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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:20,889 --> 00:00:23,968 Did our universe have a beginning? 2 00:00:23,969 --> 00:00:26,729 Why is there a universe like this one? 3 00:00:29,289 --> 00:00:35,449 If time began at the big bang, then was there a time before time? 4 00:00:36,769 --> 00:00:41,129 Why are there rivers and flows and filaments of galaxies? 5 00:00:42,169 --> 00:00:45,009 Is there an end of the universe? Is our universe eternal? 6 00:00:46,969 --> 00:00:50,048 I'm on tour in Australia, 7 00:00:50,049 --> 00:00:55,048 talking to audiences and scientists about two fundamental questions - 8 00:00:55,049 --> 00:00:56,688 how did the universe begin... 9 00:00:56,689 --> 00:00:59,088 Like in the big bang, it feels audacious. 10 00:00:59,089 --> 00:01:01,928 ...and how will it end? 11 00:01:01,929 --> 00:01:03,928 Life on earth will become very problematic. 12 00:01:03,929 --> 00:01:06,008 In the last decade, 13 00:01:06,009 --> 00:01:10,008 we've been able to probe these ideas in unprecedented detail. 14 00:01:10,009 --> 00:01:12,888 So, this IS the oldest light in the universe. 15 00:01:12,889 --> 00:01:15,528 This is the story of our scientific quest 16 00:01:15,529 --> 00:01:18,529 to understand the origin of the universe. 17 00:01:47,169 --> 00:01:50,168 Of all the questions in science, 18 00:01:50,169 --> 00:01:52,888 the question of the origin of the universe 19 00:01:52,889 --> 00:01:55,568 is one that I think needs no motivation. 20 00:01:55,569 --> 00:01:59,208 Every human culture has its own creation story, 21 00:01:59,209 --> 00:02:00,848 and science is no different. 22 00:02:00,849 --> 00:02:04,288 For the best part of 100 years, we've had the theory 23 00:02:04,289 --> 00:02:07,008 that the universe began in the big bang. 24 00:02:07,009 --> 00:02:09,488 But in the last decade or so, 25 00:02:09,489 --> 00:02:12,008 new precision measurements of the cosmos, 26 00:02:12,009 --> 00:02:14,568 coupled with theoretical developments, 27 00:02:14,569 --> 00:02:18,848 have given us an unprecedented and detailed picture 28 00:02:18,849 --> 00:02:20,969 of the origin of the universe. 29 00:02:31,129 --> 00:02:33,168 If this were a lesser program, 30 00:02:33,169 --> 00:02:35,648 we would start it in a deep voice going, 31 00:02:35,649 --> 00:02:39,968 "There was a time... with no time." 32 00:02:39,969 --> 00:02:45,568 "There was a place... not in space." 33 00:02:45,569 --> 00:02:51,208 "THAT is the time before time" 34 00:02:51,209 --> 00:02:54,728 "and place without space" 35 00:02:54,729 --> 00:02:56,809 "that we call the big bang." 36 00:02:57,849 --> 00:02:59,569 That's not what we're doing, though. 37 00:03:01,489 --> 00:03:03,008 I think if you ask the question, 38 00:03:03,009 --> 00:03:06,168 "WHY do you want to know the origins of the universe?" 39 00:03:06,169 --> 00:03:08,968 I suppose the answer has to be curiosity. 40 00:03:08,969 --> 00:03:12,328 It's surely something that must occur to everybody at some point - 41 00:03:12,329 --> 00:03:14,009 why do we exist? 42 00:03:21,009 --> 00:03:22,488 When I think of a scientist, 43 00:03:22,489 --> 00:03:26,928 I think of an adult who still has the soul of curiosity of a child. 44 00:03:26,929 --> 00:03:31,889 So I think it's very natural to ask, how did it all get here? 45 00:03:33,729 --> 00:03:36,688 Indigenous Australians have been observing the stars 46 00:03:36,689 --> 00:03:38,928 for more than 40,000 years, 47 00:03:38,929 --> 00:03:41,488 and, like many ancient cultures, 48 00:03:41,489 --> 00:03:45,289 have a number of creation stories based on the night sky. 49 00:03:46,449 --> 00:03:49,448 It's the story of 'arang' - the emu. 50 00:03:49,449 --> 00:03:51,568 The emu sacrificed his wings 51 00:03:51,569 --> 00:03:55,328 and was given an eternal place in the southern skies. 52 00:03:55,329 --> 00:04:00,328 Forever you will be seen running across the night sky 53 00:04:00,329 --> 00:04:04,809 and marked as 'dyurra' - the stars. 54 00:04:08,769 --> 00:04:10,888 I've always liked creation stories. 55 00:04:10,889 --> 00:04:14,168 I like reading about them from across the world. 56 00:04:14,169 --> 00:04:15,848 Why do we do it? 57 00:04:15,849 --> 00:04:20,088 Why do we build telescopes to look back to the edge of time? 58 00:04:20,089 --> 00:04:23,008 Why do we measure the expansion rate of the universe 59 00:04:23,009 --> 00:04:24,728 and build theories to explain it? 60 00:04:24,729 --> 00:04:29,048 But the answer is because that's what we've always done. 61 00:04:29,049 --> 00:04:30,768 And the evidence for that is 62 00:04:30,769 --> 00:04:36,049 that every culture you study across the world has a creation story. 63 00:04:38,129 --> 00:04:40,328 And the most wonderful thing 64 00:04:40,329 --> 00:04:43,128 about living in the 21st century, with modern science, 65 00:04:43,129 --> 00:04:46,169 is that we also have a creation story. 66 00:04:48,529 --> 00:04:51,209 You've probably heard it described as 'the big bang'. 67 00:04:53,689 --> 00:04:55,288 But what is the big bang? 68 00:04:55,289 --> 00:04:59,488 And what do we know about the origin of the universe? 69 00:04:59,489 --> 00:05:03,328 With observations and mathematical theorising, 70 00:05:03,329 --> 00:05:06,728 we have a good sense that about 13.8 billion years ago, 71 00:05:06,729 --> 00:05:11,088 the universe was incredibly dense and it was incredibly hot. 72 00:05:11,089 --> 00:05:14,128 Hot! Give me some heat! Give me some density! 73 00:05:14,129 --> 00:05:18,048 Give me some violations of the laws of particle physics. 74 00:05:18,049 --> 00:05:22,208 It underwent a rapid swelling that's called the big bang. 75 00:05:22,209 --> 00:05:23,768 So, what's the big bang? 76 00:05:23,769 --> 00:05:26,168 And the answer is I don't know what the big bang is. 77 00:05:26,169 --> 00:05:28,128 I just know what came after the big bang, 78 00:05:28,129 --> 00:05:31,368 where we have a universe that's expanding very quickly, 79 00:05:31,369 --> 00:05:32,888 it's really hot. 80 00:05:32,889 --> 00:05:34,808 These things, we do know. 81 00:05:34,809 --> 00:05:36,929 It's the things that come after that we understand. 82 00:05:38,649 --> 00:05:41,328 You can trace everything back and you get to a point 83 00:05:41,329 --> 00:05:44,328 where the universe had to have been hot and small and dense 84 00:05:44,329 --> 00:05:48,568 and something happened that made that expand, right? 85 00:05:48,569 --> 00:05:52,928 And so that's this idea that became known as 'the hot big bang'. 86 00:05:52,929 --> 00:05:54,328 I'm liking the big bang. 87 00:05:54,329 --> 00:05:57,049 That just feels right. It feels audacious. 88 00:05:59,969 --> 00:06:04,529 It's common to think of the big bang as the start of time itself. 89 00:06:07,209 --> 00:06:10,609 The moment when everything came from nothing. 90 00:06:12,769 --> 00:06:16,288 But there are cosmologists who think there may be more to it - 91 00:06:16,289 --> 00:06:19,248 that the thing we used to call 'the big bang' 92 00:06:19,249 --> 00:06:22,968 was an event in a pre-existing universe 93 00:06:22,969 --> 00:06:25,289 and not the beginning at all. 94 00:06:29,489 --> 00:06:32,008 But how can we be so confident? 95 00:06:32,009 --> 00:06:34,848 How can we even dare to speak of things 96 00:06:34,849 --> 00:06:37,769 that happened almost 14 billion years ago? 97 00:06:42,369 --> 00:06:45,928 In 1927, the astronomer Edwin Hubble noticed 98 00:06:45,929 --> 00:06:49,608 that the light from distant galaxies is stretched. 99 00:06:49,609 --> 00:06:54,928 That means that space is expanding - our universe is expanding. 100 00:06:54,929 --> 00:06:58,488 So, you run time backwards in your mind's eye, 101 00:06:58,489 --> 00:07:00,088 that means that in the past, 102 00:07:00,089 --> 00:07:02,808 the distances between the galaxies was smaller, 103 00:07:02,809 --> 00:07:06,488 and you can imagine a time when the distances were so small 104 00:07:06,489 --> 00:07:09,688 that everything is effectively on top of each other. 105 00:07:09,689 --> 00:07:14,048 That implies that our universe had a beginning, 106 00:07:14,049 --> 00:07:16,608 there was a day without a yesterday, 107 00:07:16,609 --> 00:07:19,289 and that is what we call the big bang. 108 00:07:20,449 --> 00:07:24,048 More than 30 years after Hubble made his observations, 109 00:07:24,049 --> 00:07:25,888 cosmologists remained divided 110 00:07:25,889 --> 00:07:28,928 about whether the big bang theory was correct. 111 00:07:28,929 --> 00:07:30,688 More evidence was needed. 112 00:07:30,689 --> 00:07:33,008 And it came in the 1960s, 113 00:07:33,009 --> 00:07:36,689 with the discovery of a mysterious faint signal. 114 00:07:38,369 --> 00:07:42,609 We call it the cosmic microwave background radiation. 115 00:07:43,929 --> 00:07:49,328 It's seen as a faint glow, coming literally from everywhere in the sky, 116 00:07:49,329 --> 00:07:54,529 but not being emitted from any particular star, galaxy or object. 117 00:07:56,809 --> 00:08:00,008 So, this is the oldest light in the universe. 118 00:08:00,009 --> 00:08:05,688 There are photons that have travelled 13.8 billion years from over there 119 00:08:05,689 --> 00:08:09,488 and 13.8 billion years from over there, 120 00:08:09,489 --> 00:08:13,249 and they're carrying information about the beginning of time. 121 00:08:14,329 --> 00:08:18,288 One of the many remarkable things about the cosmic microwave background 122 00:08:18,289 --> 00:08:20,608 is the story of its discovery, 123 00:08:20,609 --> 00:08:23,888 because it was found entirely by accident. 124 00:08:23,889 --> 00:08:28,048 We had this result. We couldn't find any explanation for it. 125 00:08:28,049 --> 00:08:31,809 We couldn't make it go away. What were we going to do with this thing? 126 00:08:34,649 --> 00:08:38,208 So, where did the cosmic microwave background come from? 127 00:08:38,209 --> 00:08:42,808 And why do we consider it such strong evidence for the big bang theory? 128 00:08:42,809 --> 00:08:47,288 So, the picture is this - the universe is expanding and cooling. 129 00:08:47,289 --> 00:08:50,688 In the first few minutes, it's extremely hot, 130 00:08:50,689 --> 00:08:53,728 and then the universe is filled by what's called a plasma - 131 00:08:53,729 --> 00:08:56,968 so, it's too hot for atoms to form. 132 00:08:56,969 --> 00:09:01,088 380,000 years after the big bang, it's cool enough for atoms to form, 133 00:09:01,089 --> 00:09:05,168 the universe becomes almost instantly transparent, 134 00:09:05,169 --> 00:09:07,048 so light can travel in straight lines, 135 00:09:07,049 --> 00:09:09,848 and it will continue to travel in straight lines 136 00:09:09,849 --> 00:09:12,648 for the rest of the expansion history of the universe 137 00:09:12,649 --> 00:09:17,649 and it can enter our telescopes here on Earth 13.8 billion years later. 138 00:09:19,409 --> 00:09:23,248 The cosmic microwave background is considered such strong evidence 139 00:09:23,249 --> 00:09:24,728 in large part because 140 00:09:24,729 --> 00:09:28,208 the big bang theory predicted that it should exist. 141 00:09:28,209 --> 00:09:31,088 It was first observed in the mid-1960s, 142 00:09:31,089 --> 00:09:34,288 and it's only then, really, just before I was born, 143 00:09:34,289 --> 00:09:39,448 that the idea that the universe began at a hot, dense origin 144 00:09:39,449 --> 00:09:41,008 really took hold. 145 00:09:41,009 --> 00:09:43,968 It's an almost overwhelming piece of evidence, 146 00:09:43,969 --> 00:09:48,408 because you're seeing the afterglow of that earliest of times. 147 00:09:48,409 --> 00:09:50,928 We can take pictures of that light in great detail now. 148 00:09:50,929 --> 00:09:52,568 We don't see it as a hum. 149 00:09:52,569 --> 00:09:55,808 We can photograph, essentially, the universe as it was, 150 00:09:55,809 --> 00:09:59,128 the whole sky looking out into the universe, 151 00:09:59,129 --> 00:10:02,649 and see it as it was when that first light was released. 152 00:10:04,849 --> 00:10:08,088 This remarkable baby photograph of the universe 153 00:10:08,089 --> 00:10:11,128 confirmed that we had the basics right. 154 00:10:11,129 --> 00:10:14,888 But its great detail presented fresh challenges. 155 00:10:14,889 --> 00:10:16,968 As we often find with science, 156 00:10:16,969 --> 00:10:21,489 when you answer one set of questions, new ones arise. 157 00:10:24,729 --> 00:10:28,448 This idea that the universe had a beginning in the big bang 158 00:10:28,449 --> 00:10:31,328 is in some ways unsatisfactory. 159 00:10:31,329 --> 00:10:34,728 It raises a series of childlike questions. 160 00:10:34,729 --> 00:10:37,168 Like, if the universe had a beginning, 161 00:10:37,169 --> 00:10:39,008 then what happened before the beginning? 162 00:10:39,009 --> 00:10:40,528 What caused it? 163 00:10:40,529 --> 00:10:45,408 If time emerged at the big bang, then was there a time before time? 164 00:10:45,409 --> 00:10:50,449 How can the universe appear spontaneously out of nothing at all? 165 00:10:55,369 --> 00:10:57,448 Was there a before? 166 00:10:57,449 --> 00:10:59,728 Well, that is a philosophical question, 167 00:10:59,729 --> 00:11:02,448 unless you can come up with a theory 168 00:11:02,449 --> 00:11:05,449 that predicts something that you can test against observation. 169 00:11:10,689 --> 00:11:13,008 The clues which point the way to a theory 170 00:11:13,009 --> 00:11:15,328 of what came before the big bang 171 00:11:15,329 --> 00:11:19,568 can be found in problems with the big bang theory itself. 172 00:11:19,569 --> 00:11:23,968 There are two problems with the standard big bang model. 173 00:11:23,969 --> 00:11:27,288 They're called the horizon problem and the flatness problem. 174 00:11:27,289 --> 00:11:32,088 You can picture the horizon problem as follows. 175 00:11:32,089 --> 00:11:37,128 If you look at the universe as far as the eye can see in that direction, 176 00:11:37,129 --> 00:11:40,368 which is to say the cosmic microwave background, 177 00:11:40,369 --> 00:11:45,648 then it's the same temperature to one part in 100,000 178 00:11:45,649 --> 00:11:49,688 as the universe as far as the eye can see in that direction, 179 00:11:49,689 --> 00:11:52,608 which is the cosmic microwave background. 180 00:11:52,609 --> 00:11:56,648 But those two points on the sky are separated today 181 00:11:56,649 --> 00:12:00,168 by 90 billion light-years. 182 00:12:00,169 --> 00:12:05,008 That means if you've got a universe that's been expanding sedately 183 00:12:05,009 --> 00:12:07,648 and is only 13.8 billion years old, 184 00:12:07,649 --> 00:12:11,609 those two points could never have been in contact with each other. 185 00:12:13,209 --> 00:12:15,808 Which means there's no explanation 186 00:12:15,809 --> 00:12:19,609 for how they could be so precisely the same. 187 00:12:21,129 --> 00:12:23,328 And then there's the flatness problem. 188 00:12:23,329 --> 00:12:28,048 When you look at our universe, it appears to be completely flat. 189 00:12:28,049 --> 00:12:29,888 Which seems very strange, 190 00:12:29,889 --> 00:12:33,608 because it could have been curved like the surface of a sphere 191 00:12:33,609 --> 00:12:37,288 or curved like the surface of a saddle. 192 00:12:37,289 --> 00:12:41,968 A solution can be found in a theory known as inflation, 193 00:12:41,969 --> 00:12:45,848 which suggests that there was a time in the history of the universe 194 00:12:45,849 --> 00:12:50,288 when the universe wasn't just expanding sedately as it is today - 195 00:12:50,289 --> 00:12:53,089 it was expanding incredibly fast. 196 00:12:55,049 --> 00:12:58,488 By "fast", I mean that it was doubling in size 197 00:12:58,489 --> 00:13:01,928 every 10 to the -37 seconds. 198 00:13:01,929 --> 00:13:06,248 That's one ten-million-million- million-million-million-millionths 199 00:13:06,249 --> 00:13:07,769 of a second. 200 00:13:13,129 --> 00:13:16,728 Why does that solve the horizon and flatness problems? 201 00:13:16,729 --> 00:13:22,048 Well, first of all, it suggests the universe has to be extremely big - 202 00:13:22,049 --> 00:13:25,368 way bigger than the piece we can see today. 203 00:13:25,369 --> 00:13:27,929 And that means that it's always gonna look flat. 204 00:13:29,249 --> 00:13:31,768 Think about an analogy with the surface of the Earth. 205 00:13:31,769 --> 00:13:35,088 This little piece of the Earth here looks flat, 206 00:13:35,089 --> 00:13:37,888 even though we know the Earth's curved. 207 00:13:37,889 --> 00:13:42,488 Why? Because it's very small compared to the size of the Earth. 208 00:13:42,489 --> 00:13:47,008 So it is, according to the theory of inflation, for our universe. 209 00:13:47,009 --> 00:13:49,448 It also solves our horizon problem, 210 00:13:49,449 --> 00:13:52,688 because it says that that piece of the sky, 211 00:13:52,689 --> 00:13:55,288 which is so far away from that piece, 212 00:13:55,289 --> 00:13:57,848 were once in contact with each other. 213 00:13:57,849 --> 00:14:00,928 They could jiggle around and get to the same temperature, 214 00:14:00,929 --> 00:14:02,809 but then they were ripped apart. 215 00:14:08,129 --> 00:14:10,248 It's mind-boggling, 216 00:14:10,249 --> 00:14:15,008 but it's important to say that if we are right about inflation, 217 00:14:15,009 --> 00:14:18,888 then this violent rapid expansion must have occurred 218 00:14:18,889 --> 00:14:22,169 BEFORE the thing we used to call 'the big bang'. 219 00:14:23,969 --> 00:14:26,848 So, what is our current theory? 220 00:14:26,849 --> 00:14:28,208 This theory called inflation 221 00:14:28,209 --> 00:14:30,888 that says there was something going on before, 222 00:14:30,889 --> 00:14:34,048 I suppose that thing we used to call 'the big bang', or is that... 223 00:14:34,049 --> 00:14:36,008 Yeah, yeah, the hot big bang. 224 00:14:36,009 --> 00:14:38,688 I make that distinction by saying "hot big bang" versus "big bang", 225 00:14:38,689 --> 00:14:41,128 because 'hot big bang' does imply, sort of, 226 00:14:41,129 --> 00:14:43,648 the universe is in a fireball kind of state. 227 00:14:43,649 --> 00:14:44,928 Yeah. 228 00:14:44,929 --> 00:14:47,888 Yeah, the reason we know that something happened before 229 00:14:47,889 --> 00:14:51,368 is we can look at that primordial fireball state. 230 00:14:51,369 --> 00:14:52,928 Like, we can actually see it. 231 00:14:52,929 --> 00:14:54,848 Because we can see the cosmic microwave background, 232 00:14:54,849 --> 00:14:58,248 which is the, sort of, afterglow of that time 233 00:14:58,249 --> 00:15:00,288 when the whole universe was hot and dense. 234 00:15:00,289 --> 00:15:03,488 The, sort of, important point there is that it was expanding so fast 235 00:15:03,489 --> 00:15:06,128 that things that were connected to each other before, 236 00:15:06,129 --> 00:15:07,888 close enough together to communicate, 237 00:15:07,889 --> 00:15:10,288 to come into equilibrium, to be the same temperature, 238 00:15:10,289 --> 00:15:12,288 rapidly come out of contact. Yeah. 239 00:15:12,289 --> 00:15:14,808 And so that's why now when we look at the sky 240 00:15:14,809 --> 00:15:17,648 and we see that two different parts of the universe 241 00:15:17,649 --> 00:15:19,928 that should never have been in contact with each other 242 00:15:19,929 --> 00:15:21,288 are the same temperature, 243 00:15:21,289 --> 00:15:23,728 it's because you can dial back the expansion 244 00:15:23,729 --> 00:15:26,128 and find that they were never in contact, 245 00:15:26,129 --> 00:15:28,488 but then there's this extra secret time at the beginning 246 00:15:28,489 --> 00:15:30,208 where they did communicate, 247 00:15:30,209 --> 00:15:32,848 and then they just were, sort of, pulled apart so quickly 248 00:15:32,849 --> 00:15:36,248 that, you know, we can only infer that that happened 249 00:15:36,249 --> 00:15:40,089 by the fact that they must have been in contact at some point. 250 00:15:41,569 --> 00:15:44,968 So inflation leads to a massive universe. 251 00:15:44,969 --> 00:15:50,088 Galaxies way beyond the horizon, way beyond the part that we can see, 252 00:15:50,089 --> 00:15:52,448 possibly infinite in extent. 253 00:15:52,449 --> 00:15:54,448 And that's one of the things inflation does. 254 00:15:54,449 --> 00:15:58,248 So, it tell us that the universe should be significantly bigger 255 00:15:58,249 --> 00:15:59,969 than the patch we can see. 256 00:16:06,129 --> 00:16:08,408 Uh, look, I'll probably just stop 257 00:16:08,409 --> 00:16:09,888 and have a look at the stars on the way home. 258 00:16:09,889 --> 00:16:11,888 It was... yeah, it was really mind-expanding stuff. 259 00:16:11,889 --> 00:16:14,808 Did you understand it all? I wouldn't say I understood it ALL. 260 00:16:14,809 --> 00:16:16,288 Excellent. Very good show. Yes. 261 00:16:16,289 --> 00:16:18,168 Did you understand it all? No. 262 00:16:18,169 --> 00:16:19,929 I'm so confused! 263 00:16:21,809 --> 00:16:24,208 After entertaining the people of Canberra, 264 00:16:24,209 --> 00:16:28,208 I've made my way to Tidbinbilla, just outside the capital. 265 00:16:28,209 --> 00:16:30,568 It's home to one of the most important 266 00:16:30,569 --> 00:16:32,888 deep-space tracking stations on earth, 267 00:16:32,889 --> 00:16:36,728 and it's a must-see for an astronomy geek like me. 268 00:16:36,729 --> 00:16:39,368 I always find these places exciting. 269 00:16:39,369 --> 00:16:42,528 If you're a space geek... ..and you look out here, 270 00:16:42,529 --> 00:16:44,288 that big dish you can see 271 00:16:44,289 --> 00:16:48,568 is the only dish in the world that can talk to Voyager 2. 272 00:16:48,569 --> 00:16:52,328 So, that iconic spacecraft, I've followed that since 1977, 273 00:16:52,329 --> 00:16:53,888 since I was nine years old. 274 00:16:53,889 --> 00:16:58,048 We're still in contact with it now, beyond the edge of the solar system, 275 00:16:58,049 --> 00:17:02,008 with its tiny transmitter - about 16 watts of power, 276 00:17:02,009 --> 00:17:05,288 and THAT dish is the way that we talk to Voyager. 277 00:17:05,289 --> 00:17:09,568 AND - in the background is a famous dish. 278 00:17:09,569 --> 00:17:13,328 It's called Honeysuckle, and that dish is the Apollo dish. 279 00:17:13,329 --> 00:17:15,928 So, when you hear Apollo 11 on the moon 280 00:17:15,929 --> 00:17:18,488 and you hear the last words of NASA 281 00:17:18,489 --> 00:17:20,888 as Apollo 13 came back into the atmosphere, 282 00:17:20,889 --> 00:17:23,808 the last contact as it re-entered and the last words you hear 283 00:17:23,809 --> 00:17:25,888 is, "Lost contact at Honeysuckle" - 284 00:17:25,889 --> 00:17:28,368 and that dish through the trees is that dish. 285 00:17:28,369 --> 00:17:30,569 Farewell, Aquarius, and we thank you. 286 00:17:32,649 --> 00:17:36,409 OK, IOS in a minute or a minute and a half. 287 00:17:37,569 --> 00:17:39,089 It's exciting. 288 00:17:40,929 --> 00:17:43,409 - And welcome home. - Thank you. 289 00:17:52,409 --> 00:17:54,568 Well, it's all very well saying that the universe underwent 290 00:17:54,569 --> 00:17:58,048 a period of rapid expansion sometime before the big bang, 291 00:17:58,049 --> 00:18:03,968 but we need some kind of mechanism that might cause that to happen. 292 00:18:03,969 --> 00:18:06,928 And we have one - off the shelf, if you like - 293 00:18:06,929 --> 00:18:08,528 from particle physics. 294 00:18:08,529 --> 00:18:10,689 It's a thing called a scalar field. 295 00:18:11,929 --> 00:18:17,488 You could picture it as a sort of still ocean filling space, 296 00:18:17,489 --> 00:18:19,529 and we call it the inflaton field. 297 00:18:22,369 --> 00:18:24,328 The thing about that type of field 298 00:18:24,329 --> 00:18:26,968 is we know it had to go away at some point, 299 00:18:26,969 --> 00:18:29,368 or else the universe would still be exponentially expanding. 300 00:18:29,369 --> 00:18:31,448 If you have an energy 301 00:18:31,449 --> 00:18:34,728 that is uniformly spread out through a region of space, 302 00:18:34,729 --> 00:18:38,488 it can yield a new kind of gravity - repulsive gravity. 303 00:18:38,489 --> 00:18:41,968 Gravity that doesn't pull things together but pushes things apart. 304 00:18:41,969 --> 00:18:46,648 So, they presuppose that this kind of... fuel, if you would, 305 00:18:46,649 --> 00:18:48,168 called the inflaton field, 306 00:18:48,169 --> 00:18:51,328 but it's like a fuel that generates this repulsive gravity, 307 00:18:51,329 --> 00:18:54,769 is what drove the universe to start expanding in the first place. 308 00:18:57,849 --> 00:19:01,608 The idea that inflation is driven by the inflaton field 309 00:19:01,609 --> 00:19:04,488 leads to one of the most remarkable predictions 310 00:19:04,489 --> 00:19:06,328 in the history of cosmology - 311 00:19:06,329 --> 00:19:09,848 which is supported by observation. 312 00:19:09,849 --> 00:19:12,128 Now, you can think of the inflaton field 313 00:19:12,129 --> 00:19:16,288 as a sort of a still ocean filling space, 314 00:19:16,289 --> 00:19:21,368 but quantum theory tells us there's no such thing as a still ocean - 315 00:19:21,369 --> 00:19:24,169 every ocean has ripples in it. 316 00:19:26,049 --> 00:19:28,808 Now, what do those ripples correspond to? 317 00:19:28,809 --> 00:19:31,088 They mean that the inflaton field 318 00:19:31,089 --> 00:19:35,088 is a little bit bigger in some regions than others. 319 00:19:35,089 --> 00:19:37,848 So that means that at the end of inflation 320 00:19:37,849 --> 00:19:39,608 and at the start of the big bang, 321 00:19:39,609 --> 00:19:42,208 some bits of the universe will have expanded 322 00:19:42,209 --> 00:19:43,968 a little bit more than others 323 00:19:43,969 --> 00:19:47,928 and they will be a little less dense than the others. 324 00:19:47,929 --> 00:19:52,048 So, at the big bang, you get a very natural prediction 325 00:19:52,049 --> 00:19:56,448 that some regions of the universe are slightly denser 326 00:19:56,449 --> 00:19:58,409 than other regions of the universe. 327 00:20:01,729 --> 00:20:04,848 Now, imagine what happens as this universe expands and cools. 328 00:20:04,849 --> 00:20:07,888 Those denser regions get denser, 329 00:20:07,889 --> 00:20:13,008 and eventually, they collapse to form the galaxies, the stars. 330 00:20:13,009 --> 00:20:15,088 The fluctuations in the early universe 331 00:20:15,089 --> 00:20:17,488 led to the structures that we see today - 332 00:20:17,489 --> 00:20:19,208 including, of course, us. 333 00:20:19,209 --> 00:20:23,449 Without those seeds, without that structure, we wouldn't exist. 334 00:20:32,729 --> 00:20:36,168 Although inflationary cosmology does have its critics, 335 00:20:36,169 --> 00:20:40,448 this idea that the universe underwent a violent expansion 336 00:20:40,449 --> 00:20:43,088 before the hot big bang 337 00:20:43,089 --> 00:20:45,369 is now accepted by many cosmologists. 338 00:20:46,409 --> 00:20:49,888 But a more speculative addition to the theory exists, 339 00:20:49,889 --> 00:20:54,368 and it opens the doors to an intriguing possibility - 340 00:20:54,369 --> 00:20:58,368 ours may not be the only universe. 341 00:20:58,369 --> 00:21:01,528 If the theory of inflation is correct, 342 00:21:01,529 --> 00:21:03,448 then you could ask the question, 343 00:21:03,449 --> 00:21:07,528 how long was inflation going on for before the big bang? 344 00:21:07,529 --> 00:21:09,448 And the answer is we don't know. 345 00:21:09,449 --> 00:21:12,888 We have a minimum time, which is quite short, actually - 346 00:21:12,889 --> 00:21:16,448 about 10 to the -35 seconds or so - 347 00:21:16,449 --> 00:21:18,888 but it could have been much longer than that. 348 00:21:18,889 --> 00:21:20,808 And so you ask the question, 349 00:21:20,809 --> 00:21:23,888 could it have been going on for an indefinite period of time? 350 00:21:23,889 --> 00:21:26,648 Could you push the origin of the universe 351 00:21:26,649 --> 00:21:30,168 back and back and back into the infinite past, 352 00:21:30,169 --> 00:21:32,168 so we have an eternal universe? 353 00:21:32,169 --> 00:21:36,848 The answer is we don't know. There's theoretical speculation either way. 354 00:21:36,849 --> 00:21:41,528 But imagine if the universe IS in fact eternal. 355 00:21:41,529 --> 00:21:43,289 There may not have BEEN a beginning. 356 00:21:50,409 --> 00:21:52,608 So, this picture of inflation, 357 00:21:52,609 --> 00:21:54,928 I suppose there are two ways of looking at it. 358 00:21:54,929 --> 00:21:57,888 There's one that this universe is all there is 359 00:21:57,889 --> 00:22:00,848 and it inflates and then slows down and... there we are, 360 00:22:00,849 --> 00:22:04,288 but there are other possibilities, aren't there? 361 00:22:04,289 --> 00:22:05,888 Yeah, for sure. 362 00:22:05,889 --> 00:22:07,488 And the other possibilities suggest 363 00:22:07,489 --> 00:22:10,968 that we're one of a grand collection of universes - 364 00:22:10,969 --> 00:22:12,368 we're part of a multiverse. 365 00:22:12,369 --> 00:22:15,928 And again, it's not an idea that comes out of wild theorising, 366 00:22:15,929 --> 00:22:17,568 it comes right from the math. 367 00:22:17,569 --> 00:22:20,288 You see, when you try to explain 368 00:22:20,289 --> 00:22:22,968 how the universe - say, our universe - got started, 369 00:22:22,969 --> 00:22:27,288 and you have this repulsive gravity coming from the inflaton field, 370 00:22:27,289 --> 00:22:29,448 it causes space to expand, 371 00:22:29,449 --> 00:22:32,608 but the math shows that it's such an efficient process 372 00:22:32,609 --> 00:22:36,448 that you can virtually never fully use up the fuel 373 00:22:36,449 --> 00:22:38,688 that generated our expansion, 374 00:22:38,689 --> 00:22:41,768 so our big bang happens, but there's still some fuel left over. 375 00:22:41,769 --> 00:22:44,608 What does it do? It can generate ANOTHER big bang. 376 00:22:44,609 --> 00:22:46,288 So you get this wonderful process 377 00:22:46,289 --> 00:22:49,488 of big bang after big bang after big bang, 378 00:22:49,489 --> 00:22:52,888 yielding universe after universe after universe. 379 00:22:52,889 --> 00:22:55,248 And that's just this natural outcome 380 00:22:55,249 --> 00:22:58,168 of trying to explain the big bang in OUR universe. 381 00:22:58,169 --> 00:23:00,048 You're naturally led to the possibility 382 00:23:00,049 --> 00:23:02,289 that it simply is not a one-time event. 383 00:23:06,649 --> 00:23:08,208 Well, here is Earth, 384 00:23:08,209 --> 00:23:09,888 and we would think it's special, 385 00:23:09,889 --> 00:23:12,008 because we happen to be pretty close to it, 386 00:23:12,009 --> 00:23:14,968 then you realise, "Oh, it's one of eight planets." 387 00:23:14,969 --> 00:23:16,808 "But our sun..." 388 00:23:16,809 --> 00:23:20,128 "No, no, it's one of 100 billion other suns." 389 00:23:20,129 --> 00:23:21,528 "The galaxy...!" 390 00:23:21,529 --> 00:23:24,688 "No, it's one of 100 billion galaxies." 391 00:23:24,689 --> 00:23:26,288 "The universe!" 392 00:23:26,289 --> 00:23:29,648 Well, is it just gonna stop there and we have only one universe? 393 00:23:29,649 --> 00:23:31,888 The trend line tells us, 394 00:23:31,889 --> 00:23:34,649 why shouldn't there be multiple universes? 395 00:23:41,329 --> 00:23:45,448 If you look out onto this universe, the one in which we live, 396 00:23:45,449 --> 00:23:49,728 and you ask the question, could it have been any different? 397 00:23:49,729 --> 00:23:52,488 What would it have looked like if gravity was a bit stronger? 398 00:23:52,489 --> 00:23:54,688 Or there was a little more dark energy? 399 00:23:54,689 --> 00:23:58,888 Or the force of electromagnetism was a little bit weaker? 400 00:23:58,889 --> 00:24:03,489 Very quickly, you get to a universe which would not permit life to exist. 401 00:24:04,849 --> 00:24:08,088 So it's a legitimate question to ask - are we lucky? 402 00:24:08,089 --> 00:24:12,808 But in theories that allow you to have multiple universes, 403 00:24:12,809 --> 00:24:15,448 such as the inflationary multiverse, 404 00:24:15,449 --> 00:24:17,848 then it CAN be the case 405 00:24:17,849 --> 00:24:21,528 that the different bubble-universes have different laws of physics 406 00:24:21,529 --> 00:24:23,288 and it CAN be the case 407 00:24:23,289 --> 00:24:26,928 that the mechanism that produces those universes 408 00:24:26,929 --> 00:24:28,928 provides a very natural way 409 00:24:28,929 --> 00:24:32,328 of exploring the landscape of the laws of physics. 410 00:24:32,329 --> 00:24:34,928 So that then means that we're not lucky at all, 411 00:24:34,929 --> 00:24:36,888 our existence is inevitable, 412 00:24:36,889 --> 00:24:40,808 because every possible universe with every possible combination 413 00:24:40,809 --> 00:24:43,888 of physical constants and dark energy and masses of the particles - 414 00:24:43,889 --> 00:24:46,368 every one exists. 415 00:24:46,369 --> 00:24:50,808 And not only that, but every one of those is being created 416 00:24:50,809 --> 00:24:53,208 essentially an infinite number of times 417 00:24:53,209 --> 00:24:56,608 and will go on being created into the indefinite future. 418 00:24:56,609 --> 00:24:59,768 And THAT is the inflationary multiverse. 419 00:24:59,769 --> 00:25:02,849 So it says our existence is inevitable. 420 00:25:04,529 --> 00:25:06,569 "How does that make you feel?" 421 00:25:12,649 --> 00:25:16,208 We may never know if our existence is inevitable. 422 00:25:16,209 --> 00:25:20,968 We may never have a complete theory of the origin of the universe. 423 00:25:20,969 --> 00:25:24,969 But it is remarkable that we've made so much progress. 424 00:25:28,529 --> 00:25:30,448 The big bang as we see it 425 00:25:30,449 --> 00:25:32,888 was created in a very special way. 426 00:25:32,889 --> 00:25:36,648 The present understanding is that inflation can do that. 427 00:25:36,649 --> 00:25:40,288 So... that's what I would hang my hat on right now. 428 00:25:40,289 --> 00:25:42,248 But I wouldn't be surprised 429 00:25:42,249 --> 00:25:46,208 if there are changes in the future in our understanding. 430 00:25:46,209 --> 00:25:49,768 One day, some smart person will come along and solve it for you. 431 00:25:49,769 --> 00:25:53,128 That's the beautiful thing of how science works. 432 00:25:53,129 --> 00:25:55,048 The set of questions we're asking now 433 00:25:55,049 --> 00:25:58,448 get us to a new vista, a new place to stand, 434 00:25:58,449 --> 00:26:00,008 and on a new place to stand, 435 00:26:00,009 --> 00:26:02,168 there are other questions we haven't even dreamt of yet 436 00:26:02,169 --> 00:26:03,888 that I'm sure will be more important 437 00:26:03,889 --> 00:26:05,809 than whatever we think we're answering today. 438 00:26:08,129 --> 00:26:11,888 I think cosmology is the most remarkable of the sciences. 439 00:26:11,889 --> 00:26:15,088 I mean, not only are we able to look up into the sky 440 00:26:15,089 --> 00:26:19,328 and collect the light from the most distant galaxies, 441 00:26:19,329 --> 00:26:22,608 and even - in the form of the cosmic microwave background - 442 00:26:22,609 --> 00:26:25,808 from close to the origin of the universe itself, 443 00:26:25,809 --> 00:26:29,648 but we're able to decode the messages that it contains 444 00:26:29,649 --> 00:26:34,888 and build plausible theories of the origin of the universe. 445 00:26:34,889 --> 00:26:38,288 You know, I think our situation was beautifully summed up 446 00:26:38,289 --> 00:26:41,408 by the Belgian priest and mathematician Georges Lemaitre, 447 00:26:41,409 --> 00:26:44,248 one of the fathers of the big bang theory. 448 00:26:44,249 --> 00:26:47,768 He said, "Standing on a well-cooled cinder," 449 00:26:47,769 --> 00:26:50,368 "we see the slow fading of the suns" 450 00:26:50,369 --> 00:26:53,808 "and try to recall the vanished brilliance" 451 00:26:53,809 --> 00:26:56,169 "of the origin of the worlds." 452 00:27:11,689 --> 00:27:14,689 Is there an end of the universe? Is our universe eternal? 453 00:27:16,409 --> 00:27:18,809 The universe literally tears itself apart. 454 00:27:19,889 --> 00:27:22,809 Will there be stars and galaxies? 455 00:27:24,009 --> 00:27:27,889 What is the fate of the universe? How will it all end? 456 00:27:36,769 --> 00:27:38,728 Captions by Ericsson Access Services 457 00:27:38,729 --> 00:27:41,288 Copyright Australian Broadcasting Corporation 39011

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