For BTZ-like black holes in Einstein-bumblebee gravity, the conserved charges, central charges, and entropy all acquire factors of the Lorentz-violating parameter, and the near-horizon extremal case admits a Virasoro-Kac-Moody U(1) algebra.
Gravitational waves in general relativity. 8. Waves in asymptotically flat space-times,
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Conserved charges and asymptotic symmetries of BTZ-like black holes in Einstein-bumblebee gravity
For BTZ-like black holes in Einstein-bumblebee gravity, the conserved charges, central charges, and entropy all acquire factors of the Lorentz-violating parameter, and the near-horizon extremal case admits a Virasoro-Kac-Moody U(1) algebra.