A simple model of a supernova

Details A simple model of a supernova A simple model of a supernova

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.155..271a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 155, no. 2, May 1989, p. 271-293.

Physics

9

Gravitational Collapse, Relativistic Theory, Stellar Models, Supernovae, Einstein Equations, Equations Of State, Field Theory (Physics), Magnetohydrodynamics, Space-Time Functions, Stellar Cores

Scientific paper

An exact analytical solution to Einstein's field equations is presented and used to construct a model for a collapsing star. The radius of the core is plotted as a function of time. Also, the decrease in the velocity of collapse is plotted as a function of increases in the adiabtic index, indicating a stiffening of the equation of state. The model neglects mass ejection and luminosity.

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