Neutrino transport during the core bounce phase of a type II supernova explosion

Details Neutrino transport during the core bounce phase of a type II supernova explosion Neutrino transport during the core bounce phase of a type II supernova explosion

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...342..416g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 342, July 1, 1989, p. 416-429.

Statistics

Computation

20

Monte Carlo Method, Neutrinos, Nuclear Astrophysics, Stellar Models, Supernovae, Computational Astrophysics, Energy Spectra, Scattering, Stellar Cores

Scientific paper

A Monte Carlo study of neutrino transport in the vicinity of the outward-moving core bounce shock of a Type II SN is discussed. The method takes into account energy gains and losses produced by first-order Fermi shock acceleration and inelastic collisions with nuclei and electrons. Sources of neutrino opacity considered include scattering off electrons, nucleons, and nuclei, the absorption of electron neutrinos, and neutrino pair annihilation. Previous SN models have been used to determine the time-integrated energy spectra of the three neutrino flavors in order to determine the conditions in the star's collapsing core.

Affiliated with

Also associated with

No associations

Rating

Neutrino transport during the core bounce phase of a type II supernova explosion 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 Neutrino transport during the core bounce phase of a type II supernova explosion, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrino transport during the core bounce phase of a type II supernova explosion will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1703630