A comparative study on generalized model of anisotropic compact star satisfying the Karmarkar condition
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TLDR
In this paper, a non-singular solution satisfying the Karmarkar condition is presented, which yields finite values of metric potentials, density, pressure, redshift, etc.Abstract:
A new solution satisfying the Karmarkar condition is presented here. We were first to have discovered a hypergeometric function metric potential representing embedding class I spacetime. This new solution yields finite values of metric potentials, density, pressure, redshift, etc. and hence a non-singular solution. The solution is well behaved with respect to the parameter $$n=12$$
to $$n=24$$
corresponding to a stable configuration of mass $$2.01M_\odot $$
and radius 9.1 km. The internal properties of the solution are very different for $$n=12$$
to $$n=24$$
; however, the total mass and radius is independent of the parameter n. The energy conditions are also holds good by the solution which thus can represent a physically viable matter distribution. The equilibrium condition and stability are also discussed through TOV-equation, cracking method and $$\Gamma >4/3$$
. The static stability criterion is also well satisfied and the turning point corresponds to $$4.46M_\odot $$
for a radius of 9.1 km.read more
Citations
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Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
Roy P. Kerr,Roy P. Kerr +1 more
Journal ArticleDOI
Generalized relativistic anisotropic compact star models by gravitational decoupling
TL;DR: In this paper, the Maurya-Gupta isotropic fluid solution to the Einstein field equations was extended to an aniso-tropic domain by using the minimal geometric deformation approach.
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
Class I approach as MGD generator
TL;DR: In this article, a relativistic anisotropic admissible compact structure is constructed by combining the class I approach with gravitational decoupling in order to generate the deformation function f(r).
Journal ArticleDOI
A completely deformed anisotropic class one solution for charged compact star: a gravitational decoupling approach
TL;DR: In this paper, a new completely deformed embedding class one solution for the compact star in the framework of charged anisotropic matter distribution was investigated by using Ovalle (Phys Lett B 788:213, 2019) approach.
References
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Gravitational field of a spinning mass as an example of algebraically special metrics
Roy P. Kerr,Roy P. Kerr +1 more
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