Dynamics of neutrino driven type-II supernovae.

Details Dynamics of neutrino driven type-II supernovae. Dynamics of neutrino driven type-II supernovae.

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993nuas.symp...18j&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: Neutrinos, Supernovae: Shock Waves

Scientific paper

The currently most promising model to explain the explosion of massive stars (8 Msun ⪉ M ⪉ 25 Msun) in type-II supernovae is the "delayed mechanism" by neutrino heating. The author has investigated the formation and evolution of the hot bubble region around the newly born neutron star by long-time hydrodynamical simulations carried out under the assumption of spherical symmetry.

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