A numerical model for stellar core collapse calculations

Details A numerical model for stellar core collapse calculations A numerical model for stellar core collapse calculations

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apjs...50..115b&link_type=abstract

Astrophysical Journal Supplement Series, vol. 50, Oct. 1982, p. 115-159.

Computer Science

Numerical Analysis

97

Cores, Gravitational Collapse, Hydrodynamics, Numerical Analysis, Stellar Evolution, Stellar Models, Elastic Scattering, Electron Capture, Electron Scattering, Equations Of State, Mean Free Path, Neutrinos, Nuclear Scattering, Pair Production, Thermonuclear Reactions

Scientific paper

A method for calculating stellar core collapse is discussed which emphasizes physical approximations and numerical methods. Collapse is modeled in terms of hydrodynamics coupled to radiation transport of all neutrino types. The latter are not assumed to be in thermal equilibrium. Analytic approximations used for the equations of state are discussed. The overall approach includes all of the physical processes which we believe are important for stellar core collapse.

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