In 5D Einstein-Bumblebee gravity, Kerr/CFT microscopic entropy of constructed rotating black holes matches Komar-integral entropy but not Wald entropy.
Spontaneous Lorentz violation, Nambu-Goldstone modes, and gravity,
2 Pith papers cite this work. Polarity classification is still indexing.
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EHT angular diameter data yield upper bounds on the holonomy correction b (e.g., b ≤ 0.1319M at a=0 for M87*) showing nonzero b remains consistent with observations for RHCBH spacetimes.
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Rotating Black Holes and the Kerr/CFT Correspondence in Einstein-Bumblebee Gravity
In 5D Einstein-Bumblebee gravity, Kerr/CFT microscopic entropy of constructed rotating black holes matches Komar-integral entropy but not Wald entropy.
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Testing loop quantum gravity through EHT observations of M87* and Sgr A* using rotating holonomy-corrected black holes
EHT angular diameter data yield upper bounds on the holonomy correction b (e.g., b ≤ 0.1319M at a=0 for M87*) showing nonzero b remains consistent with observations for RHCBH spacetimes.