A new class of bipolar vacuum gravitational fields

Details A new class of bipolar vacuum gravitational fields A new class of bipolar vacuum gravitational fields

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982rspsa.382..221d&link_type=abstract

Royal Society (London), Proceedings, Series A - Mathematical and Physical Sciences, vol. 382, no. 1782, July 8, 1982, p. 221-229

Mathematics

26

Asymptotic Methods, Einstein Equations, Gravitational Fields, Numerical Integration, Space-Time Functions, Transformations (Mathematics), Harmonic Functions, Potential Theory, Vacuum Effects

Scientific paper

The Ernst potential and the full four-dimensional metric are presented for a stationary axisymmetric solution of the vacuum Einstein equations, which were obtained by application of two rank-zero H.K.X. transformations (Hoenselaers, Kinnersley and Xanthopolous, 1979) to the general static Weyl solution. A suitable Ehlers transformation ensures asymptotic flatness.

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