Abstract
Exact solutions to Einstein–Maxwell systems play an important role in relativistic astrophysics. In this paper, a new technique to generate exact solutions to the Einstein–Maxwell system is proposed. Corresponding to a spherically symmetric charged fluid sphere, by specifying the electric field and for a particular form of the metric potential \(g_{rr}\), a new solution is obtained in terms of hypergeometric functions. Subsequently, for specific choice of model parameters, many closed-form solutions are developed. In the process, it is possible to regain a number of well-known stellar models which had been developed earlier with or without the presence of charge following the Vaidya and Tikekar ansatz for compact stars (J. Astrophys. Astron. 3:325 (1982); J. Math. Phys. 31:2454 (1990)). It is shown that the new class of solutions can be used as viable models for compact stars for a wide range of values of the model parameters. Physical behaviour of the resultant stellar configurations are studied.
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Acknowledgements
RS gratefully acknowledges the support from the Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune, India, under its Visiting Research Associateship Programme.
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Thirukkanesh, S., Saparamadu, I., Sharma, R. et al. Models for charged relativistic spheres via hyper-geometric equations. Pramana - J Phys 96, 183 (2022). https://doi.org/10.1007/s12043-022-02424-w
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DOI: https://doi.org/10.1007/s12043-022-02424-w