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.
Hod, Analytic treatment of the system of a Kerr-Newman black hole and a charged massive scalar field , Phys
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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.