Return to Video

The discovery that could rewrite physics

  • 0:01 - 0:04
    If you look deep into the night sky,
  • 0:04 - 0:06
    you see stars,
  • 0:06 - 0:09
    and if you look further, you see more stars,
  • 0:09 - 0:11
    and further, galaxies, and
    further, more galaxies.
  • 0:11 - 0:15
    But if you keep looking further and further,
  • 0:15 - 0:18
    eventually you see nothing for a long while,
  • 0:18 - 0:22
    and then finally you see a
    faint, fading afterglow,
  • 0:22 - 0:25
    and it's the afterglow of the Big Bang.
  • 0:25 - 0:28
    Now, the Big Bang was an era in the early universe
  • 0:28 - 0:30
    when everything we see in the night sky
  • 0:30 - 0:33
    was condensed into an incredibly small,
  • 0:33 - 0:37
    incredibly hot, incredibly roiling mass,
  • 0:37 - 0:40
    and from it sprung everything we see.
  • 0:40 - 0:43
    Now, we've mapped that afterglow
  • 0:43 - 0:44
    with great precision,
  • 0:44 - 0:46
    and when I say we, I mean people who aren't me.
  • 0:46 - 0:48
    We've mapped the afterglow
  • 0:48 - 0:49
    with spectacular precision,
  • 0:49 - 0:51
    and one of the shocks about it
  • 0:51 - 0:54
    is that it's almost completely uniform.
  • 0:54 - 0:56
    Fourteen billion light years that way
  • 0:56 - 0:58
    and 14 billion light years that way,
  • 0:58 - 0:59
    it's the same temperature.
  • 0:59 - 1:02
    Now it's been 14 billion years
  • 1:02 - 1:04
    since that Big Bang,
  • 1:04 - 1:07
    and so it's got faint and cold.
  • 1:07 - 1:09
    It's now 2.7 degrees.
  • 1:09 - 1:11
    But it's not exactly 2.7 degrees.
  • 1:11 - 1:14
    It's only 2.7 degrees to about
  • 1:14 - 1:15
    10 parts in a million.
  • 1:15 - 1:16
    Over here, it's a little hotter,
  • 1:16 - 1:18
    and over there, it's a little cooler,
  • 1:18 - 1:21
    and that's incredibly important
    to everyone in this room,
  • 1:21 - 1:23
    because where it was a little hotter,
  • 1:23 - 1:25
    there was a little more stuff,
  • 1:25 - 1:26
    and where there was a little more stuff,
  • 1:26 - 1:28
    we have galaxies and clusters of galaxies
  • 1:28 - 1:30
    and superclusters
  • 1:30 - 1:32
    and all the structure you see in the cosmos.
  • 1:32 - 1:35
    And those small, little, inhomogeneities,
  • 1:35 - 1:38
    20 parts in a million,
  • 1:38 - 1:40
    those were formed by quantum mechanical wiggles
  • 1:40 - 1:42
    in that early universe that were stretched
  • 1:42 - 1:45
    across the size of the entire cosmos.
  • 1:45 - 1:46
    That is spectacular,
  • 1:46 - 1:48
    and that's not what they found on Monday;
  • 1:48 - 1:50
    what they found on Monday is cooler.
  • 1:50 - 1:52
    So here's what they found on Monday:
  • 1:52 - 1:56
    Imagine you take a bell,
  • 1:56 - 1:57
    and you whack the bell with a hammer.
  • 1:57 - 1:59
    What happens? It rings.
  • 1:59 - 2:01
    But if you wait, that ringing fades
  • 2:01 - 2:03
    and fades and fades
  • 2:03 - 2:05
    until you don't notice it anymore.
  • 2:05 - 2:07
    Now, that early universe was incredibly dense,
  • 2:07 - 2:10
    like a metal, way denser,
  • 2:10 - 2:12
    and if you hit it, it would ring,
  • 2:12 - 2:14
    but the thing ringing would be
  • 2:14 - 2:16
    the structure of space-time itself,
  • 2:16 - 2:19
    and the hammer would be quantum mechanics.
  • 2:19 - 2:21
    What they found on Monday
  • 2:21 - 2:23
    was evidence of the ringing
  • 2:23 - 2:25
    of the space-time of the early universe,
  • 2:25 - 2:27
    what we call gravitational waves
  • 2:27 - 2:29
    from the fundamental era,
  • 2:29 - 2:31
    and here's how they found it.
  • 2:31 - 2:33
    Those waves have long since faded.
  • 2:33 - 2:34
    If you go for a walk,
  • 2:34 - 2:36
    you don't wiggle.
  • 2:36 - 2:39
    Those gravitational waves in the structure of space
  • 2:39 - 2:42
    are totally invisible for all practical purposes.
  • 2:42 - 2:45
    But early on, when the universe was making
  • 2:45 - 2:47
    that last afterglow,
  • 2:47 - 2:48
    the gravitational waves
  • 2:48 - 2:51
    put little twists in the structure
  • 2:51 - 2:53
    of the light that we see.
  • 2:53 - 2:56
    So by looking at the night sky deeper and deeper --
  • 2:56 - 2:58
    in fact, these guys spent
    three years on the South Pole
  • 2:58 - 3:01
    looking straight up through the coldest, clearest,
  • 3:01 - 3:03
    cleanest air they possibly could find
  • 3:03 - 3:06
    looking deep into the night sky and studying
  • 3:06 - 3:09
    that glow and looking for the faint twists
  • 3:09 - 3:12
    which are the symbol, the signal,
  • 3:12 - 3:13
    of gravitational waves,
  • 3:13 - 3:16
    the ringing of the early universe.
  • 3:16 - 3:17
    And on Monday, they announced
  • 3:17 - 3:19
    that they had found it.
  • 3:19 - 3:22
    And the thing that's so spectacular about that to me
  • 3:22 - 3:24
    is not just the ringing, though that is awesome.
  • 3:24 - 3:26
    The thing that's totally amazing,
  • 3:26 - 3:28
    the reason I'm on this stage, is because
  • 3:28 - 3:31
    what that tells us is something
    deep about the early universe.
  • 3:31 - 3:33
    It tells us that we
  • 3:33 - 3:34
    and everything we see around us
  • 3:34 - 3:37
    are basically one large bubble --
  • 3:37 - 3:39
    and this is the idea of inflation—
  • 3:39 - 3:43
    one large bubble surrounded by something else.
  • 3:43 - 3:45
    This isn't conclusive evidence for inflation,
  • 3:45 - 3:47
    but anything that isn't inflation that explains this
  • 3:47 - 3:49
    will look the same.
  • 3:49 - 3:50
    This is a theory, an idea,
  • 3:50 - 3:52
    that has been around for a while,
  • 3:52 - 3:53
    and we never thought we we'd really see it.
  • 3:53 - 3:55
    For good reasons, we thought we'd never see
  • 3:55 - 3:57
    killer evidence, and this is killer evidence.
  • 3:57 - 3:59
    But the really crazy idea
  • 3:59 - 4:02
    is that our bubble is just one bubble
  • 4:02 - 4:07
    in a much larger, roiling pot of universal stuff.
  • 4:07 - 4:09
    We're never going to see the stuff outside,
  • 4:09 - 4:11
    but by going to the South Pole
    and spending three years
  • 4:11 - 4:14
    looking at the detailed structure of the night sky,
  • 4:14 - 4:16
    we can figure out
  • 4:16 - 4:19
    that we're probably in a universe
    that looks kind of like that.
  • 4:19 - 4:21
    And that amazes me.
  • 4:21 - 4:23
    Thanks a lot.
  • 4:23 - 4:26
    (Applause)
Title:
The discovery that could rewrite physics
Speaker:
Allan Adams
Description:

On March 17, 2014, a group of physicists announced a thrilling discovery: the “smoking gun” data for the idea of an inflationary universe, a clue to the Big Bang. For non-physicists, what does it mean? TED asked Allan Adams to briefly explain the results, in this improvised talk illustrated by Randall Munroe of xkcd.

more » « less
Video Language:
English
Team:
closed TED
Project:
TEDTalks
Duration:
04:42

English subtitles

Revisions Compare revisions