ABOUT THE SPEAKER
Allan Adams - Theoretical physicist
Allan Adams is a theoretical physicist working at the intersection of fluid dynamics, quantum field theory and string theory.

Why you should listen

Allan Adams is a theoretical physicist working at the intersection of fluid dynamics, quantum field theory and string theory. His research in theoretical physics focuses on string theory both as a model of quantum gravity and as a strong-coupling description of non-gravitational systems.

Like water, string theory enjoys many distinct phases in which the low-energy phenomena take qualitatively different forms. In its most familiar phases, string theory reduces to a perturbative theory of quantum gravity. These phases are useful for studying, for example, the resolution of singularities in classical gravity, or the set of possibilities for the geometry and fields of spacetime. Along these lines, Adams is particularly interested in microscopic quantization of flux vacua, and in the search for constraints on low-energy physics derived from consistency of the stringy UV completion.

In other phases, when the gravitational interactions become strong and a smooth spacetime geometry ceases to be a good approximation, a more convenient description of string theory may be given in terms of a weakly-coupled non-gravitational quantum field theory. Remarkably, these two descriptions—with and without gravity—appear to be completely equivalent, with one remaining weakly-coupled when its dual is strongly interacting. This equivalence, known as gauge-gravity duality, allows us to study strongly-coupled string and quantum field theories by studying perturbative features of their weakly-coupled duals. Gauge-gravity duals have already led to interesting predictions for the quark-gluon plasma studied at RHIC. A major focus of Adams's present research is to use such dualities to find weakly-coupled descriptions of strongly-interacting condensed matter systems which can be realized in the lab.
More profile about the speaker
Allan Adams | Speaker | TED.com
TED2014

Allan Adams: The discovery that could rewrite physics

艾伦•亚当斯: 可能改写物理学的发现

Filmed:
1,865,923 views

2014年3月17日,一群物理学家宣布了一个振奋人心的发现:宇宙暴涨理论的铁证数据,也是宇宙大爆炸的一条线索。对非物理学家们而言,这是什么意思呢?TED 邀请了艾伦.亚当斯在这个即兴演讲中简要地解释这样的发现,插图由 xkcd 的兰德尔•门罗绘制。
- Theoretical physicist
Allan Adams is a theoretical physicist working at the intersection of fluid dynamics, quantum field theory and string theory. Full bio

Double-click the English transcript below to play the video.

00:12
If you look deep into the night sky天空,
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抬头仰望夜空,
00:16
you see stars明星,
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你会看到星星。
00:18
and if you look further进一步, you see more stars明星,
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如果你看得远一些,你会看到更多的星星,
00:20
and further进一步, galaxies星系, and
further进一步, more galaxies星系.
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再远一些,你会看到星系,
更远一些,你会看到更多的星系。
00:22
But if you keep looking further进一步 and further进一步,
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但是如果你一直看下去,
00:26
eventually终于 you see nothing for a long while,
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最终会有一段时间内你什么也看不到,
00:29
and then finally最后 you see a
faint, fading衰退 afterglow余辉,
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最终你会看到一阵微弱的,若隐若现的余辉,
00:34
and it's the afterglow余辉 of the Big Bang.
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那是宇宙大爆炸的余辉。
00:37
Now, the Big Bang was an era时代 in the early universe宇宙
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大爆炸时期是宇宙的早期,
00:40
when everything we see in the night sky天空
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那时候我们现在能看到的夜空中的一切
00:42
was condensed冷凝 into an incredibly令人难以置信 small,
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还是一团极小的、
00:44
incredibly令人难以置信 hot, incredibly令人难以置信 roiling横摇 mass,
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极热的滚滚的东西,
00:48
and from it sprung弹性 everything we see.
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而从那里产生了我们现在看得到的一切。
00:51
Now, we've我们已经 mapped映射 that afterglow余辉
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如今,我们已经能够非常精确地
00:54
with great precision精确,
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测绘这个余辉,
00:56
and when I say we, I mean people who aren't me.
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当我说“我们”的时候,其实并不包括我。
00:58
We've我们已经 mapped映射 the afterglow余辉
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我们极其精确地
01:00
with spectacular壮观 precision精确,
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测绘了这个余辉,
01:01
and one of the shocks震荡 about it
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其中一个让人非常震惊的发现是,
01:02
is that it's almost几乎 completely全然 uniform制服.
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它几乎是完全一致的。
01:05
Fourteen十四 billion十亿 light years年份 that way
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往这边140亿光年,
01:07
and 14 billion十亿 light years年份 that way,
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往那边140亿光年,
01:09
it's the same相同 temperature温度.
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都是一样的温度。
01:11
Now it's been 14 billion十亿 years年份
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如今从大爆炸以来,
01:14
since以来 that Big Bang,
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130亿年已经过去了,
01:16
and so it's got faint and cold.
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它已经变得微弱、寒冷。
01:18
It's now 2.7 degrees.
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现在是2.7度。
01:21
But it's not exactly究竟 2.7 degrees.
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但它并不是确切的2.7度。
01:23
It's only 2.7 degrees to about
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只有大约百万分之十的部分
01:25
10 parts部分 in a million百万.
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是2.7度。
01:27
Over here, it's a little hotter,
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这边稍微热一些,
01:28
and over there, it's a little cooler冷却器,
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那边稍微冷一些,
01:30
and that's incredibly令人难以置信 important重要
to everyone大家 in this room房间,
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而这对在座的每一位都非常重要,
01:33
because where it was a little hotter,
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因为那些稍微热一点的地方
01:35
there was a little more stuff东东,
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有更多的东西,
01:36
and where there was a little more stuff东东,
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而有更多东西的地方
01:38
we have galaxies星系 and clusters集群 of galaxies星系
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则有星系、星系团
01:40
and superclusters超星系团
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和超星系团,
01:41
and all the structure结构体 you see in the cosmos宇宙.
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以及你在宇宙中看到的所有其他东西。
01:44
And those small, little, inhomogeneities不均匀性,
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而那些小小的不均匀的东西,
01:47
20 parts部分 in a million百万,
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百万分之二十的部分,
01:49
those were formed形成 by quantum量子 mechanical机械 wiggles
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是由量子力学的作用形成的,
01:52
in that early universe宇宙 that were stretched拉伸
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是整个宇宙体系的
01:54
across横过 the size尺寸 of the entire整个 cosmos宇宙.
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早期宇宙。
01:56
That is spectacular壮观,
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这非常震撼,
01:58
and that's not what they found发现 on Monday星期一;
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不过他们星期一发现的不是这个,
01:59
what they found发现 on Monday星期一 is cooler冷却器.
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他们星期一的发现更震撼。
02:02
So here's这里的 what they found发现 on Monday星期一:
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接下来我要讲的就是他们星期一的发现:
02:04
Imagine想像 you take a bell,
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想象一口钟,
02:07
and you whack重打 the bell with a hammer锤子.
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你用锤子敲了一下这口钟。
02:09
What happens发生? It rings戒指.
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发生了什么?它发出了响声。
02:11
But if you wait, that ringing铃声 fades
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但是如果你等着,这个响声会退去,
02:13
and fades and fades
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慢慢退去,
02:14
until直到 you don't notice注意 it anymore.
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直到你完全听不见。
02:16
Now, that early universe宇宙 was incredibly令人难以置信 dense稠密,
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早期的宇宙非常的致密,
02:19
like a metal金属, way denser更密集,
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像一块金属,不过致密得多,
02:21
and if you hit击中 it, it would ring,
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如果你敲它,它会发出响声,
02:23
but the thing ringing铃声 would be
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发出的响声就是
02:25
the structure结构体 of space-time时空 itself本身,
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时空架构,
02:27
and the hammer锤子 would be quantum量子 mechanics机械学.
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而用的锤子就是量子力学。
02:30
What they found发现 on Monday星期一
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他们星期一的发现就是找到了
02:32
was evidence证据 of the ringing铃声
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早期宇宙的
02:35
of the space-time时空 of the early universe宇宙,
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时空响声的证据,
02:37
what we call gravitational引力 waves波浪
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我们称之为引力波,
02:39
from the fundamental基本的 era时代,
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它来自于一个非常重要的时期,
02:40
and here's这里的 how they found发现 it.
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他们是如何发现的呢?
02:42
Those waves波浪 have long since以来 faded褪色.
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那些引力波早就已经退去了。
02:45
If you go for a walk步行,
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如果你去散步,
02:46
you don't wiggle摆动.
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你不会晃来晃去。
02:48
Those gravitational引力 waves波浪 in the structure结构体 of space空间
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这些宇宙中的引力波
02:50
are totally完全 invisible无形 for all practical实际的 purposes目的.
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在现实中是完全感受不到的。
02:53
But early on, when the universe宇宙 was making制造
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但是在早期,也就是当宇宙在形成
02:56
that last afterglow余辉,
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它的余辉时,
02:58
the gravitational引力 waves波浪
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这些引力波
03:00
put little twists曲折 in the structure结构体
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在我们所能看到的光的
03:03
of the light that we see.
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结构中加了点小漩涡。
03:04
So by looking at the night sky天空 deeper更深 and deeper更深 --
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所以通过反复观察夜空,
03:07
in fact事实, these guys spent花费
three years年份 on the South Pole
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事实上,这些人在南极花了三年的时间
03:10
looking straight直行 up through通过 the coldest最冷, clearest最明显,
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抬头仰望夜空,那里有他们能找到的
03:13
cleanest干净 air空气 they possibly或者 could find
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最寒冷、清澈和干净的大气,
03:15
looking deep into the night sky天空 and studying研究
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他们抬头仰望夜空并研究
03:17
that glow辉光 and looking for the faint twists曲折
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那个余辉,
03:21
which哪一个 are the symbol符号, the signal信号,
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寻找引力波的印迹,
03:23
of gravitational引力 waves波浪,
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也就是那些微弱的漩涡,
03:25
the ringing铃声 of the early universe宇宙.
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早期宇宙的响声。
03:27
And on Monday星期一, they announced公布
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星期一,他们宣布
03:29
that they had found发现 it.
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他们找到了。
03:31
And the thing that's so spectacular壮观 about that to me
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最让我震惊的
03:33
is not just the ringing铃声, though虽然 that is awesome真棒.
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不只是这个响声,虽然这也非常棒。
03:36
The thing that's totally完全 amazing惊人,
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最让我震惊的是,
03:37
the reason原因 I'm on this stage阶段, is because
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也是我在这个台上的原因,因为
03:39
what that tells告诉 us is something
deep about the early universe宇宙.
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这告诉了我们更多关于早期宇宙的东西。
03:43
It tells告诉 us that we
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它告诉我们
03:44
and everything we see around us
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我们周围看到的一切
03:46
are basically基本上 one large bubble泡沫 --
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其实就是一个大泡泡——
03:49
and this is the idea理念 of inflation通货膨胀
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这也是宇宙暴涨理论认为的——
03:51
one large bubble泡沫 surrounded包围 by something else其他.
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一个被其他东西围绕的大泡泡。
03:55
This isn't conclusive确凿 evidence证据 for inflation通货膨胀,
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这并不足以证明宇宙暴涨理论,
03:57
but anything that isn't inflation通货膨胀 that explains说明 this
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不过任何试图解释此现象的非宇宙暴涨理论
03:59
will look the same相同.
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看上去也会差不多。
04:00
This is a theory理论, an idea理念,
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这是一个理论,一个想法,
04:02
that has been around for a while,
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它已经存在了一段时间了,
04:03
and we never thought we we'd星期三 really see it.
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我们从来没有想过我们会真的看到它(被证明的一天)。
04:05
For good reasons原因, we thought we'd星期三 never see
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这是有原因的,因为我们觉得我们永远不会找到
04:07
killer凶手 evidence证据, and this is killer凶手 evidence证据.
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有说服力的证据,而这就是非常有说服力的证据。
04:09
But the really crazy idea理念
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但是更疯狂的是,
04:11
is that our bubble泡沫 is just one bubble泡沫
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我们的泡泡只是一个
04:14
in a much larger, roiling横摇 pot of universal普遍 stuff东东.
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更大的滚滚宇宙中的其中一个泡泡。
04:18
We're never going to see the stuff东东 outside,
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我们永远看不到外面的泡泡,
04:20
but by going to the South Pole
and spending开支 three years年份
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但是去南极并在那里待上三年,
04:23
looking at the detailed详细 structure结构体 of the night sky天空,
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研究夜空的具体构成,
04:25
we can figure数字 out
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我们会发现
04:27
that we're probably大概 in a universe宇宙
that looks容貌 kind of like that.
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我们大概就处在一个看上去像这样的宇宙里边。
04:30
And that amazes惊讶 me.
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而这让我震撼不已。
04:33
Thanks谢谢 a lot.
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非常感谢。
04:34
(Applause掌声)
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(掌声)
Translated by Peipei Xiang
Reviewed by Isabel Lin

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ABOUT THE SPEAKER
Allan Adams - Theoretical physicist
Allan Adams is a theoretical physicist working at the intersection of fluid dynamics, quantum field theory and string theory.

Why you should listen

Allan Adams is a theoretical physicist working at the intersection of fluid dynamics, quantum field theory and string theory. His research in theoretical physics focuses on string theory both as a model of quantum gravity and as a strong-coupling description of non-gravitational systems.

Like water, string theory enjoys many distinct phases in which the low-energy phenomena take qualitatively different forms. In its most familiar phases, string theory reduces to a perturbative theory of quantum gravity. These phases are useful for studying, for example, the resolution of singularities in classical gravity, or the set of possibilities for the geometry and fields of spacetime. Along these lines, Adams is particularly interested in microscopic quantization of flux vacua, and in the search for constraints on low-energy physics derived from consistency of the stringy UV completion.

In other phases, when the gravitational interactions become strong and a smooth spacetime geometry ceases to be a good approximation, a more convenient description of string theory may be given in terms of a weakly-coupled non-gravitational quantum field theory. Remarkably, these two descriptions—with and without gravity—appear to be completely equivalent, with one remaining weakly-coupled when its dual is strongly interacting. This equivalence, known as gauge-gravity duality, allows us to study strongly-coupled string and quantum field theories by studying perturbative features of their weakly-coupled duals. Gauge-gravity duals have already led to interesting predictions for the quark-gluon plasma studied at RHIC. A major focus of Adams's present research is to use such dualities to find weakly-coupled descriptions of strongly-interacting condensed matter systems which can be realized in the lab.
More profile about the speaker
Allan Adams | Speaker | TED.com

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