Axisymmetric Stability of Kerr Black Holes

Details Axisymmetric Stability of Kerr Black Holes Axisymmetric Stability of Kerr Black Holes

Feb 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974phrvl..32..243f&link_type=abstract

Physical Review Letters, vol. 32, Issue 5, pp. 243-245

Physics

4

Scientific paper

A variational expression is used to prove that all axisymmetric modes of
the Kerr sequence of rotating black holes are stable.

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