Why neutrinos matter - Sílvia Bravo Gallart

Zašto su neutrini važni? - Silvija Bravo Galart (Sílvia Bravo Gallart)

448,339 views

2015-04-28 ・ TED-Ed


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Why neutrinos matter - Sílvia Bravo Gallart

Zašto su neutrini važni? - Silvija Bravo Galart (Sílvia Bravo Gallart)

448,339 views ・ 2015-04-28

TED-Ed


Please double-click on the English subtitles below to play the video.

Prevodilac: Tijana Mihajlović Lektor: Mile Živković
00:06
They're everywhere, but you will never see one.
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Svuda su, ali nikada nećete videti neki.
00:10
Trillions of them are flying through you right this second,
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Trilioni njih proleću kroz vas upravo ove sekunde,
00:13
but you can't feel them.
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ali ne možete da ih osetite.
00:15
These ghost particles are called neutrinos and if we can catch them,
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Ove fantomske čestice zovu se neutrini i ako bismo ih uhvatili,
00:19
they can tell us about the furthest reaches
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mogle bi nam reći o najdaljim prostranstvima
00:21
and most extreme environments of the universe.
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i najekstremnijim okruženjima u svemiru.
00:25
Neutrinos are elementary particles,
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Neutrini su elementarne čestice,
00:27
meaning that they can't be subdivided into other particles the way atoms can.
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što znači da se ne mogu dodatno deliti na druge delove na koje atomi mogu.
00:32
Elementary particles are the smallest known building blocks
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Osnovne čestice najmanje su gradivne jedinice
00:35
of everything in the universe,
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svega u svemiru,
00:37
and the neutrino is one of the smallest of the small.
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a neutrino je najmanji među malima.
00:41
A million times less massive than an electron,
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Milion puta manje mase nego elektron,
00:44
neutrinos fly easily through matter, unaffected by magnetic fields.
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neutrini lako proleću kroz materiju, bez uticaja magnetnog polja na njih.
00:48
In fact, they hardly ever interact with anything.
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U stvari, oni jedva da saobraćaju sa nečim.
00:51
That means that they can travel through the universe in a straight line
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To znači da mogu putovati kroz svemir pravolinijski
00:55
for millions, or even billions, of years,
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milionima, čak i milijardama godina,
00:58
safely carrying information about where they came from.
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bezbedno prenoseći informacije o tome odakle su došli.
01:02
So where do they come from?
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Pa, odakle dolaze?
01:04
Pretty much everywhere.
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Skoro odasvud.
01:06
They're produced in your body from the radioactive decay of potassium.
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Proizvode se u vašem telu kroz radioaktivno raspadanje kalijuma.
01:10
Cosmic rays hitting atoms in the Earth's atmosphere
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Kosmički zraci koji udaraju u atome u Zemljinoj atmosferi
01:14
create showers of them.
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stvaraju kiše neutrina.
01:16
They're produced by nuclear reactions inside the sun
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Proizvode ih nuklearne reakcije unutar Sunca
01:19
and by radioactive decay inside the Earth.
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i radioaktivno raspadanje unutar Zemlje.
01:22
And we can generate them in nuclear reactors
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Možemo da ih proizvedemo i u nuklearnim reaktorima
01:24
and particle accelerators.
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i akceleratorima čestica.
01:26
But the highest energy neutrinos are born far out in space
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Međutim, neutrini sa navišom energijom rađaju se daleko u svemiru
01:30
in environments that we know very little about.
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u okruženjima o kojima znamo veoma malo.
01:34
Something out there, maybe supermassive black holes,
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Nešto što se tamo nalazi, možda supermasivne crne rupe,
01:37
or maybe some cosmic dynamo we've yet to discover,
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ili možda nekakav svemirski generator koji tek treba da otkrijemo
01:41
accelerates cosmic rays to energies over a million times greater
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ubrzava kosmičke zrake do energija koje su preko milion puta veće
01:45
than anything human-built accelerators have achieved.
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od bilo čega što su akceleratori koje su ljudi izgradili postigli.
01:49
These cosmic rays, most of which are protons,
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Ovi kosmički zraci, od kojih su većina protoni,
01:52
interact violently with the matter and radiation around them,
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ostvaruju snažnu interakciju sa materijom i radijacijom oko sebe,
01:56
producing high-energy neutrinos,
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proizvodeći visokoenergetske neutrine,
01:58
which propagate out like cosmic breadcrumbs
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koji se razmnožavaju kao kosmičke mrvice
02:00
that can tell us about the locations
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koje nam mogu doneti podatke o mestima
02:02
and interiors of the universe's most powerful cosmic engines.
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i unutrašnjostima svemirskih najmoćnijih mašina,
02:07
That is, if we can catch them.
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to jest, ako uspemo da ih uhvatimo.
02:09
Neutrinos' limited interactions with other matter
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Ograničena interakcija neutrina sa drugom materijom
02:12
might make them great messengers,
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mogla bi ih učiniti sjajnim glasnicima,
02:14
but it also makes them extremely hard to detect.
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ali ih čini i jako teškim za uočavanje.
02:17
One way to do so is to put a huge volume of pure transparent material in their path
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Jedan način da se to uradi je da se na njihov put postavi
ogromna zapremina čistog providnog materijala
02:22
and wait for a neutrino to reveal itself
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i da se čeka da se neutrino otkrije
02:24
by colliding with the nucleus of an atom.
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kroz sudaranje sa jezgrom atoma.
02:27
That's what's happening in Antarctica at IceCube,
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To je ono što se dešava na Antartici u Ajskjubu,
02:30
the world's largest neutrino telescope.
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najvećem svetskom teleskopu za neutrine.
02:33
It's set up within a cubic kilometer of ice
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To je postavka u kubnom kilometru leda
02:35
that has been purified by the pressure
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koja je pročišćena pritiskom nastalim od snega i leda
02:37
of thousands of years of accumulated ice and snow,
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starih hiljadama godina,
02:40
to the point where it's one of the clearest solids on Earth.
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dotle da je postao jedan od najčistijih čvrstih materijala na Zemlji.
02:44
And even though it's shot through with boreholes holding over 5,000 detectors,
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Ipak, iako ima bušotine koje sadrže preko 5000 detektora,
02:48
most of the cosmic neutrinos racing through IceCube will never leave a trace.
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većina kosmičkih neutrina koji protrče kroz Ajskjub
nikada neće ostaviti trag.
02:53
But about ten times a year,
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Ipak, oko deset puta tokom godine,
02:55
a single high-energy neutrino collides with a molecule of ice,
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poneki visokoenergetski neutrino sudari se sa molekulom leda,
02:59
shooting off sparks of charged subatomic particles
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ispaljujući iskre naelektrisanih subatomskih čestica
03:02
that travel faster through the ice than light does.
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koje putuju kroz led brže nego svetlo.
03:06
In a similar way to how a jet that exceeds the speed of sound
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Slično načinu na koji mlaznjak proizvodi zvučni zid
03:09
produces a sonic boom,
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kada probije brzinu zvuka,
03:11
these superluminal charged particles leave behind a cone of blue light,
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ove superluminalne naelektrisane čestice ostavljaju za sobom
03:15
kind of a photonic boom.
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nekakvu fotosku eksploziju.
03:18
This light spreads through IceCube,
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Ovo svetlo se širi kroz Ajskjub,
03:20
hitting some of its detectors located over a mile beneath the surface.
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udarajući u neke od njegovih detektora
koji se nalaze na kilometre ispod površine.
03:23
Photomultiplier tubes amplify the signal,
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Fotomultiplikatorske cevi pojačavaju signal,
03:27
which contains information about the charged particles' paths and energies.
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koji sadrži informacije o putevima i energiji naelektrisanih čestica.
03:32
The data are beamed to astrophysicists around the world
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Podaci se usmeravaju ka astrofizičarima širom sveta
03:35
who look at the patterns of light
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koji pregledaju obrazac svetla
03:36
for clues about the neutrinos that produced them.
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da bi našli zaključke o neutrinima koji su ih stvorili.
03:39
These super energetic collisions are so rare
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Ovi superenergetski sudari su toliko retki
03:42
that IceCube's scientists give each neutrino nicknames,
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da naučnici sa Ajskjuba daju nadimak svakom neutrinu,
03:46
like Big Bird and Dr. Strangepork.
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kao što su Velika ptica ili dr. Čudnosvinjetić.
03:49
IceCube has already observed
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Ajskjub je već primetio
03:50
the highest energy cosmic neutrinos ever seen.
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kosmičke neutrine sa najvišom energijom ikada viđenom.
03:54
The neutrinos it detects should finally tell us where cosmic rays come from
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Neutrini koje detektuje bi konačno trebalo da nam pruže podatke
o tome odakle dolaze kosmički zraci
03:58
and how they reached such extreme energies.
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i kako dostižu tako visoke energije.
04:02
Light, from infrared, to x-rays, to gamma rays,
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Svetlo, od infracrvenog, preko x-zraka do gama zraka,
04:06
has given us increasingly energetic
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daje nam sve energičnije i konstantno iznenađujuće
04:08
and continuously surprising views of the universe.
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poglede na svemir.
04:11
We are now at the dawn of the age of neutrino astronomy,
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Sada se nalazimo na početku doba astronomije neutrina
04:14
and we have no idea what revelations IceCube
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i ne znamo šta nam otkrića Ajskjuba
04:17
and other neutrino telescopes may bring us
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i drugih teleskopa za neutrine mogu doneti
04:19
about the universe's most violent, most energetic phenomena.
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o svemirskim najsnažnijim pojavama sa najvišom energijom.
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