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Parametrized Black Hole Quasinormal Ringdown Formalism for Higher Overtones
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We investigate the parametrized black hole quasinormal ringdown formalism, which is a robust framework used to analyze quasinormal modes in systems that closely resemble general relativity, paying particular attention to the higher overtones. We find that larger deviations from the general relativity case typically appear in the quasinormal frequencies for the higher overtones. This growing tendency for higher overtones can be understood using an analytical method, and its relations to previous works are briefly discussed. Our findings indicate that we can impose a strong constraint on gravity theories by considering the overtones of quasinormal modes.
Forward citations
Cited by 4 Pith papers
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GW250114's fundamental ringdown mode bounds theory-agnostic deviations from the Teukolsky equation to be consistent with zero at characteristic scales of 60-100 km.
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Reanalyzing the ringdown signal of GW150914 using the F-statistic method
Applying the F-statistic method to GW150914's ringdown yields FIC = -0.3 for adding the first overtone, consistent with no overtone, while an injection with an overtone yields FIC = 0.3.
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