Exact physical Maxwell-Einstein Tolman-VII solution and its use in stellar models
- 24 February 2012
- journal article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 339 (2) , 329-338
Abstract
No abstract availableKeywords
This publication has 45 references indexed in Scilit:
- A class of well behaved charged superdense star models of embedding class oneAstrophysics and Space Science, 2011
- Charged analogues of Schwarzschild interior solution in terms of pressureAstrophysics and Space Science, 2011
- New class of Well behaved exact solutions of relativistic charged white-dwarf star with perfect fluidAstrophysics and Space Science, 2011
- A class of regular and well behaved charge analogue of Kuchowicz’s relativistic super-dense star modelAstrophysics and Space Science, 2010
- Transforming the Einstein static universe into physically acceptable static fluid spheresPhysical Review D, 2008
- Instability of extremal relativistic charged spheresPhysical Review D, 2001
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equationsComputer Physics Communications, 1998
- A class of new exact solutions in general relativityJournal of Physics A: General Physics, 1982
- Charged fluid sphere in general relativityJournal of Mathematical Physics, 1979
- A fluid sphere in general relativityJournal of Mathematical Physics, 1974