Abstract
In this paper, we generate exact solutions for anisotropic fluid spheres in the context of General Relativity. Some well-studied stellar solutions are shown to be subsets of the developed solution. Ours is a three-parameter (M, R, and A) family of solutions where M is the mass, R is the radius and the parameter A fixes the anisotropy. We demonstrate how the developed solutions can be utilized to model compact objects such as neutron and quark stars, particularly by considering the estimated masses and radii of PSR \(J0030+0451\), PSR \(J0348+0432\), PSR \(J0740+6620\) and SMC X \(-1\). We also obtain the maximum compactness bound for our class of stars which might be treated as an anisotropic generalization of the well-known Buchdahl compactness bound.
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Acknowledgements
RS gratefully acknowledge support from the Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune, Govt. of India, under its Visiting Research Associateship Programme. We are also grateful to the anonymous referees for providing valuable suggestions.
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Thirukkanesh, S., Ghosh, A. & Sharma, R. A physically viable model for a compact star and its compactness bound. Eur. Phys. J. Plus 138, 588 (2023). https://doi.org/10.1140/epjp/s13360-023-04216-6
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DOI: https://doi.org/10.1140/epjp/s13360-023-04216-6