Incompressibility of hot nuclear matter, general relativistic stellar collapse and shock propagation

Details Incompressibility of hot nuclear matter, general relativistic stellar collapse and shock propagation Incompressibility of hot nuclear matter, general relativistic stellar collapse and shock propagation

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...90..283m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 90, no. 2, Oct. 1991, p. 283-299. Research supported by CICY

Astronomy and Astrophysics

Astrophysics

6

Gravitational Collapse, Incompressible Flow, Nuclear Astrophysics, Relativistic Effects, Shock Wave Propagation, Supernovae, Computerized Simulation, Magnetohydrodynamics, Neutrinos, Stellar Cores, Stellar Models, Stellar Radiation

Scientific paper

Research was carried out on the effect of considering two extreme kinds
of Skyrme-type nuclear interactions on the outcome of stellar core
collapsing models. Particular attention was given to dissociation
effects generated by the shock. Neutrinos transport is included via a
multigroup trapping scheme.

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