General relativistic neutrino hydrodynamics: the physics of and numerical techniques for modeling stellar collapse and the early cooling of neutron stars.

Details General relativistic neutrino hydrodynamics: the physics of and numerical techniques for modeling stellar collapse and the early cooling of neutron stars. General relativistic neutrino hydrodynamics: the physics of and numerical techniques for modeling stellar collapse and the early cooling of neutron stars.

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994supe.conf..787s&link_type=abstract

Les Houches Ecole d'Eté de Physique Théorique. Session 54: Supernovae, p. 787 - 807

Astronomy and Astrophysics

Astrophysics

Neutrinos: Stellar Collapse, Neutrinos: Hydrodynamics, Neutrinos: Propagation, Neutrinos: Relativistic Astrophysics, Neutrinos: Interactions

Scientific paper

Contents: 1. Introduction.

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