This paper discusses the evolution of a thin spherically symmetric self gravitating phantom shell around the charged shell. The general equations describing the motion of shell with a general form of equation of state are derived. The different types of space-time R± and T± regions and shell motion are classified depending on the parameters of the problem. The mechanical stability analysis of this spherically symmetric thin shell with charge in Reissner- Nordstrom (RN) to linearized spherically symmetric perturbation about static equilibrium solution is carried out.
Published in | American Journal of Astronomy and Astrophysics (Volume 3, Issue 3) |
DOI | 10.11648/j.ajaa.20150303.14 |
Page(s) | 50-55 |
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), 2015. Published by Science Publishing Group |
General Relativity, Astrophysics, Cosmology, Phantom Energy
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APA Style
Ali Eid. (2015). Stability of Charged Shell Supported by a Phantom Energy. American Journal of Astronomy and Astrophysics, 3(3), 50-55. https://doi.org/10.11648/j.ajaa.20150303.14
ACS Style
Ali Eid. Stability of Charged Shell Supported by a Phantom Energy. Am. J. Astron. Astrophys. 2015, 3(3), 50-55. doi: 10.11648/j.ajaa.20150303.14
AMA Style
Ali Eid. Stability of Charged Shell Supported by a Phantom Energy. Am J Astron Astrophys. 2015;3(3):50-55. doi: 10.11648/j.ajaa.20150303.14
@article{10.11648/j.ajaa.20150303.14, author = {Ali Eid}, title = {Stability of Charged Shell Supported by a Phantom Energy}, journal = {American Journal of Astronomy and Astrophysics}, volume = {3}, number = {3}, pages = {50-55}, doi = {10.11648/j.ajaa.20150303.14}, url = {https://doi.org/10.11648/j.ajaa.20150303.14}, eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajaa.20150303.14}, abstract = {This paper discusses the evolution of a thin spherically symmetric self gravitating phantom shell around the charged shell. The general equations describing the motion of shell with a general form of equation of state are derived. The different types of space-time R± and T± regions and shell motion are classified depending on the parameters of the problem. The mechanical stability analysis of this spherically symmetric thin shell with charge in Reissner- Nordstrom (RN) to linearized spherically symmetric perturbation about static equilibrium solution is carried out.}, year = {2015} }
TY - JOUR T1 - Stability of Charged Shell Supported by a Phantom Energy AU - Ali Eid Y1 - 2015/05/15 PY - 2015 N1 - https://doi.org/10.11648/j.ajaa.20150303.14 DO - 10.11648/j.ajaa.20150303.14 T2 - American Journal of Astronomy and Astrophysics JF - American Journal of Astronomy and Astrophysics JO - American Journal of Astronomy and Astrophysics SP - 50 EP - 55 PB - Science Publishing Group SN - 2376-4686 UR - https://doi.org/10.11648/j.ajaa.20150303.14 AB - This paper discusses the evolution of a thin spherically symmetric self gravitating phantom shell around the charged shell. The general equations describing the motion of shell with a general form of equation of state are derived. The different types of space-time R± and T± regions and shell motion are classified depending on the parameters of the problem. The mechanical stability analysis of this spherically symmetric thin shell with charge in Reissner- Nordstrom (RN) to linearized spherically symmetric perturbation about static equilibrium solution is carried out. VL - 3 IS - 3 ER -