Evolution of contracting white dwarfs as presupernovae of Type I

Details Evolution of contracting white dwarfs as presupernovae of Type I Evolution of contracting white dwarfs as presupernovae of Type I

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976phdt.........9k&link_type=abstract

Ph.D. Thesis California Univ., Berkeley.

Computer Science

Stellar Evolution, Supernovae, White Dwarf Stars, Electron Capture, Stellar Mass, Stellar Models

Scientific paper

The possibility is considered through a numerical investigation that the progenitors of Type I supernovae are certain white dwarfs which become dynamically unstable due to e(-) captures by certain stable nuclei in their interiors. Detailed evolutionary sequences of white dwarf models were calculated with the Henyey method including composition changes which correspond to various e(-) captures.

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