Extremization of mass of charged superdense star models describe by Durgapal type space-time metric

DOI10.1007/s10509-011-0736-4zbMath1230.85015OpenAlexW2016207926MaRDI QIDQ659977

Y. K. Gupta, Sunil Kumar Maurya

Publication date: 24 January 2012

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

Full work available at URL: https://doi.org/10.1007/s10509-011-0736-4

zbMATH Keywords

general relativitycanonical coordinatescharged fluidssuperdense star

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (8)

Well behaved charged generalization of Buchdahl's fluid spheres ⋮ A new family of polynomial solutions for charged fluid spheres ⋮ Some exact relativistic models of electrically charged self-bound stars ⋮ Exact physical Maxwell-Einstein Tolman-VII solution and its use in stellar models ⋮ On charged analogues of Matese and Whitman interior solutions in general relativity ⋮ Exact well behaved solutions of Einstein-Maxwell equations for relativistic charged superdense star models ⋮ A family of well behaved charge analogues of Durgapal's perfect fluid exact solution in general relativity ⋮ Relativistic modeling of Vela X-1 using the Karmarkar condition

Cites Work

• Well behaved parametric class of relativistic charged fluid ball in general relativity
• Well behaved class of charge analogue of heintzmann's relativistic exact solution
• On a family of well behaved perfect fluid balls as astrophysical objects in general relativity
• A class of regular and well behaved relativistic super-dense star models
• New class of regular and well behaved exact solutions in general relativity
• Variety of well behaved parametric classes of relativistic charged fluid spheres in general relativity
• Equilibrium of a static charged perfect fluid sphere
• Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations

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