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Anisotropic stars with non-static conformal symmetry

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 solutions including drawbacks of the model have been explored and discussed. For this purpose we have provided the energy conditions, TOV-equations and other physical requirements and thus thoroughly investigated stability, mass-radius relation and surface redshift of the model. It is observed that most of the features are well matched with the compact stars, like quark/strange stars.

preprint2015arXivOpen access
Dibyendu SheeFarook RahamanB. K. GuhaSaibal Ray
gr-qc
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Open access4 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
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Dibyendu SheeFarook RahamanB. K. GuhaSaibal Ray

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