PARABOLOIDAL SPACE–TIMES AND RELATIVISTIC MODELS OF STRANGE STARS

DOI10.1142/S021827180600884XzbMath1106.85300MaRDI QIDQ3430044

Kanti Jotania, Ramesh Tikekar

Publication date: 20 March 2007

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

zbMATH Keywords

equation of staterelativistic starsstrange starssuperdense starsrelativistic stellar models

Mathematics Subject Classification ID

Galactic and stellar structure (85A15)

Related Items (11)

Anisotropic quintessence strange stars in \(f(T)\) gravity with modified Chaplygin gas ⋮ ANALYTICAL MODELS FOR QUARK STARS ⋮ Models of anisotropic stars in spherically symmetric space-time ⋮ Strange star with Krori–Barua potential in the presence of anisotropy ⋮ Hybrid star model with quark matter and baryonic matter in minimally coupled \(f ( R )\) gravity ⋮ A class of super dense stars models using charged analogues of hajj-boutros type relativistic fluid solutions ⋮ Possible features of galactic halo with electric field and observational constraints ⋮ NON-ADIABATIC GRAVITATIONAL COLLAPSE OF A SUPERDENSE STAR ⋮ A relativistic two-parameter core-envelope model of compact stars ⋮ An analytical anisotropic compact stellar model of embedding class I ⋮ Relativistic strange stars in Tolman-Kuchowicz spacetime

Cites Work

• On most general exact solution for Vaidya-Tikekar isentropic superdense star
• Exact model for a relativistic star
• General solution for a relativistic star
• Exact solutions for the Tikekar superdense star

This page was built for publication: PARABOLOIDAL SPACE–TIMES AND RELATIVISTIC MODELS OF STRANGE STARS