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arXiv · 2604.19692

QPOs from the Viscous Transonic Accretion Flow Around a Spinning Black Hole

Sanjit Debnath·Indranil Chattopadhyay·Soumyadip Mandal·Raj Kishor Joshi·Priyesh Kumar Tripathi·M. Saleem Khan
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Abstract

We investigate the dynamics of transonic advective accretion flows around spinning black holes in the presence of viscosity. The spacetime of a Kerr black hole is approximated using a pseudo-potential. We study viscously driven shock oscillations over a range of black hole spin parameters. Our results show that the frequency range of quasi-periodic oscillations (QPOs) obtained from the power density spectra depends strongly on the black hole spin. Low-spin systems predominantly exhibit low-frequency QPOs, whereas rapidly rotating black holes (greater than 0.9 Kerr parameter) produce QPOs spanning a broad range from low to high frequencies, comparable to those observed in black hole X-ray binaries. We further obtain a correlation between the QPO frequency and the power-law photon index by computing the spectrum for a 10 solar mass black hole.

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Sanjit Debnath, Indranil Chattopadhyay, Soumyadip Mandal, Raj Kishor Joshi, Priyesh Kumar Tripathi, M. Saleem Khan. 2026-04-21. QPOs from the Viscous Transonic Accretion Flow Around a Spinning Black Hole. https://arxiv.org/abs/2604.19692

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