摘要: The equations describing the hydrostatic equilibrium (mass continuity and Tolman–Oppenheimer–Volkoff) of a static anisotropic general relativistic fluid sphere are obtained in D (D⩾4) space–time dimensions presence cosmological constant. formalism thus developed is used to study homogeneous constant density charged spheres with neutral isotropic core higher dimensions. For these configurations particular choice proper charge complete solution coupled Einstein–Maxwell obtained.
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