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It is known that approximating the Regge-Wheeler Potential with step functions significantly modifies the Schwarzschild black hole quasinormal mode spectrum.
1904
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2009
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2011
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2006
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M. Maggiore, “Physical Interpretation of the Spectrum of Black Hole Quasinormal Modes”,
2008
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K. Lin and W.-L. Qian, “A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes”,
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A.F. Cardona and C. Molina, “Quasinormal modes of generalized Pöschl-Teller potentials”,
2017
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