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Anisotropic compact stellar solution in general relativity
We present herein a new class of singularity-free interior solutions to describe realistic
anisotropic compact stellar objects with spherically symmetric matter distribution. A specific …
anisotropic compact stellar objects with spherically symmetric matter distribution. A specific …
Moment of inertia of slowly rotating anisotropic neutron stars in gravity
Within the framework of f (R, T) theories of gravity, we investigate the hydrostatic equilibrium
of anisotropic neutron stars with a physically relevant equation of state (EoS) for the radial …
of anisotropic neutron stars with a physically relevant equation of state (EoS) for the radial …
Study of anisotropic compact stars by exploring tidal deformability
In this paper, the effect of anisotropy on the tidal deformability of a compact neutron star is
investigated. In particular, it is possible to quantify the tidal Love number, which is defined by …
investigated. In particular, it is possible to quantify the tidal Love number, which is defined by …
Charged anisotropic fluid spheres with conformal symmetry
We generate charged anisotropic exact models to the Einstein–Maxwell field equations for
static spacetime with a conformal Killing vector. The Einstein–Maxwell field equations are …
static spacetime with a conformal Killing vector. The Einstein–Maxwell field equations are …
Charged conformal stars and equation of state
Charged anisotropic fluid spheres admitting a conformal Killing vector with a linear equation
of state are generated. Our approach incorporates a conformal symmetry and an equation of …
of state are generated. Our approach incorporates a conformal symmetry and an equation of …
Central pressure-dependent compact anisotropic stellar model and its tidal Love number
We develop an anisotropic compact stellar model by assuming a Buchdahl ansazt (Phys.
Rev. 116: 1027–1034, 1959)-type metric potential and a particular radial pressure profile …
Rev. 116: 1027–1034, 1959)-type metric potential and a particular radial pressure profile …
Relativistic models of anisotropic superdense star in the regime of Karmarkar's condition
We obtained a new class of solutions for a relativistic anisotropic compact star by utilizing
the Karmarkar embedding condition. To obtain the closed-form solution a suitable form of …
the Karmarkar embedding condition. To obtain the closed-form solution a suitable form of …
[PDF][PDF] Critical Compactness Bound of a Select Class of Compact Stars
S Barman, R Sharma - 2023 - preprints.org
Tolman VII solution [1] is an exact analytic solution to the Einstein field equations describing
1 the space-time of a static spherically symmetric distribution of matter. The solution has …
1 the space-time of a static spherically symmetric distribution of matter. The solution has …