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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Numerical BHL accretion simulations in disformal Kerr spacetime produce QPO frequencies consistent with observations from GRS 1915+105, M82 X-1, NGC 5408 X-1, and RE J1034+396.
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