Abstract
Rahaman et al. (Astrophys. Space. Sci. 331:191–197, 2010) discussed some classical electron models (CEM) in general relativity. Bijalwan (Astrophys. Space. Sci. 334:139–143, 2011) present a general exact solution of the Einstein-Maxwell equations in terms of pressure. We showed that charged fluid solutions in terms of pressure are not reducible to a well behaved neutral counter part for a spatial component of metrice λ. Hence, these solutions represent an electron model in general relativity. We illustrated solutions in terms of pressure briefly with de-Sitter equation of state and charged analogues of Kohler Chao interior solution as a special cases.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Bijalwan, N.: Astrophys. Space Sci. 334, 139–143 (2011)
Dionysiou, D.D.: Astrophys. Space Sci. 85, 331 (1982)
Finch, M.R., Skea, J.E.F.: Class. Quantum Gravity 4, 467 (1989)
Florides, P.S.: J. Phys. A, Math. Gen. 16, 1419 (1983)
Kohler, M., Chao, K.L.Z.: Naturforsch Set. A 20, 1537 (1965)
Rahaman, F., Jamil, M., Chakraborty, K.: Astrophys. Space Sci. 331, 191–197 (2010)
Tiwari, R.N., Rao, J.R., Kanakamedala, R.R.: Phys. Rev. D 30, 489 (1984)
Tiwari, R.N., Ray, S.: Astrophys. Space Sci. 182, 105 (1991)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Bijalwan, N. Exact solutions: classical electron model. Astrophys Space Sci 336, 485–489 (2011). https://doi.org/10.1007/s10509-011-0796-5
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10509-011-0796-5