activity
20132026
most citedModelling of anisotropic compact stars of emebedding class one

129 citations · 1.7k across the 48 of their papers we have counts for

collaborators
Showing 2014Show all

6 papers · 1 filter

gr-qc2014★ 82 cited

Singularity free anisotropic strange quintessence star

Piyali Bhar

Present paper provides a new model of anisotropic strange star corresponding to the exterior schwarzschild metric. The Einstein field equations have been solved by utilizing the Kr…

physics.gen-ph2014★ 35 cited

Exact solution of a (2 + 1) dimensional anisotropic star in Finch and Skea spacetime

Piyali Bhar, Farook Rahaman, Ritabrata Biswas +1

We provide a new class of interior solution of a (2 + 1) dimensional anisotropic star in Finch and Skea spacetime corresponding to the BTZ black hole. We have developed the model b…

physics.gen-ph2014★ 34 cited

Search of wormholes in different dimensional non-commutative inspired space-time with lorentzian distribution

Piyali Bhar, Farook Rahaman

In this paper we are searching whether the wormhole solutions exists in different dimensional non- commutative inspired spacetimes. It is well known that the noncommutativity of th…

physics.gen-ph2014★ 56 cited

The Dark Energy Star and Stability analysis

Piyali Bhar, Farook Rahaman

We have proposed a new model of dark energy star consisting of five zones namely, solid core of constant energy density, the thin shell between core and interior, an inhomogeneous…

physics.gen-ph2014★ 9 cited

Noncommutative geometry inspired 3-dimensional charged black hole solution in an anti-de Sitter background space-time

Farook Rahaman, Piyali Bhar, Ranjan Sharma +1

We report a 3D charged black hole solution in an anti desetter space inspired by noncommutative geometry.In this construction,the black hole exhibits two horizon which turn into a…

gr-qc2014★ 54 cited

Vaidya-Tikekar Type Superdense Star Admitting Conformal Motion in Presence of Quintessence Field

Piyali Bhar

To explain the reason of accelerated expansion of our universe dark energy is a suitable candidate. Motivated by this concept in the present paper we have obtained a new model of a…