For Kerr-AdS black holes crossing the Hawking-Reall bound, stationary gravitational modes exist for all sufficiently large azimuthal numbers, and the parameters accumulate on the threshold as the azimuthal number grows.
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Stationary gravitational modes on Kerr-anti-de Sitter spacetimes
For Kerr-AdS black holes crossing the Hawking-Reall bound, stationary gravitational modes exist for all sufficiently large azimuthal numbers, and the parameters accumulate on the threshold as the azimuthal number grows.