On a family of well behaved perfect fluid balls as astrophysical objects in general relativity

DOI10.1007/S10509-011-0705-YzbMath1241.85007OpenAlexW2007846964MaRDI QIDQ416228

Y. K. Gupta, Sunil Kumar Maurya

Publication date: 9 May 2012

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

Full work available at URL: https://doi.org/10.1007/s10509-011-0705-y

zbMATH Keywords

general relativitycanonical coordinatessuperdense 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) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (7)

Some charged polytropic models ⋮ Description of the interior of the neutron star in EXO 1785-248 by mean of the Karmarkar condition ⋮ Some exact relativistic models of electrically charged self-bound stars ⋮ Exact physical Maxwell-Einstein Tolman-VII solution and its use in stellar models ⋮ A new well behaved exact solution in general relativity for perfect fluid ⋮ Compact models with regular charge distributions ⋮ Extremization of mass of charged superdense star models describe by Durgapal type space-time metric

Cites Work

• Physics of neutron star crusts
• On most general exact solution for Vaidya-Tikekar isentropic superdense star
• Some new exact solutions with finite central parameters and uniform radial motion of sound
• General Relativistic Fluid Spheres
• General solution for a relativistic star
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• Radially Symmetric Distributions of Matter

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