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Journal ArticleDOI

Exact Relativistic Model for a Superdense Star

TLDR
In this article, a static spherically symmetric model based on an exact solution of Einstein's equations is given which will permit densities of the order of 2 × 1014 gm cm-3, radii of a few kilometers and masses up to about four times the solar mass.
Abstract
Assuming that the physical 3-spacet = const in a superdense star is spheroidal, a static spherically symmetric model based on an exact solution of Einstein’s equations is given which will permit densities of the order of 2 × 1014 gm cm-3, radii of the order of a few kilometers and masses up to about four times the solar mass.

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Citations
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Anisotropic Model of Super Dense Star with Linearized Core and Van der Waals Envelope

TL;DR: In this paper , a core envelope model of a super dense spherically symmetric compact star is developed by considering anisotropic matter configuration, where the core is represented by a linear equation of state (EOS), whereas the Van der Waals EOS is used in the envelope region.
Journal ArticleDOI

Dependence of maximum mass of strange star on finite strange quark mass (m s ≠ 0)

TL;DR: Li et al. as discussed by the authors analyzed a class of compact objects in spheroidal geometry described by Vaidya-Tikekar model and MIT bag model equation of state considering the finite mass of strange quark (m s).
Journal ArticleDOI

A note on exact spherically symmetric interior solutions in higher dimensions

TL;DR: In this article, a method of constructing a new family of higher-dimensional perfect-fluid spheres from a known Tolman-type solution is presented, with spheroidal geometry on the hypersurfacest = constant.
Journal ArticleDOI

Study of anisotropic stellar objects, a revisit to Buchdahl metric potential

TL;DR: In this paper , the authors explore anisotropic compact stellar models in the framework of general theory of relativity with [Formula: see text] component governed by Buchdahl ansatz.
References
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Journal ArticleDOI

Static Solutions of Einstein's Field Equations for Spheres of Fluid

TL;DR: In this article, a method is developed for treating Einstein's field equations, applied to static spheres of fluid, in such a manner as to provide explicit solutions in terms of known analytic functions.
Journal ArticleDOI

Maximum Mass of a Neutron Star

TL;DR: On the basis of the theory of relativity, the principle of causality, and Le Chatelier's principle, it was shown in this article that the maximum mass of the equilibrium configuration of a neutron star cannot be larger than $3.2{M}_{[m?]}