Two- and three-dimensional simulations of convection in protoneutron stars.

Details Two- and three-dimensional simulations of convection in protoneutron stars. Two- and three-dimensional simulations of convection in protoneutron stars.

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993nuas.symp...27m&link_type=abstract

"Nuclear Astrophysics, Proceedings of the 7th Workshop held 22-27 March 1993 at Ringberg Castle, Tegernsee,

Astronomy and Astrophysics

Astrophysics

Supernovae: Hydrodynamics, Supernovae: Convection, Supernovae: Neutron Stars

Scientific paper

The author presents some results from hydrodynamical simulations of
supernova explosions, which clearly show the existence of convective
instabilities in the mantle of the collapsing stellar core.

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