Solar neutrino

Solar neutrino

.

The main contribution comes from the so-called proton-proton chain reaction. The net reaction is:: 4 p + 2e = He + 2 u_e ! ,or in words:: 4 protons + 2 electrons = Helium + 2 electron neutrinos.

Neutrinos from the proton-proton process have energy up to 400 keV. There are also several other significant production mechanisms, with energies up to 10 MeV. [A. Bellerive, [http://arxiv.org/abs/hep-ex/0312045 Review of solar neutrino experiments] . Int.J.Mod.Phys. A19 (2004) 1167-1179]

The number of neutrinos can be predicted by the Standard Solar Model. The detected number of electron neutrinos was only 1/3 of the predicted number, and this was known as the solar neutrino problem. It led to the idea of neutrino oscillation and the fact that neutrinos can change flavour. This was confirmed when the total flux of solar neutrinos of all types was measured and it agreed with the earlier predictions of expected electron neutrino flux, as seen by Sudbury Neutrino Observatory, and thus confirmed that neutrinos have mass.

ee also

* Neutrino detection

References


Wikimedia Foundation. 2010.

Игры ⚽ Нужно решить контрольную?

Look at other dictionaries:

  • Solar neutrino unit — (SNU) is a new unit defined for convenience, which is more suitable for very low event rates.In principle there are two ways of detecting solar neutrinos: radiochemical and real time experiments. The principle of radiochemical experiments is the… …   Wikipedia

  • Solar neutrino problem — The solar neutrino problem was a major discrepancy between measurements of the numbers of neutrinos flowing through the earth and theoretical models of the solar interior, lasting from the mid 1960s to about 2002. The discrepancy has since been… …   Wikipedia

  • Solar neutrino unit — Le solar neutrino unit (abréviation SNU, parfois snu) est une unité de mesure non reconnue par le système international d unités, destinée à décrire le taux d événement captés par un détecteur de neutrinos émis par le Soleil. Les neutrinos sont… …   Wikipédia en Français

  • solar neutrino unit — (snu)    a unit used by astrophysicists to measure the rate at which neutrinos from the Sun are detected on Earth. Neutrinos are elementary particles with no charge and little or no mass (in 1999 it was reported that neutrinos do have a small… …   Dictionary of units of measurement

  • solar neutrino unit — …   Useful english dictionary

  • Neutrino oscillation — is a quantum mechanical phenomenon predicted by Bruno Pontecorvo[1] whereby a neutrino created with a specific lepton flavor (electron, muon or tau) can later be measured to have a different flavor. The probability of measuring a particular… …   Wikipedia

  • Neutrino astronomy — is the branch of astronomy that observes astronomical objects with neutrino detectors in special observatories. Nuclear reactions in stars and supernova explosions produce very large numbers of neutrinos, a very few of which may be detected by a… …   Wikipedia

  • Neutrino — Klassifikation Elementarteilchen Fermion Lepton Eigenschaften Ladung neutral Masse (E …   Deutsch Wikipedia

  • Neutrino — For other uses, see Neutrino (disambiguation). Neutrino/Antineutrino The first use of a hydrogen bubble chamber to detect neutrinos, on November 13, 1970. A neutrino hit a proton in a hydrogen atom. The collision occurred at the point where three …   Wikipedia

  • Neutrino detector — The Sudbury Neutrino Observatory, a 12 meter sphere filled with heavy water surrounded by light detectors located 2000 meters below the ground in Sudbury, Ontario, Canada. A neutrino detector is a physics apparatus designed to study neutrinos.… …   Wikipedia

Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”