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.
Carter, Phys
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No evidence for physics beyond general relativity is found in the analysis of 15 GW events from GWTC-3, with consistency in residuals, PN parameters, and remnant properties.
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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.
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Tests of General Relativity with GWTC-3
No evidence for physics beyond general relativity is found in the analysis of 15 GW events from GWTC-3, with consistency in residuals, PN parameters, and remnant properties.