Ringdown analysis of GW250114 with orthonormal modes
Abstract
GW250114 is the loudest gravitational wave event to date observed by LIGO-Virgo-KAGRA Collaboration. Owing to its high signal-to-noise ratio (SNR), previous analyses based on quasinormal mode (QNM) superpositions have suggested evidence of the fundamental and the first overtone of the ℓ=m=2 mode in this event. However, QNMs are not orthogonal and the inclusion of multiple QNMs induces correlations among them, which can hinder the robust identification of subdominant QNMs. To address this challenge, we apply an analysis based on orthonormalized QNMs [S. Morisaki et al., Phys. Rev. D 112, 124083 (2025)] to GW250114. We find that, in the model including three ℓ=m=2 QNMs up to the second overtone, the first overtone of the ℓ=m=2 mode is more strongly supported than in previous nonorthogonal analyses, with the inferred significance increasing from 82.5% to 99.9%. Furthermore, we estimate deviations from the Kerr prediction using the orthonormal QNM framework and find no significant deviation, consistent with previous analyses. These results demonstrate that the orthonormal QNM framework provides a more robust way to identify subdominant modes in high-SNR ringdown signals, highlighting its potential for future gravitational wave observations.
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BibTeX
@misc{suzuki2026ringdown,
title = {{Ringdown analysis of GW250114 with orthonormal modes}},
author = {Motoki Suzuki and Kei-ichiro Kubota and Soichiro Morisaki and Hayato Motohashi and Daiki Watarai},
howpublished = {arXiv},
year = {2026},
month = aug,
doi = {10.48550/arxiv.2605.03576},
eprint = {2605.03576},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2605.03576},
}
RIS
TY - UNPB
TI - Ringdown analysis of GW250114 with orthonormal modes
AU - Motoki Suzuki
AU - Kei-ichiro Kubota
AU - Soichiro Morisaki
AU - Hayato Motohashi
AU - Daiki Watarai
PY - 2026
DA - 2026/08/28
PB - arXiv
DO - 10.48550/arxiv.2605.03576
UR - https://arxiv.org/abs/2605.03576
AB - GW250114 is the loudest gravitational wave event to date observed by LIGO-Virgo-KAGRA Collaboration. Owing to its high signal-to-noise ratio (SNR), previous analyses based on quasinormal mode (QNM) superpositions have suggested evidence of the fundamental and the first overtone of the ℓ=m=2 mode in this event. However, QNMs are not orthogonal and the inclusion of multiple QNMs induces correlations among them, which can hinder the robust identification of subdominant QNMs. To address this challenge, we apply an analysis based on orthonormalized QNMs [S. Morisaki et al., Phys. Rev. D 112, 124083 (2025)] to GW250114. We find that, in the model including three ℓ=m=2 QNMs up to the second overtone, the first overtone of the ℓ=m=2 mode is more strongly supported than in previous nonorthogonal analyses, with the inferred significance increasing from 82.5% to 99.9%. Furthermore, we estimate deviations from the Kerr prediction using the orthonormal QNM framework and find no significant deviation, consistent with previous analyses. These results demonstrate that the orthonormal QNM framework provides a more robust way to identify subdominant modes in high-SNR ringdown signals, highlighting its potential for future gravitational wave observations.
ER -