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

Alans Adamss: Atklājums, kas varētu pārrakstīt fiziku

Filmed:
1,865,923 views

2014. gada 17. martā grupa fiziķu paziņoja par satriecošu atklājumu: datiem, kas tieši pierāda Visuma sākotnēji straujo izplešanos un norāda uz Lielo sprādzienu. Ko tas nozīmē nefiziķiem? TED aicināja Alanu Adamsu īsi izskaidrot šos rezultātus. Improvizēto runu ilustrējis Rendals Munro no „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 deepdziļi into the night skydebesis,
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Ieskatoties naksnīgu debešu tālēs,
00:16
you see starszvaigznes,
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redzamas zvaigznes.
00:18
and if you look furthertālāk, you see more starszvaigznes,
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Ieskatoties vērīgāk,
redzams vairāk zvaigžņu,
un tālāk – galaktikas,
un vēl tālāk – vēl vairāk galaktiku.
00:20
and furthertālāk, galaxiesgalaktikas, and
furthertālāk, more galaxiesgalaktikas.
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00:22
But if you keep looking furthertālāk and furthertālāk,
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Bet, skatoties arvien tālāk un tālāk,
00:26
eventuallybeidzot you see nothing for a long while,
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galu galā ilgu laiku nav redzams nekas,
00:29
and then finallybeidzot you see a
faintvājš, fadingizbalēšanu afterglowvakara blāzma,
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līdz visbeidzot redzama
blāva, dziestoša atblāzma,
00:34
and it's the afterglowvakara blāzma of the BigLiels BangSprādziena.
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un tā ir Lielā sprādziena atblāzma.
00:37
Now, the BigLiels BangSprādziena was an eralaikmets in the earlyagri universevisums
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Lielais sprādziens
bija agrīnā Visuma laikmets,
00:40
when everything we see in the night skydebesis
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kad viss naksnīgajās debesīs redzamais
00:42
was condensedsaīsinātu into an incrediblyneticami smallmazs,
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bija saspiests ārkārtīgi mazā,
00:44
incrediblyneticami hotkarsts, incrediblyneticami roilingroling massmasa,
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ārkārtīgi karstā, ārkārtīgi blīvā masā,
00:48
and from it sprungieplīsis everything we see.
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un no tās radās viss redzamais.
00:51
Now, we'vemēs esam mappedkartētas that afterglowvakara blāzma
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Šo atblāzmu esam ļoti precīzi kartējuši,
00:54
with great precisionprecizitāte,
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00:56
and when I say we, I mean people who aren'tnav me.
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un ar „mēs” es domāju cilvēkus,
kas neesmu es.
00:58
We'veMēs esam mappedkartētas the afterglowvakara blāzma
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Šo atblāzmu mēs esam kartējuši
ar izcilu precizitāti,
01:00
with spectaculariespaidīgs precisionprecizitāte,
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01:01
and one of the shocksElektrošoks about it
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un viena no tās satriecošajām iezīmēm ir,
ka tā ir gandrīz viendabīga.
01:02
is that it's almostgandrīz completelypilnīgi uniformvienota.
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01:05
FourteenČetrpadsmit billionmiljardi lightgaisma yearsgadiem that way
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14 miljardu gaismas gadu attālumā turp
01:07
and 14 billionmiljardi lightgaisma yearsgadiem that way,
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un 14 miljardus gaismas gadu turp
01:09
it's the samepats temperaturetemperatūra.
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temperatūra ir vienāda.
01:11
Now it's been 14 billionmiljardi yearsgadiem
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Kopš Lielā sprādziena
ir pagājuši 14 miljardi gadu,
01:14
sincekopš that BigLiels BangSprādziena,
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01:16
and so it's got faintvājš and coldauksts.
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tāpēc Visums ir kļuvis blāvs un auksts.
Tagad tā temperatūra
ir –270,4 grādi pēc Celsija.
01:18
It's now 2.7 degreesgrādi.
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01:21
But it's not exactlytieši tā 2.7 degreesgrādi.
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Bet tā nav precīzi –270,4 grādi.
01:23
It's only 2.7 degreesgrādi to about
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Mīnus 270,4 grādi ir tikai
ap desmit daļiņām uz miljonu.
01:25
10 partsdaļas in a millionmiljons.
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01:27
Over here, it's a little hottervēl karstāk,
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Šeit ir mazdrusciņ karstāks
un tur – mazdrusciņ aukstāks,
01:28
and over there, it's a little coolerdzesētājs,
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01:30
and that's incrediblyneticami importantsvarīgs
to everyonevisi in this roomistaba,
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un tas ikvienam klātesošajam
ir ārkārtīgi svarīgi,
01:33
because where it was a little hottervēl karstāk,
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jo vietās, kur bija mazliet karstāks,
01:35
there was a little more stuffstuff,
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bija mazliet vairāk matērijas,
01:36
and where there was a little more stuffstuff,
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un tur, kur matērijas bija vairāk,
01:38
we have galaxiesgalaktikas and clustersklasteri of galaxiesgalaktikas
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ir galaktikas un galaktiku kopas,
01:40
and superclusterssuperclusters
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un superkopas,
01:41
and all the structurestruktūra you see in the cosmoskosmosā.
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un visas kosmosā sastopamās struktūras.
01:44
And those smallmazs, little, inhomogeneitiesinhomogeneities,
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Un šīs mazās, sīkās neviendabības,
01:47
20 partsdaļas in a millionmiljons,
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20 daļiņas uz miljonu,
01:49
those were formedizveidota by quantumkvantu mechanicalmehānisks wigglesWiggles
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veidoja kvantu mehāniskie vilnīši
agrīnajā Visumā,
01:52
in that earlyagri universevisums that were stretchedizstiepts
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kas izplatījās visā kosmosā.
01:54
acrosspāri the sizeIzmērs of the entireviss cosmoskosmosā.
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01:56
That is spectaculariespaidīgs,
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Tas ir satriecoši,
01:58
and that's not what they foundatrasts on MondayPirmdiena;
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bet tas nav tas, ko viņi atklāja pirmdien;
01:59
what they foundatrasts on MondayPirmdiena is coolerdzesētājs.
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pirmdien atklātais ir vēl satriecošāks.
02:02
So here'sšeit ir what they foundatrasts on MondayPirmdiena:
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Lūk, ko viņi atklāja pirmdien –
02:04
ImagineIedomājieties you take a bellzvans,
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iedomājieties, ka jums ir zvans
02:07
and you whackdauzīt the bellzvans with a hammerāmurs.
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un jūs iebliežat pa šo zvanu ar āmuru.
02:09
What happensnotiek? It ringsgredzeni.
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Kas notiek? Tas iezvanās.
02:11
But if you wait, that ringingzvana fadesizzūd
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Taču nogaidot zvana skaņa pieklust,
02:13
and fadesizzūd and fadesizzūd
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klūst arvien klusāka un klusāka,
02:14
untillīdz you don't noticepaziņojums it anymorevairs.
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līdz vairs nav dzirdama.
02:16
Now, that earlyagri universevisums was incrediblyneticami denseblīvs,
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Redziet, agrīnais Visums
bija ārkārtīgi blīvs,
02:19
like a metalmetāls, way denserbiezajiem,
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kā metāls, daudz blīvāks,
02:21
and if you hitsist it, it would ringgredzens,
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un, ja pa to uzsistu, tas iezvanītos,
02:23
but the thing ringingzvana would be
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taču zvanīšana izpaustos
02:25
the structurestruktūra of space-timetelpas un laika itselfpati par sevi,
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kā pašas laiktelpas struktūra,
02:27
and the hammerāmurs would be quantumkvantu mechanicsmehānika.
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un āmurs būtu kvantu mehānika.
02:30
What they foundatrasts on MondayPirmdiena
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Pirmdien atklātais
02:32
was evidencepierādījumi of the ringingzvana
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pierādīja agrīnā Visuma
laiktelpas zvanīšanu,
02:35
of the space-timetelpas un laika of the earlyagri universevisums,
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02:37
what we call gravitationalgravitācijas wavesviļņi
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mūsu tā sauktos gravitācijas viļņus
02:39
from the fundamentalfundamentāls eralaikmets,
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no sākotnējā laikmeta.
02:40
and here'sšeit ir how they foundatrasts it.
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Lūk, kā tos atklāja.
02:42
Those wavesviļņi have long sincekopš fadedizbalējuši.
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Šie viļņi jau sen ir norimuši.
02:45
If you go for a walkstaigāt,
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Izejot pastaigā,
02:46
you don't wigglevalstīties.
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jūs neviļņojaties.
02:48
Those gravitationalgravitācijas wavesviļņi in the structurestruktūra of spacetelpa
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Šie gravitācijas viļņi telpas struktūrā
02:50
are totallypilnīgi invisibleneredzams for all practicalpraktiska purposesmērķiem.
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jebkurā praktiskā nozīmē ir neredzami.
02:53
But earlyagri on, when the universevisums was makingveidošana
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Bet pirmsākumos,
Visumam radot pēdējo atblāzmu,
02:56
that last afterglowvakara blāzma,
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02:58
the gravitationalgravitācijas wavesviļņi
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gravitācijas viļņi
03:00
put little twistsvijas in the structurestruktūra
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izraisīja sīkas svārstības
mums redzamās gaismas struktūrā.
03:03
of the lightgaisma that we see.
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03:04
So by looking at the night skydebesis deeperdziļāk and deeperdziļāk --
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Tāpēc, ieskatoties naksnīgajās debesīs
arvien dziļāk un dziļāk...
03:07
in factfakts, these guys spentiztērēti
threetrīs yearsgadiem on the SouthSouth PolePole
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šie puiši patiesībā pavadīja
trīs gadus Dienvidpolā,
03:10
looking straighttaisni up throughcauri the coldestaukstākais, clearestskaidrāka,
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veroties augšup, aukstākajā, skaidrākajā,
03:13
cleanestvistīrāko airgaiss they possiblyiespējams could find
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tīrākajā gaisā, kādu vien varēja atrast,
03:15
looking deepdziļi into the night skydebesis and studyingmācās
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skatoties dziļi naksnīgajās debesīs
un pētot šo atblāzmu, un meklējot
gandrīz nemanāmās svārstības,
03:17
that glowblāzma and looking for the faintvājš twistsvijas
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03:21
whichkas are the symbolsimbols, the signalsignāls,
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kas ir simbols, pazīme
03:23
of gravitationalgravitācijas wavesviļņi,
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gravitācijas viļņiem,
03:25
the ringingzvana of the earlyagri universevisums.
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agrīnā Visuma zvanīšanai.
03:27
And on MondayPirmdiena, they announcedpaziņoja
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Un pirmdien viņi paziņoja,
03:29
that they had foundatrasts it.
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ka ir to atraduši.
03:31
And the thing that's so spectaculariespaidīgs about that to me
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Un, manuprāt, satriecošākais
03:33
is not just the ringingzvana, thoughtomēr that is awesomesatriecošs.
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ir ne tikai pati zvanīšana,
lai gan arī tā ir lieliska.
03:36
The thing that's totallypilnīgi amazingpārsteidzošs,
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Tas absolūti satriecošais,
03:37
the reasoniemesls I'm on this stageposms, is because
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iemesls, kāpēc stāvu uz šīs skatuves,
03:39
what that tellsstāsta us is something
deepdziļi about the earlyagri universevisums.
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ir, ka tas atklāj ko ievērojamu
par agrīno Visumu.
03:43
It tellsstāsta us that we
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Tas atklāj, ka mēs
03:44
and everything we see around us
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un it viss mums apkārt redzamais,
03:46
are basicallybūtībā one largeliels bubbleburbulis --
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būtībā ir viens liels burbulis –
03:49
and this is the ideaideja of inflationinflācija
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un šī ideja par straujo izplešanos –
03:51
one largeliels bubbleburbulis surroundedapkārt by something elsecits.
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viens liels burbulis,
kam apkārt ir kaut kas cits.
03:55
This isn't conclusivepārliecinoši evidencepierādījumi for inflationinflācija,
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Tas nav galīgs šīs izplešanās pierādījums,
03:57
but anything that isn't inflationinflācija that explainsskaidro this
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taču jebkas, kas nav izplešanās
un kas šo izskaidros,
03:59
will look the samepats.
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izskatīsies tāpat.
04:00
This is a theoryteorija, an ideaideja,
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Tā ir teorija, ideja,
kas pastāv jau kādu laiku,
04:02
that has been around for a while,
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04:03
and we never thought we we'dmēs gribētu really see it.
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un mēs nedomājām,
ka reiz to patiešām ieraudzīsim.
04:05
For good reasonsiemeslu dēļ, we thought we'dmēs gribētu never see
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Domājām, ka nekad negūsim
pārliecinošus pierādījumus,
04:07
killerslepkava evidencepierādījumi, and this is killerslepkava evidencepierādījumi.
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bet te nu tie ir.
04:09
But the really crazytraks ideaideja
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Taču patiešām trakā ideja
04:11
is that our bubbleburbulis is just one bubbleburbulis
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ir, ka mūsu burbulis
ir tikai viens burbulis
04:14
in a much largerlielāks, roilingroling potpods of universaluniversāls stuffstuff.
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daudz lielākā un mutuļojošā
Visuma matērijas katlā.
04:18
We're never going to see the stuffstuff outsideārpusē,
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Mēs nekad neieraudzīsim ārpus tā esošo,
04:20
but by going to the SouthSouth PolePole
and spendingizdevumi threetrīs yearsgadiem
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taču, dodoties uz Dienvidpolu
un pavadot trīs gadus,
pētot struktūras tā naksnīgajās debesīs,
04:23
looking at the detaileddetalizēts structurestruktūra of the night skydebesis,
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04:25
we can figureskaitlis out
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varam secināt,
04:27
that we're probablydroši vien in a universevisums
that looksizskatās kindlaipns of like that.
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ka, iespējams, atrodamies Visumā,
kas izskatās apmēram šādi.
04:30
And that amazespārsteidz me.
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Un tas mani sajūsmina!
04:33
Thankspaldies a lot.
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Liels paldies.
04:34
(ApplauseAplausi)
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(Aplausi)
Translated by Ilze Garda
Reviewed by Kristaps Kadiķis

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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