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Analytical model of low-mass strange stars using Tolman space–time in \((2+1)\) dimensions

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Abstract

It is hard to explain low-mass strange stars. In this paper, we have modelled these low-mass strange stars using the Tolman IV metric in (\(2+1\)) dimensions. We found that the presence of attractive or positive anisotropic force is the cause for the lower mass of the strange stars in our model. We have also found that the cosmological constant has a significant role in the mass–radius relationship of the stars. We have used our model to predict the radius of a few low-mass strange stars. Our approach is helpful for predicting the crucial parameters of the low-mass strange stars.

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Acknowledgements

MM is thankful to CSIR (Grant No. -09/1157(0007)/2019-EMR-I) for providing financial support. MK is grateful to the Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune, India for providing Associateship programme under which a part of this work was carried out.

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Authors and Affiliations

  1. Department of Physics, Cooch Behar Panchanan Barma University, Vivekananda Street, Cooch Behar, 736 101, India

    Taniya Kundu & Prabir Kumar Haldar

  2. Department of Physics, Aliah University, IIA/27, New Town, Kolkata, 700 160, India

    Masum Murshid & Mehedi Kalam

Authors
  1. Taniya Kundu
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  2. Masum Murshid
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  3. Prabir Kumar Haldar
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  4. Mehedi Kalam
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Correspondence to Mehedi Kalam.

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Kundu, T., Murshid, M., Haldar, P.K. et al. Analytical model of low-mass strange stars using Tolman space–time in \((2+1)\) dimensions. Pramana - J Phys 98, 75 (2024). https://doi.org/10.1007/s12043-024-02741-2

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  • DOI: https://doi.org/10.1007/s12043-024-02741-2

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