Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates

Ksh. Newton Singh; Narendra Pradhan; Manuel Malaver

doi:doi:10.11648/j.ijass.s.2015030101.13

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Modeling Anisotropic Charged Neutron Star in Isotropic Coordinates

Ksh. Newton Singh, Narendra Pradhan, Manuel Malaver

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

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
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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

Ksh. Newton Singh

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

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

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

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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}
}

Copy | Download

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  -

Copy | Download