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Relativistic Modelling for Anisotropic Stellar Object

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Advances in Mathematical Modelling, Applied Analysis and Computation (ICMMAAC 2023)

Part of the book series: Lecture Notes in Networks and Systems ((LNNS,volume 953))

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Abstract

In this study, closed-form solutions for a spherically symmetric anisotropic matter distribution were obtained using the space-time geometry of Finch-Skea. We have shown that the class of solutions can be employed as strong models for 4U 1820-30, 4U 1608-52, Cen X-3 pulsars by looking at its physical admissibility. Using graphs, we have examined the many physical properties of our model, including energy density, pressures, anisotropy factor, mass, energy conditions, equilibrium, and stability analysis.

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Authors and Affiliations

  1. Department of Physics, Malaviya National Institute of Technology, Jaipur, 302017, India

    Ankita Jangid & K. K. Venkataratnam

Authors
  1. Ankita Jangid
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  2. K. K. Venkataratnam
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Corresponding author

Correspondence to Ankita Jangid .

Editor information

Editors and Affiliations

  1. Department of Mathematics, JECRC University, Jaipur, Rajasthan, India

    Jagdev Singh

  2. Department of Mathematics, University of Memphis, Memphis, TN, USA

    George A. Anastassiou

  3. Department of Computer Science and Mathematics, Lebanese American University, Beirut, Lebanon

    Dumitru Baleanu

  4. Department of Mathematics, University of Rajasthan, Jaipur, Rajasthan, India

    Devendra Kumar

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Jangid, A., Venkataratnam, K.K. (2024). Relativistic Modelling for Anisotropic Stellar Object. In: Singh, J., Anastassiou, G.A., Baleanu, D., Kumar, D. (eds) Advances in Mathematical Modelling, Applied Analysis and Computation . ICMMAAC 2023. Lecture Notes in Networks and Systems, vol 953. Springer, Cham. https://doi.org/10.1007/978-3-031-56304-1_3

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  • DOI: https://doi.org/10.1007/978-3-031-56304-1_3

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  • Publisher Name: Springer, Cham

  • Print ISBN: 978-3-031-56303-4

  • Online ISBN: 978-3-031-56304-1

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