Abstract
We present a class of new relativistic solutions with anisotropic fluid for compact stars in hydrostatic equilibrium. The interior space-time geometry considered here for compact objects are described by parameters namely, λ, k, A, R and n. The values of the geometrical parameters are determined here for obtaining a class of physically viable stellar models. The energy-density, radial pressure and tangential pressure are finite and positive inside the anisotropic stars. Considering some stars of known mass we present stellar models which describe compact astrophysical objects with nuclear density.
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Acknowledgements
BCP would like to acknowledge TWAS-UNESCO for supporting a visit to Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing where the work is completed. BCP would like to thank University Grants Commission, New Delhi for financial support (Grant no. F.42-783/2013(SR)). RD is also thankful to UGC, New Delhi and Physics Department, North Bengal University for providing research facilities. The authors would like to thank the referee for constructive suggestions.
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Paul, B.C., Deb, R. Relativistic solutions of anisotropic compact objects. Astrophys Space Sci 354, 421–430 (2014). https://doi.org/10.1007/s10509-014-2097-2
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DOI: https://doi.org/10.1007/s10509-014-2097-2