Charged analogues of Schwarzschild interior solution in terms of pressure

DOI10.1007/s10509-011-0780-0zbMath1269.83042OpenAlexW2072537742MaRDI QIDQ432207

Naveen Bijalwan

Publication date: 3 July 2012

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-011-0780-0

zbMATH Keywords

exact solutionSchwarzschildgeneral relativityReissner-Nordstromcharge fluids

Mathematics Subject Classification ID

Black holes (83C57) Electromagnetic fields in general relativity and gravitational theory (83C50) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)

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Binding energy in self-gravitating charged plane symmetric systems, Anisotropic compact star model on Finch-Skea space-time, Exact solutions: neutral and charged static perfect fluids with pressure, Exact physical Maxwell-Einstein Tolman-VII solution and its use in stellar models

Cites Work

• Static electrically charged fluids in terms of pressure: general property
• Closed form Vaidya-Tikekar type charged fluid spheres with pressure
• Sharp bounds on the critical stability radius for relativistic charged spheres
• Nonsingular charged analogues of Schwarzschild's interior solution
• The physical properties of an analytic model for a relativistic star
• Interior Weyl-type solutions to the Einstein-Maxwell field equations.
• A class of charged analogues of Durgapal and Fuloria superdense star