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Charged analogue of Vlasenko–Pronin superdense star with variable cosmological term

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Abstract

The set of three static spherically symmetric solutions of the Einstein–Maxwell field equations by Maurya and Gupta, Astrophys. Space Sci. 333, 149 (2011) are modified by introducing the variable cosmological term. Motivated by Tiwari et al, Indian J. Pure Appl. Math. 31, 1017 (2000), some particular values of the cosmological term are taken to obtain well-behaved solutions of the Einstein–Maxwell field equations. All the results given by Maurya and Gupta can be obtained as particular cases of our solutions by choosing a cosmological term equal to zero.

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Acknowledgements

Authors are grateful to the unknown referee for the valuable comments and suggestions.

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Authors and Affiliations

  1. School of Natural Sciences, National University of Sciences and Technology, Islamabad, Pakistan

    TOOBA FEROZE & GHAZALA NAZEER

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  1. TOOBA FEROZE
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  2. GHAZALA NAZEER
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Correspondence to TOOBA FEROZE.

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FEROZE, T., NAZEER, G. Charged analogue of Vlasenko–Pronin superdense star with variable cosmological term. Pramana - J Phys 86, 789–800 (2016). https://doi.org/10.1007/s12043-015-1085-6

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  • DOI: https://doi.org/10.1007/s12043-015-1085-6

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