The following is a summary and article by AI based on a transcript of the video "The Universe’s Second, Bigger Bang". Due to the limitations of AI, please be careful to distinguish the correctness of the content.
00:00 | Nearly 100 years ago, we started telling ourselves a particular story |
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00:04 | about the beginning of everything. |
00:05 | And it’s a story that starts with a hot, unthinkably dense ball of matter, |
00:10 | and ends with right now. |
00:12 | You probably know it best as the Big Bang Theory. |
00:15 | And while different scientists may play around with slightly different versions of it, |
00:19 | it does a pretty solid job of explaining all the stuff we see in the universe today. |
00:23 | But there’s a lot of stuff we don’t see, too. |
00:26 | Like, after the Big Bang Theory first came about, |
00:28 | our picture of the universe expanded to include a strange substance called dark matter, |
00:33 | whose presence we can detect, but not the stuff itself. |
00:36 | And so far, this mysterious form of matter has just been folded into the Big Bang. |
00:40 | Most theoretical astrophysicists have carried on assuming |
00:43 | that everything popped into existence during that one moment. |
00:47 | But what if this story we’ve told ourselves for generations…about how stars and planets |
00:51 | and galaxies came to be…isn’t true for their dark matter cousins? |
00:56 | Recently, some scientists have proposed that the Big Bang was followed by a |
01:00 | “dark Big Bang,” which not only spawned all the matter belonging to this |
01:03 | dark sector of reality, but spawned more matter than was made in the original. |
01:08 | And if they’re right, studying the Universe’s second, |
01:11 | bigger bang could help us solve the mystery of what dark matter even is. |
01:15 | [♪ INTRO] |
01:19 | Now before we can talk about the Dark Big Bang, |
01:21 | we need to talk about the original Big Bang. |
01:23 | In 1931, a Belgian scientist/priest named Georges Lemaître |
01:28 | made a simple conclusion. |
01:30 | Because humanity had recently discovered that the universe was expanding, |
01:34 | as opposed to just always being there, and all he needed to do was hit rewind. |
01:38 | The universe got smaller and smaller until he hit the beginning of time. |
01:42 | So Lemaître proposed a “primeval atom.” |
01:45 | A super dense point that had the whole universe packed inside it. |
01:49 | And some version of that has been our universe origin story ever since. |
01:53 | In the early days, scientists hypothesized that the universe’s energy started off |
01:57 | packed inside a singularity, an infinitely dense, hot point. |
02:01 | And in this version of the story, the Big Bang was the moment |
02:04 | when that singularity exploded to create the universe. |
02:08 | That story explained the expanding universe pretty well overall, |
02:11 | but it came with some thorny problems. |
02:14 | Like the fact that the very concept of an infinitely dense point just… |
02:18 | doesn’t exist physically. |
02:19 | And if you take our best models of the universe |
02:21 | and try to rewind the clock all the way to zero, the whole thing breaks before it gets there. |
02:26 | The laws of physics spit out nonsense. |
02:29 | So the modern concept of the Big Bang is a little different. |
02:33 | It puts the Big Bang after a brief period in the universe’s ancient history called inflation. |
02:38 | In this version of the story, there was a sliver of a second at the beginning of time when |
02:43 | the universe expanded exponentially in size, and it did so faster than the speed of light. |
02:48 | No one knows what triggered this inflation or what came before it. |
02:52 | But within less than a billionth of a billionth of a trillionth of a second, it was over. |
02:57 | And it was only then that all the energy driving this breakneck expansion |
03:02 | turned into matter and light, giving way to the Big Bang, |
03:05 | and giving rise to all the stuff that is out there, today. |
03:08 | The thing is, the picture gets a little fuzzy when we try to extend it |
03:11 | to the stuff we can’t see, which makes up a big piece of the pie. |
03:15 | For example, for every gram of regular, visible matter, cosmologists believe that |
03:20 | there are around five grams of so-called dark matter…an invisible substance that, |
03:25 | at least as far as we know, only interacts with objects through gravity. |
03:29 | We can watch it make stars at the edges of galaxies |
03:31 | rotate faster than they would otherwise. |
03:34 | And we can see how it warps spacetime, bending light that passes by it. |
03:38 | But we’ve never detected it directly. |
03:40 | So even though it’s been taunting astronomers for nearly 100 years, |
03:44 | no one knows what dark matter is. |
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04:50 | And let’s get back to it! |
04:52 | It’s part of what astronomers call the dark sector, the part of the universe |
04:56 | that’s made up of mysterious substances that we’ve never explored directly, |
05:01 | yet is most of reality as we know it. |
05:03 | The dark sector makes up around 95% of the universe, |
05:07 | but all we know about it is how it pushes and pulls on the rest of the universe… |
05:11 | the part that’s made up of regular matter and energy and light. |
05:14 | So, the idea that everything in the dark sector |
05:17 | was born during the Big Bang is as good a guess as any. |
05:20 | But it’s still just a guess. |
05:22 | There’s no actual reason why it has to be that way. |
05:24 | We can’t observe the moments immediately after the Big Bang, |
05:27 | because it was so hot and dense that space was completely opaque. |
05:31 | Light couldn’t shine through the universe. |
05:33 | So we don’t even know for sure what regular matter was doing, |
05:36 | let alone if dark matter was there interacting with it. |
05:39 | And, considering that regular and dark matter barely interact with each other anyway, |
05:43 | some scientists are considering whether dark matter could have emerged at a later time, |
05:47 | in what they call the Dark Big Bang. |
05:49 | It’s all hypothetical at this point. |
05:50 | But as long as they’ve got this idea on the table, |
05:53 | their task is to figure out how a Dark Big Bang might have gone down if it did happen. |
05:58 | It’s kind of like your lunch is missing, and you’re trying to figure out if your dog ate it. |
06:02 | To solve the mystery, you might start by imagining the potential clues to look for: |
06:07 | For example, you know your dog is a messy eater, so if it really did eat your BLT, |
06:12 | it probably left some crumbs behind. |
06:14 | Plus, it’s not supposed to eat human food, so it might get an upset stomach. |
06:18 | Or at the very least, it might not be as hungry when dinnertime rolls around. |
06:22 | And astronomers are taking the same general approach here. |
06:25 | They’re trying to paint a picture of the hypothetical Dark Big Bang |
06:29 | so that observers can look for any crumbs that suggest it really happened. |
06:33 | And one crucial detail is when it happened. |
06:36 | Hypothetically, anyway. |
06:37 | Cosmologists know that dark matter played a big role in seeding the large-scale structure |
06:42 | of the universe today: It helped draw regular matter into the massive web |
06:46 | of galaxy clusters that stretches as far as we can see. |
06:50 | So it had to have been around early enough to play that role |
06:53 | and fit into our models of how that structure evolved. |
06:56 | And according to computer models, |
06:57 | a dark big bang most likely took place a mere month after the regular one. |
07:02 | But a question that’s far more important than the when is the what. |
07:05 | What, if anything, actually happened? |
07:08 | The team proposing this dark hypothesis suggests that, |
07:11 | prior to this second “bang”, there was a dark matter vacuum. |
07:14 | Now a vacuum is what we think of as pure emptiness. |
07:17 | So in this dark matter vacuum there would have been some regular matter, |
07:20 | but it would have been empty of dark matter. |
07:22 | But according to quantum mechanics, nothing is truly empty. |
07:26 | Even so-called empty space is frothing with particles that spontaneously… |
07:30 | and incredibly briefly…pop in and out of existence. |
07:34 | So a vacuum still has at least some amount of energy in it. |
07:37 | But that “at least” is important, because a vacuum can have different energy states. |
07:42 | While it likes to be in the lowest energy state possible, |
07:45 | better known as a true vacuum, it doesn’t have to be. |
07:48 | And scientists refer to that situation as a false vacuum. |
07:51 | You can think of a false vacuum like a pothole on an inclined street. |
07:55 | If a ball gets stuck in the pothole, whether it got kicked up the hill |
07:58 | or was rolling down the hill, it can stay stuck for a long time. |
08:02 | But as soon as a car or a gust of wind nudges the ball out of the pothole, |
08:06 | it will roll down the street and wind up resting at wherever the bottom of the hill is. |
08:10 | Because the bottom of the hill is at a lower energy state than the pothole. |
08:14 | Now, the energy state of a vacuum is a little harder to picture, |
08:18 | but the basic concept is the same: A false vacuum may be stable for a long time, |
08:23 | but it can suddenly drop to a lower energy state. |
08:26 | And this is called a phase transition. |
08:28 | On Earth, we’re familiar with certain types of phase transitions that happen in chemistry, |
08:33 | like when liquid water vaporizes into a gas or freezes into a solid. |
08:37 | And cosmological phase transitions aren’t completely dissimilar. |
08:40 | They’re also sudden changes in the form and properties of matter. |
08:44 | Some theorists hypothesize that during the original Big Bang, |
08:47 | a phase transition transformed a false vacuum into a smattering of particles, |
08:52 | not unlike how a gas condenses into a liquid. |
08:55 | And in this hypothetical Dark Big Bang, something similar may have happened, too. |
08:59 | Just like a pot of water that’s beginning to boil, |
09:01 | a false vacuum on the verge of a phase change begins to bubble. |
09:05 | And, yes, the cosmologists actually refer to them as bubbles. |
09:08 | They’re little spots where the vacuum starts dropping to a lower-energy state. |
09:12 | And as they expand at near-light speed and bump into each other, |
09:16 | these bubbles collapse the false vacuum into a true vacuum. |
09:19 | Now, in the case of the hypothetical dark matter vacuum, the energy from these |
09:23 | expanding bubbles gets released as dark matter and dark radiation…much like the matter |
09:28 | and light released in the collapse of the vacuum that created the Big Bang. |
09:32 | But exactly what comes out of this dark phase transition depends on how it plays out. |
09:37 | In one hypothetical scenario, bubbles could slam together fast enough |
09:41 | that their energy can turn directly into humongous dark matter particles |
09:45 | that are up to 10 trillion times the mass of a proton. |
09:48 | The authors of this Dark Big Bang hypothesis |
09:51 | have affectionately dubbed them dark-zillas. |
09:53 | But if the phase transition plays out more slowly, |
09:56 | the colliding bubbles will first create a hot plasma in the dark sector. |
10:00 | And while the plasma is hot, small dark matter particles |
10:04 | will emerge from interactions within it. |
10:06 | It’s this kind of transition that could create the most popular candidates |
10:09 | for dark matter particles out there, today. |
10:11 | They’re known as WIMPS, or weakly interacting massive particles, and scientists are |
10:16 | actively searching for them with a bunch of different experiments around the world. |
10:20 | Eventually, the plasma cools, slowing down the interactions taking place |
10:24 | within the plasma, and ending the creation of more dark matter. |
10:28 | But that’s just two scenarios of many. |
10:30 | And right now, theorists aren’t sure which, if any, might be right. |
10:33 | But they hope they’ll find evidence that points them in the right direction. |
10:36 | Because remember, even though this is all hypothetical, and it all happened at a time we |
10:40 | can’t observe directly, it’s like the dog that ate your sandwich when you weren’t looking. |
10:44 | The Dark Big Bang would have left behind some crumbs. |
10:48 | And while those bubbles that carry out the phase transition |
10:50 | between a false vacuum and a real vacuum are invisible, |
10:53 | they would have generated gravitational waves as they collided. |
10:57 | Gravitational waves are ripples that warp spacetime as they pass through it, |
11:01 | subtly pinching and stretching the distances between objects. |
11:05 | And thanks to advancements in technology, |
11:06 | scientists are getting better and better at detecting tinier and tinier signals. |
11:11 | Like in 2023, a massive international collaboration called NANOGrav |
11:15 | announced they had successfully detected |
11:17 | a sort of gravitational wave background noise coming from all around us. |
11:22 | Buried within that signal would be gravitational waves created during the Big Bang. |
11:27 | And eventually more detailed studies |
11:28 | will help scientists tease apart exactly what made them. |
11:31 | And maybe one day, they’ll reveal there really was a second Big Bang. |
11:36 | Or maybe they won’t. |
11:37 | Cosmologists don’t need a Dark Big Bang |
11:39 | to explain how we got a universe full of dark matter. |
11:42 | And there are plenty of alternate proposals that I don’t have time to dive into, here. |
11:46 | Like primordial black holes, or a kind of ultradense matter called “quark nuggets”. |
11:51 | But I’m pulling for you Dark Big Bang, |
11:53 | if only to read all the fun sequel names that people put in the comments. |
11:58 | [♪ OUTRO] |