The laws of physics may permit a neutrino with a mass to change from one type into another,
so electron neutrinos may simply transform themselves into undetectable muon or tau neutrinos before they fly across the 150 million kilometres of space between the Sun and the Earth.
Not exact matches
But the weak nuclear force — responsible for making neutrons decay into protons,
electrons and
neutrinos — might not be
so essential (SN: 4/29/17, p. 22).
But if they are within 100,000 times or
so the mass of normal
neutrinos — or a few thousand
electron volts — most should still exist, with some occasionally decaying into lighter
neutrinos and X-ray photons.
In the paper, Glashow and Cohen point out that if
neutrinos can travel faster than light, then when they do
so they should sometimes radiate an
electron paired with its antimatter equivalent — a positron — through a process called Cerenkov radiation, which is analogous to a sonic boom.
So rather than, say, a 10 percent chance of an
electron neutrino turning into a muon
neutrino, for example, physicists wonder if the odds are lower that an
electron antineutrino turns into a muon antineutrino.
Carrying no electrical charge,
neutrinos are attracted neither to protons nor
electrons,
so they don't interact with electromagnetic fields.
Since 1998, physicists have also known that
neutrinos can change type as they zing along at near light - speed,
so that a muon
neutrino can become an
electron neutrino, and
so on.
For example,
electron neutrinos born in the sun morph into other flavors before they reach Earth,
so that fewer
electron neutrinos arrive than would otherwise be expected.
In doing
so, Daya Bay researchers searched for a faster, smaller oscillation imposed on top of the longer, slower one that accounts for the disappearance of
electron neutrinos from the sun, which is dominated by a different mixing angle.
In addition to these particles, there are heavier particles, which don't appear in ordinary matter because there's
so heavy; they're unstable and they decay into the particle's I mentioned —
electrons,
neutrinos and the two lightest types of quarks.
So in the very early Universe, some 17 keV
neutrinos could have been transformed into
electron neutrinos before they could decay, adding to the pressure of the big bang.
Although the mass of such a
neutrino is small (17 keV compared with about 500 keV for an
electron),
neutrinos are thought to be
so common in the Universe that they could have a profound influence on the way the Universe has evolved.