4 A source of a quasi – spherical space – time : The case for the M – Q solution
نویسندگان
چکیده
We present a physically reasonable source for an static, axially– symmetric solution to the Einstein equations. Arguments are provided , supporting our belief that the exterior space–time produced by such source, describing a quadrupole correction to the Schwarzschild metric, is particularly suitable (among known solutions of the Weyl family) for discussing the properties of quasi–spherical gravitational fields.
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