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- W2144344886 abstract "The observed quasi-periodic oscillations (QPOs) in low-mass X-raybinaries have been suggested to be probably related to the characteristicoscillation modes in the inner part ofa relativistic accretion disk. In this paper we study the trapped feature of these oscillation modes by considering the radial perturbations and viscosity effects. We find that the trappedoscillations are amplified significantly when the viscosity parameterincreases and the trapped size varies when the radial wavenumber and Mach number change. Our results support that the stablehundred-hertz QPOs and their low fractional rms amplitudes found intwo Galactic microquasars may be explained by some trapped non-damping oscillation modes in the inner part of accretiondisks around rotating black holes." @default.
- W2144344886 created "2016-06-24" @default.
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- W2144344886 date "2001-01-01" @default.
- W2144344886 modified "2023-09-25" @default.
- W2144344886 title "Trapped Disk Oscillations and Stable QPOs in Microquasars" @default.
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- W2144344886 doi "https://doi.org/10.1007/978-94-010-0700-9_43" @default.
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