Validity of analytic continuation from bound states to quasinormal modes
Determine rigorous conditions under which the analytic continuation that maps bound-state energies of inverted black hole perturbation potentials to quasinormal mode frequencies is valid, specifying its domain of applicability for cases such as the inverted Regge–Wheeler and modified Pöschl–Teller potentials and in regimes exhibiting spectral instability.
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The inability to find the modes, together with open questions about the validity of the analytic continuation itself, has led to some ambiguity and subsequent criticism.
We were unable to obtain stable results with this approach. If such a procedure exists, it appears to be more complicated than calculating the quasi-bound states directly by numerical shooting and matching solutions of the Riccati equation.