Abstract
Einstein–Maxwell field equations corresponding to a higher-dimensional description of static spherically symmetric space–time are solved under two specific sets of conditions: (i) ρ ≠ 0, ν′ = 0 and (ii) ρ = 0, ν′ ≠ 0, where ρ and ν represent the mass density and metric potential. The solution sets thus obtained satisfy the criteria of being an electromagnetic mass model such that the gravitational mass vanishes for the vanishing charge density σ and also the space–time becomes flat. Physical features related to other parameters are also discussed.
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