TYPE II CHARGED GENERALISATION OF DURGAPAL’S SOLUTIONS FOR n ≥ 2
Abstract
We investigate the equilibrium configuration of a spherically symmetric charged fluid with a metric of the form ds^2=-e^λ(r) dr^2-r^2 (dθ^2+sin^2θ dϕ^2 )+e^ν(r) dt^2. Using e^ν = A^2 (1 + x)^n where x+Cr^2, the coupled Einstein-Maxwell equations are reformulated in terms of a first-order linear differential equation for Z = e^(-λ). The general solution to this equation is derived, admitting integration constants and coefficients defined through recurrence relations. We explore a specific case with n=2 and an electric filed E^2= (α^2 C_x)/(2(1+x))resulting in explicit expressions for the metric components, matter density ρ and pressure p.
References
I. M.C.Durgapal, A Class of new exact solutions in general relativity, Journal of Physics A:Mathematical and General, Vol.15(8),pp 2637, 1982.
II. P.C.Vaidya, Ramesh Tikekar, Exact Relativistic Model for a Superdense Star, Journal of Astro- physics and Astronomy, 3, 325-334 (1982).
III. Sabu M.C, A study of Some Spacetimes of Gravitational Significance, (1998).
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