The symmetries of Kerr black holes

Details The symmetries of Kerr black holes The symmetries of Kerr black holes

Jun 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973cmaph..33..129h&link_type=abstract

Communications in Mathematical Physics, Volume 33, Issue 2, pp.129-133

Mathematics

Mathematical Physics

23

Scientific paper

The Kerr solution describes, in Einstein's theory, the gravitational
field of a rotating black hole. The axial symmetry and stationarity of
the solution are shown here to arise in a simple way from properties of
the curvature tensor.

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