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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A recurring 0.03 Hz radio QPO was detected in the 2025 flare of GRS 1915+105 at >5.9 sigma in one epoch, identical across S- and X-bands and prior years, indicating an intrinsic accretion-jet timescale.
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Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts
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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A 0.03 Hz Radio Quasi-periodic Oscillation During the 2025 Flare of GRS 1915+105
A recurring 0.03 Hz radio QPO was detected in the 2025 flare of GRS 1915+105 at >5.9 sigma in one epoch, identical across S- and X-bands and prior years, indicating an intrinsic accretion-jet timescale.