Evolution and explosion of massive stars

Details Evolution and explosion of massive stars Evolution and explosion of massive stars

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...7932142w&link_type=abstract

Presented at the 13th Texas Symp. on Relativistic Astrophys., Munich, 14-19 Dec. 1979

Other

Hydrodynamic Equations, Mathematical Models, Stellar Evolution, Stellar Mass Ejection, Convection, Gravitational Collapse, Nuclear Reactions, Supernovae, Time Dependence

Scientific paper

An attempt is reported to build self-consistent evolutionary models of complete massive stars, starting from their observable zero-age main sequence configurations, and evolving through their various hydrostatic nuclear burning stages, iron core collapse, bounce, outward-going shock formation, and finally, explosive nucleosynthesis and supernovae light curve formation. The nodel incorporates implicit hydrodynamics with a treatment of time dependent convection and semiconvection, and a careful treatment of the complexities of the advanced stages of stellar burning. The model was used to completely evolve population I stars of 15 and 25 M/sub solar mass/, with excellent agreement with the known properties and the prediction of other properties.

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