Geometry of rotating charged bubbles in general relativity

Details Geometry of rotating charged bubbles in general relativity Geometry of rotating charged bubbles in general relativity

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990gregr..22..827l&link_type=abstract

General Relativity and Gravitation, Volume 22, Issue 7, pp.827-831

Physics

1

Scientific paper

It is shown that the spatial geometry of the bubbles with a constant radial coordinater o, embedded in the Kerr-Newman manifold, does not depend on the mass and charge of this solution when referred to a coordinate frame rigidly rotating with the angular velocityω =a(r{0/2+a} 2)-1. The corresponding line element is found to be identical to the one obtained by Smarr for the surface geometry of a charged rotating black hole.

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