Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvl..61.2171s&link_type=abstract
Physical Review Letters (ISSN 0031-9007), vol. 61, Nov. 7, 1988, p. 2171-2174.
Astronomy and Astrophysics
Astrophysics
2
Neutrinos, Nuclear Astrophysics, Plasma Density, Supernovae, Correlation, Density (Mass/Volume), Transport Properties
Scientific paper
The effects of interactions on the density fluctuations of an n, p, e plasma are calculated. The scattering of neutrinos arising from the Fermi part of the neutral current interactions with protons, under supernova conditions, is practically extinguished by Coulomb effects in the plasma. Charged-current reactions are discussed in terms of off-diagonal density fluctuations. Inclusion of the symmetry energy term in the nuclear interaction gives rise to a large reduction in the Fermi part of the cross section for nu + n yields e(-) + p.
No associations
LandOfFree
Diagonal and off-diagonal density fluctuations in hot nuclear matter, and applications to neutrino transport in supernovae 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 Diagonal and off-diagonal density fluctuations in hot nuclear matter, and applications to neutrino transport in supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Diagonal and off-diagonal density fluctuations in hot nuclear matter, and applications to neutrino transport in supernovae will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1827920