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Why neutrinos matter - Sílvia Bravo Gallart

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

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Video Language:
English
Team:
closed TED
Project:
TED-Ed
Duration:
04:41

English subtitles

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