International Journal of Astrophysics and Space Science

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Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates

Received: 17 November 2014    Accepted: 19 November 2014    Published: 19 December 2014
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Abstract

We present a spherically symmetric solution of the general relativistic field equations in isotropic coordinates for charged fluid with pressure anisotropy, compatible with a super dense star modeling. Further, we have constructed an anisotropic model of super dense star with all degree of suitability. We also observed that by increasing anisotropy, the maximum mass of super dense stars also decreases.

DOI 10.11648/j.ijass.s.2015030101.13
Published in International Journal of Astrophysics and Space Science (Volume 3, Issue 1-1, February 2015)

This article belongs to the Special Issue Compact Objects in General Relativity

Page(s) 13-20
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Isotropic Coordinates, Charged Fluid, Anisotropic Model, Super Dense Star

References
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Author Information
  • Department of Physics, National Defence Academy, Khadakwasla, Pune-411023, India

  • Department of Physics, National Defence Academy, Khadakwasla, Pune-411023, India

  • Department of Basic Sciences, Maritime University of the Caribbean, Catia la Mar, Venezuela

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    Ksh. Newton Singh, Narendra Pradhan, Manuel Malaver. (2014). Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates. International Journal of Astrophysics and Space Science, 3(1-1), 13-20. https://doi.org/10.11648/j.ijass.s.2015030101.13

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    ACS Style

    Ksh. Newton Singh; Narendra Pradhan; Manuel Malaver. Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates. Int. J. Astrophys. Space Sci. 2014, 3(1-1), 13-20. doi: 10.11648/j.ijass.s.2015030101.13

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    AMA Style

    Ksh. Newton Singh, Narendra Pradhan, Manuel Malaver. Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates. Int J Astrophys Space Sci. 2014;3(1-1):13-20. doi: 10.11648/j.ijass.s.2015030101.13

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  • @article{10.11648/j.ijass.s.2015030101.13,
      author = {Ksh. Newton Singh and Narendra Pradhan and Manuel Malaver},
      title = {Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates},
      journal = {International Journal of Astrophysics and Space Science},
      volume = {3},
      number = {1-1},
      pages = {13-20},
      doi = {10.11648/j.ijass.s.2015030101.13},
      url = {https://doi.org/10.11648/j.ijass.s.2015030101.13},
      eprint = {https://download.sciencepg.com/pdf/10.11648.j.ijass.s.2015030101.13},
      abstract = {We present a spherically symmetric solution of the general relativistic field equations in isotropic coordinates for charged fluid with pressure anisotropy, compatible with a super dense star modeling. Further, we have constructed an anisotropic model of super dense star with all degree of suitability. We also observed that by increasing anisotropy, the maximum mass of super dense stars also decreases.},
     year = {2014}
    }
    

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    T1  - Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates
    AU  - Ksh. Newton Singh
    AU  - Narendra Pradhan
    AU  - Manuel Malaver
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    JF  - International Journal of Astrophysics and Space Science
    JO  - International Journal of Astrophysics and Space Science
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    EP  - 20
    PB  - Science Publishing Group
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    UR  - https://doi.org/10.11648/j.ijass.s.2015030101.13
    AB  - We present a spherically symmetric solution of the general relativistic field equations in isotropic coordinates for charged fluid with pressure anisotropy, compatible with a super dense star modeling. Further, we have constructed an anisotropic model of super dense star with all degree of suitability. We also observed that by increasing anisotropy, the maximum mass of super dense stars also decreases.
    VL  - 3
    IS  - 1-1
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