Axion hair for Kerr black holes

Details Axion hair for Kerr black holes Axion hair for Kerr black holes

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phlb..251...34c&link_type=abstract

Physics Letters B, Volume 251, Issue 1, p. 34-38.

Physics

38

Scientific paper

We consider axion fields with Lorentz Chern-Simons coupling to gravity. In Kerr black hole background metrics this coupling gives a non-vanishing source term for the axion field. For the case of a slowly rotating black hole, we explicitly calculate the long range axion field strength ``hair'' produced. We believe that this represents the first known example of stable, dynamical, non-gauge ``hair'' exhibited by a black hole.

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