Time-dependent neutrino transport out of dense stellar cores

Details Time-dependent neutrino transport out of dense stellar cores Time-dependent neutrino transport out of dense stellar cores

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..71..219l&link_type=abstract

Astrophysics and Space Science, vol. 71, no. 1, Aug. 1980, p. 219-227.

Astronomy and Astrophysics

Astrophysics

1

Boltzmann Transport Equation, Gravitational Collapse, Neutrinos, Particle Emission, Stellar Cores, Stellar Radiation, Supernovae, Scattering, Time Dependence

Scientific paper

Time-dependent neutrino transport out of an optically thick neutronized stellar core is calculated in order to study the effects of neutrino degeneracy and of source depletion. It is found that neutrino trapping inhibits further neutrino emission until neutrinos peel out of the outer zones of the core, exposing successively inner zones. The effect of neutrino Fermi statistics is to considerably retard the disperse neutrino leakage out of the core, making neutrino transport insignificant during fast stages of core collapse.

Affiliated with

Also associated with

No associations

Rating

Time-dependent neutrino transport out of dense stellar cores 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 Time-dependent neutrino transport out of dense stellar cores, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Time-dependent neutrino transport out of dense stellar cores will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1273676