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

Allan Adams: A descoberta que pode revolucionar a física

Filmed:
1,865,923 views

Em 17 de março de 2014, um grupo de físicos anunciou uma descoberta emocionante: as informações que indicam, sem sombra de dúvida, um universo inflacionário, uma pista do Big Bang. Para os leigos, o que isso significa? O TED pediu que Allan Adams explicasse brevemente os resultados nesta palestra improvisada, ilustrada por Randall Munroe do xkcd.
- 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,
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Se olharmos o céu noturno lá longe,
00:16
you see stars,
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vemos estrelas,
00:18
and if you look further, you see more stars,
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e se olharmos mais longe,
vemos mais estrelas,
00:20
and further, galaxies, and
further, more galaxies.
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e mais longe, galáxias,
e mais longe, mais galáxias.
00:22
But if you keep looking further and further,
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Mas se continuarmos olhando
cada vez mais longe,
00:26
eventually you see nothing for a long while,
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chega uma hora em que não vemos
nada por um tempo,
00:29
and then finally you see a
faint, fading afterglow,
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até que, finalmente, vemos um brilho
fraco, quase desaparecendo
00:34
and it's the afterglow of the Big Bang.
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e esse é o brilho do Big Bang.
00:37
Now, the Big Bang was an era in the early universe
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Bem, o Big Bang foi uma época
no início do universo
00:40
when everything we see in the night sky
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quando tudo que vemos no céu noturno
00:42
was condensed into an incredibly small,
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estava condensado em uma massa
00:44
incredibly hot, incredibly roiling mass,
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incrivelmente pequena, quente e turva
00:48
and from it sprung everything we see.
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e dela surgiu tudo o que vemos.
00:51
Now, we've mapped that afterglow
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Bem, nós mapeamos esse brilho
00:54
with great precision,
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com grande precisão,
00:56
and when I say we, I mean people who aren't me.
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e quando digo nós,
quero dizer pessoas que não sou eu.
00:58
We've mapped the afterglow
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Nós mapeamos o brilho
01:00
with spectacular precision,
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com precisão espetacular,
01:01
and one of the shocks about it
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e uma das grandes surpresas
01:02
is that it's almost completely uniform.
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é que ele é quase completamente uniforme.
01:05
Fourteen billion light years that way
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14 bilhões de anos-luz para lá
01:07
and 14 billion light years that way,
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e 14 bilhões de anos-luz para cá,
01:09
it's the same temperature.
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é a mesma temperatura.
01:11
Now it's been 14 billion years
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Agora já se passaram 14 bilhões de anos
01:14
since that Big Bang,
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desde o Big Bang,
01:16
and so it's got faint and cold.
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e assim ele ficou fraco e frio.
01:18
It's now 2.7 degrees.
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Atualmente são 2,7 graus.
01:21
But it's not exactly 2.7 degrees.
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Mas não 2,7 graus exatamente.
01:23
It's only 2.7 degrees to about
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São só 2,7 graus mais ou menos
01:25
10 parts in a million.
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em 10 partes por milhão.
01:27
Over here, it's a little hotter,
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Para cá é um pouco mais quente,
01:28
and over there, it's a little cooler,
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e para lá, um pouco mais frio,
01:30
and that's incredibly important
to everyone in this room,
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e isso é incrivelmente importante
a todos neste salão,
01:33
because where it was a little hotter,
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porque onde estava um pouco mais quente,
01:35
there was a little more stuff,
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havia mais matéria,
01:36
and where there was a little more stuff,
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e onde havia mais matéria,
01:38
we have galaxies and clusters of galaxies
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nós temos as galáxias
e os conjuntos de galáxias
01:40
and superclusters
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e superconjuntos
01:41
and all the structure you see in the cosmos.
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e toda a estrutura que vemos no cosmo.
01:44
And those small, little, inhomogeneities,
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E aquelas pequenas heterogeneidades,
01:47
20 parts in a million,
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20 partes por milhão,
01:49
those were formed by quantum mechanical wiggles
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elas foram formadas por torções quânticas
01:52
in that early universe that were stretched
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naquele universo primitivo
que estava em expansão
01:54
across the size of the entire cosmos.
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ao longo de todo o comprimento do cosmo.
01:56
That is spectacular,
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Isso é espetacular.
01:58
and that's not what they found on Monday;
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E não foi isso que eles descobriram
na segunda-feira;
01:59
what they found on Monday is cooler.
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o que descobriram é mais legal.
02:02
So here's what they found on Monday:
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Foi isto que eles descobriram na segunda:
02:04
Imagine you take a bell,
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Imaginem um sino,
02:07
and you whack the bell with a hammer.
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e vocês acertam o sino com um martelo.
02:09
What happens? It rings.
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O que acontece? Ele ressoa.
02:11
But if you wait, that ringing fades
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Mas se esperarmos, o som diminui
02:13
and fades and fades
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e diminui cada vez mais
02:14
until you don't notice it anymore.
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até que nem conseguimos mais notar.
02:16
Now, that early universe was incredibly dense,
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Agora, o universo primitivo
era incrivelmente denso,
02:19
like a metal, way denser,
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como um metal, muito mais denso,
02:21
and if you hit it, it would ring,
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e se o acertássemos, ele ressoaria,
02:23
but the thing ringing would be
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mas a coisa que ressoaria seria
02:25
the structure of space-time itself,
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a própria estrutura do espaço-tempo,
02:27
and the hammer would be quantum mechanics.
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e o martelo seria a mecânica quântica.
02:30
What they found on Monday
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O que descobriram segunda-feira
02:32
was evidence of the ringing
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foi evidência da ressonância
02:35
of the space-time of the early universe,
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do espaço-tempo do universo primitivo,
02:37
what we call gravitational waves
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o que chamamos de ondas gravitacionais
02:39
from the fundamental era,
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do período fundamental,
02:40
and here's how they found it.
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e foi assim que eles descobriram.
02:42
Those waves have long since faded.
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Essas ondas diminuíram há muito tempo.
02:45
If you go for a walk,
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Se você sair para uma caminhada,
02:46
you don't wiggle.
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você não se contorce.
02:48
Those gravitational waves in the structure of space
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Essas ondas gravitacionais
na estrutura do espaço
02:50
are totally invisible for all practical purposes.
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são totalmente invisíveis
para todos os propósitos práticos.
02:53
But early on, when the universe was making
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Mas no início, quando o universo
emitia aquele último brilho,
02:56
that last afterglow,
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02:58
the gravitational waves
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as ondas gravitacionais
03:00
put little twists in the structure
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colocaram pequenas torções na estrutura
03:03
of the light that we see.
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da luz que nós vemos.
03:04
So by looking at the night sky deeper and deeper --
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Então, ao olhar para o céu noturno
cada vez mais longe...
03:07
in fact, these guys spent
three years on the South Pole
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Na verdade, estes caras passaram
três anos no Polo Sul,
03:10
looking straight up through the coldest, clearest,
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olhando diretamente para cima
pelo ar mais frio,
03:13
cleanest air they possibly could find
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mais claro e mais limpo
que se pode encontrar
03:15
looking deep into the night sky and studying
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olhando lá longe no céu noturno
e estudando
03:17
that glow and looking for the faint twists
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aquele brilho e procurando
essas pequenas torções
03:21
which are the symbol, the signal,
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que são o símbolo, o sinal,
03:23
of gravitational waves,
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das ondas gravitacionais,
03:25
the ringing of the early universe.
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a ressonância do universo primitivo.
03:27
And on Monday, they announced
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E na segunda-feira, eles anunciaram
03:29
that they had found it.
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que o encontraram.
03:31
And the thing that's so spectacular about that to me
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E o que eu acho mais espetacular nisso
03:33
is not just the ringing, though that is awesome.
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não é somente a ressonância, que é incrível.
03:36
The thing that's totally amazing,
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O que é mais maravilhoso,
03:37
the reason I'm on this stage, is because
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a razão pela qual estou aqui no palco,
03:39
what that tells us is something
deep about the early universe.
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é que isso nos diz algo
profundo sobre o universo primitivo.
03:43
It tells us that we
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Isso nos diz que nós
03:44
and everything we see around us
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e tudo que vemos ao nosso redor
03:46
are basically one large bubble --
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somos basicamente uma grande bolha,
03:49
and this is the idea of inflation—
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e essa é a ideia de inflação --
03:51
one large bubble surrounded by something else.
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uma grande bolha rodeada de alguma coisa.
03:55
This isn't conclusive evidence for inflation,
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Essa não é evidência conclusiva
para a inflação,
03:57
but anything that isn't inflation that explains this
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mas qualquer coisa que não seja inflação
que explique isso
03:59
will look the same.
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teria a mesma aparência.
04:00
This is a theory, an idea,
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Essa é uma teoria, uma ideia,
04:02
that has been around for a while,
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que está por aí há um tempo,
04:03
and we never thought we we'd really see it.
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e nunca imaginamos que realmente veríamos.
04:05
For good reasons, we thought we'd never see
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Por bons motivos,
pensamos que nunca veríamos
04:07
killer evidence, and this is killer evidence.
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evidência definitiva,
e isso é evidência definitiva.
04:09
But the really crazy idea
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Mas a ideia muito louca
04:11
is that our bubble is just one bubble
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é que nossa bolha é só uma bolha
04:14
in a much larger, roiling pot of universal stuff.
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num poço muito grande e turvo
de matéria universal.
04:18
We're never going to see the stuff outside,
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Nós nunca vamos ver o que está lá fora,
04:20
but by going to the South Pole
and spending three years
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mas indo ao Polo Sul e passando três anos
04:23
looking at the detailed structure of the night sky,
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observando a estrutura
detalhada do céu noturno,
04:25
we can figure out
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nós podemos entender
04:27
that we're probably in a universe
that looks kind of like that.
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que estamos num universo
que é mais ou menos assim.
04:30
And that amazes me.
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E isso me surpreende.
04:33
Thanks a lot.
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Muito obrigado.
04:34
(Applause)
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(Aplausos)
Translated by Gustavo Rocha
Reviewed by Nadja Nathan

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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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