Supernova explosions - The role of a Rayleigh-Taylor instability

Details Supernova explosions - The role of a Rayleigh-Taylor instability Supernova explosions - The role of a Rayleigh-Taylor instability

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...27..571b&link_type=abstract

(International Astronomical Union, Colloquium on Stellar Hydrodynamics, 58th, Los Alamos, N. Mex., Aug. 12-15, 1980.) Space Scie

Astronomy and Astrophysics

Astronomy

4

Convective Flow, Gravitational Collapse, Neutrinos, Supernovae, Taylor Instability, Cores, Energy Transfer, Entropy, Leptons, Momentum Transfer, Shock Waves, Stellar Evolution

Scientific paper

A two-dimensional hydrodynamic study indicates that convectively
unstable gradients which develop during core collapse and bounce give
rise to large scale core overturn. It is also shown that the concomitant
release of neutrinos can deposit large amounts of energy and momentum in
the infalling envelope and give rise to a powerful supernova explosion.

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