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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.

Published in International Journal of Astrophysics and Space Science (Volume 3, Issue 1-1)

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

DOI 10.11648/j.ijass.s.2015030101.13
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), 2014. Published by Science Publishing Group

Keywords

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

References
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  • APA Style

    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://article.sciencepublishinggroup.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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  • TY  - JOUR
    T1  - Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates
    AU  - Ksh. Newton Singh
    AU  - Narendra Pradhan
    AU  - Manuel Malaver
    Y1  - 2014/12/19
    PY  - 2014
    N1  - https://doi.org/10.11648/j.ijass.s.2015030101.13
    DO  - 10.11648/j.ijass.s.2015030101.13
    T2  - International Journal of Astrophysics and Space Science
    JF  - International Journal of Astrophysics and Space Science
    JO  - International Journal of Astrophysics and Space Science
    SP  - 13
    EP  - 20
    PB  - Science Publishing Group
    SN  - 2376-7022
    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
    ER  - 

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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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