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A perfect-fluid spacetime for a slightly deformed mass

    https://doi.org/10.1142/9789814759816_0048Cited by:0 (Source: Crossref)
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    Abstract:

    We present approximate exterior and interior solutions of Einstein's equations which describe the gravitational field of a static deformed mass distribution. The deformation of the source is taken into account up to the first order in the quadrupole.