Relativistic modelling of a superdense star containing a charged perfect fluid
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Publication:1933367
DOI10.1134/S0202289312030073zbMath1258.83017OpenAlexW2057896960MaRDI QIDQ1933367
Publication date: 23 January 2013
Published in: Gravitation \& Cosmology (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1134/s0202289312030073
Electromagnetic fields in general relativity and gravitational theory (83C50) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)
Related Items (5)
An exact family of Einstein-Maxwell Wyman-Adler solution in general relativity ⋮ Compact stars described by a charged model ⋮ Some exact relativistic models of electrically charged self-bound stars ⋮ A well-behaved class of charged analogue of Durgapal solution ⋮ An isotropic analytical model for charged stars
Cites Work
- Radiating gravitational collapse with an initial inhomogeneous energy density distribution
- New class of well behaved exact solutions of relativistic charged white-dwarf star with perfect fluid
- Radiating gravitational collapse with shear viscosity revisited
- Relativistic model of radiating massive fluid sphere
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- Some new exact solutions with finite central parameters and uniform radial motion of sound
- Horizon-free gravitational collapse of radiating fluid sphere
- On a stationary system with spherical symmetry consisting of many gravitating masses
- Magnetic tension and gravitational collapse
- On Continued Gravitational Contraction
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