1 00:00:00,240 --> 00:00:05,600 Speaker 1: Now here's a highlight from coast to coast am on iHeartRadio. 2 00:00:05,000 --> 00:00:08,000 Speaker 2: Proper number off faster than light. How your shadow can 3 00:00:08,039 --> 00:00:11,119 Speaker 2: do it but you can't is really good. Is this 4 00:00:11,320 --> 00:00:14,400 Speaker 2: a material taken from lectures that you've given or you've 5 00:00:14,400 --> 00:00:15,720 Speaker 2: pulled it together over the years. 6 00:00:17,000 --> 00:00:19,160 Speaker 3: Well, I've always had interest. For many many years, I 7 00:00:19,239 --> 00:00:22,159 Speaker 3: had an interest, and I've actually published on some of 8 00:00:22,160 --> 00:00:27,000 Speaker 3: the strange aspects in science journals, some of the strange 9 00:00:27,040 --> 00:00:30,840 Speaker 3: aspects that shadows and laser spots can do when they 10 00:00:31,000 --> 00:00:35,080 Speaker 3: when they go faster than lights. Because even the physics community, 11 00:00:35,320 --> 00:00:37,680 Speaker 3: once they see the logic, they don't disagree with it, 12 00:00:37,760 --> 00:00:40,360 Speaker 3: but they're unaware of it. So if you were to 13 00:00:40,400 --> 00:00:43,360 Speaker 3: go and speak to someone you know that's versed in physics, 14 00:00:43,400 --> 00:00:45,320 Speaker 3: they would say, oh, no, no, that can't happen. But 15 00:00:45,400 --> 00:00:48,360 Speaker 3: once you explain to them the logic of how it 16 00:00:48,400 --> 00:00:51,680 Speaker 3: does happen, they'll say, oh, yeah, yeah, that's kind of cool. 17 00:00:52,040 --> 00:00:54,520 Speaker 3: And it is. So it's really strange. It's it's one 18 00:00:54,560 --> 00:00:57,400 Speaker 3: of these untold stories out there that there's this whole 19 00:00:57,920 --> 00:01:01,240 Speaker 3: universe of things that happen faster than light that we 20 00:01:01,320 --> 00:01:04,640 Speaker 3: don't know. For instance, when you turn on a room 21 00:01:04,720 --> 00:01:08,000 Speaker 3: light the room. At first the room is completely dark, 22 00:01:08,160 --> 00:01:12,320 Speaker 3: and after a second, for sure the room is completely illuminated. Well, 23 00:01:12,480 --> 00:01:17,040 Speaker 3: the boundary between dark and light moves across the law 24 00:01:17,760 --> 00:01:21,479 Speaker 3: faster than light. So if you could see at those speeds, 25 00:01:21,760 --> 00:01:24,280 Speaker 3: you would be able to see a much different universe. 26 00:01:24,400 --> 00:01:26,840 Speaker 3: You would see lots of things moving faster than light 27 00:01:26,880 --> 00:01:28,920 Speaker 3: all the time. And so one of the reasons why 28 00:01:28,959 --> 00:01:31,399 Speaker 3: we can't do it, why we can't see it, is 29 00:01:31,400 --> 00:01:35,080 Speaker 3: because our brains and minds are so slow. That would 30 00:01:35,120 --> 00:01:39,360 Speaker 3: mean that it just doesn't come through. But now with 31 00:01:39,480 --> 00:01:43,840 Speaker 3: modern technology, we can have times rapid time lapse photography 32 00:01:43,880 --> 00:01:44,720 Speaker 3: and see these things. 33 00:01:45,800 --> 00:01:49,080 Speaker 2: You drop a lot of really cool historical facts in 34 00:01:49,120 --> 00:01:52,320 Speaker 2: the book about you know, the the understanding of the 35 00:01:52,320 --> 00:01:55,520 Speaker 2: speed of light, how it developed and changed over the centuries. 36 00:01:56,000 --> 00:01:58,600 Speaker 2: Maybe let's start there, I mean, tell us a little 37 00:01:58,600 --> 00:02:00,600 Speaker 2: bit about and what you cover in the talk about 38 00:02:01,000 --> 00:02:03,600 Speaker 2: the first folks to try to measure the speed light, 39 00:02:03,680 --> 00:02:06,360 Speaker 2: is it Galileo or even before that. 40 00:02:07,320 --> 00:02:10,359 Speaker 3: People have been been speculating about the speed of light 41 00:02:10,440 --> 00:02:16,440 Speaker 3: since since in most of recorded history. For instance, as 42 00:02:16,440 --> 00:02:20,120 Speaker 3: you noted, let's see Aristotle and you clip back in 43 00:02:20,840 --> 00:02:26,079 Speaker 3: the you know BC times they sort of thought that. 44 00:02:26,160 --> 00:02:28,480 Speaker 3: They sort of thought that what happens is light doesn't 45 00:02:28,520 --> 00:02:31,120 Speaker 3: come from an object, from a star, or from a 46 00:02:31,200 --> 00:02:34,560 Speaker 3: light to you. Light goes from your eye to the 47 00:02:34,560 --> 00:02:38,040 Speaker 3: object you're seeing. And for most of human history that's 48 00:02:38,120 --> 00:02:41,480 Speaker 3: the way humans thought. It was. Every now and then 49 00:02:41,520 --> 00:02:43,440 Speaker 3: someone would say, no it I think it's the other way. 50 00:02:43,480 --> 00:02:46,240 Speaker 3: But that was not what most people believed. And it 51 00:02:46,280 --> 00:02:51,160 Speaker 3: was only around one thousand a d that that it 52 00:02:51,200 --> 00:02:53,680 Speaker 3: was more and more realized that no, no, no, that 53 00:02:53,680 --> 00:02:56,000 Speaker 3: that's not the way it is. Light actually comes goes 54 00:02:56,040 --> 00:02:59,320 Speaker 3: from something and comes to us, and that's when so 55 00:02:59,639 --> 00:03:02,359 Speaker 3: back in the DC times, people thought, well, the Steed 56 00:03:02,440 --> 00:03:05,160 Speaker 3: light must be infinite, because when your eyes are closed, 57 00:03:05,160 --> 00:03:07,080 Speaker 3: you don't see something, and then when you open your eyes, 58 00:03:07,160 --> 00:03:08,760 Speaker 3: then light goes out from your eyes and you can 59 00:03:08,800 --> 00:03:11,560 Speaker 3: see things, even stars that are far away. Therefore, the 60 00:03:11,600 --> 00:03:15,600 Speaker 3: speedelite must be effectically infinite. But once people realized that 61 00:03:15,880 --> 00:03:18,880 Speaker 3: light was coming from other things into their eye, then 62 00:03:18,919 --> 00:03:22,000 Speaker 3: people realize, well, maybe it's not infinite, maybe it's it's 63 00:03:22,000 --> 00:03:24,960 Speaker 3: got some speed. But for many years they just couldn't 64 00:03:25,000 --> 00:03:28,080 Speaker 3: measured it. It was so fast, as I like to tell 65 00:03:28,120 --> 00:03:33,160 Speaker 3: my students, there's really only three numbers in conceptual astrosoutics. 66 00:03:33,160 --> 00:03:36,360 Speaker 3: One is infinity, which means it was really too fast 67 00:03:36,440 --> 00:03:39,440 Speaker 3: or too big to measure. One is one means that 68 00:03:39,520 --> 00:03:41,680 Speaker 3: we measured it. It's one of those, and the other 69 00:03:41,800 --> 00:03:45,080 Speaker 3: is zero. The third number and astrophys this is zero 70 00:03:45,160 --> 00:03:47,200 Speaker 3: because it means it's too small to measure. It might 71 00:03:47,240 --> 00:03:50,200 Speaker 3: be there, we don't know its size, but it's effectively zero. 72 00:03:50,640 --> 00:03:52,920 Speaker 3: So for a lot of human history, the speedlite was 73 00:03:52,960 --> 00:03:55,520 Speaker 3: infinite because it was just too fast to measure. We 74 00:03:56,080 --> 00:03:59,680 Speaker 3: couldn't do it. So people like Galileo they tried to 75 00:03:59,720 --> 00:04:02,920 Speaker 3: do it. They would go to the mountaintops or hilltops, 76 00:04:02,960 --> 00:04:05,000 Speaker 3: and then someone else could in another hilltop, and they 77 00:04:05,000 --> 00:04:09,520 Speaker 3: had lanterns, and they had black things they could, you know, 78 00:04:09,560 --> 00:04:11,640 Speaker 3: they could put over the lanterns. And so they would 79 00:04:11,680 --> 00:04:14,760 Speaker 3: make deal feel you and your your hilltop. When you 80 00:04:15,000 --> 00:04:18,760 Speaker 3: see me uncover my lanterns, you uncover your lantern and 81 00:04:18,960 --> 00:04:22,080 Speaker 3: I'll count the amount of seconds it takes before I 82 00:04:22,120 --> 00:04:24,919 Speaker 3: can see your lanterns. And so Galileo did this and 83 00:04:25,000 --> 00:04:28,000 Speaker 3: other people did this, and they found out wall it 84 00:04:28,040 --> 00:04:30,480 Speaker 3: was out a second. No, it's about two seconds. No, 85 00:04:30,560 --> 00:04:32,440 Speaker 3: it's about half a second. And they realized they weren't 86 00:04:32,440 --> 00:04:36,120 Speaker 3: getting a consistent answer, and Galileo realized that, no, I 87 00:04:36,200 --> 00:04:38,479 Speaker 3: just don't believe it. It was infinitely fast. What we're 88 00:04:38,520 --> 00:04:42,039 Speaker 3: really measuring is how long it takes to uncover the lanterns. 89 00:04:42,040 --> 00:04:44,240 Speaker 3: They're not really measuring anything to do with the state 90 00:04:44,279 --> 00:04:48,040 Speaker 3: of light. So many efforts measured the super fast speed 91 00:04:48,040 --> 00:04:52,960 Speaker 3: of light just fouled until suddenly, in the sixteen hundred, 92 00:04:53,320 --> 00:04:56,799 Speaker 3: someone who was not famous just happened to be doing 93 00:04:56,839 --> 00:05:00,560 Speaker 3: something that some people didn't, you know, think would be 94 00:05:00,600 --> 00:05:03,120 Speaker 3: all that interesting, and they got a result that they 95 00:05:03,120 --> 00:05:07,479 Speaker 3: didn't understand. But that result was the door. That door 96 00:05:07,800 --> 00:05:11,040 Speaker 3: was that we went through is the finite speed of light. 97 00:05:11,440 --> 00:05:14,840 Speaker 3: And that person was Olay Roamer and a Roamer. What 98 00:05:14,880 --> 00:05:17,320 Speaker 3: they were doing is they were just watching the moons 99 00:05:17,320 --> 00:05:19,840 Speaker 3: of Jupiter. And when the moons of Jupiter, particularly Iisle, 100 00:05:19,920 --> 00:05:23,000 Speaker 3: would go behind Jupiter go in front of Jupiter, and 101 00:05:23,600 --> 00:05:26,760 Speaker 3: Romer noticed it was just something odd about the timing 102 00:05:26,839 --> 00:05:30,200 Speaker 3: of these eclipses, and the eclipses would take longer in 103 00:05:30,279 --> 00:05:34,160 Speaker 3: some circumstances and shorter in other circumstances, and it just 104 00:05:34,200 --> 00:05:37,479 Speaker 3: didn't seem to make sense. And so meanwhile, on the 105 00:05:37,520 --> 00:05:40,200 Speaker 3: other people on the next bill trying to uncover lanterns, 106 00:05:40,600 --> 00:05:42,720 Speaker 3: but the roamer was saying, hey, wait a minute, can 107 00:05:42,760 --> 00:05:45,760 Speaker 3: you understand this? And the answer it turns out that 108 00:05:45,839 --> 00:05:49,320 Speaker 3: Olay Rummer was actually the first to discover the finite 109 00:05:49,400 --> 00:05:52,719 Speaker 3: speed of light, and to measure it was in a 110 00:05:52,760 --> 00:05:56,480 Speaker 3: small fraction of the not super actively, but relatively accurately, 111 00:05:57,680 --> 00:06:01,400 Speaker 3: like but we know it today. The discovery was just 112 00:06:01,480 --> 00:06:06,400 Speaker 3: a bit of a surprise, and it advanced human knowledge 113 00:06:06,800 --> 00:06:08,919 Speaker 3: in a great way by just a sort of a 114 00:06:08,960 --> 00:06:10,080 Speaker 3: thirddipitous results. 115 00:06:11,320 --> 00:06:13,280 Speaker 2: You write a couple of different places in the book 116 00:06:13,320 --> 00:06:15,600 Speaker 2: about there being more than one speed of light? Can 117 00:06:15,640 --> 00:06:16,320 Speaker 2: you explain that? 118 00:06:17,680 --> 00:06:17,880 Speaker 1: Yes? 119 00:06:17,960 --> 00:06:20,040 Speaker 3: So now we know in modern science we know a 120 00:06:20,040 --> 00:06:22,760 Speaker 3: lot about the speed of lighte. And we know that 121 00:06:23,000 --> 00:06:26,080 Speaker 3: the speed a light in objects. So when you look 122 00:06:26,160 --> 00:06:29,320 Speaker 3: through water, the speed light and water is not the 123 00:06:29,360 --> 00:06:32,200 Speaker 3: same as the speed a light in air or in vacuum. 124 00:06:32,520 --> 00:06:34,760 Speaker 3: Speed light through air and vacuum are actually very similar. 125 00:06:34,760 --> 00:06:37,960 Speaker 3: It's a very small fractional percentage difference between us. But 126 00:06:38,040 --> 00:06:42,560 Speaker 3: in water it's like third flower. But there's different even 127 00:06:42,640 --> 00:06:45,200 Speaker 3: kinds of light. We now know things about the way 128 00:06:45,320 --> 00:06:48,640 Speaker 3: light works, and there's phases, and there's something called the 129 00:06:48,640 --> 00:06:50,880 Speaker 3: group velocity. The group colosity is more of us how 130 00:06:50,880 --> 00:06:52,960 Speaker 3: long it will take light to go from you to 131 00:06:53,040 --> 00:06:55,760 Speaker 3: a mirror to bounce back. If you measure that speed, 132 00:06:55,920 --> 00:06:58,320 Speaker 3: which we can now do with great accuracy, you're measuring 133 00:06:58,320 --> 00:07:00,880 Speaker 3: the group philosity of light. Also thing it's called the 134 00:07:00,920 --> 00:07:03,960 Speaker 3: phase velocity. Words, if you measure how much light is deflected, 135 00:07:04,680 --> 00:07:07,279 Speaker 3: that tells. But that's not all that important. 136 00:07:07,320 --> 00:07:07,440 Speaker 1: Really. 137 00:07:07,480 --> 00:07:10,440 Speaker 3: It's important for understanding the details of physics and how 138 00:07:10,560 --> 00:07:13,840 Speaker 3: things work. But in terms of the conceptual speed light, 139 00:07:13,880 --> 00:07:16,560 Speaker 3: we now know that the speed light and glass is 140 00:07:16,600 --> 00:07:19,440 Speaker 3: different than the speed light and water, and the speed 141 00:07:19,520 --> 00:07:21,400 Speaker 3: light and water is different than the speed a light 142 00:07:21,440 --> 00:07:23,560 Speaker 3: and air, which is slightly different than the speed light 143 00:07:23,600 --> 00:07:26,360 Speaker 3: and vacuum. And the fastest that we know that anything 144 00:07:26,400 --> 00:07:29,480 Speaker 3: can pass you by is the speed a light in vacuum, 145 00:07:29,480 --> 00:07:31,840 Speaker 3: and so we call that the speed of light, but 146 00:07:31,880 --> 00:07:35,240 Speaker 3: it really means fastest speed that we know of in 147 00:07:35,320 --> 00:07:38,000 Speaker 3: terms of something that has energy and mass can go. 148 00:07:38,800 --> 00:07:41,240 Speaker 2: Understand the speed of light is not just an exercise 149 00:07:41,320 --> 00:07:43,600 Speaker 2: in and of itself. I mean it helps to understand 150 00:07:43,920 --> 00:07:47,160 Speaker 2: the much bigger picture of the universe we live in 151 00:07:47,200 --> 00:07:48,640 Speaker 2: and the nature of reality. 152 00:07:48,800 --> 00:07:53,360 Speaker 3: Right, Yeah, so light is just a fundamental thing. It's 153 00:07:53,400 --> 00:07:57,440 Speaker 3: one of the used to dominate the universe. The photons 154 00:07:57,440 --> 00:07:59,280 Speaker 3: that the make up light used to have the most 155 00:07:59,400 --> 00:08:02,040 Speaker 3: energy in the unit. But now the universe has evolved 156 00:08:02,080 --> 00:08:06,200 Speaker 3: that the light has has become less comparatively energetic where 157 00:08:06,200 --> 00:08:08,800 Speaker 3: it's mass, and now something called dark energy have not 158 00:08:08,920 --> 00:08:13,000 Speaker 3: diluted like light. So now light is there's lots of 159 00:08:13,120 --> 00:08:17,400 Speaker 3: there's like billions of pieces of photons for every atom 160 00:08:17,600 --> 00:08:20,080 Speaker 3: in that we know of. But still the amount of 161 00:08:20,160 --> 00:08:23,600 Speaker 3: energy in light is down, has gone down down a lot, 162 00:08:24,320 --> 00:08:28,640 Speaker 3: and so now light is more isn't most useful for 163 00:08:28,800 --> 00:08:32,120 Speaker 3: its mass and its energy doesn't the energy it has, 164 00:08:32,160 --> 00:08:34,000 Speaker 3: it's most useful for what it can tell us because 165 00:08:34,040 --> 00:08:37,120 Speaker 3: it's acrossed the universe from far away, and so when 166 00:08:37,120 --> 00:08:39,600 Speaker 3: we look at it near and far and we can 167 00:08:39,640 --> 00:08:42,520 Speaker 3: try to decode what it is. Light was created someplace, 168 00:08:42,679 --> 00:08:45,560 Speaker 3: Light was reflected from someplace, was emitted in some place, 169 00:08:45,880 --> 00:08:48,800 Speaker 3: and we we we pieced together the universe from the 170 00:08:48,880 --> 00:08:50,120 Speaker 3: light we see pretty much. 171 00:08:51,640 --> 00:08:54,080 Speaker 2: You have some fun exercises in the book. There's no 172 00:08:54,120 --> 00:08:55,600 Speaker 2: way we can cover all of them, but one of 173 00:08:55,600 --> 00:08:57,960 Speaker 2: them early in the book is an aside where you 174 00:08:58,440 --> 00:09:00,640 Speaker 2: the title is nothing can go fast faster than light, 175 00:09:00,679 --> 00:09:03,240 Speaker 2: which is I think probably the general assumption that most 176 00:09:03,280 --> 00:09:06,400 Speaker 2: of us non scientists would suggest. But you say that, 177 00:09:06,440 --> 00:09:09,280 Speaker 2: if you were to head into local university and ask 178 00:09:09,360 --> 00:09:13,320 Speaker 2: a random physics student if anything or if shadows could 179 00:09:13,320 --> 00:09:15,120 Speaker 2: go faster than light, you're probably going to get an 180 00:09:15,120 --> 00:09:17,360 Speaker 2: answer no, nothing would go faster than light. But they'd 181 00:09:17,360 --> 00:09:18,199 Speaker 2: be wrong, right. 182 00:09:19,200 --> 00:09:23,839 Speaker 3: Yes, they would be wrong. So it's an amazing thing. 183 00:09:23,840 --> 00:09:28,319 Speaker 3: I've given talks and I've had you know, good physicists 184 00:09:28,320 --> 00:09:30,760 Speaker 3: in the audience object saying oh no, that can't happen, 185 00:09:30,800 --> 00:09:32,640 Speaker 3: and then when I try to detail it, they don't 186 00:09:32,679 --> 00:09:34,600 Speaker 3: even want to let me continue. So we get into 187 00:09:34,640 --> 00:09:37,840 Speaker 3: an awkward part where I say, oh no. But then 188 00:09:38,280 --> 00:09:44,000 Speaker 3: I think at another university that has justice prestigious scientists 189 00:09:44,040 --> 00:09:45,480 Speaker 3: and they a lot of it, they say, oh, yeah, this 190 00:09:45,559 --> 00:09:48,040 Speaker 3: is really interesting, this is really great. So yeah, if 191 00:09:48,080 --> 00:09:50,640 Speaker 3: you were to go to this experiment, you might find 192 00:09:50,679 --> 00:09:53,200 Speaker 3: people there who would seem to disagree with this, but 193 00:09:53,400 --> 00:09:55,199 Speaker 3: unless what you can do is you can tell them 194 00:09:55,280 --> 00:09:57,840 Speaker 3: to look up my articles, not only my articles, there 195 00:09:57,840 --> 00:10:01,160 Speaker 3: are other articles, and then to read this book. And 196 00:10:01,400 --> 00:10:05,400 Speaker 3: it really it makes it very clear and it's been 197 00:10:05,440 --> 00:10:08,720 Speaker 3: measured in the last too, that shadows and laser spots 198 00:10:08,760 --> 00:10:11,480 Speaker 3: and illumination fronts, like when you turn on the light 199 00:10:11,480 --> 00:10:14,120 Speaker 3: in the room, they all can move, and they do 200 00:10:14,240 --> 00:10:16,160 Speaker 3: move faster than life. 201 00:10:16,480 --> 00:10:18,840 Speaker 2: And you say, you write that you've submitted papers to 202 00:10:18,920 --> 00:10:23,440 Speaker 2: recognize physics journals and had them rejected because that editors say, 203 00:10:23,640 --> 00:10:25,720 Speaker 2: oh no, there's no way this paper is flawed because 204 00:10:25,760 --> 00:10:28,040 Speaker 2: nothing can go faster than light. They're wrong. 205 00:10:28,240 --> 00:10:32,160 Speaker 3: Yeah, that has happened too. So what happens is we 206 00:10:32,160 --> 00:10:35,800 Speaker 3: we have editors that know. So when you send in 207 00:10:36,320 --> 00:10:38,480 Speaker 3: use some research, you send it into a journal. So 208 00:10:38,600 --> 00:10:41,760 Speaker 3: the journal you send it into the editor signs an editor. 209 00:10:41,880 --> 00:10:44,240 Speaker 3: Then the editor has what's called referees. You can picture 210 00:10:44,240 --> 00:10:46,080 Speaker 3: there are scientists and sit around with stripes on them 211 00:10:46,080 --> 00:10:49,319 Speaker 3: and they advise the editor as to whether this piece 212 00:10:49,360 --> 00:10:51,959 Speaker 3: of science writing that was submitted to journal should be 213 00:10:52,000 --> 00:10:55,040 Speaker 3: published or not. Many things submitted to journals are not 214 00:10:55,160 --> 00:10:59,960 Speaker 3: published because the editor, on advice of the referee usually said, 215 00:11:00,080 --> 00:11:04,040 Speaker 3: oh no. So we now know for some journals some 216 00:11:04,320 --> 00:11:07,280 Speaker 3: editors are are cluing and they understand what we're doing 217 00:11:07,320 --> 00:11:09,400 Speaker 3: and that this is correct. But if we get the 218 00:11:09,400 --> 00:11:11,680 Speaker 3: wrong editor and the wrong editor submits it to the 219 00:11:11,720 --> 00:11:16,320 Speaker 3: wrong referee, then we just get back a wrote rejection 220 00:11:16,679 --> 00:11:19,480 Speaker 3: which we know to try to push pass. We try 221 00:11:19,520 --> 00:11:21,840 Speaker 3: to find we asked that editors send to a different 222 00:11:21,840 --> 00:11:26,240 Speaker 3: referee where we ask that another editor takeover. And so 223 00:11:27,280 --> 00:11:29,360 Speaker 3: since we are able to publish our stuff, that is 224 00:11:29,679 --> 00:11:33,640 Speaker 3: a successful tactic. But you're right, we've gotten just you know, 225 00:11:33,760 --> 00:11:36,280 Speaker 3: back an immediate thing saying oh no, this can't be 226 00:11:36,400 --> 00:11:39,680 Speaker 3: right because someone hasn't thought it through. They just they 227 00:11:39,880 --> 00:11:42,920 Speaker 3: remember some you know, some adage that says nothing to 228 00:11:43,000 --> 00:11:45,800 Speaker 3: go faster than light, but which is nothing can pack 229 00:11:45,840 --> 00:11:48,120 Speaker 3: with masks can pack you faster than lights. So far 230 00:11:48,160 --> 00:11:49,920 Speaker 3: as we know, we don't have any examples of that. 231 00:11:50,080 --> 00:11:53,720 Speaker 3: But shadows can go way, the spots can go, things 232 00:11:53,760 --> 00:11:56,520 Speaker 3: can go, and these things can be very very interesting 233 00:11:56,760 --> 00:11:58,880 Speaker 3: and tell us things about the universe that we didn't 234 00:11:58,920 --> 00:11:59,480 Speaker 3: know before. 235 00:12:00,360 --> 00:12:03,040 Speaker 2: Yeah, you have one experiment in the book that where 236 00:12:03,040 --> 00:12:05,280 Speaker 2: you point a laser pointer at the moon and it 237 00:12:05,360 --> 00:12:07,280 Speaker 2: can go. You can whip it around and it could 238 00:12:07,280 --> 00:12:10,160 Speaker 2: go faster than the speed of light RT. 239 00:12:10,240 --> 00:12:14,640 Speaker 3: Yeah. So one of my favorite favorite thought experiments, and 240 00:12:14,640 --> 00:12:17,000 Speaker 3: there's a lot of conceptual thought experiments in the book, 241 00:12:17,080 --> 00:12:20,120 Speaker 3: is let's say you're seat here on your here on Earth, 242 00:12:20,160 --> 00:12:23,480 Speaker 3: and let's say there is this big dome out one 243 00:12:23,559 --> 00:12:25,960 Speaker 3: light year away. So if it's one light year away, 244 00:12:26,040 --> 00:12:29,240 Speaker 3: it takes light a whole year to get there. So 245 00:12:29,400 --> 00:12:31,959 Speaker 3: now you have your laser pointer. Uh, so you take 246 00:12:31,960 --> 00:12:34,440 Speaker 3: your laser pointer and you point it at one spot 247 00:12:34,440 --> 00:12:37,040 Speaker 3: in the dome. And even though you point it there, 248 00:12:37,040 --> 00:12:39,080 Speaker 3: it's going to take a year for light to get there. 249 00:12:39,280 --> 00:12:41,640 Speaker 3: But then in one second, you take your laser pointer 250 00:12:41,760 --> 00:12:43,559 Speaker 3: and you shift it around to one hundred and eighty 251 00:12:43,600 --> 00:12:46,800 Speaker 3: degrees around to the to the other side of the dome. 252 00:12:47,360 --> 00:12:50,760 Speaker 3: So after a year that takes like to get there, 253 00:12:50,800 --> 00:12:53,240 Speaker 3: the laser spot will cross. We'll go all the way 254 00:12:53,280 --> 00:12:59,120 Speaker 3: around that dome in a second. But that dome has 255 00:12:59,360 --> 00:13:02,120 Speaker 3: has a rate, has a circumference greater than a light year, 256 00:13:02,160 --> 00:13:05,520 Speaker 3: So that spot is moving greater than a light year 257 00:13:05,559 --> 00:13:08,800 Speaker 3: in a second, which means the spot has a superluminal speed. 258 00:13:09,080 --> 00:13:12,840 Speaker 3: Now there's no information being created on the dome that's 259 00:13:12,920 --> 00:13:16,760 Speaker 3: moving on the dome faster than light. The laser spot 260 00:13:16,920 --> 00:13:19,800 Speaker 3: is the superposition of unrelated photons that are hitting at 261 00:13:19,800 --> 00:13:23,520 Speaker 3: different places, and so that is what is appearing appearing 262 00:13:23,760 --> 00:13:28,400 Speaker 3: to move faster than light. But yes, there's these things. 263 00:13:28,440 --> 00:13:30,079 Speaker 3: You know, we don't have a dome out at one 264 00:13:30,160 --> 00:13:33,920 Speaker 3: light year, but these thought experiments are very clear demonstrations 265 00:13:33,960 --> 00:13:37,520 Speaker 3: that things laser spots can move. So if you take 266 00:13:37,520 --> 00:13:39,760 Speaker 3: your laser spot, maybe we don't have a dome light 267 00:13:39,800 --> 00:13:42,360 Speaker 3: year away. What we do have is things that are 268 00:13:42,360 --> 00:13:44,680 Speaker 3: closer to the moon. If you just try your local 269 00:13:44,800 --> 00:13:46,679 Speaker 3: wall and you take your laser pointer and you s 270 00:13:46,679 --> 00:13:48,959 Speaker 3: creep it around the wall, you can't move your arm 271 00:13:49,040 --> 00:13:51,520 Speaker 3: fast enough to make it go faster than light. Unfortunately, 272 00:13:51,760 --> 00:13:53,920 Speaker 3: but the moon is far enough away that if you 273 00:13:53,960 --> 00:13:56,400 Speaker 3: take your laser pointer and you sweep it past the 274 00:13:56,440 --> 00:13:59,679 Speaker 3: moon at a reasonable speed not too fast, that that 275 00:13:59,720 --> 00:14:02,880 Speaker 3: layer spot, if you could see it, would move faster 276 00:14:02,920 --> 00:14:04,040 Speaker 3: than light across the moon. 277 00:14:05,440 --> 00:14:07,520 Speaker 2: You have a chapter that deals with how to make 278 00:14:07,559 --> 00:14:11,120 Speaker 2: a magnetic field move faster than light? So what is 279 00:14:11,160 --> 00:14:13,880 Speaker 2: there a simple answer to that, a simple explanation that 280 00:14:13,920 --> 00:14:14,840 Speaker 2: we would understand. 281 00:14:15,760 --> 00:14:20,560 Speaker 3: Well, that's a tough one because okay, yeah, the magnetic 282 00:14:20,640 --> 00:14:23,480 Speaker 3: kal minds are actually not something you can grab onto. 283 00:14:23,640 --> 00:14:28,600 Speaker 3: There are conceptual lines of h of uh that has 284 00:14:28,600 --> 00:14:31,240 Speaker 3: something to do with magnetism. So yeah, so we draw 285 00:14:31,320 --> 00:14:33,760 Speaker 3: them in and then when the ninetism changes, you turn 286 00:14:33,800 --> 00:14:35,880 Speaker 3: a magnet or something like that. Yeah, these magnetic kial 287 00:14:35,960 --> 00:14:38,760 Speaker 3: minds can can move faster than light. That that's very clear, 288 00:14:39,000 --> 00:14:41,720 Speaker 3: but it's not that easy to explain. So I did 289 00:14:41,800 --> 00:14:43,840 Speaker 3: could go do some effort in the book to do it, 290 00:14:43,960 --> 00:14:45,440 Speaker 3: but I don't know if that would work here in 291 00:14:45,480 --> 00:14:47,160 Speaker 3: the in the Coast to Coast forum. 292 00:14:47,200 --> 00:14:49,960 Speaker 2: Okay, very well, you know you do touch on here 293 00:14:50,000 --> 00:14:56,520 Speaker 2: and there the differences between relativity and quantum mechanics, and 294 00:14:57,000 --> 00:14:59,080 Speaker 2: try as I might to get my head around it, 295 00:14:59,160 --> 00:15:01,200 Speaker 2: I just can't do it. But it seems to be 296 00:15:01,320 --> 00:15:04,560 Speaker 2: a lot of what quantum mechanics concludes to be real 297 00:15:04,640 --> 00:15:07,640 Speaker 2: and true is at odds with what we think of 298 00:15:07,680 --> 00:15:10,080 Speaker 2: as relativity. I don't know how they coexist, but they. 299 00:15:10,000 --> 00:15:14,080 Speaker 3: Do, right, Yeah, so they are not in We don't 300 00:15:14,080 --> 00:15:18,120 Speaker 3: always know how they interact, and we're sometimes surprised. But 301 00:15:18,280 --> 00:15:22,560 Speaker 3: there is quantum mechanics does not contradict special relativity. In fact, 302 00:15:22,520 --> 00:15:28,960 Speaker 3: there's there are types of quantum mechanics, quantum electrodynamics and 303 00:15:28,960 --> 00:15:33,120 Speaker 3: and things like that that incorporates special relativity into them. 304 00:15:33,840 --> 00:15:37,960 Speaker 3: The classic quantum mechanics, the Schrodinger equation, it's called that 305 00:15:38,240 --> 00:15:41,880 Speaker 3: can be brought into conflict with the concepts of special relativity. 306 00:15:41,920 --> 00:15:46,680 Speaker 3: But physicists do know that special relativity is right and 307 00:15:46,720 --> 00:15:49,280 Speaker 3: that it does fit into quantum mechanics. But that doesn't 308 00:15:49,320 --> 00:15:52,880 Speaker 3: mean there's there's some really strange quantum mechanics experiments out 309 00:15:52,880 --> 00:15:57,080 Speaker 3: there that it appears that information is being transferred faster 310 00:15:57,120 --> 00:15:59,320 Speaker 3: than light, but it is not when it is when 311 00:15:59,320 --> 00:16:02,160 Speaker 3: it's looked at it very detailed, it's just the appearance 312 00:16:02,200 --> 00:16:04,960 Speaker 3: that it is. It's not really going faster than life. 313 00:16:05,000 --> 00:16:07,920 Speaker 3: And how that is is just absolutely fascinating. How it 314 00:16:08,040 --> 00:16:11,560 Speaker 3: seems like something on one side and something far away. 315 00:16:11,800 --> 00:16:14,040 Speaker 3: They seem like they know about each other, but they're 316 00:16:14,120 --> 00:16:17,320 Speaker 3: not communicating. And so if you look at the details 317 00:16:17,360 --> 00:16:18,920 Speaker 3: of it, which I try to explain in some of 318 00:16:18,960 --> 00:16:21,760 Speaker 3: the chapters in my book, you can see that there's 319 00:16:21,920 --> 00:16:25,720 Speaker 3: no real communication going on there. There's correlations which we 320 00:16:25,760 --> 00:16:28,720 Speaker 3: don't understand why this correlation, but there's no communication. 321 00:16:29,600 --> 00:16:32,880 Speaker 1: Listen to more Coast to Coast AM every weeknight at 322 00:16:32,880 --> 00:16:36,520 Speaker 1: oneam Eastern and go to Coast to coastam dot com 323 00:16:36,520 --> 00:16:36,960 Speaker 1: for more