Physics of type II supernova explosions

Details Physics of type II supernova explosions Physics of type II supernova explosions

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ppas.book...79s&link_type=abstract

IN: Particle physics and astrophysics - Current viewpoints (A90-35283 15-90). Berlin and New York, Springer-Verlag, 1989, p. 79-

Astronomy and Astrophysics

Astrophysics

1

Gravitational Collapse, Stellar Cores, Stellar Evolution, Stellar Mass, Supernova 1987A, Neutrinos, Stellar Models

Scientific paper

The present consideration of the physical bases for type II SN explosions notes that the total number of associated events as a function of time, as well as the average neutrino energy and the total neutrino luminosity, are all satisfactorily explained by the standard model of core collapse and neutro-star formation. No exotic physical phenomena beyond the standard model are required, and the data extant are held not to imply the existence of a nonvanishing neutrino mass. It is judged unfortunate that none of the current computer simulations lead to an explosion for the mass range of progenitor stars inferred from SN 1987A.

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