Rayleigh-Taylor convective overturn in stellar collapse

Details Rayleigh-Taylor convective overturn in stellar collapse Rayleigh-Taylor convective overturn in stellar collapse

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234l.183b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 234, Dec. 15, 1979, p. L183-L186. Research supported by the Minister

Astronomy and Astrophysics

Astrophysics

24

Gravitational Collapse, Neutrinos, Stellar Models, Supernovae, Astrophysics, Convection, Hydrodynamics

Scientific paper

Rayleigh-Taylor convective overturn in collapsing stellar cores is
modeled with a one-dimensional parametrization. The results of a
numerical hydrodynamic study are very encouraging and indicate that such
an overturn could well be a dominant feature in the supernova explosion
mechanism.

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