Core collapse, bounce and shock propagation

Details Core collapse, bounce and shock propagation Core collapse, bounce and shock propagation

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...27..537b&link_type=abstract

(International Astronomical Union, Colloquium on Stellar Hydrodynamics, 58th, Los Alamos, N. Mex., Aug. 12-15, 1980.) Space Scie

Astronomy and Astrophysics

Astrophysics

2

Astrophysics, Gravitational Collapse, Shock Wave Propagation, Supernovae, Adiabatic Conditions, Astronomical Models, Iron, Metallic Stars

Scientific paper

Recent developments in the physics input for iron core collapse models of type II supernovae are reviewed. The effect of these developments on collapse calculations is also discussed. The inner core collapses homologously, with little change in specific entropy, bounces in the neighborhood of nuclear density, and sets up an outward moving shock. In adiabatic models an explosion may result. The inclusion of neutrino effects may produce substantial shock damping. Current results indicate that core collapse, bounce and shock propagation does not produce an explosion when neutrino effects are included.

Affiliated with

Also associated with

No associations

Rating

Core collapse, bounce and shock propagation 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 Core collapse, bounce and shock propagation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Core collapse, bounce and shock propagation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-758291