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,
0
928
3492
Ako se duboko zagledate u nebo noću,
vidite zvezde,
00:16
you see starsЗвездице,
1
4420
1616
00:18
and if you look furtherдаље, you see more starsЗвездице,
2
6036
2572
ako pogledate dalje, videćete još zvezda,
00:20
and furtherдаље, galaxiesгалаксије, and
furtherдаље, more galaxiesгалаксије.
3
8608
2159
dalje su galaksije,
a dalje od toga još galaksija.
00:22
But if you keep looking furtherдаље and furtherдаље,
4
10767
3873
Ali ako nastavite da gledate
dalje i dalje,
00:26
eventuallyконачно you see nothing for a long while,
5
14640
3116
u jednom trenutku nećete
videti ništa neko vreme
00:29
and then finallyконачно you see a
faintнесвестица, fadingбледи afterglowodsjaj,
6
17756
4462
i onda konačno vidite slab sjaj
koji nestaje,
00:34
and it's the afterglowodsjaj of the BigVeliki BangPrasak.
7
22218
3024
to je sjaj koji prati Veliki prasak.
00:37
Now, the BigVeliki BangPrasak was an eraера in the earlyрано universeуниверзум
8
25242
2817
Veliki prasak je bio doba
u ranom periodu univerzuma
00:40
when everything we see in the night skyнебо
9
28059
2171
kada je sve što vidimo na noćnom nebu
00:42
was condensedSkraжena into an incrediblyневероватно smallмали,
10
30230
2410
bilo zbijeno u neverovatno malu,
00:44
incrediblyневероватно hotвруће, incrediblyневероватно roilingроилинг massмаса,
11
32640
4326
neverovatno vrelu, zamućenu masu
00:48
and from it sprungoslobodila everything we see.
12
36966
2692
iz koje je nastalo sve što vidimo.
00:51
Now, we'veми смо mappedmapirano that afterglowodsjaj
13
39658
2859
Taj prateći sjaj smo mapirali
00:54
with great precisionпрецизност,
14
42517
1679
sa velikom preciznošću,
00:56
and when I say we, I mean people who aren'tнису me.
15
44196
2044
a kada kažem "mi",
mislim na ljude koji nisu ja.
00:58
We'veMoramo mappedmapirano the afterglowodsjaj
16
46240
1876
Mapirali smo prateći sjaj
01:00
with spectacularспектакуларно precisionпрецизност,
17
48116
1322
sa spektakularnom preciznošću,
i jedan od šokova je to
01:01
and one of the shocksšokove about it
18
49438
1548
01:02
is that it's almostскоро completelyу потпуности uniformуниформе.
19
50986
2946
što je skoro u potpunosti ujednačen.
01:05
FourteenČetrnaest billionмилијарде lightсветло yearsгодине that way
20
53932
1958
14 milijardi svetlostnih godina
u tom pravcu
01:07
and 14 billionмилијарде lightсветло yearsгодине that way,
21
55890
1860
i još toliko u drugom pravcu,
01:09
it's the sameисти temperatureтемпература.
22
57750
1408
temperatura je ista.
01:11
Now it's been 14 billionмилијарде yearsгодине
23
59158
3314
Prošlo je 14 milijardi godina
01:14
sinceОд that BigVeliki BangPrasak,
24
62472
1818
od Velikog praska,
01:16
and so it's got faintнесвестица and coldхладно.
25
64290
2472
tako da je on oslabio i ohladio se.
01:18
It's now 2.7 degreesстепени.
26
66762
2308
Sada je 2,7 stepeni.
01:21
But it's not exactlyбаш тако 2.7 degreesстепени.
27
69070
2280
Ali nije tačno toliko.
01:23
It's only 2.7 degreesстепени to about
28
71350
2294
Samo je 2,7 stepeni na otprilike
01:25
10 partsделови in a millionмилиона.
29
73644
1842
deseti deo miliona.
01:27
Over here, it's a little hottertoplije,
30
75486
994
Ovde je malo vrelije,
01:28
and over there, it's a little coolerхладније,
31
76480
1868
a tamo je malo hladnije,
01:30
and that's incrediblyневероватно importantважно
to everyoneсви in this roomсоба,
32
78348
3088
a to je veoma bitno
za sve u ovoj prostoriji,
01:33
because where it was a little hottertoplije,
33
81436
1724
jer tamo gde je malo vrelije,
01:35
there was a little more stuffствари,
34
83160
1696
tu je bilo malo više stvari,
01:36
and where there was a little more stuffствари,
35
84856
1567
a gde je bilo malo više stvari,
01:38
we have galaxiesгалаксије and clustersкластери of galaxiesгалаксије
36
86423
1969
imali smo galaksije i skupove galaksija
01:40
and superclusterssuperclusters
37
88392
1252
i superskupove
01:41
and all the structureструктура you see in the cosmosкосмос.
38
89644
2708
i svu strukturu koju vidite u kosmosu.
01:44
And those smallмали, little, inhomogeneitiesinhomogeneities,
39
92352
3112
Te malene nehomogenosti,
01:47
20 partsделови in a millionмилиона,
40
95464
2282
20 delova miliona,
01:49
those were formedформирана by quantumквант mechanicalмеханички wigglesnemirko
41
97746
2754
to se formiralo mrdanjem
u kvantnoj mehanici
01:52
in that earlyрано universeуниверзум that were stretchedистегнута
42
100500
1808
u tom ranom univerzumu, i to se razvuklo
01:54
acrossпреко the sizeвеличине of the entireцео cosmosкосмос.
43
102308
2279
preko dužine celog kosmosa.
01:56
That is spectacularспектакуларно,
44
104587
1714
To je spektakularno
01:58
and that's not what they foundнашао on MondayU ponedeljak;
45
106301
1665
i to nisu pronašli u ponedeljak,
01:59
what they foundнашао on MondayU ponedeljak is coolerхладније.
46
107966
2036
ono što su tad pronašli
je još više kul.
02:02
So here'sево what they foundнашао on MondayU ponedeljak:
47
110002
2266
Ovo su otkrili tada:
02:04
ImagineZamislite you take a bellзвоно,
48
112268
3503
zamislite da uzmete zvono
02:07
and you whackударац the bellзвоно with a hammerчекић.
49
115771
1611
i udarite ga čekićem.
02:09
What happensсе дешава? It ringsпрстенови.
50
117382
1676
Šta se dešava?
Ono zvoni.
02:11
But if you wait, that ringingzvoni fadesбледи
51
119058
2208
Ali ako sačekate,
ta zvonjava se utišava
02:13
and fadesбледи and fadesбледи
52
121266
1620
i polako slabi i slabi
02:14
untilсве док you don't noticeобјава it anymoreвише.
53
122886
1942
dok je više ne primećujete.
02:16
Now, that earlyрано universeуниверзум was incrediblyневероватно denseгусто,
54
124828
2648
Taj rani univerzum
je bio neverovatno gust,
02:19
like a metalметал, way densergušće,
55
127476
2079
poput metala, i još gušći,
02:21
and if you hitхит it, it would ringпрстен,
56
129555
2405
i zvonio bi kada ga udarite,
02:23
but the thing ringingzvoni would be
57
131960
1863
ali ono što zvoni je bila
02:25
the structureструктура of space-timeprostor-vremena itselfсам,
58
133823
2088
sama struktura prostor-vreme,
02:27
and the hammerчекић would be quantumквант mechanicsmehanika.
59
135911
2816
a čekić bi bila kvantna mehanika.
02:30
What they foundнашао on MondayU ponedeljak
60
138727
1931
U ponedeljak su otkrili
02:32
was evidenceдоказ of the ringingzvoni
61
140658
2362
dokaz o zvonjavi
02:35
of the space-timeprostor-vremena of the earlyрано universeуниверзум,
62
143020
2315
prostor-vreme ranog univerzuma,
02:37
what we call gravitationalгравитационо wavesталаси
63
145335
2105
ono što zovemo gravitacionim talasima
02:39
from the fundamentalфундаментално eraера,
64
147440
1520
iz fundamentalnog doba,
02:40
and here'sево how they foundнашао it.
65
148960
1975
a ovako su ih otkrili.
02:42
Those wavesталаси have long sinceОд fadedizbledela.
66
150935
2072
Ti talasi su davno utihnuli.
02:45
If you go for a walkходати,
67
153007
1488
Ako se prošetate,
02:46
you don't wiggleBudi brza.
68
154495
1588
nećete mrdati.
02:48
Those gravitationalгравитационо wavesталаси in the structureструктура of spaceпростор
69
156083
2748
Ti gravitacioni talasi u strukturi svemira
02:50
are totallyтотално invisibleневидљив for all practicalпрактично purposesсврхе.
70
158831
2774
su apsolutno nevidljivi
za sve praktične primene.
02:53
But earlyрано on, when the universeуниверзум was makingстварање
71
161605
2904
Ali u ranom vremenu
kada je univerzum pravio
02:56
that last afterglowodsjaj,
72
164509
2370
taj poslednji prateći sjaj,
02:58
the gravitationalгравитационо wavesталаси
73
166879
1558
gravitacioni talasi
03:00
put little twistsobrtima in the structureструктура
74
168437
2863
napravili su male vrtloge u strukturi
03:03
of the lightсветло that we see.
75
171300
1527
svetla koje vidimo.
03:04
So by looking at the night skyнебо deeperдубље and deeperдубље --
76
172827
2966
Gledajući dublje i dublje u noćno nebo,
03:07
in factчињеница, these guys spentпотрошено
threeтри yearsгодине on the SouthJug PolePol
77
175793
2638
zapravo, ovi ljudi su proveli
tri godine na Južnom polu
03:10
looking straightравно up throughкроз the coldestнајхладнији, clearestkristalno jasno,
78
178431
2589
gledajući pravo gore
kroz najhladniji, najjasniji
03:13
cleanestnajčistiju airваздух they possiblyмогуће could find
79
181020
2350
i najčistiji vazduh koji su mogli da nađu
03:15
looking deepдубоко into the night skyнебо and studyingстудирање
80
183370
2429
i gledaju duboko u noćno nebo
i proučavajući
03:17
that glowsjaj and looking for the faintнесвестица twistsobrtima
81
185799
3376
taj sjaj i gledajući u blage vrtloge
03:21
whichкоја are the symbolсимбол, the signalсигнал,
82
189175
2348
koji su znak i signal
03:23
of gravitationalгравитационо wavesталаси,
83
191523
1820
gravitacionih talasa,
03:25
the ringingzvoni of the earlyрано universeуниверзум.
84
193343
2341
zvonjave ranog univerzuma.
03:27
And on MondayU ponedeljak, they announcedнајавио
85
195684
1787
U ponedeljak su objavili
03:29
that they had foundнашао it.
86
197471
1744
da su ga našli.
03:31
And the thing that's so spectacularспектакуларно about that to me
87
199215
2427
Meni je tu spektakularna
03:33
is not just the ringingzvoni, thoughипак that is awesomeсупер.
88
201642
2748
ne samo zvonjava, iako je i to super.
03:36
The thing that's totallyтотално amazingНевероватно,
89
204390
1358
Ono što je neverovatno,
03:37
the reasonразлог I'm on this stageфаза, is because
90
205748
2102
razlog zbog kojeg sam ovde,
03:39
what that tellsкаже us is something
deepдубоко about the earlyрано universeуниверзум.
91
207850
3468
je što nam to kaže
nešto duboko o ranom univerzumu.
03:43
It tellsкаже us that we
92
211318
1664
Kaže nam da smo mi
03:44
and everything we see around us
93
212982
1436
i sve oko nas
03:46
are basicallyу основи one largeвелики bubbleмехур --
94
214418
2954
zapravo jedan veliki mehur -
03:49
and this is the ideaидеја of inflationинфлација
95
217372
1756
i to je ova ideja naduvavanja -
03:51
one largeвелики bubbleмехур surroundedокружен by something elseдруго.
96
219128
3892
jedan veliki mehur
okružen nečim drugim.
03:55
This isn't conclusivedefinitivan evidenceдоказ for inflationинфлација,
97
223020
2130
Ovo nisu konačni dokazi
o tom naduvavanju,
03:57
but anything that isn't inflationинфлација that explainsobjašnjava this
98
225150
2174
ali sve što nije naduvavanje
a objašnjava ovo
03:59
will look the sameисти.
99
227324
1317
će izgledati isto.
04:00
This is a theoryтеорија, an ideaидеја,
100
228641
1645
Ovo je teorija, ideja
koja postoji već neko vreme
04:02
that has been around for a while,
101
230286
1224
i nikada nismo mislili da
ćemo je zaista videti.
04:03
and we never thought we we'dми смо really see it.
102
231510
1725
04:05
For good reasonsразлоге, we thought we'dми смо never see
103
233235
1838
Iz dobrih razloga, mislili smo
da nikada nećemo videti
04:07
killerубица evidenceдоказ, and this is killerубица evidenceдоказ.
104
235073
2248
odlične dokaze,
a ovo je upravo to.
04:09
But the really crazyлуд ideaидеја
105
237321
2010
Ali je zaista luda ideja
04:11
is that our bubbleмехур is just one bubbleмехур
106
239331
3032
da je naš mehur samo jedan mehur
04:14
in a much largerвеће, roilingроилинг potпот of universalуниверзалан stuffствари.
107
242363
4626
u puno većem, zamućenom kazanu
stvari u univerzumu.
04:18
We're never going to see the stuffствари outsideспоља,
108
246989
1826
Nikada nećemo videti ono spolja,
04:20
but by going to the SouthJug PolePol
and spendingтрошење threeтри yearsгодине
109
248815
2574
ali time što odemo na Južni pol
i provedemo tri godine
04:23
looking at the detaileddetaljne structureструктура of the night skyнебо,
110
251389
2560
posmatrajući detaljnu
strukturu noćnog neba,
04:25
we can figureфигура out
111
253949
1856
možemo da otkrijemo
04:27
that we're probablyвероватно in a universeуниверзум
that looksизглед kindкинд of like that.
112
255805
3090
da smo verovatno u univerzumu
koji je nalik tome.
04:30
And that amazesамазес me.
113
258895
2422
I to me zapanjuje.
04:33
ThanksHvala ti a lot.
114
261317
1336
Hvala vam mnogo.
04:34
(ApplauseAplauz)
115
262653
2936
(Aplauz)
Translated by Mile Živković
Reviewed by Anca Dimovska

▲Back to top

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