Some Properties of Kerr Geometry with a Repulsive Cosmological Constant

Details Some Properties of Kerr Geometry with a Repulsive Cosmological Constant Some Properties of Kerr Geometry with a Repulsive Cosmological Constant

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.2282p&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

Mathematics

Logic

Stationary Observers, Black Hole, Kerr Geometry, Cosmological Constant, Kerr-De Sitter Geometry

Scientific paper

We summarize general properties of the Kerr-de Sitter geometry, i.e., Kerr geometry in the presence of a repulsive cosmological constant. An interesting difference between Kerr geometry and Kerr-de Sitter geometry has been found -- namely, the condition of free fall (vanishing 4-acceleration) is satisfied for stationary observers located on the axis of symmetry above the horizon.

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