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A model for anisotropic strange stars | | Debabrata Deb
; Sourav Roy Chowdhury
; Saibal Ray
; Farook Rahaman
; B.K. Guha
; | | Date: |
30 May 2016 | | Abstract: | We attempt to find a singularity free interior solution for a neutral and
static stellar model. We consider that (i) the star is made up of anisotropic
fluid and (ii) the MIT bag model can be used. The total system is defined by
assuming the density profile given by Mak and Harko cite{Mak2002}, which
satisfies all the physical conditions of a stellar system and is stable by
nature. We find that those stellar systems which obey such a non-linear density
function must have maximum anisotropy at the surface. We also perform several
tests for physical features of the proposed model and show that these are
mostly acceptable within certain range. As a special mention, from our
investigation we find that the maximum mass and radius of the quark star are
$11.811 km$ and $3.53 {M}_{odot}$ respectively. | | Source: | arXiv, 1606.0713 | | Services: | Forum | Review | PDF | Favorites | |
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