The Evolution of Luminosity for Spherically Symmetric Superdense Configurations in Einstein Theory of Gravitation

Details The Evolution of Luminosity for Spherically Symmetric Superdense Configurations in Einstein Theory of Gravitation The Evolution of Luminosity for Spherically Symmetric Superdense Configurations in Einstein Theory of Gravitation

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.491s&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We report the equations of superdense stellar structure and evolution for spherically symmetric configurations in the framework of Einstein theory. They are formulated in notation which makes easy contact with Newtonian theory.The problem was solved for arbitrary Equation of State. Equations for absorption coefficient and opacity of matter are added. The sources of luminosity are considered spherically symmetric.Evolution picture for luminosity is numerically generated and is compared with luminosity evolution of EV Lac-type objects. We discuss results of simulation for entire luminosity of star.

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