, it seems like, well, 550 00:29:20,320 --> 00:29:22,280 Speaker 1: it's just so easy, you know, They're just so easy 551 00:29:22,320 --> 00:29:26,760 Speaker 1: to blame. They're so neutral, They're they're being sneaky about something. 552 00:29:26,840 --> 00:29:29,520 Speaker 1: You those neutrinos are hiding something. I can smell it. 553 00:29:29,840 --> 00:29:33,520 Speaker 1: Never trust someone without an opinion, Isn't that what I 554 00:29:33,600 --> 00:29:37,520 Speaker 1: just said? But you know, it's like wondering, why are 555 00:29:37,600 --> 00:29:40,080 Speaker 1: humans more right handed than left handed. There's something going 556 00:29:40,160 --> 00:29:43,280 Speaker 1: on there. There's a clue to brain physiology or something. 557 00:29:43,800 --> 00:29:45,960 Speaker 1: So we wonder why is there more matter? Why is 558 00:29:46,000 --> 00:29:48,680 Speaker 1: time flow forwards? And one simple way to sort of 559 00:29:48,960 --> 00:29:51,520 Speaker 1: get rid of that question is to say, well, maybe 560 00:29:51,560 --> 00:29:55,400 Speaker 1: it's not actually in asymmetry. Maybe there's another universe where 561 00:29:55,480 --> 00:30:00,240 Speaker 1: time flows backwards and it's filled with anti partic like 562 00:30:00,360 --> 00:30:03,080 Speaker 1: somehow we started together but then we got split off. Yeah, 563 00:30:03,240 --> 00:30:06,480 Speaker 1: at the Big Bang two universes were created, one made 564 00:30:06,520 --> 00:30:09,040 Speaker 1: of matter where time flows forwards, and one made of 565 00:30:09,080 --> 00:30:13,719 Speaker 1: antimatter where time flows back. Why but then but um, 566 00:30:13,920 --> 00:30:15,720 Speaker 1: and we're right on top of each other and right 567 00:30:15,800 --> 00:30:18,000 Speaker 1: next to each other. No neither. I mean that doesn't 568 00:30:18,040 --> 00:30:20,280 Speaker 1: really make any sense. It's like, you know, time is 569 00:30:20,320 --> 00:30:22,719 Speaker 1: flowing backwards, it's a different part of space. I mean, 570 00:30:22,800 --> 00:30:25,440 Speaker 1: it's parallel in a sense that it's like not here, 571 00:30:25,640 --> 00:30:27,920 Speaker 1: it's not there, it's not right next to you, it's 572 00:30:27,960 --> 00:30:31,720 Speaker 1: not anywhere in our space. It's like where is yesterday? 573 00:30:31,880 --> 00:30:33,360 Speaker 1: I don't know. It's not to my left or to 574 00:30:33,480 --> 00:30:36,400 Speaker 1: my right. You know, it's backwards and behind me. It's 575 00:30:36,480 --> 00:30:39,040 Speaker 1: behind me, just like the south pole is belowing. But 576 00:30:39,160 --> 00:30:41,760 Speaker 1: if time is flowing backwards and to be ahead of you. Right, 577 00:30:42,280 --> 00:30:45,400 Speaker 1: So this is like the South Pole universe. It started 578 00:30:45,440 --> 00:30:47,280 Speaker 1: at the Big Bang going the other way and is 579 00:30:47,360 --> 00:30:51,240 Speaker 1: dominated by antimatter. Okay, so wait, So the theory is 580 00:30:51,400 --> 00:30:55,400 Speaker 1: then that these two neutrinos came from this other universe. 581 00:30:55,920 --> 00:30:59,000 Speaker 1: That's the idea is if there's this parallel universe, that 582 00:30:59,040 --> 00:31:01,400 Speaker 1: means that there's a symmetry to the universe that you know, 583 00:31:01,800 --> 00:31:05,080 Speaker 1: matter has antimatter, and that suggests that there are other 584 00:31:05,240 --> 00:31:09,080 Speaker 1: kinds of neutrinos in our universe, that the neutrino has 585 00:31:09,160 --> 00:31:13,000 Speaker 1: some really heavy partner because they make the other universe work. 586 00:31:13,280 --> 00:31:16,520 Speaker 1: You need these heavy neutrinos in our universe. That's what 587 00:31:16,600 --> 00:31:19,760 Speaker 1: the equations would suggest. Like if you invert the equations, 588 00:31:19,840 --> 00:31:22,040 Speaker 1: then you get a heavy neutrina. That's right, because there 589 00:31:22,080 --> 00:31:24,720 Speaker 1: has to be some other neutrino for that universe to have, 590 00:31:25,480 --> 00:31:27,920 Speaker 1: and so it has to be possible in our universe. 591 00:31:28,040 --> 00:31:31,200 Speaker 1: Just like our universe is mostly matter, not antimatter, the 592 00:31:31,240 --> 00:31:33,600 Speaker 1: other one is mostly antimatter, but we can still have 593 00:31:33,720 --> 00:31:37,960 Speaker 1: antimatter in our universe, and so their version of neutrinos 594 00:31:38,040 --> 00:31:42,080 Speaker 1: could also exist in our universe, and those neutrinos would 595 00:31:42,120 --> 00:31:45,640 Speaker 1: be super duper heavy. They'd be like really really massive, 596 00:31:46,000 --> 00:31:48,880 Speaker 1: unlike our neutrinos talking about well, you know, we talked 597 00:31:48,880 --> 00:31:51,280 Speaker 1: about this on that episode, Like these neutrinos could be 598 00:31:52,120 --> 00:31:55,600 Speaker 1: ridiculously massive, like thousands or millions of times heavier than 599 00:31:55,640 --> 00:31:58,240 Speaker 1: anything we've seen, or even more, you know, up to 600 00:31:58,360 --> 00:32:00,680 Speaker 1: like you can have a single particle has like the 601 00:32:00,840 --> 00:32:02,920 Speaker 1: mass of a whole city. These things could we what 602 00:32:03,360 --> 00:32:06,520 Speaker 1: could be really really heavy just in its resting match, 603 00:32:06,600 --> 00:32:10,080 Speaker 1: just in its resting mass. Yeah, because remember a particles mass, 604 00:32:10,120 --> 00:32:12,160 Speaker 1: it's not like how much stuff is there in it. 605 00:32:12,280 --> 00:32:14,840 Speaker 1: It's just some weird interaction with the Higgs field. And 606 00:32:14,920 --> 00:32:17,120 Speaker 1: so in a sense, it could be anything. We have 607 00:32:17,240 --> 00:32:20,400 Speaker 1: no clue why particles have this mass or that mass 608 00:32:20,520 --> 00:32:22,600 Speaker 1: or the other mass. It's all a mystery. So you 609 00:32:22,680 --> 00:32:25,080 Speaker 1: can set them to be anything. There's very few rules. 610 00:32:25,480 --> 00:32:28,800 Speaker 1: So this parallel universe that we're imagining, it's just kind 611 00:32:28,840 --> 00:32:32,080 Speaker 1: of the same, but it has a different preference, right, Yeah, 612 00:32:32,400 --> 00:32:35,160 Speaker 1: when the universe started, it's not like the universe decided 613 00:32:35,480 --> 00:32:38,200 Speaker 1: I'm going to have matter instead of antimatter. It did both. 614 00:32:38,600 --> 00:32:40,880 Speaker 1: It's like we'll do matter and we'll do antimatter. We'll 615 00:32:40,920 --> 00:32:43,080 Speaker 1: cover both of our basics. We have two verses, Yeah, 616 00:32:43,120 --> 00:32:45,040 Speaker 1: we are in this. Why why buy one when you 617 00:32:45,120 --> 00:32:49,200 Speaker 1: can buy two for the same physics, That's right. You know, 618 00:32:49,280 --> 00:32:51,280 Speaker 1: if you're going to go universe shopping, go to costco 619 00:32:52,600 --> 00:32:55,040 Speaker 1: r Yeah, yeah, you save shipping. Well, we just said 620 00:32:55,040 --> 00:32:59,440 Speaker 1: that in parallel Dannie. So if there's a parallel universe, 621 00:32:59,800 --> 00:33:03,200 Speaker 1: then it suggests the existence of these really heavy neutrinos. 622 00:33:03,720 --> 00:33:07,080 Speaker 1: And they could be the dark mouth like they could 623 00:33:07,120 --> 00:33:09,520 Speaker 1: be Yeah, there's a lot of steps here. They could 624 00:33:09,520 --> 00:33:13,000 Speaker 1: be the dark mount And if so, then they're really heavy. 625 00:33:13,080 --> 00:33:16,520 Speaker 1: They interact gravitationally. They could be collecting at the center 626 00:33:16,680 --> 00:33:20,200 Speaker 1: of the Earth like like the Sun, Like they're hanging 627 00:33:20,240 --> 00:33:22,320 Speaker 1: out at the center of the Earth. They're coming along 628 00:33:22,360 --> 00:33:24,400 Speaker 1: with us as we go around the Sun. Yeah, because 629 00:33:24,520 --> 00:33:27,800 Speaker 1: that's where things do gravitationally, is they clump together, and 630 00:33:27,880 --> 00:33:31,000 Speaker 1: the Earth is a big gravitational blob, and these neutrinos 631 00:33:31,080 --> 00:33:33,240 Speaker 1: don't feel the Earth in any way. They just sort 632 00:33:33,280 --> 00:33:35,640 Speaker 1: of passed through. The only thing they feel is it's gravity. 633 00:33:36,240 --> 00:33:38,840 Speaker 1: And so the Sun and also the Earth and all 634 00:33:38,840 --> 00:33:42,680 Speaker 1: the other planets might have collected these very heavy dark 635 00:33:42,800 --> 00:33:46,000 Speaker 1: matter neutrinos at the center. Wait, you just called it 636 00:33:46,120 --> 00:33:49,480 Speaker 1: in the same name. They're dark matter neutrinos, meaning neutrinos 637 00:33:49,560 --> 00:33:52,280 Speaker 1: that maybe explain dark matter. Yes, because we know that 638 00:33:52,360 --> 00:33:54,280 Speaker 1: there's a lot of missing stuff in the universe. We 639 00:33:54,360 --> 00:33:57,160 Speaker 1: know there's a lot of mass out there we cannot see. 640 00:33:57,480 --> 00:33:59,320 Speaker 1: We don't know what it is. We're looking for it. 641 00:33:59,400 --> 00:34:01,239 Speaker 1: We think maybe it's this, maybe it's that, Maybe it's 642 00:34:01,280 --> 00:34:04,560 Speaker 1: primordial black holes. One idea is maybe it's some weird, 643 00:34:04,640 --> 00:34:07,240 Speaker 1: new kind of very heavy neutrino we've never seen. And 644 00:34:07,320 --> 00:34:10,279 Speaker 1: these neutrinos are pretty suspicious. There's a lot of ifs here, right, 645 00:34:10,840 --> 00:34:13,960 Speaker 1: if there's a parallel universe. They are explaining matter and 646 00:34:14,000 --> 00:34:17,640 Speaker 1: antimatter time and also dark matter. Are they also involved 647 00:34:17,640 --> 00:34:20,680 Speaker 1: in dark energy? They kill JFK, that's what I think. 648 00:34:21,160 --> 00:34:25,360 Speaker 1: And the dinosaurs. Dinosaurs anyway, these things hanging out this 649 00:34:25,480 --> 00:34:26,919 Speaker 1: end of the Earth, they have a lot of energy, 650 00:34:27,000 --> 00:34:28,600 Speaker 1: have a lot of mass just sort of stored up 651 00:34:28,640 --> 00:34:32,000 Speaker 1: inside them. They're like very tightly coiled springs. So what 652 00:34:32,160 --> 00:34:35,520 Speaker 1: happens when they decay, Like some particles, they eventually decay. 653 00:34:35,640 --> 00:34:39,520 Speaker 1: Very heavy particles often decay. They can decay into normal neutrinos, 654 00:34:39,920 --> 00:34:42,680 Speaker 1: But normal lutrinos have very low mass, and so they 655 00:34:42,719 --> 00:34:45,680 Speaker 1: would have to decay into very high energy, very fast 656 00:34:45,840 --> 00:34:49,759 Speaker 1: moving neutrinos. So the mass of these mysterious dark matter 657 00:34:49,840 --> 00:34:53,480 Speaker 1: neutrinos gets turned into the energy, the kinetic energy the 658 00:34:53,560 --> 00:34:57,800 Speaker 1: motion of these very light normal neutrinos. Well, okay, I 659 00:34:57,840 --> 00:35:02,520 Speaker 1: guess maybe first of all these neutrinos, why don't they 660 00:35:02,640 --> 00:35:05,480 Speaker 1: decay more? I thought the universe didn't like like big 661 00:35:05,600 --> 00:35:08,160 Speaker 1: massive things hanging out. Yeah, that's a great question. The 662 00:35:08,320 --> 00:35:11,640 Speaker 1: universe doesn't like big massive things hanging out. But big 663 00:35:11,719 --> 00:35:14,719 Speaker 1: massive things hanging out can only turn into lighter things 664 00:35:14,800 --> 00:35:16,279 Speaker 1: if they have a way to do it, if there's 665 00:35:16,320 --> 00:35:19,640 Speaker 1: some interaction, some process. They use a photon to use 666 00:35:19,680 --> 00:35:22,359 Speaker 1: a w or z so you can keep something that's 667 00:35:22,440 --> 00:35:24,919 Speaker 1: very heavy, you can keep it stable if you turn 668 00:35:25,040 --> 00:35:27,799 Speaker 1: off all of its ways of decaying. So we don't 669 00:35:27,840 --> 00:35:29,560 Speaker 1: know anything about these things. They could have like a 670 00:35:29,719 --> 00:35:33,920 Speaker 1: very hard time decaying into these neutrinos, But also we 671 00:35:34,000 --> 00:35:36,279 Speaker 1: don't know, like it could be that it happens all 672 00:35:36,320 --> 00:35:38,120 Speaker 1: the time. There just aren't that many of them in 673 00:35:38,200 --> 00:35:40,120 Speaker 1: the center of the Earth mat Maybe there's only forty 674 00:35:40,160 --> 00:35:42,120 Speaker 1: of them and the decay once a year, And can 675 00:35:42,239 --> 00:35:44,480 Speaker 1: the universe be making these or can these only be 676 00:35:44,600 --> 00:35:47,200 Speaker 1: made in the big band universe? Probably wouldn't be making 677 00:35:47,280 --> 00:35:49,359 Speaker 1: these anymore. They would be primordial. They would have been 678 00:35:49,400 --> 00:35:52,640 Speaker 1: made in the early universe and then still existing. So 679 00:35:52,800 --> 00:35:54,680 Speaker 1: that means that if it is dark matter, then that 680 00:35:54,760 --> 00:35:57,439 Speaker 1: means the dark matter would be disappearing. Yes, dark matter 681 00:35:57,440 --> 00:36:00,359 Speaker 1: would be disappearing, but very slowly. Right like we know matter, 682 00:36:00,440 --> 00:36:03,640 Speaker 1: if it exists, is cosmologically stable, like it was made 683 00:36:03,840 --> 00:36:06,400 Speaker 1: very early on in the universe, and not much of 684 00:36:06,440 --> 00:36:10,239 Speaker 1: it or if any has disappeared, And so these neutrinos, 685 00:36:10,680 --> 00:36:14,000 Speaker 1: if they do decay, it can't happen very often. So actually, 686 00:36:14,040 --> 00:36:15,920 Speaker 1: if we saw two of them in the last twenty years, 687 00:36:16,000 --> 00:36:18,040 Speaker 1: that suggests there must be a lot of them if 688 00:36:18,120 --> 00:36:20,839 Speaker 1: they exist in the center of the Earth, I see, 689 00:36:20,880 --> 00:36:22,880 Speaker 1: all right, So then that's how you connect the thoughts, 690 00:36:23,080 --> 00:36:26,880 Speaker 1: is that we saw these two neutrino pings and we're like, 691 00:36:26,920 --> 00:36:29,480 Speaker 1: where they come from. They couldn't have come from anywhere 692 00:36:29,480 --> 00:36:31,160 Speaker 1: that we know of, So maybe they said they came 693 00:36:31,200 --> 00:36:33,080 Speaker 1: from the center of the Earth and they were made 694 00:36:33,120 --> 00:36:35,560 Speaker 1: by these two heavy neutrinos that are hanging out there, 695 00:36:35,640 --> 00:36:38,440 Speaker 1: that's right, And if those two heavy neutrinos do exist, 696 00:36:38,719 --> 00:36:41,600 Speaker 1: there are a clue that maybe the universe has this 697 00:36:41,760 --> 00:36:45,480 Speaker 1: symmetry after all, that maybe there is another universe out 698 00:36:45,520 --> 00:36:48,319 Speaker 1: there that started the Big Bang going the other way. 699 00:36:48,680 --> 00:36:51,120 Speaker 1: But you know that's also a reach. Yeah. I'm having 700 00:36:51,160 --> 00:36:53,640 Speaker 1: trouble with that one because it just means that these 701 00:36:53,680 --> 00:36:56,200 Speaker 1: having neutrinos exist. It's like saying that because we can 702 00:36:56,280 --> 00:36:58,719 Speaker 1: see antimatter, that means there's another universe. But that's not 703 00:36:58,800 --> 00:37:01,160 Speaker 1: really the case, is it right? You cannot conclude that 704 00:37:01,200 --> 00:37:04,080 Speaker 1: there's a parallel universe, even if you proved that there 705 00:37:04,120 --> 00:37:06,719 Speaker 1: are super heavy neutrinos at the center of the Earth 706 00:37:06,800 --> 00:37:10,000 Speaker 1: decaying into normal neutrinos, because there are other explanations that 707 00:37:10,120 --> 00:37:13,160 Speaker 1: are not as bonkers and crazy. Is a parallel universe 708 00:37:13,440 --> 00:37:17,080 Speaker 1: I see, So that the parallel universe is just one 709 00:37:17,480 --> 00:37:21,480 Speaker 1: maybe possible explanation for why our universe has the light 710 00:37:21,600 --> 00:37:24,279 Speaker 1: neutrinos and not the heavy neutrinos. But we do have 711 00:37:24,360 --> 00:37:26,800 Speaker 1: the haaving neutrinos, So I guess I'm complu we have 712 00:37:26,880 --> 00:37:28,719 Speaker 1: the light neutrinos, we don't know if we have the 713 00:37:28,800 --> 00:37:31,600 Speaker 1: heavy neutrinos in our universe. Like, that's one idea it 714 00:37:31,719 --> 00:37:34,400 Speaker 1: could be, and one reason to explain it is like 715 00:37:34,520 --> 00:37:37,000 Speaker 1: maybe there's a parallel universe and that requires us to 716 00:37:37,040 --> 00:37:39,239 Speaker 1: have heavy neutrinos. But there are other theories that have 717 00:37:39,360 --> 00:37:41,960 Speaker 1: heavy neutrinos in them also. I mean, what happened is 718 00:37:42,320 --> 00:37:45,279 Speaker 1: Anita saw these weird neutrinos. A bunch of very well 719 00:37:45,360 --> 00:37:47,520 Speaker 1: meaning theorists who've been working on this idea of a 720 00:37:47,600 --> 00:37:50,080 Speaker 1: parallel universe said, hey, wait a second, I like that 721 00:37:50,360 --> 00:37:53,359 Speaker 1: that could be explained by our theory. Here's a fun, 722 00:37:53,480 --> 00:37:55,879 Speaker 1: crazy theory that could explain it that we've been working 723 00:37:55,920 --> 00:37:58,520 Speaker 1: on for ten years and involves a cool parallel universe. 724 00:37:58,719 --> 00:38:01,440 Speaker 1: They wrote this paper. Then science journalism was like, now, 725 00:38:01,560 --> 00:38:05,160 Speaker 1: so it discovered a parallel universe, and so you know, 726 00:38:05,520 --> 00:38:09,879 Speaker 1: they screamed like that, like like like very excited kids. 727 00:38:10,000 --> 00:38:11,920 Speaker 1: Yeah exactly. There was a lot of journalistic jumping up 728 00:38:11,960 --> 00:38:14,719 Speaker 1: and down. All right, Well, it seems like a reach. 729 00:38:14,800 --> 00:38:19,319 Speaker 1: It seems like you're extrapolating two signals to the whole 730 00:38:19,360 --> 00:38:23,560 Speaker 1: existence over this new particle, to the whole existence of 731 00:38:23,600 --> 00:38:27,520 Speaker 1: apparallel universe. That's right, every step there is a reach, right, 732 00:38:27,640 --> 00:38:30,480 Speaker 1: just because you see these two new particles doesn't mean 733 00:38:30,920 --> 00:38:33,800 Speaker 1: that there's anything new. It could be experimental error. It 734 00:38:33,880 --> 00:38:37,720 Speaker 1: could just be luck. Or it could be some heavy 735 00:38:37,800 --> 00:38:40,240 Speaker 1: new particle in the center of the Earth, which could 736 00:38:40,440 --> 00:38:44,640 Speaker 1: be maybe a new trino, which could maybe potentially give 737 00:38:44,719 --> 00:38:48,400 Speaker 1: credence to this crazy, fun, silly theory about a parallel universe. 738 00:38:48,640 --> 00:38:51,080 Speaker 1: But I guess maybe why does it have to come 739 00:38:51,120 --> 00:38:53,560 Speaker 1: from the center of the Earth. Is that the only explanation? Well, 740 00:38:53,560 --> 00:38:55,600 Speaker 1: because we only see them coming up from the earth, Like, 741 00:38:55,680 --> 00:38:58,080 Speaker 1: we don't see them skimming the earth. We don't see 742 00:38:58,120 --> 00:39:00,319 Speaker 1: them coming in any other direction. We only see them 743 00:39:00,400 --> 00:39:02,759 Speaker 1: coming straight up from underground, because that's the only place 744 00:39:02,800 --> 00:39:05,120 Speaker 1: where we have the camera, isn't it. The camera can 745 00:39:05,120 --> 00:39:08,719 Speaker 1: see these things coming even straight down or sideways or 746 00:39:08,800 --> 00:39:11,560 Speaker 1: coming up from the ice and just skimming it like 747 00:39:11,840 --> 00:39:13,920 Speaker 1: just along the horizon. But they don't see anything in 748 00:39:14,000 --> 00:39:17,320 Speaker 1: those directions. They see only these very high energy netrinos 749 00:39:17,360 --> 00:39:21,200 Speaker 1: coming straight up from the Earth. All right, Well, what 750 00:39:21,280 --> 00:39:22,960 Speaker 1: else could they be? One thing is they could be 751 00:39:23,000 --> 00:39:26,680 Speaker 1: experimental error. I mean, the two out in twenty years 752 00:39:26,840 --> 00:39:28,759 Speaker 1: does seem sort of like a blip. Yeah, it does 753 00:39:28,800 --> 00:39:30,879 Speaker 1: seem like a blip. And so you have to ask, like, well, 754 00:39:30,920 --> 00:39:33,799 Speaker 1: how well do we know these things? Sometimes there's something rare, 755 00:39:33,960 --> 00:39:36,399 Speaker 1: but when you spot it, you're pretty sure. Like if 756 00:39:36,440 --> 00:39:39,279 Speaker 1: you discover a unicorn. Yeah, they're hard to find, but 757 00:39:39,480 --> 00:39:41,400 Speaker 1: when you get one in your lab, you can pretty 758 00:39:41,400 --> 00:39:44,800 Speaker 1: well tell us in uniform. You seem to speak from experience. 759 00:39:46,239 --> 00:39:48,520 Speaker 1: That's my dream, you know, the one day discover unicorn. 760 00:39:49,160 --> 00:39:51,879 Speaker 1: And so what do we actually know about these things? Really, 761 00:39:51,960 --> 00:39:54,680 Speaker 1: the measurements we have come from these antennas and they're 762 00:39:54,680 --> 00:39:58,400 Speaker 1: pretty good, but they can get spoofed. Like one scenario 763 00:39:58,760 --> 00:40:01,239 Speaker 1: is these things come from the center of the Earth. 764 00:40:01,400 --> 00:40:04,600 Speaker 1: They came from straight down, like maybe a high energy 765 00:40:04,640 --> 00:40:08,279 Speaker 1: neutrino came straight down and hit the ice and the 766 00:40:08,360 --> 00:40:11,640 Speaker 1: signals sort of reflected in the ice and then came 767 00:40:11,680 --> 00:40:14,280 Speaker 1: back up and then it was captured by the balloon, 768 00:40:14,360 --> 00:40:16,120 Speaker 1: so it looked like it came out of the ice, 769 00:40:16,400 --> 00:40:19,279 Speaker 1: but actually the original particle was coming straight down. Oh, 770 00:40:19,880 --> 00:40:23,160 Speaker 1: so that can happen. They can bounce. That totally happens. 771 00:40:23,200 --> 00:40:26,880 Speaker 1: They can bounce, But this experiment can usually tell because 772 00:40:27,040 --> 00:40:30,520 Speaker 1: there's a polarity to this signal. The signals effectively spin 773 00:40:30,600 --> 00:40:32,920 Speaker 1: in a certain way because of the Earth's magnetic field, 774 00:40:33,120 --> 00:40:35,800 Speaker 1: and if they hit the ice and bounce, that polarity flips. 775 00:40:36,280 --> 00:40:39,320 Speaker 1: It's like when light bounces off of water, it changes 776 00:40:39,440 --> 00:40:42,239 Speaker 1: this polarity, and so they can see this, and so 777 00:40:42,480 --> 00:40:44,520 Speaker 1: they see this. Actually all the time, they see cosmic 778 00:40:44,600 --> 00:40:47,520 Speaker 1: rays coming from space that bounce off the ice up 779 00:40:47,560 --> 00:40:49,640 Speaker 1: to the experiment and then they remove them. But for 780 00:40:49,840 --> 00:40:52,600 Speaker 1: these two weird neutrinos, they don't see that, so it 781 00:40:52,719 --> 00:40:56,080 Speaker 1: doesn't look like they bounced, right. But you know, how 782 00:40:56,160 --> 00:40:59,759 Speaker 1: well do we really understand the details of Antarctic ice? 783 00:41:00,120 --> 00:41:03,279 Speaker 1: Could there be something weird going on? Occasionally it gets 784 00:41:03,360 --> 00:41:06,800 Speaker 1: double reflected or something, right, there's always a possibility. I 785 00:41:06,880 --> 00:41:09,520 Speaker 1: think they came from a parallel universe data with a 786 00:41:09,600 --> 00:41:13,440 Speaker 1: different polarity. I'll call New Scientists magazine. Okay, a parallel 787 00:41:13,600 --> 00:41:17,200 Speaker 1: universe where everybody likes bananas and DC makes better movies 788 00:41:17,239 --> 00:41:20,840 Speaker 1: than Mardel. Impossible. That just breaks the laws of physics. 789 00:41:21,560 --> 00:41:24,839 Speaker 1: Al Right, Well, um, it sounds like it's pretty tantalizing, 790 00:41:24,920 --> 00:41:28,080 Speaker 1: I guess, but it's sort of build upon two measurements, 791 00:41:28,800 --> 00:41:32,360 Speaker 1: and it's kind of extrapolating a lot from two measurements 792 00:41:32,480 --> 00:41:36,680 Speaker 1: to new particles, to the whole different universe. It's like 793 00:41:36,719 --> 00:41:38,800 Speaker 1: a lot of ifs there and a lot of like 794 00:41:39,040 --> 00:41:41,040 Speaker 1: maybes built on top of each other, and a lot 795 00:41:41,120 --> 00:41:43,880 Speaker 1: of people doing very careful work, Like the experimentalists have 796 00:41:43,960 --> 00:41:46,080 Speaker 1: been building this thing and running it for twenty years, 797 00:41:46,400 --> 00:41:50,280 Speaker 1: and their papers are totally solid. They very carefully understood 798 00:41:50,320 --> 00:41:52,640 Speaker 1: the source of these things. And in their papers, you know, 799 00:41:52,719 --> 00:41:54,960 Speaker 1: they say exactly how well they know things and how 800 00:41:55,000 --> 00:41:57,520 Speaker 1: well they don't know things. And then the theorists also 801 00:41:57,600 --> 00:42:00,239 Speaker 1: pretty well behaved. They were just like suggesting and I dea. 802 00:42:00,280 --> 00:42:02,960 Speaker 1: They're not claiming to discovery the parallel universe. They to say, 803 00:42:03,239 --> 00:42:06,239 Speaker 1: here's a possible fun explanation, and then you know, it 804 00:42:06,320 --> 00:42:08,800 Speaker 1: trickled out in the mainstream press and they're hitting the 805 00:42:08,880 --> 00:42:12,560 Speaker 1: parallel universe button a little too hard, all right, But um, 806 00:42:12,680 --> 00:42:15,319 Speaker 1: I guess what's interesting is that it might be possible, right, 807 00:42:15,480 --> 00:42:18,160 Speaker 1: this could be how we discovered a parallel universe. It's 808 00:42:18,200 --> 00:42:21,040 Speaker 1: definitely something interesting. At the most boring end of the spectrum, 809 00:42:21,080 --> 00:42:24,640 Speaker 1: we've learned something interesting about Antarctic ice. You know. More 810 00:42:24,760 --> 00:42:27,040 Speaker 1: interesting is like, hey, maybe there is some weird new 811 00:42:27,160 --> 00:42:30,040 Speaker 1: kind of particle, or maybe there is some new source 812 00:42:30,160 --> 00:42:32,319 Speaker 1: of really high energy to trinos out there we've never 813 00:42:32,400 --> 00:42:36,000 Speaker 1: seen before, or maybe it's something crazy in bonkers, right, 814 00:42:36,120 --> 00:42:38,719 Speaker 1: We can't rule out the parallel universe scenario. It is 815 00:42:38,800 --> 00:42:42,719 Speaker 1: one explanation for these particles I see. And so this 816 00:42:43,120 --> 00:42:47,000 Speaker 1: parallel universe, it is one word. Time flows backwards too, 817 00:42:47,239 --> 00:42:49,279 Speaker 1: It's not just like a copy of ours. It's also 818 00:42:49,400 --> 00:42:54,840 Speaker 1: running backwards. Yeah, time flows backwards and antimatter dominates, and 819 00:42:54,920 --> 00:42:57,120 Speaker 1: that provides a nice symmetry, you know. It's like it 820 00:42:57,239 --> 00:42:59,680 Speaker 1: answers the question of why does time flow forwards and 821 00:42:59,719 --> 00:43:01,919 Speaker 1: why we have matter or not antimatter. And it doesn't 822 00:43:01,920 --> 00:43:03,719 Speaker 1: tell you why did the universe split, but it tells 823 00:43:03,719 --> 00:43:05,680 Speaker 1: you at least it covered both of its basis. It 824 00:43:05,719 --> 00:43:08,840 Speaker 1: doesn't have like a preference for forward flowing time or 825 00:43:09,120 --> 00:43:12,800 Speaker 1: for matter over antimatter. And that just feels somehow more natural. 826 00:43:13,440 --> 00:43:16,040 Speaker 1: Maybe twitter and that universe is like full of positivity 827 00:43:16,160 --> 00:43:23,080 Speaker 1: and well meaning people. Yeah, then maybe I prefer that universe. Yeah, 828 00:43:23,200 --> 00:43:26,960 Speaker 1: let's move to that one. I think there's a portal 829 00:43:27,000 --> 00:43:28,640 Speaker 1: at the center of the Earth. Oh, there you go. 830 00:43:29,080 --> 00:43:32,520 Speaker 1: You just gotta get past those having neutrinos and step through. 831 00:43:33,080 --> 00:43:35,680 Speaker 1: That's right. Effectively, there are bouncers to the parallel universe, 832 00:43:35,800 --> 00:43:37,600 Speaker 1: or maybe we can take a balloon or like an 833 00:43:37,600 --> 00:43:40,560 Speaker 1: anti balloon, take an anti balloon to the center of 834 00:43:40,719 --> 00:43:43,200 Speaker 1: the Earth and then you step through. Well, would you 835 00:43:43,280 --> 00:43:45,840 Speaker 1: call a balloon that floats below the south pole and 836 00:43:45,880 --> 00:43:50,880 Speaker 1: anti balloon anyway? Because it's going down. Oh, you're right, 837 00:43:51,040 --> 00:43:55,319 Speaker 1: you're right. You just turn it on me. Yeah, all right. 838 00:43:55,880 --> 00:43:59,840 Speaker 1: So I guess the very take is interesting results, solid signs, 839 00:44:00,040 --> 00:44:03,239 Speaker 1: interesting results. But maybe the science journalism they're got a 840 00:44:03,280 --> 00:44:05,520 Speaker 1: little too excited, a little too excited. I love the 841 00:44:05,640 --> 00:44:09,240 Speaker 1: enthusiasm of science journalism, but please let's keep it realistic, 842 00:44:09,640 --> 00:44:11,480 Speaker 1: all right. Well, they did say in the headline, we 843 00:44:11,600 --> 00:44:13,960 Speaker 1: may have spotted a parallel universe. They did add the 844 00:44:14,040 --> 00:44:18,480 Speaker 1: main Yeah. May it may covers everything, right, I might 845 00:44:18,560 --> 00:44:21,440 Speaker 1: have an unicorn right here next to me. I may 846 00:44:21,480 --> 00:44:24,840 Speaker 1: be totally lying to you, all right. Hopefully that covered 847 00:44:24,880 --> 00:44:27,520 Speaker 1: the questions that our readers had about these headlines, and 848 00:44:27,680 --> 00:44:29,400 Speaker 1: maybe I got you to think a little bit about 849 00:44:29,560 --> 00:44:31,040 Speaker 1: what could be out there and not out there. And 850 00:44:31,120 --> 00:44:33,440 Speaker 1: if you see something in the science headlines that you 851 00:44:33,560 --> 00:44:36,080 Speaker 1: don't understand and you'd like to hear about, please send 852 00:44:36,120 --> 00:44:39,319 Speaker 1: it to us. Two questions at Daniel and Jorge dot Com. 853 00:44:39,680 --> 00:44:41,759 Speaker 1: We'll break it down for you. Thanks for joining us, 854 00:44:42,400 --> 00:44:52,600 Speaker 1: see you next time. Thanks for listening, and remember that 855 00:44:52,760 --> 00:44:55,480 Speaker 1: Daniel and Jorge Explain the Universe is a production of 856 00:44:55,600 --> 00:44:58,959 Speaker 1: by Heart Radio. For more podcast from my heart Radio, 857 00:44:59,120 --> 00:45:02,640 Speaker 1: visit the i heart Radio app, Apple Podcasts, or wherever 858 00:45:02,800 --> 00:45:04,440 Speaker 1: you listen to your favorite shows.