On the dynamics of a thin spherically symmetric radiating shell,its classical model,and relativistic effects |
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Authors: | Mario Castagnino Norberto Umerez |
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Affiliation: | (1) Instituto de Física de Rosario (CONICET-U.N.R.), v. Pellegrini 250, 2000 Rosario, Argentina;(2) Instituto de Astronomia Física del Espacio, Casilla de Correo 67-Sucursal 28, 1428 Buenos Aires, Argentina;(3) Instituto de Astronomía Física del Espacio, Casilla de Correo 67-Sucursal 28, 1428 Buenos Aires, Argentina |
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Abstract: | A general relativity model of nova and supernova explosions is studied and improved. Its classical limit is found, and the magnitude of the velocity and mass necessary to detect relativistic effects are computed. |
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