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

Alan Adams (Allan Adams): Otkriće koje bi moglo da iz korena izmeni fiziku

Filmed:
1,865,923 views

17. marta 2014., grupa fizičara objavila je uzbudljivo otkriće - ključne podatke za ideju o naduvanom univerzumu, dokaz za Veliki prasak. Šta to znači za one koji nisu fizičari? TED je zamolio Alana Adamsa da ukratko objasni rezultate, u ovom improvizovanom govoru koji je ilustrovao Rendal Manro sa sajta 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 deepдубоко into the night skyнебо,
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Ako se duboko zagledate u nebo noću,
vidite zvezde,
00:16
you see starsЗвездице,
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00:18
and if you look furtherдаље, you see more starsЗвездице,
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ako pogledate dalje, videćete još zvezda,
00:20
and furtherдаље, galaxiesгалаксије, and
furtherдаље, more galaxiesгалаксије.
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dalje su galaksije,
a dalje od toga još galaksija.
00:22
But if you keep looking furtherдаље and furtherдаље,
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Ali ako nastavite da gledate
dalje i dalje,
00:26
eventuallyконачно you see nothing for a long while,
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u jednom trenutku nećete
videti ništa neko vreme
00:29
and then finallyконачно you see a
faintнесвестица, fadingбледи afterglowodsjaj,
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i onda konačno vidite slab sjaj
koji nestaje,
00:34
and it's the afterglowodsjaj of the BigVeliki BangPrasak.
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to je sjaj koji prati Veliki prasak.
00:37
Now, the BigVeliki BangPrasak was an eraера in the earlyрано universeуниверзум
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Veliki prasak je bio doba
u ranom periodu univerzuma
00:40
when everything we see in the night skyнебо
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kada je sve što vidimo na noćnom nebu
00:42
was condensedSkraжena into an incrediblyневероватно smallмали,
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bilo zbijeno u neverovatno malu,
00:44
incrediblyневероватно hotвруће, incrediblyневероватно roilingроилинг massмаса,
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neverovatno vrelu, zamućenu masu
00:48
and from it sprungoslobodila everything we see.
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iz koje je nastalo sve što vidimo.
00:51
Now, we'veми смо mappedmapirano that afterglowodsjaj
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Taj prateći sjaj smo mapirali
00:54
with great precisionпрецизност,
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sa velikom preciznošću,
00:56
and when I say we, I mean people who aren'tнису me.
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a kada kažem "mi",
mislim na ljude koji nisu ja.
00:58
We'veMoramo mappedmapirano the afterglowodsjaj
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Mapirali smo prateći sjaj
01:00
with spectacularспектакуларно precisionпрецизност,
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sa spektakularnom preciznošću,
i jedan od šokova je to
01:01
and one of the shocksšokove about it
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01:02
is that it's almostскоро completelyу потпуности uniformуниформе.
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što je skoro u potpunosti ujednačen.
01:05
FourteenČetrnaest billionмилијарде lightсветло yearsгодине that way
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14 milijardi svetlostnih godina
u tom pravcu
01:07
and 14 billionмилијарде lightсветло yearsгодине that way,
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i još toliko u drugom pravcu,
01:09
it's the sameисти temperatureтемпература.
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temperatura je ista.
01:11
Now it's been 14 billionмилијарде yearsгодине
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Prošlo je 14 milijardi godina
01:14
sinceОд that BigVeliki BangPrasak,
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od Velikog praska,
01:16
and so it's got faintнесвестица and coldхладно.
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tako da je on oslabio i ohladio se.
01:18
It's now 2.7 degreesстепени.
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Sada je 2,7 stepeni.
01:21
But it's not exactlyбаш тако 2.7 degreesстепени.
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Ali nije tačno toliko.
01:23
It's only 2.7 degreesстепени to about
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Samo je 2,7 stepeni na otprilike
01:25
10 partsделови in a millionмилиона.
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deseti deo miliona.
01:27
Over here, it's a little hottertoplije,
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Ovde je malo vrelije,
01:28
and over there, it's a little coolerхладније,
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a tamo je malo hladnije,
01:30
and that's incrediblyневероватно importantважно
to everyoneсви in this roomсоба,
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a to je veoma bitno
za sve u ovoj prostoriji,
01:33
because where it was a little hottertoplije,
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jer tamo gde je malo vrelije,
01:35
there was a little more stuffствари,
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tu je bilo malo više stvari,
01:36
and where there was a little more stuffствари,
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a gde je bilo malo više stvari,
01:38
we have galaxiesгалаксије and clustersкластери of galaxiesгалаксије
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imali smo galaksije i skupove galaksija
01:40
and superclusterssuperclusters
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i superskupove
01:41
and all the structureструктура you see in the cosmosкосмос.
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i svu strukturu koju vidite u kosmosu.
01:44
And those smallмали, little, inhomogeneitiesinhomogeneities,
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Te malene nehomogenosti,
01:47
20 partsделови in a millionмилиона,
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20 delova miliona,
01:49
those were formedформирана by quantumквант mechanicalмеханички wigglesnemirko
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to se formiralo mrdanjem
u kvantnoj mehanici
01:52
in that earlyрано universeуниверзум that were stretchedистегнута
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u tom ranom univerzumu, i to se razvuklo
01:54
acrossпреко the sizeвеличине of the entireцео cosmosкосмос.
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preko dužine celog kosmosa.
01:56
That is spectacularспектакуларно,
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To je spektakularno
01:58
and that's not what they foundнашао on MondayU ponedeljak;
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i to nisu pronašli u ponedeljak,
01:59
what they foundнашао on MondayU ponedeljak is coolerхладније.
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ono što su tad pronašli
je još više kul.
02:02
So here'sево what they foundнашао on MondayU ponedeljak:
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Ovo su otkrili tada:
02:04
ImagineZamislite you take a bellзвоно,
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zamislite da uzmete zvono
02:07
and you whackударац the bellзвоно with a hammerчекић.
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i udarite ga čekićem.
02:09
What happensсе дешава? It ringsпрстенови.
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Šta se dešava?
Ono zvoni.
02:11
But if you wait, that ringingzvoni fadesбледи
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Ali ako sačekate,
ta zvonjava se utišava
02:13
and fadesбледи and fadesбледи
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i polako slabi i slabi
02:14
untilсве док you don't noticeобјава it anymoreвише.
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dok je više ne primećujete.
02:16
Now, that earlyрано universeуниверзум was incrediblyневероватно denseгусто,
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Taj rani univerzum
je bio neverovatno gust,
02:19
like a metalметал, way densergušće,
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poput metala, i još gušći,
02:21
and if you hitхит it, it would ringпрстен,
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i zvonio bi kada ga udarite,
02:23
but the thing ringingzvoni would be
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ali ono što zvoni je bila
02:25
the structureструктура of space-timeprostor-vremena itselfсам,
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sama struktura prostor-vreme,
02:27
and the hammerчекић would be quantumквант mechanicsmehanika.
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a čekić bi bila kvantna mehanika.
02:30
What they foundнашао on MondayU ponedeljak
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U ponedeljak su otkrili
02:32
was evidenceдоказ of the ringingzvoni
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dokaz o zvonjavi
02:35
of the space-timeprostor-vremena of the earlyрано universeуниверзум,
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prostor-vreme ranog univerzuma,
02:37
what we call gravitationalгравитационо wavesталаси
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ono što zovemo gravitacionim talasima
02:39
from the fundamentalфундаментално eraера,
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iz fundamentalnog doba,
02:40
and here'sево how they foundнашао it.
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a ovako su ih otkrili.
02:42
Those wavesталаси have long sinceОд fadedizbledela.
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Ti talasi su davno utihnuli.
02:45
If you go for a walkходати,
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Ako se prošetate,
02:46
you don't wiggleBudi brza.
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nećete mrdati.
02:48
Those gravitationalгравитационо wavesталаси in the structureструктура of spaceпростор
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Ti gravitacioni talasi u strukturi svemira
02:50
are totallyтотално invisibleневидљив for all practicalпрактично purposesсврхе.
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su apsolutno nevidljivi
za sve praktične primene.
02:53
But earlyрано on, when the universeуниверзум was makingстварање
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Ali u ranom vremenu
kada je univerzum pravio
02:56
that last afterglowodsjaj,
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taj poslednji prateći sjaj,
02:58
the gravitationalгравитационо wavesталаси
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gravitacioni talasi
03:00
put little twistsobrtima in the structureструктура
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napravili su male vrtloge u strukturi
03:03
of the lightсветло that we see.
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svetla koje vidimo.
03:04
So by looking at the night skyнебо deeperдубље and deeperдубље --
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Gledajući dublje i dublje u noćno nebo,
03:07
in factчињеница, these guys spentпотрошено
threeтри yearsгодине on the SouthJug PolePol
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zapravo, ovi ljudi su proveli
tri godine na Južnom polu
03:10
looking straightравно up throughкроз the coldestнајхладнији, clearestkristalno jasno,
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gledajući pravo gore
kroz najhladniji, najjasniji
03:13
cleanestnajčistiju airваздух they possiblyмогуће could find
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i najčistiji vazduh koji su mogli da nađu
03:15
looking deepдубоко into the night skyнебо and studyingстудирање
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i gledaju duboko u noćno nebo
i proučavajući
03:17
that glowsjaj and looking for the faintнесвестица twistsobrtima
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taj sjaj i gledajući u blage vrtloge
03:21
whichкоја are the symbolсимбол, the signalсигнал,
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koji su znak i signal
03:23
of gravitationalгравитационо wavesталаси,
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gravitacionih talasa,
03:25
the ringingzvoni of the earlyрано universeуниверзум.
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zvonjave ranog univerzuma.
03:27
And on MondayU ponedeljak, they announcedнајавио
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U ponedeljak su objavili
03:29
that they had foundнашао it.
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da su ga našli.
03:31
And the thing that's so spectacularспектакуларно about that to me
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Meni je tu spektakularna
03:33
is not just the ringingzvoni, thoughипак that is awesomeсупер.
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ne samo zvonjava, iako je i to super.
03:36
The thing that's totallyтотално amazingНевероватно,
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Ono što je neverovatno,
03:37
the reasonразлог I'm on this stageфаза, is because
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razlog zbog kojeg sam ovde,
03:39
what that tellsкаже us is something
deepдубоко about the earlyрано universeуниверзум.
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je što nam to kaže
nešto duboko o ranom univerzumu.
03:43
It tellsкаже us that we
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Kaže nam da smo mi
03:44
and everything we see around us
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i sve oko nas
03:46
are basicallyу основи one largeвелики bubbleмехур --
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zapravo jedan veliki mehur -
03:49
and this is the ideaидеја of inflationинфлација
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i to je ova ideja naduvavanja -
03:51
one largeвелики bubbleмехур surroundedокружен by something elseдруго.
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jedan veliki mehur
okružen nečim drugim.
03:55
This isn't conclusivedefinitivan evidenceдоказ for inflationинфлација,
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Ovo nisu konačni dokazi
o tom naduvavanju,
03:57
but anything that isn't inflationинфлација that explainsobjašnjava this
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ali sve što nije naduvavanje
a objašnjava ovo
03:59
will look the sameисти.
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će izgledati isto.
04:00
This is a theoryтеорија, an ideaидеја,
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Ovo je teorija, ideja
koja postoji već neko vreme
04:02
that has been around for a while,
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i nikada nismo mislili da
ćemo je zaista videti.
04:03
and we never thought we we'dми смо really see it.
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04:05
For good reasonsразлоге, we thought we'dми смо never see
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Iz dobrih razloga, mislili smo
da nikada nećemo videti
04:07
killerубица evidenceдоказ, and this is killerубица evidenceдоказ.
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odlične dokaze,
a ovo je upravo to.
04:09
But the really crazyлуд ideaидеја
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Ali je zaista luda ideja
04:11
is that our bubbleмехур is just one bubbleмехур
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da je naš mehur samo jedan mehur
04:14
in a much largerвеће, roilingроилинг potпот of universalуниверзалан stuffствари.
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u puno većem, zamućenom kazanu
stvari u univerzumu.
04:18
We're never going to see the stuffствари outsideспоља,
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Nikada nećemo videti ono spolja,
04:20
but by going to the SouthJug PolePol
and spendingтрошење threeтри yearsгодине
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ali time što odemo na Južni pol
i provedemo tri godine
04:23
looking at the detaileddetaljne structureструктура of the night skyнебо,
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posmatrajući detaljnu
strukturu noćnog neba,
04:25
we can figureфигура out
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možemo da otkrijemo
04:27
that we're probablyвероватно in a universeуниверзум
that looksизглед kindкинд of like that.
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da smo verovatno u univerzumu
koji je nalik tome.
04:30
And that amazesамазес me.
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I to me zapanjuje.
04:33
ThanksHvala ti a lot.
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Hvala vam mnogo.
04:34
(ApplauseAplauz)
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(Aplauz)
Translated by Mile Živković
Reviewed by Anca Dimovska

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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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