Physics
Scientific paper
Aug 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997gregr..29..991m&link_type=abstract
General Relativity and Gravitation, Volume 29, Issue 8, p.991-996
Physics
4
Scientific paper
An exact asymptotically flat 3-parameter solution of the Einstein--Max\-well equations is presented that reduces to the Bonnor magnetic dipole solution in the magnetostatic limit, and to the Tomimatsu-Sato $\delta=2$ solution in the stationary pure vacuum limit. This solution is the simplest possible one admitting the polynomial representation in the spheroidal coordinates ($x,y$) and able to describe the exterior field of a magnetized spinning mass. A multipole criterion for the choice of the parameters in the Einstein--Maxwell spacetimes is also formulated.
Manko Vladimir S.
Ruiz Eduardo
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