2006/12/27 by Alikram N. Aliev, Aliev, Alikram N.
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics (astro-ph) #Black Holes and Theoretical Physics #FOS: Physical sciences #Pulsars and Gravitational Waves Research
paper · pdf · doi:10.48550/arxiv.astro-ph/0612730
openalex publication_date 2006/12/27 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We briefly discuss the theory of epicyclic motion near rotating black holes and its relation to the origin of high frequency Quasi-Periodic Oscillations (QPOs) seen in many cases of accreting black hole binaries. We also point out some new frequency ratios predicted by the theory.