Abstract
A new type of embedding class-I representing anisotropic fluid distribution is presented. The new solution is free from singularity and also satisfies all physical criteria. It also satisfies all energy conditions such as SEC, WEC, NEC and DEC. The solution so obtained is used to optimize mass and radius of some well compact stars candidates like, Her X-1, SAX J1808.4-3658, RX J1856.5-3754, PSR J1614-2230 and PSR J0348+0432.
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Acknowledgements
Authors are grateful to the anonymous referee(s) for rigorous review, constructive comments and useful suggestions. The authors also acknowledge their gratitude to Vice Admiral G Ashok Kumar, AVSM, VSM, the Commandant National Defence Academy Khadakwasla Pune for his motivation and encouragement.
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Singh, K.N., Pant, N. A new analytic solution representing anisotropic stellar objects in embedding class I. Astrophys Space Sci 361, 177 (2016). https://doi.org/10.1007/s10509-016-2765-5
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DOI: https://doi.org/10.1007/s10509-016-2765-5