Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star

A. H. M. Mahbubur Rahman; M. Rubayet Rahman; A. S. M. Mohiul Islam

doi:doi:10.11648/j.ijass.20140203.12

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Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star

A. H. M. Mahbubur Rahman, M. Rubayet Rahman, A. S. M. Mohiul Islam

Published in International Journal of Astrophysics and Space Science (Volume 2, Issue 3)

Received: 25 July 2014 Accepted: 9 August 2014 Published: 20 August 2014

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Abstract

The exact analytical Wyman-Adler’s relativistic solution describing the interior of a charged spherical strange star candidate is found under the assumption and existence of two parameters K and m. The interior self-bound star matter, pressure, energy density and the adiabatic sound speed are represented in terms of simple algebraic function. The analytic solution depicts a unique static charged configuration of quark matter with radius R~9 km and total mass M~2.5M¬¬⊙. And try to investigate the velocity of sound approximately 1/√3 which is similar to the attitude of SQM (Strange Quark matter). Based on analytic model in the recent work, the applicable values of physical quantities have been calculated by accepting the estimated masses and radii of some well-known strange star candidates like PSR J1903+327, Her X-1, Cen X-3, EXO 1785-248. The equation of state of the charge matter distribution may play a major role in the study of the interior structure of highly compact charge stellar object in astrophysical study.

Published in	International Journal of Astrophysics and Space Science (Volume 2, Issue 3)
DOI	10.11648/j.ijass.20140203.12
Page(s)	46-55
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

Exact Solution, Einstein-Maxwell, Reissner–Nordström, Relativistic Astrophysics, Compact Star, Equation of State

References

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A. H. M. Mahbubur Rahman, M. Rubayet Rahman, A. S. M. Mohiul Islam. (2014). Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star. International Journal of Astrophysics and Space Science, 2(3), 46-55. https://doi.org/10.11648/j.ijass.20140203.12

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ACS Style

A. H. M. Mahbubur Rahman; M. Rubayet Rahman; A. S. M. Mohiul Islam. Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star. Int. J. Astrophys. Space Sci. 2014, 2(3), 46-55. doi: 10.11648/j.ijass.20140203.12

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AMA Style

A. H. M. Mahbubur Rahman, M. Rubayet Rahman, A. S. M. Mohiul Islam. Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star. Int J Astrophys Space Sci. 2014;2(3):46-55. doi: 10.11648/j.ijass.20140203.12

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@article{10.11648/j.ijass.20140203.12,
  author = {A. H. M. Mahbubur Rahman and M. Rubayet Rahman and A. S. M. Mohiul Islam},
  title = {Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {2},
  number = {3},
  pages = {46-55},
  doi = {10.11648/j.ijass.20140203.12},
  url = {https://doi.org/10.11648/j.ijass.20140203.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20140203.12},
  abstract = {The exact analytical Wyman-Adler’s relativistic solution describing the interior of a charged spherical strange star candidate is found under the assumption and existence of two parameters K and m. The interior self-bound star matter, pressure, energy density and the adiabatic sound speed are represented in terms of simple algebraic function. The analytic solution depicts a unique static charged configuration of quark matter with radius R~9 km and total mass M~2.5M¬¬⊙. And try to investigate the velocity of sound approximately 1/√3 which is similar to the attitude of SQM (Strange Quark matter). Based on analytic model in the recent work, the applicable values of physical quantities have been calculated by accepting the estimated masses and radii of some well-known strange star candidates like PSR J1903+327, Her X-1, Cen X-3, EXO 1785-248. The equation of state of the charge matter distribution may play a major role in the study of the interior structure of highly compact charge stellar object in astrophysical study.},
 year = {2014}
}

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TY - JOUR
T1 - Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star
AU - A. H. M. Mahbubur Rahman
AU - M. Rubayet Rahman
AU - A. S. M. Mohiul Islam
Y1 - 2014/08/20
PY - 2014
N1 - https://doi.org/10.11648/j.ijass.20140203.12
DO - 10.11648/j.ijass.20140203.12
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 - 46
EP - 55
PB - Science Publishing Group
SN - 2376-7022
UR - https://doi.org/10.11648/j.ijass.20140203.12
AB - The exact analytical Wyman-Adler’s relativistic solution describing the interior of a charged spherical strange star candidate is found under the assumption and existence of two parameters K and m. The interior self-bound star matter, pressure, energy density and the adiabatic sound speed are represented in terms of simple algebraic function. The analytic solution depicts a unique static charged configuration of quark matter with radius R~9 km and total mass M~2.5M¬¬⊙. And try to investigate the velocity of sound approximately 1/√3 which is similar to the attitude of SQM (Strange Quark matter). Based on analytic model in the recent work, the applicable values of physical quantities have been calculated by accepting the estimated masses and radii of some well-known strange star candidates like PSR J1903+327, Her X-1, Cen X-3, EXO 1785-248. The equation of state of the charge matter distribution may play a major role in the study of the interior structure of highly compact charge stellar object in astrophysical study.
VL - 2
IS - 3
ER -

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Author Information

A. H. M. Mahbubur Rahman

Department of Civil Engineering, Southern University Bangladesh, Bangladesh
M. Rubayet Rahman

Faculty of Math and Science, Asian University for Women, Bangladesh
A. S. M. Mohiul Islam

Department of Mathematics, University of Chittagong, Bangladesh

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APA Style

A. H. M. Mahbubur Rahman, M. Rubayet Rahman, A. S. M. Mohiul Islam. (2014). Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star. International Journal of Astrophysics and Space Science, 2(3), 46-55. https://doi.org/10.11648/j.ijass.20140203.12

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ACS Style

A. H. M. Mahbubur Rahman; M. Rubayet Rahman; A. S. M. Mohiul Islam. Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star. Int. J. Astrophys. Space Sci. 2014, 2(3), 46-55. doi: 10.11648/j.ijass.20140203.12

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AMA Style

A. H. M. Mahbubur Rahman, M. Rubayet Rahman, A. S. M. Mohiul Islam. Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star. Int J Astrophys Space Sci. 2014;2(3):46-55. doi: 10.11648/j.ijass.20140203.12

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@article{10.11648/j.ijass.20140203.12,
  author = {A. H. M. Mahbubur Rahman and M. Rubayet Rahman and A. S. M. Mohiul Islam},
  title = {Well Behaved Charge Analogues of Wyman-Adler Exact Solution for a Self-Bound Star},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {2},
  number = {3},
  pages = {46-55},
  doi = {10.11648/j.ijass.20140203.12},
  url = {https://doi.org/10.11648/j.ijass.20140203.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20140203.12},
  abstract = {The exact analytical Wyman-Adler’s relativistic solution describing the interior of a charged spherical strange star candidate is found under the assumption and existence of two parameters K and m. The interior self-bound star matter, pressure, energy density and the adiabatic sound speed are represented in terms of simple algebraic function. The analytic solution depicts a unique static charged configuration of quark matter with radius R~9 km and total mass M~2.5M¬¬⊙. And try to investigate the velocity of sound approximately 1/√3 which is similar to the attitude of SQM (Strange Quark matter). Based on analytic model in the recent work, the applicable values of physical quantities have been calculated by accepting the estimated masses and radii of some well-known strange star candidates like PSR J1903+327, Her X-1, Cen X-3, EXO 1785-248. The equation of state of the charge matter distribution may play a major role in the study of the interior structure of highly compact charge stellar object in astrophysical study.},
 year = {2014}
}

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