Fundamental stationary scalar clouds exist around rotating BTZ-like black holes in Einstein-bumblebee gravity, with the Lorentz-breaking parameter and angular quantum number having opposite effects and sometimes producing degenerate cloud lines.
Carter, in Black Holes, Proceedings of 1972 Session of Ecole d’ete de Physique Theorique, edited by C
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Stationary scalar clouds around a rotating BTZ-like black hole in the Einstein-bumblebee gravity
Fundamental stationary scalar clouds exist around rotating BTZ-like black holes in Einstein-bumblebee gravity, with the Lorentz-breaking parameter and angular quantum number having opposite effects and sometimes producing degenerate cloud lines.