The Extreme Energies Lines in the Solar Neutrino Spectrum

Details The Extreme Energies Lines in the Solar Neutrino Spectrum The Extreme Energies Lines in the Solar Neutrino Spectrum

2010-05-19

arxiv.org/abs/1005.3458v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Scientific paper

Tritium chain of the hydrogen cycle in the Sun including reactions ^3He(e^-,{\nu}_(e))^(3)H(p,{\gamma})^(4)He is considered. At the distance of 1 a.u. the flux of tritium neutrinos is equal to 8.1\cdot 10^(4) cm^(-2)s^(-1). It is an order of magnitude higher than the flux of the (hep)-neutrinos. Radial distribution of ^(3)H-neutrinos yield inside the Sun and their energy spectrum which has a form of line at the energy of (2,5 {\div} 3,0) keV are calculated. The flux of thermal tritium neutrinos is accompanied by a very weak flux of antineutrinos (~ 10^(3) cm^(-2)year^(-1)) with energy lower than 18,6 keV. These antineutrinos are produced during Urca processes ^3He<=>^3H. The flux of the neutrinos of maximum possible energy (line 19,8 MeV) produced due to the (heep)-reaction (related to the (hep)-process) is estimated

Affiliated with

Also associated with

No associations

Rating

The Extreme Energies Lines in the Solar Neutrino Spectrum does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Extreme Energies Lines in the Solar Neutrino Spectrum, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Extreme Energies Lines in the Solar Neutrino Spectrum will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-479910