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| Format: | Preprint |
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2026
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| Online Access: | https://arxiv.org/abs/2605.25623 |
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| _version_ | 1866913161357033472 |
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| author | Guo, Shitong Miao, Yan-Gang |
| author_facet | Guo, Shitong Miao, Yan-Gang |
| contents | Black-hole spectroscopy aims to infer properties of the remnant spacetime from the quasinormal-mode (QNM) spectrum of the gravitational-wave ringdown signal. In most implementations, however, this inference is performed with waveform models that already incorporate Kerr or other theory-specific QNM spectral relations, thereby entangling spectral measurement with remnant or beyond-Kerr parameter inference. At the same time, conventional ringdown analyses commonly excise the pre-merger data, which in principle contain information about the excitation amplitudes and phases of the QNMs. We introduce \texttt{SPRING} (\textit{Spectral-level Pre-merger-informed RINGdown inference}), a framework designed to separate ringdown spectral inference from theory-side interpretation while propagating pre-merger information through amplitude-scale estimation. As a demonstration, we apply \texttt{SPRING} to GW250114 using an agnostic two-component damped-sinusoid (2DS) model for Kerr remnant inference. \texttt{SPRING} improves the Bayesian support for the agnostic 2DS signal model relative to analyses that do not use pre-merger information, with an increase of \(Δ\ln B\sim 5\)--\(10\). The resulting remnant posterior remains closely consistent with the inspiral-merger-ringdown estimate, despite the extra freedom introduced by the second DS component. This work bridges pre-merger information and ringdown inference, establishing a fully spectral-level route for future black-hole spectroscopy. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2605_25623 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | A pre-merger-informed spectral-level ringdown inference framework for black-hole spectroscopy Guo, Shitong Miao, Yan-Gang General Relativity and Quantum Cosmology High Energy Physics - Theory Black-hole spectroscopy aims to infer properties of the remnant spacetime from the quasinormal-mode (QNM) spectrum of the gravitational-wave ringdown signal. In most implementations, however, this inference is performed with waveform models that already incorporate Kerr or other theory-specific QNM spectral relations, thereby entangling spectral measurement with remnant or beyond-Kerr parameter inference. At the same time, conventional ringdown analyses commonly excise the pre-merger data, which in principle contain information about the excitation amplitudes and phases of the QNMs. We introduce \texttt{SPRING} (\textit{Spectral-level Pre-merger-informed RINGdown inference}), a framework designed to separate ringdown spectral inference from theory-side interpretation while propagating pre-merger information through amplitude-scale estimation. As a demonstration, we apply \texttt{SPRING} to GW250114 using an agnostic two-component damped-sinusoid (2DS) model for Kerr remnant inference. \texttt{SPRING} improves the Bayesian support for the agnostic 2DS signal model relative to analyses that do not use pre-merger information, with an increase of \(Δ\ln B\sim 5\)--\(10\). The resulting remnant posterior remains closely consistent with the inspiral-merger-ringdown estimate, despite the extra freedom introduced by the second DS component. This work bridges pre-merger information and ringdown inference, establishing a fully spectral-level route for future black-hole spectroscopy. |
| title | A pre-merger-informed spectral-level ringdown inference framework for black-hole spectroscopy |
| topic | General Relativity and Quantum Cosmology High Energy Physics - Theory |
| url | https://arxiv.org/abs/2605.25623 |