Abstract
We analyze GW150914 postmerger data to understand if ringdown overtone detection claims are robust. We find no evidence in favor of an overtone in the data after the waveform peak. Around the peak, the Bayes factor does not indicate the presence of an overtone, while the support for a nonzero amplitude is sensitive to changes in the starting time much smaller than the overtone damping time. This suggests that claims of an overtone detection are noise dominated. We perform GW150914-like injections in neighboring segments of the real detector noise, and we show that noise can indeed induce artificial evidence for an overtone.
- Received 10 January 2022
- Revised 29 March 2022
- Accepted 7 July 2022
DOI:https://doi.org/10.1103/PhysRevLett.129.111102
© 2022 American Physical Society
Physics Subject Headings (PhySH)
synopsis
To Hear or Not to Hear Overtones in Black Hole Mergers
Published 9 September 2022
A new analysis questions whether researchers found so-called overtones in the first detected gravitational-wave signal from a black hole merger.
See more in Physics