Author:
Herrera L.,Jiménez J.,Barreto W.
Abstract
The effects of viscosity on the gravitational collapse of a radiating sphere are calculated by extending the Herrera–Jiménez–Ruggeri method to the case of viscous fluids. An explicit model is worked out, indicating that when both the shear and bulk viscosity are nonvanishing, the final configuration is less compact than that corresponding to a nonviscous fluid.
Publisher
Canadian Science Publishing
Subject
General Physics and Astronomy
Cited by
14 articles.
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