The LQG parameter ξ enlarges equatorial bound orbit energy ranges, confines off-equatorial trajectories, and produces larger deviations from Kerr waveforms in EMRI models for two rotating LQG black holes, though signals fall below detector sensitivities.
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Disformal Kerr black holes in BHL accretion produce modified shock structures and QPO frequencies at 43-68 Hz and lower that align with observations from GRS 1915+105, M82 X-1, and similar sources via inverse-mass scaling.
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Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity
The LQG parameter ξ enlarges equatorial bound orbit energy ranges, confines off-equatorial trajectories, and produces larger deviations from Kerr waveforms in EMRI models for two rotating LQG black holes, though signals fall below detector sensitivities.
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Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts
Disformal Kerr black holes in BHL accretion produce modified shock structures and QPO frequencies at 43-68 Hz and lower that align with observations from GRS 1915+105, M82 X-1, and similar sources via inverse-mass scaling.