Nucleosynthesis in SNIa

Details Nucleosynthesis in SNIa Nucleosynthesis in SNIa

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.169...19b&link_type=abstract

(IAU, European Regional Astronomy Meeting on New Windows to the Universe, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics a

Astronomy and Astrophysics

Astrophysics

1

Nuclear Astrophysics, Nuclear Fusion, Stellar Evolution, Supernovae, Abundance, Chromium Isotopes, Iron Isotopes, Light Curve, Nickel Isotopes, Stellar Models

Scientific paper

The final products of a SNIa explosion critically depend on the degree of neutronization of the incinerated material and on the total amount of burned material. This paper studies their dependence on the velocity of the burning front and on the density at which the thermonuclear runaway starts. The abundances of Cr-54, Fe-54, 58, and Ni-58, 62 provide some constraints to the possible values of model parameters.

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