Why is our universe fine-tuned for life? | Brian Greene

4,614,840 views ・ 2012-04-23

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Translator: Jenny Zurawell
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Prevodilac: Isidora Bacic Lektor: Tatjana Jevdjic
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A few months ago
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Pre nekoliko meseci
00:17
the Nobel Prize in physics
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Nobelovu nagradu iz fizike dobila su
00:19
was awarded to two teams of astronomers
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dva tima astronoma
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for a discovery that has been hailed
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za otkriće koje je proglašeno
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as one of the most important
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jednim od najvažnijih
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astronomical observations ever.
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astronomskih zapažanja ikada.
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And today, after briefly describing what they found,
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Danas, nakon što vam ukratko objasnim šta su našli,
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I'm going to tell you about a highly controversial framework
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pričaću vam o veoma kontraverznom okviru
00:33
for explaining their discovery,
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za objašnjavanje njihovog otkrića,
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namely the possibility
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naime mogućnost
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that way beyond the Earth,
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da veoma daleko od Zemlje,
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the Milky Way and other distant galaxies,
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Mlečnog puta i ostalih udaljenih galaksija,
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we may find that our universe
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možemo utvrditi da naš univerzum
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is not the only universe,
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nije jedini univerzum,
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but is instead
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već je umesto toga
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part of a vast complex of universes
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deo ogromnog kompleksa univerzuma
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that we call the multiverse.
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koji nazivamo multiverzum.
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Now the idea of a multiverse is a strange one.
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Ideja multiverzuma je čudna.
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I mean, most of us were raised to believe
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Većina nas je odgajana da misli
00:58
that the word "universe" means everything.
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da reč "univerzum" označava sve.
01:01
And I say most of us with forethought,
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Namerno kažem većina nas,
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as my four-year-old daughter has heard me speak of these ideas since she was born.
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jer svojoj četvorogodišnjoj kćeri pričam o ovim idejama od kada se rodila.
01:07
And last year I was holding her
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Prošle godine sam je nosio
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and I said, "Sophia,
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i rekao: "Sofija,
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I love you more than anything in the universe."
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volim te više od svega u univerzumu."
01:14
And she turned to me and said, "Daddy,
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Ona me pogledala i rekla: "Tata,
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universe or multiverse?"
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u univerzumu ili multiverzumu?"
01:18
(Laughter)
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(Smeh)
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But barring such an anomalous upbringing,
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Ali ako izuzmemo takvo nestandardno odgajanje,
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it is strange to imagine
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teško je zamisliti
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other realms separate from ours,
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druge svetove odvojene od našeg,
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most with fundamentally different features,
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većinu sa bitno drugačijim karakteristikama,
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that would rightly be called universes of their own.
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koji bi sa pravom mogli da se nazovu posebni univerzumi.
01:33
And yet,
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A ipak,
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speculative though the idea surely is,
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koliko god da je ova ideja spekulativna,
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I aim to convince you
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moj je cilj da vas ubedim
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that there's reason for taking it seriously,
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da postoji razlog zašto da je shvatite ozbiljno,
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as it just might be right.
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pošto možda bude tačna.
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I'm going to tell the story of the multiverse in three parts.
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Ispričaću priču o multiverzumu u tri dela.
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In part one,
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U prvom delu,
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I'm going to describe those Nobel Prize-winning results
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opisaću rezultate za koje je dobijena Nobelova nagrada
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and to highlight a profound mystery
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i naglasiću duboku misteriju
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which those results revealed.
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koju su ti rezultati otkrili.
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In part two,
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U drugom delu,
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I'll offer a solution to that mystery.
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dajem rešenje ove misterije.
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It's based on an approach called string theory,
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Ono se zasniva na pristupu nazvanom teorija struna
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and that's where the idea of the multiverse
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i tu se ideja o multiverzumu
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will come into the story.
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uključuje u ovu priču.
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Finally, in part three,
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Na kraju, u trećem delu,
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I'm going to describe a cosmological theory
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opisaću kosmološku teoriju
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called inflation,
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koja se zove inflacija,
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which will pull all the pieces of the story together.
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koja će spojiti sve delove priče.
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Okay, part one starts back in 1929
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Ok, prvi deo počinje 1929.
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when the great astronomer Edwin Hubble
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kada je veliki astronom Edvin Habl
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realized that the distant galaxies
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shvatio da se sve daleke galaksije
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were all rushing away from us,
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brzo udaljavaju od nas
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establishing that space itself is stretching,
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i time je utvrdio da se sam svemir širi,
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it's expanding.
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da se proširuje.
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Now this was revolutionary.
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To je bilo nešto revolucionarno.
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The prevailing wisdom was that on the largest of scales
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Tada je bilo uvreženo mišljenje da je u najvećoj meri
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the universe was static.
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svemir statičan.
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But even so,
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Ali ipak,
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there was one thing that everyone was certain of:
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u jedno su svi bili sigurni:
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The expansion must be slowing down.
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širenje mora da se usporava.
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That, much as the gravitational pull of the Earth
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Kao što sila teže Zemlje
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slows the ascent of an apple tossed upward,
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usporava uspon jabuke bačene uvis,
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the gravitational pull
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tako sila težnje
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of each galaxy on every other
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svake galaksije koja utiče na sve ostale
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must be slowing
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mora da usporava
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the expansion of space.
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širenje svemira.
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Now let's fast-forward to the 1990s
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Sada hajde da uzbrzamo do 1990-ih
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when those two teams of astronomers
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kada su ta dva tima astronoma
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I mentioned at the outset
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koje sam spomenuo na početku,
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were inspired by this reasoning
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inspirisana ovim razmišljanjem,
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to measure the rate
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izmerila stopu
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at which the expansion has been slowing.
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po kojoj se širenje usporava.
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And they did this
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To su učinili
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by painstaking observations
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mukotrpnim zapažanjima
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of numerous distant galaxies,
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brojnih udaljenih galaksija,
03:17
allowing them to chart
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što im je omogućilo da prate
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how the expansion rate has changed over time.
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kako se stopa širenja promenila tokom vremena.
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Here's the surprise:
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I evo iznenađenja:
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They found that the expansion is not slowing down.
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utvrdili su da se širenje ne usporava.
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Instead they found that it's speeding up,
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Umesto toga utvrdili su da se ubrzava,
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going faster and faster.
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da je sve brže i brže.
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That's like tossing an apple upward
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To je kao da bacite jabuku na gore
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and it goes up faster and faster.
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i ona se sve više ubrzava.
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Now if you saw an apple do that,
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Kada biste videli jabuku da se tako kreće,
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you'd want to know why.
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hteli biste da znate zašto.
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What's pushing on it?
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Šta je gura na gore?
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Similarly, the astronomers' results
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Slično tome, rezultati astronoma
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are surely well-deserving of the Nobel Prize,
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su sigurno zaslužili Nobelovu nagradu,
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but they raised an analogous question.
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ali postavljaju analogno pitanje.
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What force is driving all galaxies
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Koja sila utiče na sve galaksije
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to rush away from every other
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da se međusobno udaljavaju
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at an ever-quickening speed?
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sve većom brzinom?
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Well the most promising answer
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Odgovor koji najviše obećava
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comes from an old idea of Einstein's.
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je stara Ajnštajnova ideja.
04:04
You see, we are all used to gravity
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Vidite, svi smo navikli na gravitaciju
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being a force that does one thing,
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kao silu koja radi jednu stvar,
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pulls objects together.
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međusobno privlači stvari.
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But in Einstein's theory of gravity,
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Ali prema Ajnštajnovoj teoriji gravitacije,
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his general theory of relativity,
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njegovoj opštoj teoriji relativiteta,
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gravity can also push things apart.
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gravitacija može takođe da razdvaja stvari.
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How? Well according to Einstein's math,
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Kako? Prema Ajnštajnovoj matematici,
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if space is uniformly filled
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ako je svemir uniformno popunjen
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with an invisible energy,
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nevidljivom energijom,
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sort of like a uniform, invisible mist,
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nečemu nalik uniformnoj, nevidljivoj magli,
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then the gravity generated by that mist
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onda gravitacija koju ta magla generiše
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would be repulsive,
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mora da bude odbojna,
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repulsive gravity,
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odbojna gravitacija,
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which is just what we need to explain the observations.
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što je upravo to što nam treba da objasnimo ova zapažanja.
04:38
Because the repulsive gravity
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Jer odbojna gravitacija
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of an invisible energy in space --
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nevidljive energije u svemiru --
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we now call it dark energy,
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koju sada zovemo tamnom energijom,
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but I've made it smokey white here so you can see it --
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ovde sam je prikazao dimno-belom tako da možete da je vidite -
04:47
its repulsive gravity
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njena odbojna gravitacija
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would cause each galaxy to push against every other,
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bi uticala na to da se svaka galaksija odbija od svih ostalih
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driving expansion to speed up,
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i tako ubrzava širenje,
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not slow down.
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a ne usporava.
04:55
And this explanation
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I ovo širenje
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represents great progress.
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predstavlja veliki napredak.
04:59
But I promised you a mystery
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Ali obećao sam vam misteriju
05:02
here in part one.
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u prvom delu.
05:04
Here it is.
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Evo je.
05:06
When the astronomers worked out
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Kada su astronomi izračunali
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how much of this dark energy
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koliko te tamne energije
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must be infusing space
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mora da prožima prostor
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to account for the cosmic speed up,
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da bi se kosmos ubrzao,
05:15
look at what they found.
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otkrili su sledeće.
05:24
This number is small.
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Ovo je mali broj.
05:26
Expressed in the relevant unit,
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Izražen u relevantnoj jedinici,
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it is spectacularly small.
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on je spektakularno mali.
05:30
And the mystery is to explain this peculiar number.
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Misterija je objasniti ovaj čudan broj.
05:33
We want this number
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Želimo da ovaj broj
05:35
to emerge from the laws of physics,
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nastane iz zakona fizike,
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but so far no one has found a way to do that.
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ali do sada to nikome nije uspelo.
05:40
Now you might wonder,
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Možete se zapitati,
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should you care?
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zašto je to važno?
05:45
Maybe explaining this number
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Možda je objašnjenje ovog broja
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is just a technical issue,
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samo tehničko pitanje,
05:49
a technical detail of interest to experts,
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tehnički podatak zanimljiv stručnjacima,
05:52
but of no relevance to anybody else.
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bez važnosti za nas ostale.
05:54
Well it surely is a technical detail,
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To svakako jeste tehnički podatak,
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but some details really matter.
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ali neki podaci stvarno jesu važni.
05:59
Some details provide
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Neki podaci daju
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windows into uncharted realms of reality,
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uvid u neistražene svetove realnosti
06:03
and this peculiar number may be doing just that,
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i ovaj čudan broj možda upravo to čini,
06:06
as the only approach that's so far made headway to explain it
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jer kao jedini način koji je do sada to uspešno objašnjavao,
06:09
invokes the possibility of other universes --
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poziva se na mogućnost postojanja drugih univerzuma -
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an idea that naturally emerges from string theory,
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ideja koja prirodno proističe iz teorije struna,
06:15
which takes me to part two: string theory.
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što me uvodi u drugi deo: teoriju struna.
06:18
So hold the mystery of the dark energy
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Zato nemojte zaboraviti negde u pozadini
06:22
in the back of your mind
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misteriju tamne materije,
06:24
as I now go on to tell you
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dok vam budem pričao o
06:26
three key things about string theory.
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tri ključne stvari teorije struna.
06:29
First off, what is it?
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Kao prvo, šta je to?
06:31
Well it's an approach to realize Einstein's dream
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To je pristup ka ostvarivanju Ajnštanovog sna
06:34
of a unified theory of physics,
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o jedinstvenoj teoriji u fizici,
06:37
a single overarching framework
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jednom sveobuhvatnom okviru
06:39
that would be able to describe
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koji bi mogao da opiše
06:41
all the forces at work in the universe.
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sve sile koje deluju u univerzumu.
06:43
And the central idea of string theory
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Centralna ideja teorije struna
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is quite straightforward.
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je prilično jednostavna.
06:47
It says that if you examine
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Ona kaže da ako ispitujete
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any piece of matter ever more finely,
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bilo koji delić materije sve detaljnije,
06:51
at first you'll find molecules
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prvo ćete naći molekule,
06:53
and then you'll find atoms and subatomic particles.
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a onda atome i subatomske čestice.
06:56
But the theory says that if you could probe smaller,
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Prema ovoj teoriji, ako biste mogli da ispitujete još sitnije
06:58
much smaller than we can with existing technology,
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nego što možemo postojećom tehnologijom,
07:01
you'd find something else inside these particles --
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našli biste još nešto u ovim česticama -
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a little tiny vibrating filament of energy,
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sićušno, vibrirajuće vlakno energije,
07:07
a little tiny vibrating string.
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sićušnu vibrirajuću strunu.
07:10
And just like the strings on a violin,
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I baš kao strune na violini,
07:12
they can vibrate in different patterns
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one mogu da vibriraju na različite načine
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producing different musical notes.
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proizvodeći različite muzičke note.
07:16
These little fundamental strings,
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Ove male fundamentalne strune,
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when they vibrate in different patterns,
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kada vibriraju na različite načine,
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they produce different kinds of particles --
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proizvode različite vrste čestica --
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so electrons, quarks, neutrinos, photons,
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tako se elektroni, kvarkovi, neutrini, fotoni,
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all other particles
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sve ostale čestice
07:26
would be united into a single framework,
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ujedinjuju u jedan okvir,
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as they would all arise from vibrating strings.
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pošto svi proističu iz vibrirajućih struna.
07:31
It's a compelling picture,
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To je zanimljiva slika,
07:34
a kind of cosmic symphony,
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neke vrste kosmičke simfonije,
07:36
where all the richness
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gde svo bogatstvo
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that we see in the world around us
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koje vidimo u svetu oko nas
07:40
emerges from the music
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nastaje iz muzike
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that these little, tiny strings can play.
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koje ove sićušne strune mogu da sviraju.
07:45
But there's a cost
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Ali postoji cena
07:47
to this elegant unification,
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ovog elegantnog ujedinjenja
07:49
because years of research
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jer su godine istraživanja
07:51
have shown that the math of string theory doesn't quite work.
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pokazale da matematika teorije struna ne funkcioniše baš sasvim.
07:54
It has internal inconsistencies,
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Postoje interne nedoslednosti,
07:56
unless we allow
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osim ako dopustimo
07:58
for something wholly unfamiliar --
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nešto potpuno nepoznato --
08:01
extra dimensions of space.
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dodatne dimenzije prostora.
08:04
That is, we all know about the usual three dimensions of space.
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Svi znamo za tri standardne dimenzije prostora.
08:07
And you can think about those
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Možete ih zamisliti
08:09
as height, width and depth.
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kao visinu, širinu i dubinu.
08:12
But string theory says that, on fantastically small scales,
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Ali teorija struna kaže da na fantastično maloj skali,
08:15
there are additional dimensions
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postoje dodatne dimenzije
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crumpled to a tiny size so small
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zgužvane na tako malu veličinu
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that we have not detected them.
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da ih nismo detektovali.
08:21
But even though the dimensions are hidden,
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Ali čak iako su dimenzije skrivene,
08:23
they would have an impact on things that we can observe
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one bi uticale na stvari koje možemo primetiti
08:26
because the shape of the extra dimensions
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jer oblik dodatnih dimenzija
08:29
constrains how the strings can vibrate.
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ograničava kako strune vibriraju.
08:32
And in string theory,
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A u teoriji struna,
08:34
vibration determines everything.
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vibracije određuju sve.
08:37
So particle masses, the strengths of forces,
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Tako bi masa čestica, jačina sila
08:39
and most importantly, the amount of dark energy
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i najvažnije, količina tamne materije
08:42
would be determined
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bila određena
08:44
by the shape of the extra dimensions.
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oblikom dodatnih dimenzija.
08:46
So if we knew the shape of the extra dimensions,
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Zato kada bismo znali oblik dodatnih dimenzija,
08:49
we should be able to calculate these features,
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mogli bismo da izračunamo te karakteristike,
08:52
calculate the amount of dark energy.
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da izračunamo količinu tamne energije.
08:55
The challenge
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Izazov
08:57
is we don't know
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je u tome što ne znamo
08:59
the shape of the extra dimensions.
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oblik dodatnih dimenzija.
09:02
All we have
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Sve što imamo
09:04
is a list of candidate shapes
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je spisak kandidata oblika
09:06
allowed by the math.
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koje dopušta matematika.
09:09
Now when these ideas were first developed,
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Kada su ove ideje pri put razvijene,
09:11
there were only about five different candidate shapes,
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bilo je samo oko pet različitih kandidata za oblike,
09:13
so you can imagine
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pa možete zamisliti
09:15
analyzing them one-by-one
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da ih analizirate jednog po jednog
09:17
to determine if any yield
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kako biste utvrdili da li neki daje
09:19
the physical features we observe.
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fizičke karakteristike koje smo zapazili.
09:21
But over time the list grew
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Ali tokom vremena spisak se uvećao
09:23
as researchers found other candidate shapes.
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jer su istraživači našli još kandidata za oblike.
09:25
From five, the number grew into the hundreds and then the thousands --
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Sa pet, broj je porastao na stotine i onda hiljade -
09:28
A large, but still manageable, collection to analyze,
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Što je veliki skup, ali koji se ipak može analizirati
09:31
since after all,
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jer ipak
09:33
graduate students need something to do.
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i postdiplomci moraju nešto da rade.
09:36
But then the list continued to grow
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A onda je spisak nastavio da raste
09:38
into the millions and the billions, until today.
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na milione i milijarde, do danas.
09:41
The list of candidate shapes
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Spisak kandidata za oblike
09:43
has soared to about 10 to the 500.
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je otišao za oko 10 na 500.
09:48
So, what to do?
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I šta sada?
09:51
Well some researchers lost heart,
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Neki istraživači su se obeshrabrili
09:54
concluding that was so many candidate shapes for the extra dimensions,
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i zaključili da sa toliko kandidata za oblike dodatnih dimenzija,
09:57
each giving rise to different physical features,
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gde svaki daje različite fizičke karakteristike,
10:00
string theory would never make
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teorija struna nikada neće dati
10:02
definitive, testable predictions.
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konačna predviđanja koja se mogu testirati.
10:04
But others turned this issue on its head,
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Ali drugi su obrnuli ovaj problem naglavačke
10:08
taking us to the possibility of a multiverse.
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i uveli mogućnost multiverzuma.
10:10
Here's the idea.
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Evo ideje.
10:12
Maybe each of these shapes is on an equal footing with every other.
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Možda je svaki od ovih oblika jednak svim ostalima.
10:15
Each is as real as every other,
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Svaki je realan kao i svaki drugi,
10:17
in the sense
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u smislu
10:19
that there are many universes,
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da postoje mnogi univerzumi,
10:21
each with a different shape, for the extra dimensions.
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svi različitog oblika, za dodatne dimenzije.
10:24
And this radical proposal
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Ovaj radikalni predlog
10:26
has a profound impact on this mystery:
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je imao dubok uticaj na ovu misteriju:
10:29
the amount of dark energy revealed by the Nobel Prize-winning results.
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količinu tamne energije koju su otkrili rezultati za dobijenu Nobelovu nagradu.
10:32
Because you see,
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Jer vidite,
10:34
if there are other universes,
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ako postoje drugi univerzumi
10:37
and if those universes
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i ako svaki taj univerzum
10:39
each have, say, a different shape for the extra dimensions,
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ima različit oblik za dodatne dimenzije,
10:43
then the physical features of each universe will be different,
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onda će fizičke karakteristike svakog univerzuma biti različite
10:45
and in particular,
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i konkretno,
10:47
the amount of dark energy in each universe
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količina tamne energije u svakom univerzumu
10:49
will be different.
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će se razlikovati.
10:51
Which means that the mystery
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Što znači da bi misterija
10:53
of explaining the amount of dark energy we've now measured
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objašnjenja količine tamne energije koju smo sada izmerili
10:55
would take on a wholly different character.
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imala potpuno drugačiji karakter.
10:58
In this context,
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U ovom kontekstu,
11:00
the laws of physics can't explain one number for the dark energy
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zakoni fizike ne mogu da objasne jedan broj za tamnu materiju
11:03
because there isn't just one number,
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jer ne postoji samo jedan broj,
11:06
there are many numbers.
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ima mnogo brojeva.
11:08
Which means
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To znači
11:10
we have been asking the wrong question.
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da smo postavljali pogrešno pitanje.
11:13
It's that the right question to ask is,
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Pravo pitanje koje treba postaviti jeste,
11:15
why do we humans find ourselves in a universe
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zašto se mi ljudi nalazimo u univerzumu
11:18
with a particular amount of dark energy we've measured
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sa određenom količinom tamne materije koju smo izmerili
11:21
instead of any of the other possibilities
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umesto bilo koje druge mogućnosti
11:24
that are out there?
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koja postoji?
11:26
And that's a question on which we can make headway.
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To je pitanje sa kojim možemo da napredujemo.
11:29
Because those universes
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Jer u tim univerzumima
11:31
that have much more dark energy than ours,
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koji imaju mnogo više tamne energije od naše,
11:33
whenever matter tries to clump into galaxies,
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kad god materija proba da se grupiše u galaksije,
11:36
the repulsive push of the dark energy is so strong
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snaga odbijanja tamne energije je toliko jaka
11:39
that it blows the clump apart
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da razbija tu gomilu
11:41
and galaxies don't form.
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i galaksije se ne formiraju.
11:43
And in those universes that have much less dark energy,
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U tim univerzumima koji imaju mnogo manje tamne energije,
11:46
well they collapse back on themselves so quickly
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dolazi do unutrašnjeg kolapsa tako brzo
11:48
that, again, galaxies don't form.
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da se galaksije opet ne formiraju.
11:51
And without galaxies, there are no stars, no planets
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Bez galaksija, nema zvezda, nema planeta
11:54
and no chance
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i nema šanse da
11:56
for our form of life
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naš oblik života
11:58
to exist in those other universes.
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postoji u tim drugim univerzumima.
12:00
So we find ourselves in a universe
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Zato se nalazimo u univerzumu
12:02
with the particular amount of dark energy we've measured
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sa određenom količinom tamne energije koju smo izmerili
12:05
simply because our universe has conditions
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prosto zato što naš univerzum ima uslove
12:08
hospitable to our form of life.
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koji su pogodni za naš oblik života.
12:12
And that would be that.
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To bi bilo to.
12:14
Mystery solved,
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Misterija rešena,
12:16
multiverse found.
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multiverzum nađen.
12:18
Now some find this explanation unsatisfying.
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Neki nisu zadovoljni ovim objašnjenjem.
12:23
We're used to physics
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Navikli smo da nam fizika
12:25
giving us definitive explanations for the features we observe.
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daje konačna objašnjenja odlika koje opažamo.
12:28
But the point is,
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Ali poenta je u tome,
12:30
if the feature you're observing
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da ako odlika koju zapažate
12:33
can and does take on
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može da ima i ima
12:35
a wide variety of different values
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niz različitih vrednosti
12:37
across the wider landscape of reality,
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u širokom predelu realnosti,
12:40
then thinking one explanation
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onda razmišljanje o jednom objašnjenju
12:42
for a particular value
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za određnu vrednost
12:44
is simply misguided.
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je jednostavno neispravno.
12:47
An early example
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Rani primer
12:49
comes from the great astronomer Johannes Kepler
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dolazi od velikog astronoma Johana Keplera
12:52
who was obsessed with understanding
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koji je bio opsednut razumevanjem
12:54
a different number --
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jednog drugog broja -
12:56
why the Sun is 93 million miles away from the Earth.
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zašto je Sunce udaljeno 150 miliona km od Zemlje.
13:00
And he worked for decades trying to explain this number,
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Decenijama je pokušavao da objasni ovaj broj,
13:03
but he never succeeded, and we know why.
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ali nikada nije uspeo i znamo zašto.
13:06
Kepler was asking
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Kepler je postavljao
13:08
the wrong question.
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pogrešno pitanje.
13:10
We now know that there are many planets
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Sada znamo da postoje mnoge planete
13:13
at a wide variety of different distances from their host stars.
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koje su na različitim rastojanjima od svojih matičnih zvezda.
13:16
So hoping that the laws of physics
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Zato je nadanje da će zakoni fizike
13:19
will explain one particular number, 93 million miles,
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objasniti jedan određeni broj, 150 miliona km,
13:22
well that is simply wrongheaded.
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jednostavno pogrešno.
13:25
Instead the right question to ask is,
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Umesto toga pravo pitanje jeste,
13:27
why do we humans find ourselves on a planet
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zašto se ljudi nalaze na planeti,
13:30
at this particular distance,
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na određenoj udaljenosti,
13:32
instead of any of the other possibilities?
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umesto svih ostalih mogućnosti?
13:35
And again, that's a question we can answer.
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I opet, to je pitanje na koje možemo da odgovorimo.
13:38
Those planets which are much closer to a star like the Sun
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Sve one planete koje su mnogo bliže zvezdi poput Sunca
13:41
would be so hot
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bile bi toliko tople
13:43
that our form of life wouldn't exist.
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da naš oblik života ne bi postojao.
13:45
And those planets that are much farther away from the star,
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A one planete koje su mnogo dalje od zvezde,
13:48
well they're so cold
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one su toliko hladne
13:50
that, again, our form of life would not take hold.
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da naš oblik života ne bi mogao da opstane.
13:52
So we find ourselves
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Tako da se nalazimo
13:54
on a planet at this particular distance
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na planeti pri ovoj određenoj udaljenosti
13:56
simply because it yields conditions
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prosto jer nam daje uslove
13:58
vital to our form of life.
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ključne za naš oblik života.
14:01
And when it comes to planets and their distances,
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A kada su u pitanju planete i njihova udaljenost,
14:04
this clearly is the right kind of reasoning.
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ovo je očigledno ispravan način razmišljanja.
14:08
The point is,
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Poenta je,
14:10
when it comes to universes and the dark energy that they contain,
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da kada su u pitanju univerzumi i tamna energija koju sadrže,
14:13
it may also be the right kind of reasoning.
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to takođe može biti ispravan način razmišljanja.
14:17
One key difference, of course,
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Jedna ključna razlika, naravno,
14:20
is we know that there are other planets out there,
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jeste da znamo da postoji još planeta,
14:22
but so far I've only speculated on the possibility
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ali do sada smo samo spekulisali o mogućnosti
14:25
that there might be other universes.
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da postoje drugi univerzumi.
14:27
So to pull it all together,
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Znači da bismo sve spojili,
14:29
we need a mechanism
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potreban nam je mehanizam
14:31
that can actually generate other universes.
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koji stvarno generiše druge univerzume.
14:34
And that takes me to my final part, part three.
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To me dovodi do mog konačnog dela, trećeg dela.
14:37
Because such a mechanism has been found
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Jer su takav mehanizam pronašli
14:40
by cosmologists trying to understand the Big Bang.
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kosmolozi koji pokušavaju da razumeju Veliki prasak.
14:43
You see, when we speak of the Big Bang,
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Vidite, kada govorimo o Velikom prasku,
14:45
we often have an image
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često imamo sliku
14:47
of a kind of cosmic explosion
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neke kosmičke eksplozije
14:49
that created our universe
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koja je stvorila univerzum
14:51
and set space rushing outward.
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i izbacila svemir napolje.
14:54
But there's a little secret.
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Ali postoji mala tajna.
14:56
The Big Bang leaves out something pretty important,
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Veliki prasak izostavlja nešto veoma važno,
14:59
the Bang.
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prasak.
15:01
It tells us how the universe evolved after the Bang,
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On nam govori o tome kako se univerzum razvio nakon praska,
15:04
but gives us no insight
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ali nam ne daje uvid
15:06
into what would have powered the Bang itself.
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u to šta je dalo energiju samom prasku.
15:10
And this gap was finally filled
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A ova rupa je konačno popunjena
15:12
by an enhanced version of the Big Bang theory.
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boljom verzijom teorije Velikog praska.
15:14
It's called inflationary cosmology,
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Zove se inflatorna kosmologija,
15:17
which identified a particular kind of fuel
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koja je identifikovala određenu vrstu goriva
15:21
that would naturally generate
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koje bi prirodno generisalo
15:23
an outward rush of space.
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izbijanje prostora ka spolja.
15:25
The fuel is based on something called a quantum field,
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Gorivo se zasniva na nečemu nazvanom kvantno polje,
15:28
but the only detail that matters for us
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ali jedini podatak koji nam je važan
15:31
is that this fuel proves to be so efficient
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jeste da je ovo gorivo toliko efikasno
15:34
that it's virtually impossible
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da je praktično nemoguće
15:36
to use it all up,
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da se sve potroši,
15:38
which means in the inflationary theory,
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što znači da prema inflatornoj teoriji,
15:40
the Big Bang giving rise to our universe
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Veliki prasak koji je stvorio naš univerzum
15:43
is likely not a one-time event.
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verovatno nije jedinstveni događaj.
15:46
Instead the fuel not only generated our Big Bang,
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Umesto toga gorivo je generisalo ne samo naš Veliki prasak,
15:49
but it would also generate countless other Big Bangs,
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već i bezbroj drugih Velikih praskova,
15:55
each giving rise to its own separate universe
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svaki bi stvorio svoj posebni univerzum,
15:58
with our universe becoming but one bubble
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a naš univerzum bi bio samo jedan mehur
16:00
in a grand cosmic bubble bath of universes.
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u velikoj kosmičkoj peni za kupanje univerzuma.
16:03
And now, when we meld this with string theory,
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Sada, kada spojimo ovo sa teorijom struna,
16:05
here's the picture we're led to.
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evo slike do koje dolazimo.
16:07
Each of these universes has extra dimensions.
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Svaki od ovih univerzuma ima dodatne dimenizije.
16:09
The extra dimensions take on a wide variety of different shapes.
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Ekstra dimenzije imaju niz različitih oblika.
16:12
The different shapes yield different physical features.
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Različiti oblici daju različite fizičke odlike.
16:15
And we find ourselves in one universe instead of another
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I mi smo u jednom univerzumu umesto u drugom,
16:18
simply because it's only in our universe
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jednostavno jer su samo u našem univerzumu
16:21
that the physical features, like the amount of dark energy,
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fizičke odlike, kao što je količina tamne energije,
16:24
are right for our form of life to take hold.
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pogodne za razvoj našeg oblika života.
16:28
And this is the compelling but highly controversial picture
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Ovo je zanimljiva, ali veoma kontroverzna slika
16:31
of the wider cosmos
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šireg kosmosa
16:33
that cutting-edge observation and theory
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koju su nas najnovija zapažanja i teorija
16:35
have now led us to seriously consider.
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naterali da ozbiljno razmotrimo.
16:39
One big remaining question, of course, is,
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Ostaje jedno veliko pitanje, a to je,
16:43
could we ever confirm
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da li bismo ikada mogli da potvrdimo
16:46
the existence of other universes?
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postojanje drugih univerzuma?
16:49
Well let me describe
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Objasniću vam
16:51
one way that might one day happen.
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jedan način na koji bi to moglo da se dogodi.
16:54
The inflationary theory
403
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Inflaciona teorija
16:56
already has strong observational support.
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već ima jaku podršku iz zapažanja.
16:58
Because the theory predicts
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Jer teorija predviđa
17:00
that the Big Bang would have been so intense
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da bi Veliki prasak bio toliko intenzivan
17:02
that as space rapidly expanded,
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da bi se dok se svemir brzo širio,
17:05
tiny quantum jitters from the micro world
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sićušni kvantni titraji mikro sveta
17:07
would have been stretched out to the macro world,
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proširli u makro svet,
17:10
yielding a distinctive fingerprint,
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dajući upadljiv otisak,
17:13
a pattern of slightly hotter spots and slightly colder spots,
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raspored blago toplijih tačaka i blago hladnijih tačaka,
17:15
across space,
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širom svemira,
17:17
which powerful telescopes have now observed.
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koji su sada zapazili jaki teleskopi.
17:20
Going further, if there are other universes,
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Ako idemo dalje, ako postoji još univerzuma,
17:23
the theory predicts that every so often
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teorija predviđa da se svako malo
17:25
those universes can collide.
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ti univerzumi mogu sudariti.
17:27
And if our universe got hit by another,
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I ako bi naš univerzum udario drugi,
17:29
that collision
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taj sudar
17:31
would generate an additional subtle pattern
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bi stvorio dodatan suptilan raspored
17:33
of temperature variations across space
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temperaturnih varijacija širom svemira
17:35
that we might one day
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koje bismo mogli jednog dana
17:37
be able to detect.
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da detektujemo.
17:39
And so exotic as this picture is,
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I ma koliko ova slika bila egzotična,
17:42
it may one day be grounded
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jednog dana bi mogla biti zasnovana
17:44
in observations,
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na opservacijama,
17:46
establishing the existence of other universes.
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utvrđujući postojanje drugih univerzuma.
17:49
I'll conclude
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Završiću sa
17:51
with a striking implication
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bitnim implikacijama
17:54
of all these ideas
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svih ovih ideja
17:56
for the very far future.
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za veoma daleku budućnost.
17:58
You see, we learned
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Vidite, naučili smo
18:00
that our universe is not static,
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da naš univerzum nije statičan,
18:02
that space is expanding,
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da se svemir širi,
18:04
that that expansion is speeding up
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da se to širenje ubrzava
18:06
and that there might be other universes
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i da možda postoji još univerzuma
18:08
all by carefully examining
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samo pažljivim pregledanjem
18:10
faint pinpoints of starlight
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slabašnih tačaka zvezdanog svetla
18:12
coming to us from distant galaxies.
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koje dolazi do nas iz udaljenih galaksija.
18:15
But because the expansion is speeding up,
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Pošto se širenje ubrzava,
18:18
in the very far future,
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u veoma dalekoj budućnosti
18:20
those galaxies will rush away so far and so fast
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te galaksije će se udaljiti toliko daleko i toliko brzo
18:23
that we won't be able to see them --
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da nećemo moći da ih vidimo -
18:26
not because of technological limitations,
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ne zbog tehnoloških ograničenja,
18:28
but because of the laws of physics.
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već zbog zakona fizike.
18:30
The light those galaxies emit,
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Svetlost koju te galaksije emituju,
18:32
even traveling at the fastest speed, the speed of light,
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čak i kada putuju pri najbržoj brzini, brzini svetlosti,
18:35
will not be able to overcome
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neće moći da premosti
18:37
the ever-widening gulf between us.
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sve veći jaz između nas.
18:40
So astronomers in the far future
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Zato astronomi u dalekoj budućnosti
18:42
looking out into deep space
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koji gledaju u dalek svemir
18:44
will see nothing but an endless stretch
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neće videti ništa osim beskonačnog prostranstva
18:47
of static, inky, black stillness.
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statične, mastiljave, crne tišine.
18:51
And they will conclude
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Oni će zaključiti
18:53
that the universe is static and unchanging
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da je univerzum statičan i nepromenljiv
18:55
and populated by a single central oasis of matter
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i nastanjen jednom centralnom oazom materije
18:58
that they inhabit --
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koju oni nastanjuju -
19:00
a picture of the cosmos
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slika kosmosa
19:02
that we definitively know to be wrong.
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za koju definitivno znamo da je pogrešna.
19:05
Now maybe those future astronomers will have records
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Možda će ti budući astronomi imati dokaze
19:08
handed down from an earlier era,
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prenete iz ranijeg doba,
19:10
like ours,
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poput našeg,
19:12
attesting to an expanding cosmos
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koji potvrđuju da se kosmos širi
19:14
teeming with galaxies.
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prepun galaksija.
19:16
But would those future astronomers
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Ali da li će ti budući astronomi
19:18
believe such ancient knowledge?
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verovati u to drevno znanje?
19:21
Or would they believe
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Ili će verovati
19:23
in the black, static empty universe
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u crni, statični prazni univerzum
19:26
that their own state-of-the-art observations reveal?
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koji pokazuju njihova najnovija zapažanja?
19:30
I suspect the latter.
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Nagađam da će biti ovo drugo.
19:32
Which means that we are living
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Što znači da živimo
19:34
through a remarkably privileged era
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u izuzetno privilegovanom dobu,
19:37
when certain deep truths about the cosmos
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u kome su neke suštinske istine o kosmosu
19:39
are still within reach
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i dalje na dohvat
19:41
of the human spirit of exploration.
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ljudskog istraživačkog duha.
19:43
It appears that it may not always be that way.
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Izgleda da možda neće uvek biti tako.
19:48
Because today's astronomers,
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Jer današnji astronomi su,
19:50
by turning powerful telescopes to the sky,
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usmeravajući jake teleskope ka nebu,
19:53
have captured a handful of starkly informative photons --
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uhvatili nekolicinu veoma informativnih fotona -
19:56
a kind of cosmic telegram
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vrstu kosmičkog telegrama
19:59
billions of years in transit.
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milijardi godina u tranzitu.
20:01
and the message echoing across the ages is clear.
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Poruka koja odzvanja kroz vekove je jasna.
20:05
Sometimes nature guards her secrets
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Nekada priroda štiti svoje tajne
20:08
with the unbreakable grip
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čvrstom rukom
20:10
of physical law.
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fizičkog zakona.
20:12
Sometimes the true nature of reality beckons
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Nekada nas prava priroda realnosti doziva
20:16
from just beyond the horizon.
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negde preko horizonta.
20:19
Thank you very much.
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Hvala vam puno.
20:21
(Applause)
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(Aplauz)
20:25
Chris Anderson: Brian, thank you.
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Kris Anderson: Brajane, hvala ti.
20:27
The range of ideas you've just spoken about
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Raspon ideja o kojima si nam pričao
20:29
are dizzying, exhilarating, incredible.
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je vrtoglav, uzbudljiv, neverovatan.
20:32
How do you think
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Gde misliš
20:34
of where cosmology is now,
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da je kosmologija sada,
20:36
in a sort of historical side?
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sa istorijskog aspekta?
20:38
Are we in the middle of something unusual historically in your opinion?
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Da li smo usred nečega istorijski neobičnog, prema tebi?
20:41
BG: Well it's hard to say.
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BG: Teško je reći.
20:43
When we learn that astronomers of the far future
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Kada saznamo da astronomi u dalekoj budućnosti
20:46
may not have enough information to figure things out,
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možda neće imati dovoljno informacija da saznaju stvari,
20:49
the natural question is, maybe we're already in that position
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postavlja se pitanje, možda smo već u toj poziciji
20:52
and certain deep, critical features of the universe
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i neke duboke, ključne odlike univerzuma
20:55
already have escaped our ability to understand
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su već utekle našoj sposobnosti da ih razumemo
20:58
because of how cosmology evolves.
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zbog načina na koji se kosmologija razvija.
21:00
So from that perspective,
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Iz te perspektive,
21:02
maybe we will always be asking questions
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možda ćemo uvek postavljati pitanja
21:04
and never be able to fully answer them.
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i nikada nećemo moći u potpunosti da ih razumemo.
21:06
On the other hand, we now can understand
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Sa druge strane, sada možemo da razumemo
21:08
how old the universe is.
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koliko je star univerzum.
21:10
We can understand
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Možemo razumeti
21:12
how to understand the data from the microwave background radiation
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kako da razumemo podatke mikrotalasnog pozadinskog zračenja
21:15
that was set down 13.72 billion years ago --
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koje je poslato pre 13,72 milijardi godina -
21:18
and yet, we can do calculations today to predict how it will look
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danas možemo da izračunamo kako da predvidimo kako će izgledati
21:20
and it matches.
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i poklapa se.
21:22
Holy cow! That's just amazing.
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Tako mi svega! To je neverovatno.
21:24
So on the one hand, it's just incredible where we've gotten,
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Sa jedne strane, potpuno je neverovatno dokle smo stigli,
21:27
but who knows what sort of blocks we may find in the future.
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ali ko zna na kakve prepreke možemo naići u budućnosti.
21:31
CA: You're going to be around for the next few days.
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KA: Ti ćeš biti tu narednih par dana.
21:34
Maybe some of these conversations can continue.
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Možda se neki od ovih razgovora mogu nastaviti.
21:36
Thank you. Thank you, Brian. (BG: My pleasure.)
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Hvala ti. Hvala ti, Brajane. (BG: Bilo mi je zadovoljstvo.)
21:38
(Applause)
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(Aplauz)
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