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動画の字幕をクリックしてすぐ単語の意味を調べられます!
単語帳読み込み中…
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They're everywhere, but you will never see one.
Trillions of them are flying through you right this second,
but you can't feel them.
These ghost particles are called neutrinos and if we can catch them,
they can tell us about the furthest reaches
and most extreme environments of the universe.
Neutrinos are elementary particles,
meaning that they can't be subdivided into other particles the way atoms can.
Elementary particles are the smallest known building blocks
of everything in the universe,
and the neutrino is one of the smallest of the small.
A million times less massive than an electron,
neutrinos fly easily through matter, unaffected by magnetic fields.
In fact, they hardly ever interact with anything.
That means that they can travel through the universe in a straight line
for millions, or even billions, of years,
safely carrying information about where they came from.
So where do they come from?
Pretty much everywhere.
They're produced in your body from the radioactive decay of potassium.
Cosmic rays hitting atoms in the Earth's atmosphere
create showers of them.
They're produced by nuclear reactions inside the sun
and by radioactive decay inside the Earth.
And we can generate them in nuclear reactors
and particle accelerators.
But the highest energy neutrinos are born far out in space
in environments that we know very little about.
Something out there, maybe supermassive black holes,
or maybe some cosmic dynamo we've yet to discover,
accelerates cosmic rays to energies over a million times greater
than anything human-built accelerators have achieved.
These cosmic rays, most of which are protons,
interact violently with the matter and radiation around them,
producing high-energy neutrinos,
which propagate out like cosmic breadcrumbs
that can tell us about the locations
and interiors of the universe's most powerful cosmic engines.
That is, if we can catch them.
Neutrinos' limited interactions with other matter
might make them great messengers,
but it also makes them extremely hard to detect.
One way to do so is to put a huge volume of pure transparent material in their path
and wait for a neutrino to reveal itself
by colliding with the nucleus of an atom.
That's what's happening in Antarctica at IceCube,
the world's largest neutrino telescope.
It's set up within a cubic kilometer of ice
that has been purified by the pressure
of thousands of years of accumulated ice and snow,
to the point where it's one of the clearest solids on Earth.
And even though it's shot through with boreholes holding over 5,000 detectors,
most of the cosmic neutrinos racing through IceCube will never leave a trace.
But about ten times a year,
a single high-energy neutrino collides with a molecule of ice,
shooting off sparks of charged subatomic particles
that travel faster through the ice than light does.
In a similar way to how a jet that exceeds the speed of sound
produces a sonic boom,
these superluminal charged particles leave behind a cone of blue light,
kind of a photonic boom.
This light spreads through IceCube,
hitting some of its detectors located over a mile beneath the surface.
Photomultiplier tubes amplify the signal,
which contains information about the charged particles' paths and energies.
The data are beamed to astrophysicists around the world
who look at the patterns of light
for clues about the neutrinos that produced them.
These super energetic collisions are so rare
that IceCube's scientists give each neutrino nicknames,
like Big Bird and Dr. Strangepork.
IceCube has already observed
the highest energy cosmic neutrinos ever seen.
The neutrinos it detects should finally tell us where cosmic rays come from
and how they reached such extreme energies.
Light, from infrared, to x-rays, to gamma rays,
has given us increasingly energetic
and continuously surprising views of the universe.
We are now at the dawn of the age of neutrino astronomy,
and we have no idea what revelations IceCube
and other neutrino telescopes may bring us
about the universe's most violent, most energetic phenomena.
コツ:単語をクリックしてすぐ意味を調べられます!

読み込み中…

【TED-Ed】Why neutrinos matter - Sílvia Bravo Gallart

1521 タグ追加 保存
稲葉白兎 2015 年 5 月 9 日 に公開
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