Long range neutrino forces and the lower bound on neutrino mass

Details Long range neutrino forces and the lower bound on neutrino mass Long range neutrino forces and the lower bound on neutrino mass

1996-04-30

arxiv.org/abs/hep-ph/9604443v2

Physics

High Energy Physics

High Energy Physics - Phenomenology

More detailed discussion of the blocking mechanism is given LaTeX, 7 pages, no figures

Scientific paper

Stellar objects (including our Sun, other stars of main sequence, white dwarfs, neutron stars etc.) contain strongly degenerate low energy sea of neutrinos (in neutron stars) or antineutrinos. The presence of this sea leads due to Pauli principle and thermal effects to effective blocking of the long-range neutrino forces. This blocking can resolve the problem of the unphysically large value of the self-energy of stars stipulated by many body long-range neutrino interactions. As a consequence no lower bound on the neutrino mass is inferred, in contrast with the statement by Fischbach.

Affiliated with

Also associated with

No associations

Rating

Long range neutrino forces and the lower bound on neutrino mass 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 Long range neutrino forces and the lower bound on neutrino mass, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Long range neutrino forces and the lower bound on neutrino mass will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-502198