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. |