New Models of Dark Energy Stars with Charge Distributions

Manuel Malaver; María Esculpi; Megandhren Govender

doi:doi:10.11648/j.ijass.20190702.12

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New Models of Dark Energy Stars with Charge Distributions

Manuel Malaver, María Esculpi, Megandhren Govender

Published in International Journal of Astrophysics and Space Science (Volume 7, Issue 2)

Received: 15 July 2019 Accepted: 19 August 2019 Published: 2 September 2019

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Abstract

In this paper, we have obtained a relativistic and spherically symmetric stellar configuration that describes an anisotropic fluid with a charge distribution that represents a potential model for a dark energy star and we specify particular forms in the gravitational potential and the electric field intensity which allows solve the Einstein-Maxwell field equations. The reason for proposing this model originates from the evidence that recent observational findings suggest that the universe has an accelerated cosmic expansion and the model of dark energy star is one of the most reasonable explanations of this phenomena. The field equations are integrated analytical and new stellar configurations are obtained are analyzed. For each these solutions we found that the radial pressure, the anisotropy factor, energy density, metric coefficients, mass function, charge density are regular and well behaved in the stellar interior. With the new solutions can be developed models of dark energy stars physically acceptable where the causality condition is not satisfied or the strong energy condition is violated. This model has a great application in the study of the fundamental theories of physics and cosmology. Several independent observations indicate that the greater part of the total energy density of the universe is in the form of dark energy and the rest in the form of nonbaryonic cold dark matter particles, but which have never been detected.

Published in	International Journal of Astrophysics and Space Science (Volume 7, Issue 2)
DOI	10.11648/j.ijass.20190702.12
Page(s)	18-23
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), 2019. Published by Science Publishing Group

Keywords

Stellar Configuration, Gravitational Potential, Charge Distribution, Anisotropic Fluid, Accelerated Cosmic Expansion, Einstein-Maxwell Field Equations

References

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APA Style

Manuel Malaver, María Esculpi, Megandhren Govender. (2019). New Models of Dark Energy Stars with Charge Distributions. International Journal of Astrophysics and Space Science, 7(2), 18-23. https://doi.org/10.11648/j.ijass.20190702.12

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ACS Style

Manuel Malaver; María Esculpi; Megandhren Govender. New Models of Dark Energy Stars with Charge Distributions. Int. J. Astrophys. Space Sci. 2019, 7(2), 18-23. doi: 10.11648/j.ijass.20190702.12

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AMA Style

Manuel Malaver, María Esculpi, Megandhren Govender. New Models of Dark Energy Stars with Charge Distributions. Int J Astrophys Space Sci. 2019;7(2):18-23. doi: 10.11648/j.ijass.20190702.12

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@article{10.11648/j.ijass.20190702.12,
  author = {Manuel Malaver and María Esculpi and Megandhren Govender},
  title = {New Models of Dark Energy Stars with Charge Distributions},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {7},
  number = {2},
  pages = {18-23},
  doi = {10.11648/j.ijass.20190702.12},
  url = {https://doi.org/10.11648/j.ijass.20190702.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20190702.12},
  abstract = {In this paper, we have obtained a relativistic and spherically symmetric stellar configuration that describes an anisotropic fluid with a charge distribution that represents a potential model for a dark energy star and we specify particular forms in the gravitational potential and the electric field intensity which allows solve the Einstein-Maxwell field equations. The reason for proposing this model originates from the evidence that recent observational findings suggest that the universe has an accelerated cosmic expansion and the model of dark energy star is one of the most reasonable explanations of this phenomena. The field equations are integrated analytical and new stellar configurations are obtained are analyzed. For each these solutions we found that the radial pressure, the anisotropy factor, energy density, metric coefficients, mass function, charge density are regular and well behaved in the stellar interior. With the new solutions can be developed models of dark energy stars physically acceptable where the causality condition is not satisfied or the strong energy condition is violated. This model has a great application in the study of the fundamental theories of physics and cosmology. Several independent observations indicate that the greater part of the total energy density of the universe is in the form of dark energy and the rest in the form of nonbaryonic cold dark matter particles, but which have never been detected.},
 year = {2019}
}

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TY  - JOUR
T1  - New Models of Dark Energy Stars with Charge Distributions
AU  - Manuel Malaver
AU  - María Esculpi
AU  - Megandhren Govender
Y1  - 2019/09/02
PY  - 2019
N1  - https://doi.org/10.11648/j.ijass.20190702.12
DO  - 10.11648/j.ijass.20190702.12
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  - 18
EP  - 23
PB  - Science Publishing Group
SN  - 2376-7022
UR  - https://doi.org/10.11648/j.ijass.20190702.12
AB  - In this paper, we have obtained a relativistic and spherically symmetric stellar configuration that describes an anisotropic fluid with a charge distribution that represents a potential model for a dark energy star and we specify particular forms in the gravitational potential and the electric field intensity which allows solve the Einstein-Maxwell field equations. The reason for proposing this model originates from the evidence that recent observational findings suggest that the universe has an accelerated cosmic expansion and the model of dark energy star is one of the most reasonable explanations of this phenomena. The field equations are integrated analytical and new stellar configurations are obtained are analyzed. For each these solutions we found that the radial pressure, the anisotropy factor, energy density, metric coefficients, mass function, charge density are regular and well behaved in the stellar interior. With the new solutions can be developed models of dark energy stars physically acceptable where the causality condition is not satisfied or the strong energy condition is violated. This model has a great application in the study of the fundamental theories of physics and cosmology. Several independent observations indicate that the greater part of the total energy density of the universe is in the form of dark energy and the rest in the form of nonbaryonic cold dark matter particles, but which have never been detected.
VL  - 7
IS  - 2
ER  -

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Author Information

Manuel Malaver

Bijective Physics Institute, Idrija, Slovenia
María Esculpi

Department of Applied Physics, Central University of Venezuela, Faculty of Engineering, Caracas, Venezuela
Megandhren Govender

Department of Mathematics, Statistical and Physics, Durban University of Technology, Durban, South Africa

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APA Style

Manuel Malaver, María Esculpi, Megandhren Govender. (2019). New Models of Dark Energy Stars with Charge Distributions. International Journal of Astrophysics and Space Science, 7(2), 18-23. https://doi.org/10.11648/j.ijass.20190702.12

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ACS Style

Manuel Malaver; María Esculpi; Megandhren Govender. New Models of Dark Energy Stars with Charge Distributions. Int. J. Astrophys. Space Sci. 2019, 7(2), 18-23. doi: 10.11648/j.ijass.20190702.12

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AMA Style

Manuel Malaver, María Esculpi, Megandhren Govender. New Models of Dark Energy Stars with Charge Distributions. Int J Astrophys Space Sci. 2019;7(2):18-23. doi: 10.11648/j.ijass.20190702.12

Copy | Download

@article{10.11648/j.ijass.20190702.12,
  author = {Manuel Malaver and María Esculpi and Megandhren Govender},
  title = {New Models of Dark Energy Stars with Charge Distributions},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {7},
  number = {2},
  pages = {18-23},
  doi = {10.11648/j.ijass.20190702.12},
  url = {https://doi.org/10.11648/j.ijass.20190702.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20190702.12},
  abstract = {In this paper, we have obtained a relativistic and spherically symmetric stellar configuration that describes an anisotropic fluid with a charge distribution that represents a potential model for a dark energy star and we specify particular forms in the gravitational potential and the electric field intensity which allows solve the Einstein-Maxwell field equations. The reason for proposing this model originates from the evidence that recent observational findings suggest that the universe has an accelerated cosmic expansion and the model of dark energy star is one of the most reasonable explanations of this phenomena. The field equations are integrated analytical and new stellar configurations are obtained are analyzed. For each these solutions we found that the radial pressure, the anisotropy factor, energy density, metric coefficients, mass function, charge density are regular and well behaved in the stellar interior. With the new solutions can be developed models of dark energy stars physically acceptable where the causality condition is not satisfied or the strong energy condition is violated. This model has a great application in the study of the fundamental theories of physics and cosmology. Several independent observations indicate that the greater part of the total energy density of the universe is in the form of dark energy and the rest in the form of nonbaryonic cold dark matter particles, but which have never been detected.},
 year = {2019}
}

Copy | Download

TY  - JOUR
T1  - New Models of Dark Energy Stars with Charge Distributions
AU  - Manuel Malaver
AU  - María Esculpi
AU  - Megandhren Govender
Y1  - 2019/09/02
PY  - 2019
N1  - https://doi.org/10.11648/j.ijass.20190702.12
DO  - 10.11648/j.ijass.20190702.12
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  - 18
EP  - 23
PB  - Science Publishing Group
SN  - 2376-7022
UR  - https://doi.org/10.11648/j.ijass.20190702.12
AB  - In this paper, we have obtained a relativistic and spherically symmetric stellar configuration that describes an anisotropic fluid with a charge distribution that represents a potential model for a dark energy star and we specify particular forms in the gravitational potential and the electric field intensity which allows solve the Einstein-Maxwell field equations. The reason for proposing this model originates from the evidence that recent observational findings suggest that the universe has an accelerated cosmic expansion and the model of dark energy star is one of the most reasonable explanations of this phenomena. The field equations are integrated analytical and new stellar configurations are obtained are analyzed. For each these solutions we found that the radial pressure, the anisotropy factor, energy density, metric coefficients, mass function, charge density are regular and well behaved in the stellar interior. With the new solutions can be developed models of dark energy stars physically acceptable where the causality condition is not satisfied or the strong energy condition is violated. This model has a great application in the study of the fundamental theories of physics and cosmology. Several independent observations indicate that the greater part of the total energy density of the universe is in the form of dark energy and the rest in the form of nonbaryonic cold dark matter particles, but which have never been detected.
VL  - 7
IS  - 2
ER  -

Copy | Download