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: Oppdagelsen som kunne omskrive fysikken

Filmed:
1,865,923 views

17. mars 2014 annonserte en gruppe fysikere et veldig spennende funn: selve dataene for ideen om et inflasjonsunivers, en ledetråd til Big Bang. Hva betyr dette for ikke-fysikere? TED spurte Allan Adams om å kort forklare resultatene - i denne improviserte talen, illustrert av Randall Munroe fra 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 deepdyp into the night skyhimmel,
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Hvis du stirrer dypt inn i nattehimmelen,
00:16
you see starsstjerner,
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ser du stjerner,
00:18
and if you look furtherlengre, you see more starsstjerner,
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og om du ser dypere, ser du mer stjerner,
00:20
and furtherlengre, galaxiesgalakser, and
furtherlengre, more galaxiesgalakser.
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og dypere, galakser,
og enda dypere, mer galakser.
00:22
But if you keep looking furtherlengre and furtherlengre,
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Men om du fortsetter å se dypere og dypere,
00:26
eventuallyetter hvert you see nothing for a long while,
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etter hvert ser du ingenting
en stund
00:29
and then finallyendelig you see a
faintsvime av, fadingfalming afterglowAfterglow,
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men endelig ser du en svak, falmende glød,
00:34
and it's the afterglowAfterglow of the BigStor BangBang.
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og det er gløden av
det Store Smellet (Big Bang).
00:37
Now, the BigStor BangBang was an eraera in the earlytidlig universeunivers
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Big Bang var en tid i det tidlige universet
00:40
when everything we see in the night skyhimmel
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da alt vi ser på nattehimmelen
00:42
was condensedkondensert into an incrediblyutrolig smallliten,
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var kondensert ned til et utrolig lite,
00:44
incrediblyutrolig hotvarmt, incrediblyutrolig roilingroiling massmasse,
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utrolig varmt, utrolig turbulent masse,
00:48
and from it sprungoppstått everything we see.
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og fra den massen kom alt vi ser
00:51
Now, we'vevi har mappedtilordnet that afterglowAfterglow
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Vi har kartlagt denne ettergløden,
00:54
with great precisionpresisjon,
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med stor presisjon,
00:56
and when I say we, I mean people who aren'ter ikke me.
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og når jeg sier vi, mener jeg folk som ikke er meg.
00:58
We'veVi har mappedtilordnet the afterglowAfterglow
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Vi har kartlagt ettergløden
01:00
with spectacularspektakulære precisionpresisjon,
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med utrolig presisjon,
01:01
and one of the shockssjokk about it
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og et av sjokkene vedrørende det
01:02
is that it's almostnesten completelyhelt uniformuniform.
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er at det er omtrent helt ensartet.
01:05
FourteenFjorten billionmilliarder lightlett yearsår that way
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Fjorten milliarder lysår i den retningen
01:07
and 14 billionmilliarder lightlett yearsår that way,
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og fjorten milliarder lysår i den retningen,
01:09
it's the samesamme temperaturetemperatur.
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er det samme temperatur.
01:11
Now it's been 14 billionmilliarder yearsår
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Nå har det gått 13 miliarder år
01:14
sincesiden that BigStor BangBang,
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siden Big Bang,
01:16
and so it's got faintsvime av and coldkald.
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og det har falmet og blitt kaldt.
01:18
It's now 2.7 degreesgrader.
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Det er nå 2.7 grader.
01:21
But it's not exactlynøyaktig 2.7 degreesgrader.
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Men ikke akkurat 2.7 grader.
01:23
It's only 2.7 degreesgrader to about
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Det er bare 2.7 grader i
01:25
10 partsdeler in a millionmillion.
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10 deler per million.
01:27
Over here, it's a little hottervarmere,
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Der borte er det litt varmere,
01:28
and over there, it's a little coolerkulere,
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og der borte, der er det litt kaldere,
01:30
and that's incrediblyutrolig importantviktig
to everyonealle in this roomrom,
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og det er utrolig viktig
for alle i dette rommet,
01:33
because where it was a little hottervarmere,
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fordi der det var litt varmere,
01:35
there was a little more stuffting,
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var det litt mer masse,
01:36
and where there was a little more stuffting,
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og der det var litt mer masse,
01:38
we have galaxiesgalakser and clustersklynger of galaxiesgalakser
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har vi galakser og galaksehoper
01:40
and superclusterssuperclusters
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og superhoper
01:41
and all the structurestruktur you see in the cosmoskosmos.
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og alle strukturene du ser i kosmos.
01:44
And those smallliten, little, inhomogeneitiesinhomogeneities,
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Og alle de små ugjevnhetene,
01:47
20 partsdeler in a millionmillion,
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20 deler per million,
01:49
those were formeddannet by quantumquantum mechanicalmekanisk wigglesWiggles
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de var skapt av små kvantemekaniske vridninger
01:52
in that earlytidlig universeunivers that were stretchedstrukket
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i det tidlige universet som ble strekt
01:54
acrosspå tvers the sizestørrelse of the entirehel cosmoskosmos.
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over hele kosmoset.
01:56
That is spectacularspektakulære,
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Det er spektakulært,
01:58
and that's not what they foundfunnet on MondayMandag;
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og det er ikke hva dem fant sist mandag;
01:59
what they foundfunnet on MondayMandag is coolerkulere.
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det dem fant var kulere.
02:02
So here'sher er what they foundfunnet on MondayMandag:
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Så dette er det dem fant sist mandag:
02:04
ImagineTenk you take a bellklokke,
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Tenk deg at du tar en bjelle,
02:07
and you whackknerte the bellklokke with a hammerhammer.
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og at du slår den med en hammer.
Hva skjer? Den ringer.
02:09
What happensskjer? It ringsringer.
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02:11
But if you wait, that ringingringer fadesfades
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Men hvis du venter, falmer ringingen
og den falmer og falmer
02:13
and fadesfades and fadesfades
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02:14
untilfør you don't noticelegge merke til it anymorelenger.
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til du ikke lengre merker den.
02:16
Now, that earlytidlig universeunivers was incrediblyutrolig densetett,
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Det tidlige universet var utrolig tett,
02:19
like a metalmetall, way densertettere,
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som metall, mye tettere,
02:21
and if you hittruffet it, it would ringringe,
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og hvis du slo den, ville den ringe.
02:23
but the thing ringingringer would be
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men den ringingen ville være
strukturen til romtid,
02:25
the structurestruktur of space-timerom-tid itselfseg selv,
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02:27
and the hammerhammer would be quantumquantum mechanicsmekanikk.
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og hammeren ville vært kvantemekanikk.
02:30
What they foundfunnet on MondayMandag
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Det dem fant sist mandag
02:32
was evidencebevis of the ringingringer
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var bevis for den ringingen
02:35
of the space-timerom-tid of the earlytidlig universeunivers,
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av romtid i det tidlige universet,
02:37
what we call gravitationalgravitasjons wavesbølger
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det vi kaller gravitasjonsbølger
02:39
from the fundamentalfundamental eraera,
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fra den fundamentale tiden,
02:40
and here'sher er how they foundfunnet it.
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og dette er hvordan dem fant bølgene.
02:42
Those wavesbølger have long sincesiden fadedfalmet.
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Disse bølgene har falmet for lenge siden.
02:45
If you go for a walk,
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Hvis du går en tur,
så vrir ikke kvantestrengene i deg.
02:46
you don't wigglevrikke.
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02:48
Those gravitationalgravitasjons wavesbølger in the structurestruktur of spacerom
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Disse gravitasjonsbølgene i romtiden
02:50
are totallyhelt klart invisibleusynlig for all practicalpraktisk purposesformål.
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er praktisk talt helt usynlige.
02:53
But earlytidlig on, when the universeunivers was makinglager
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Men tidlig, da universet lagde
02:56
that last afterglowAfterglow,
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den siste gløden,
02:58
the gravitationalgravitasjons wavesbølger
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lagde gravitasjonsbølgene
03:00
put little twistsvendinger in the structurestruktur
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små vridninger i strukturen
03:03
of the lightlett that we see.
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til lyset vi kan se i dag.
03:04
So by looking at the night skyhimmel deeperdypere and deeperdypere --
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Så ved å stirre inn i nattehimmelen, dypere og dypere --
03:07
in factfaktum, these guys spentbrukt
threetre yearsår on the SouthSør PolePole
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faktisk, disse karene brukte 3 år på sydpolen
03:10
looking straightrett up throughgjennom the coldestkaldeste, clearestdet klareste,
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til å se rett opp igjennom det kaldeste, klareste,
03:13
cleanestreneste airluft they possiblymuligens could find
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reneste luften dem kunne finne.
03:15
looking deepdyp into the night skyhimmel and studyingstudere
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Stirret dypt inn i nattehimmelen og studerte
03:17
that glowglød and looking for the faintsvime av twistsvendinger
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den falmede gløden og lette etter de små vridningene
03:21
whichhvilken are the symbolsymbol, the signalsignal,
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som er symbolet, signalet
03:23
of gravitationalgravitasjons wavesbølger,
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av gravitasjonsbølger,
03:25
the ringingringer of the earlytidlig universeunivers.
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av ringingen i det tidlige universet.
03:27
And on MondayMandag, they announcedannonsert
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Og sist mandag ble det annonsert
03:29
that they had foundfunnet it.
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at dem hadde funnet det.
03:31
And the thing that's so spectacularspektakulære about that to me
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Og det som er så spektakulært ved det,
for meg
03:33
is not just the ringingringer, thoughselv om that is awesomeRått.
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er ikke bare ringingen,
selv om det er utrolig kult.
03:36
The thing that's totallyhelt klart amazingfantastisk,
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Det som er helt utrolig for meg,
03:37
the reasongrunnen til I'm on this stagescene, is because
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grunnen til at jeg står på scenen, er fordi
03:39
what that tellsforteller us is something
deepdyp about the earlytidlig universeunivers.
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det forteller oss noe om det tidlige universet.
03:43
It tellsforteller us that we
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Det forteller oss at vi
og alt rundt oss
03:44
and everything we see around us
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03:46
are basicallyi utgangspunktet one largestor bubbleboble --
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er egentlig en stor boble --
og dette er idéen bak (kosmisk-)inflasjon—
03:49
and this is the ideaidé of inflationinflasjon
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03:51
one largestor bubbleboble surroundedomgitt by something elseellers.
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en stor boble omsluttet av noe annet.
03:55
This isn't conclusiveavgjørende evidencebevis for inflationinflasjon,
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Dette er ikke et avgjørende bevis for inflasjon,
03:57
but anything that isn't inflationinflasjon that explainsforklarer this
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men alt som ikke er inflasjon som forklarer dette
03:59
will look the samesamme.
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vil se likt ut.
04:00
This is a theoryteori, an ideaidé,
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Dette er en teori, en idé,
04:02
that has been around for a while,
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som har vært kjent lenge,
og vi trodde ikke vi noen gang ville få se det.
04:03
and we never thought we we'dvi vil really see it.
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For gode grunner, trodde vi ikke at vi ville se
04:05
For good reasonsgrunner, we thought we'dvi vil never see
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04:07
killermorder evidencebevis, and this is killermorder evidencebevis.
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gode beviser, og dette er gode beviser.
04:09
But the really crazygal ideaidé
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Men den sprøe idéen er at
04:11
is that our bubbleboble is just one bubbleboble
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vår boble er bare en boble
04:14
in a much largerstørre, roilingroiling potgryte of universaluniversell stuffting.
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i en mye større, turbulent kokekar av universgreier.
04:18
We're never going to see the stuffting outsideutenfor,
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Vi kommer aldri til å se det som er utenfor,
men ved å gå til sydpolen
04:20
but by going to the SouthSør PolePole
and spendingutgifter threetre yearsår
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og tilbringe tre år til å studere
strukturen av nattehimmelen,
04:23
looking at the detaileddetaljert structurestruktur of the night skyhimmel,
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04:25
we can figurefigur out
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kan vi kanskje oppdage
04:27
that we're probablysannsynligvis in a universeunivers
that looksutseende kindsnill of like that.
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at vi antakeligvis er i et univers
som ser litt slik ut.
04:30
And that amazesforundrer me.
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Og det er utrolig for meg.
04:33
Thankstakk a lot.
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Tusen takk.
04:34
(ApplauseApplaus)
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(Applaus)
Translated by Emma Vartdal
Reviewed by Victoria Heby

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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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