The hot bubble and supernova calculations

Details The hot bubble and supernova calculations The hot bubble and supernova calculations

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nyasa.617....1c&link_type=abstract

(Nonlinear astrophysical fluid dynamics; Proceedings of the 5th Florida Workshop in Nonlinear Astronomy, Gainesville, FL, Oct. 5

Astronomy and Astrophysics

Astronomy

Gravitational Collapse, Neutron Stars, Plasma Bubbles, Stellar Models, Supernovae, Thermal Plasmas, Black Holes (Astronomy), Shock Waves, Turbulent Mixing

Scientific paper

Theoretical models and numerical simulations of SN explosions caused by collapse to a neutron star are discussed in an analytical review. The focus is on the hot-bubble model developed by Wilson and Mayle (1984) and the fact that, despite the strength of the shock wave, a significant proportion of the ejected matter falls back onto the neutron star over the course of about 30 min, ultimately leading to a black hole. Particular attention is given to mixing behind the shock, turbulent mixing processes, the acceleration of the contact surface, and the relationship between entropy and mixing.

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