Abstract
Spherically symmetric solutions of the combined system of four-dimensional Einstein, Maxwell, and specific scalar-field equations are obtained by generalization of the Schwarzschild metric and its subsequent linear quasi-rotation in the (x0, x5) plane. The accurate Kramer—Legkii solution of the five-dimensional Einstein equations is used. New accurate solutions generalizing the well-known Reissner—Nordstrom and Fisher metrics are obtained.
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