Published November 1, 2019
| Version Version 1
Journal article
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Theoretical Aspects of Neutron Stars by TOV equation
Description
Attempts have been made to analyze the nature of neutron star with realistic equation
of states (EOSs), highly non-linear differential equations, 3+1 numerical relativity and
TOV (Tolman-Oppenheimer-Volkov) equations. The gravitation potential for their
formation are visualized and physical interpretation are given.
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References
- AaronSmith. (2012). "Tolman-Oppenheimer-Volkoff (TOV) Stars". Department of Astronomy, The University of Texas at Austin, Austin. Faber Joshua A & Rasio Frederic A. (2012). "Binary Neutron Star Mergers". Department of Physics and Astronomy, Northwestern University, USA. Friedman J. L, Parker L, Ipser J R. (1986). "Rapidly Rotating Neutron Stars Model". AstrophysicsJournal. J. 304, 115, Department of Physics, University of Wisconsin-Milwaukee & University of Florida, USA. Hernquist, L. (1990). " An analytical model for spherical galaxies and bulges". ApJ. Lattimer J. M &Pethick C J. (2004). "The Physics of Neutron Stars", Department of Physics & Astronomy, State University of New York at Stony Brook, USA. Lattimer J. M &Pethick M, Masak D., Yahil A. (1990). "Rapidly Rotating Pulsarsnand the Equation of States". AJ, J. 355, 241. Maccio A. V., Stinson G., Brook C. B., Wadsley J., Couchman H. M. P., Shen S., Gibson B.K., Quinn T., (2012). ApJ.