A charged anisotropic well-behaved Adler–Finch–Skea solution satisfying Karmarkar condition
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In this paper, a new well-behaved charged anisotropic solution of the field equations was discovered, which can represent a physically possible configuration with the inclusion of some net electric charge, i.e. the solution can become a wellbehaved solution with decreasing sound speed radially outward.Abstract:
In the present paper, we discover a new well-behaved charged anisotropic solution of Einstein–Maxwell’s field equations. We ansatz the metric potential g00 of the form given by Maurya el al. (Eur. Phys. J. C 76(2) (2016) 693) with n = 2. In their paper, it is mentioned that for n = 2, the solution is not well-behaved for neutral configuration as the speed of sound is nondecreasing radially outward. However, the solution can represent a physically possible configuration with the inclusion of some net electric charge, i.e. the solution can become a well-behaved solution with decreasing sound speed radially outward for a charged configuration. Due to the inclusion of electric charge, the solution leads to a very stiff equation-of-state (EoS) with the velocity of sound at the center vr02 = 0.819, vt02 = 0.923 and the compactness parameter u = 0.823 is close to the Buchdahl limit 0.889. This stiff EoS support a compact star configuration of mass 5.418M⊙ and radius of 10.1km.read more
Citations
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Anisotropic fluid spheres of embedding class one using Karmarkar condition
S. K. Maurya,Sunil D. Maharaj +1 more
TL;DR: In this article, a new anisotropic solution for spherically symmetric spacetimes was obtained by analyzing the Karmarkar embedding condition, which can be used to construct realistic static fluid spheres.
Journal ArticleDOI
Anisotropic relativistic fluid spheres: an embedding class I approach
Francisco Tello-Ortiz,S. K. Maurya,Abdelghani Errehymy,Ksh. Newton Singh,Mohammed Daoud,Mohammed Daoud +5 more
TL;DR: In this article, a well-behaved solution to Einstein's field equations describing anisotropic matter distribution was proposed in the embedding class one spacetime framework using Karmarkar's condition.
Journal ArticleDOI
Anisotropic Karmarkar stars in f ( R , T )-gravity
Monsur Rahaman,Ksh. Newton Singh,Ksh. Newton Singh,Abdelghani Errehymy,Farook Rahaman,Mohammed Daoud,Mohammed Daoud +6 more
TL;DR: In this article, the existence of compact spherical systems representing anisotropic matter distributions within the scenario of alternative theories of gravitation, specifically f(R, T) gravity theory, is studied.
Journal ArticleDOI
A comparative study on generalized model of anisotropic compact star satisfying the Karmarkar condition
TL;DR: In this paper, a non-singular solution satisfying the Karmarkar condition is presented, which yields finite values of metric potentials, density, pressure, redshift, etc.
Journal ArticleDOI
Compact stars with specific mass function
TL;DR: In this paper, a new mass function was proposed to obtain an exact analytic solution of the Einstein field equations of a compact star within embedding class one spacetime i.e., four dimensional spacetime embedded in five dimensional pseudo Euclidean space.
References
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Self‐graviting anisotropic fluids with plane symmetry
P. S. Letelier,R. Machado +1 more
TL;DR: In this paper, the general solution to Einstein's equations coupled to an anisotropic fluid described by two perfect-fluid components is obtained in the case that the space-time is plane-symmetric, each fluid component is irrotational, and each one obeys the equation of state pressure = energy density.
Journal ArticleDOI
Self-gravitating anisotropic fluids
TL;DR: In this article, the authors studied the solution to the problem of solving the equivalent problem of Einstein's equations coupled to an anisotropic fluid described by two perfect-fluid components in the case that the metric is given by four functions of two variables and each fluid component is irrotational.