Clarify mode-coupling mechanisms in non-axisymmetric disc-oscillation models
Clarify the physical mechanisms that couple axisymmetric and non-axisymmetric modes, as well as pairs of non-axisymmetric modes, in the Non-axisymmetric Disc Oscillation Models.
References
Although these models provide a natural framework for incorporating pressure effects and non-axisymmetric oscillations, their physical basis remains uncertain. In particular, the mechanisms responsible for coupling an axisymmetric mode to a non-axisymmetric mode, or coupling pairs of non-axisymmetric modes, are not yet well understood, limiting the predictive power of the model .
— Probing hairy Kerr black holes through quasi-periodic oscillations II: a study based on the resonance models
(2610.11378 - Dasgupta et al., 8 Oct 2026) in Section 3, subsection “Non-axisymmetric Disc Oscillation Model (NADO)”