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A toy model of hyperboloidal approach to quasinormal modes
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We consider a scalar field propagating in the static region of the two dimensional de Sitter space. This simple system is used to illustrate the advantages of hyperboloidal foliations in the analysis of quasinormal modes.
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Cited by 1 Pith paper
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Quasi-normal mode expansions of black hole perturbations: a hyperboloidal Keldysh's approach
A Keldysh spectral expansion built on dual pairings reproduces black hole quasinormal-mode time series, including Schwarzschild power-law tails, and supplies H^p pseudospectral and transient-growth tools.
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