Supernova explosion and neutral currents of weak interaction

Details Supernova explosion and neutral currents of weak interaction Supernova explosion and neutral currents of weak interaction

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pthph..54.1325s&link_type=abstract

Progress of Theoretical Physics, vol. 54, Nov. 1975, p. 1325-1338. Research supported by the Soryushi Shogakukai.

Physics

58

Gravitational Collapse, Neutrinos, Supernovae, Electron Capture, Graphs (Charts), Muons, Neutron Stars, Shock Fronts, Stellar Evolution, Stellar Temperature

Scientific paper

The diffusion of neutrinos in a supernova core is analyzed within the framework of Weinberg's (1967) weak-interaction theory. The hydrodynamic collapse of the core is calculated on the assumption that the core is homogeneous (one-shell model), with simultaneous allowance for electron capture by nuclei and for the reaction and diffusion of neutrinos. The computations are carried out for a range of core temperatures and for Weinberg angles of 0.45, 0.3, and 0.

Affiliated with

Also associated with

No associations

Rating

Supernova explosion and neutral currents of weak interaction 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 Supernova explosion and neutral currents of weak interaction, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Supernova explosion and neutral currents of weak interaction will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1377685