Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Shee, Dibyendu"'
Publikováno v:
Eur. Phys. J. C (2020) 80:175
In the current article, we study anisotropic spherically symmetric strange star under the background of $f(R,T)$ gravity using the metric potentials of Tolman-Kuchowicz type~\cite{Tolman1939,Kuchowicz1968} as $\lambda(r)=\ln(1+ar^2+br^4)$ and $\nu(r)
Externí odkaz:
http://arxiv.org/abs/2006.01619
This paper deals with the existence of a compact stellar object, precisely strange (quark) star, in the framework of Einstein's General Theory of Relativity with Tolman $V$ metric potential, which is one of the simplest forms of potential among his p
Externí odkaz:
http://arxiv.org/abs/2004.10480
Publikováno v:
In Environmental and Experimental Botany October 2023 214
Publikováno v:
Annals of Physics 409 (2019) 167905
In this article we propose a relativistic model of a static spherically symmetric anisotropic strange star with the help of Tolman-Kuchowicz (TK) metric potentials [Tolman, Phys. Rev. {\bf55}, 364 (1939) and Kuchowicz, Acta Phys. Pol. {\bf33}, 541 (1
Externí odkaz:
http://arxiv.org/abs/1910.00427
Publikováno v:
International Journal of Modern Physics D, Vol. 27, No. 8 (2018) 1850089 (18 pages)
In this paper we present a strange stellar model using Tolman $V$ type metric potential employing simplest form of the MIT bag equation of state (EOS) for the quark matter. We consider that the stellar system is spherically symmetric, compact and mad
Externí odkaz:
http://arxiv.org/abs/1808.02371
In the present paper we exhaustively examine the physical status of the socalled Matese-Whitman mass function [J.J. Matese and P.G. Whitman, Phys. Rev. D, 22, 1270 (1980)]. As a first step, we construct the relevant Einstein field equations with an a
Externí odkaz:
http://arxiv.org/abs/1706.00674
Publikováno v:
In Environmental and Experimental Botany March 2021 183
Publikováno v:
In Results in Physics January 2021 20
We have proposed a model for relativistic compact star with anisotropy and analytically obtained exact spherically symmetric solutions describing the interior of the dense star admitting non-static conformal symmetry. Several features of the solution
Externí odkaz:
http://arxiv.org/abs/1505.03034
Publikováno v:
In Results in Physics September 2019 14