An exact family of Einstein-Maxwell Wyman-Adler solution in general relativity

DOI10.1007/S10773-013-1538-YzbMath1272.83021OpenAlexW1975573168MaRDI QIDQ359657

Saba Fatema, Mohammad Hassan Murad

Publication date: 12 August 2013

Published in: International Journal of Theoretical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10773-013-1538-y

zbMATH Keywords

exact solutiongeneral relativitycharged fluid spherecompact objectselectrically charged strange (quark) starNordströmReissnerSchwarzschild (canonical) coordinatesstatic spherically symmetric metric

Mathematics Subject Classification ID

Black holes (83C57) Strong interaction, including quantum chromodynamics (81V05) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)

Related Items (5)

Relativistic charged stellar modeling with a perfect fluid sphere ⋮ Some exact relativistic models of electrically charged self-bound stars ⋮ A family of Finch and Skea relativistic stars ⋮ Generating interior sources for the Reissner-Nordström metric ⋮ A class of super dense stars models using charged analogues of hajj-boutros type relativistic fluid solutions

Cites Work

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• Well behaved class of charge analogue of heintzmann's relativistic exact solution
• A class of charged relativistic superdense star models
• A class of regular and well behaved relativistic super-dense star models
• Variety of well behaved parametric classes of relativistic charged fluid spheres in general relativity
• Equilibrium of a static charged perfect fluid sphere
• Sharp bounds on the critical stability radius for relativistic charged spheres
• Absolute stability limit for relativistic charged spheres
• Minimum mass-radius ratio for charged gravitational objects
• Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
• A solution for a charged sphere in general relativity
• Exact interior solutions for charged fluid spheres
• On the stability of homogeneous, spherically symmetric, charged fluids in relativity
• Relativistic modelling of a superdense star containing a charged perfect fluid
• Revisiting the classical electron model in general relativity
• Exact physical Maxwell-Einstein Tolman-VII solution and its use in stellar models
• A family of well behaved charge analogues of Durgapal's perfect fluid exact solution in general relativity
• A new well behaved class of charge analogue of Adler's relativistic exact solution
• RELATIVISTIC SOLUTION FOR A CLASS OF STATIC COMPACT CHARGED STAR IN PSEUDO-SPHEROIDAL SPACETIME
• FROM CRUST TO CORE: A BRIEF REVIEW OF QUARK MATTER IN NEUTRON STARS
• OF CHARGED STARS AND CHARGED BLACK HOLES
• General Relativistic Fluid Spheres
• ANALYTICAL MODELS FOR QUARK STARS
• Stellar Physics
• Exact solutions to Einstein's field equations for perfect spherically symmetric static fluids
• Spherical charged fluid distributions in general relativity
• Singularity-free static fluid spheres in general relativity
• Exact Solutions of Einstein's Field Equations
• Special and General Relativity
• MAXIMUM MASS OF A CLASS OF COLD COMPACT STARS
• QUARK STARS ADMITTING A ONE-PARAMETER GROUP OF CONFORMAL MOTIONS
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• Radially Symmetric Distributions of Matter

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