Local Analysis of Nonlinear Oscillations of Thin Accretion Disks

Details Local Analysis of Nonlinear Oscillations of Thin Accretion Disks Local Analysis of Nonlinear Oscillations of Thin Accretion Disks

2008-02-12

arxiv.org/abs/0802.1594v1

Publ. Astron. Soc. Japan 60, pp.605-612 (2008)

Astronomy and Astrophysics

Astrophysics

15 pages, to be published in PASJ Vol. 60 No. 3

Scientific paper

We calculated the coupling coefficients for non-linear, quasi-local
oscillatory modes of thin accretion disks. We found that several of them are
non-zero. Mode coupling is a necessary condition for a resonance, and thus our
results may be relevant for the recently discussed QPO resonance model.

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