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Can't see them, can't feel them, but know
they exist
Neutrino - the ghost particle
Neutrinos are a leptons, an elementary particle. They do not have electric
charge, and they interact with matter via the weak nuclear force. The
weakness of the weak force gives neutrinos the property that matter
is almost transparent to them. For the over a half a century scientists
believed that neutrinos are massless, and that they travel at the speed
of light
By MARIJA MITROVIĆ
from Belgrade, SERBIA
Look at your thumbnail! Did you know that in this moment about 100 billion
solar neutrinos pass through your thumbnail! You didn't noticed
that?!Maybe if you look again. Nothing? That is strange, or it's not.
Neutrinos are a leptons, an elementary particle. They do not have electric
charge, and they interact with matter via the weak nuclear force. The
weakness of the weak force gives neutrinos the property that matter
is almost transparent to them. For the over a half a century scientists
believed that neutrinos are massless, and that they travel at the speed
of light. This believes were in line with The Standard Model, a theory
which describes three of the four known fundamental interactions between
the elementary particles that make up all matter. Today we know that
neutrino has mass, but we can only estimate its value, and we know that
it is very small.
The neutrino was first postulated in December, 1930 by Wolfgang Pauli
to explain conservation of energy in beta decay. When neutron decays
into a proton and electron, we would expect that energies of electrons
emitted by beta decay had a discrete spectrum. But experiments were
in disagreement with theory. In 1911 Lise Meitner and Otto Han performed
an experiment that showed that the energies of electrons had a continuous
spectrum. To resolve this inconsistency, Pauli suggested that in addition
to electrons and protons atoms also contained an extremely light neutral
particle which he called the neutron. He suggested that this "neutron"
was also emitted during beta decay and had simply not yet been observed.
In 1931 Enrico Fermi renamed Pauli's "neutron" to neutrino.
Actually, that third particle is antiparticle of neutrino, called anti-neutrino.
Pauli believed that scientists will never detect neutrinos, because
of their "ghostly" properties. But, in 1956 Clyde Cowan, Frederic
Reines, and their colleagues preformed an neutrino experiment. In this
experiment, neutrinos created in a nuclear reactor by beta decay were
shot into protons producing neutrons and positrons (antiparticle of
electron) both of which could be detected. This way they indirectly
proved that neutrino exists. Today we know that this way they proved
existing of anti-neutrinos.
Still there was a problem of detecting neutrino. Physicist Bruno Pontecorvo,
suggested that one might be able to capture neutrinos from a reactor
using chlorine. The neutrinos from the reactor would convert some of
the chlorine atoms to argon atoms, which are radioactive and could be
counted in small quantities in small counters. One could be sensitive
to even something as weakly interacting as a neutrino if one had a huge
vat of chlorine. If we can detect neutrinos we can use them to look
deep into the Sun. How? Well, light, as we all know, doesn't penetrate
anything. If you put your hand in front of your face, others can not
see your faces; the light won't go through your hand. It doesn't penetrate
any appreciable amount of material. Neutrinos can go through unimaginable
amounts of material
without being affected. There is less than a percent chance that anything
would ever happen to them as they passed through the sun, certainly
through the Earth.
Raymond Davis Jr. was the first one who successfully detected solar
neutrinos. Davis developed an experiment based on this idea by placing
a 400 000 liters tank of dry-cleaning chemical which is a good source
of chlorine, one and a half kilometer underground in the Homestake Gold
Mine in South Dakota and developing techniques for quantitatively extracting
a few atoms of argon from the tank. The chlorine target was located
deep underground to protect it from cosmic rays. This experiment confirmed
that the sun produces neutrinos, but only about one-third of the number
of neutrinos predicted by theory of John Bahcall could be detected.
This problem was known as a "solar neutrino puzzle" and it
is resolved a few years ago, in 2001. John Bahcall predicted the number
of solar neutrinos, using all our knowledge about nuclear reaction which
are happening on Sun. So everything we knew about Sun would be brought
into the question if Davis's experiment was right. Bouth, Davis and
Bahcall insisted that they were right, and they were. Strange? Well,
actually it is not so strange. There are three known types ( flavors
) of neutrinos: electron neutrino, muon neutrino and tau neutrino, named
after their partner leptons in the Standard Model. The correspondence
between the six quarks in the Standard Model and the six leptons, among
them the three neutrinos, suggests to physicist's intuition that there
should be exactly three types of neutrino. However, actual proof that
there are only three kinds of neutrinos remains an elusive goal of particle
physics. During their trip, from the Sun to the Earth, neutrinos are
changing their flavor. This is called neutrinos oscillation. Only one
third of electron neutrinos, produced in the Sun is reaching Earth as
electron neutrinos, which we can detect. This explanation has one problem.
If neutrinos do not have a mass, they can not interact with each other,
so they can not change flavor.
The "solar neutrino puzzle" gave birth to different experiments
by scientists around the world, all working to confirm the solar neutrino
deficit and to prove that they have a mass. First came Kamiokande in
Japan, then SAGE in the former Soviet Union, GALLEX in Italy, and then
Super Kamiokande. Finally, in 2001-2002, scientists working at SNO,
the Sudbury Neutrino Observatory in Ontario, Canada, found strong evidence
that the neutrino has the ability to oscillate.
They are here, we can not see them, we can not feel them, but we know
that they exist.
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