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Ringdown overtones, black hole spectroscopy, and no-hair theorem tests · Around

2019

Ringdown overtones, black hole spectroscopy, and no-hair theorem tests

Bhagwat, Swetha, Forteza, Xisco Jimenez, Pani, Paolo et al.

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Validating the black-hole no-hair theorem with gravitational-wave observations of compact binary coalescences provides a compelling argument that the remnant object is indeed a black hole as described by the general theory of relativity.

This requires performing a spectroscopic analysis of the post-merger signal and resolving the frequencies of either different angular modes or overtones (of the same angular mode).
For a nearly-equal mass binary black-hole system, only the dominant angular mode ($l=m=2$) is sufficiently excited and the overtones are instrumental to perform this test.
Here we investigate the robustness of modelling the post-merger signal of a binary black hole coalescence as a superposition of overtones.

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