Collapse of a Relativistic Self-Gravitating Star with Radial Heat Flux : Impact of Anisotropic Stresses
Joint Authors
Source
Issue
Vol. 2013, Issue 2013 (31 Dec. 2013), pp.1-8, 8 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2013-05-22
Country of Publication
Egypt
No. of Pages
8
Main Subjects
Abstract EN
We develop a simple model for a self-gravitating spherically symmetric relativistic star which begins to collapse from an initially static configuration by dissipating energy in the form of radial heat flow.
We utilize the model to show how local anisotropy affects the collapse rate and thermal behavior of gravitationally evolving systems.
American Psychological Association (APA)
Sharma, Ranjan& Das, Shyam. 2013. Collapse of a Relativistic Self-Gravitating Star with Radial Heat Flux : Impact of Anisotropic Stresses. Journal of Gravity،Vol. 2013, no. 2013, pp.1-8.
https://search.emarefa.net/detail/BIM-489029
Modern Language Association (MLA)
Sharma, Ranjan& Das, Shyam. Collapse of a Relativistic Self-Gravitating Star with Radial Heat Flux : Impact of Anisotropic Stresses. Journal of Gravity No. 2013 (2013), pp.1-8.
https://search.emarefa.net/detail/BIM-489029
American Medical Association (AMA)
Sharma, Ranjan& Das, Shyam. Collapse of a Relativistic Self-Gravitating Star with Radial Heat Flux : Impact of Anisotropic Stresses. Journal of Gravity. 2013. Vol. 2013, no. 2013, pp.1-8.
https://search.emarefa.net/detail/BIM-489029
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-489029