Extends previous rotating acoustic geometry model with solid-body rotation term and computes quasibound spectra via analytical solutions of the scalar wave equation.
Slowly-rotating curved acoustic black holes: Quasinormal modes, Hawking–Unruh radiation, and quasibound states
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Extending the model of rotating acoustic geometries to include non-vanishing solid-body rotation: quasibound spectra
Extends previous rotating acoustic geometry model with solid-body rotation term and computes quasibound spectra via analytical solutions of the scalar wave equation.