A family of physically realizable perfect fluid spheres representing a \(quark\)-\(stars\) in general relativity

DOI10.1007/S10509-011-0810-YzbMath1238.85017OpenAlexW2044673067MaRDI QIDQ422234

Y. K. Gupta, Sunil Kumar Maurya

Publication date: 16 May 2012

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

Full work available at URL: https://doi.org/10.1007/s10509-011-0810-y

zbMATH Keywords

general relativitycanonical coordinatessuper-dense starSchwarzschild exterior metric

Mathematics Subject Classification ID

Black holes (83C57) Strong interaction, including quantum chromodynamics (81V05) 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 (2)

A new family of polynomial solutions for charged fluid spheres ⋮ Description of the interior of the neutron star in EXO 1785-248 by mean of the Karmarkar condition

Cites Work

• New class of regular and well behaved exact solutions in general relativity
• 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
• Static Solutions of Einstein's Field Equations for Spheres of Fluid

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