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Black hole spectroscopy with coherent mode stacking

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it
abstract

The measurement of multiple ringdown modes in gravitational waves from binary black hole mergers will allow for testing fundamental properties of black holes in General Relativity, and to constrain modified theories of gravity. To enhance the ability of Advanced LIGO/Virgo to perform such tasks, we propose a coherent mode stacking method to search for a chosen target mode within a collection of multiple merger events. We first rescale each signal so that the target mode in each of them has the same frequency, and then sum the waveforms constructively. A crucial element to realize this coherent superposition is to make use of a priori information extracted from the inspiral-merger phase of each event. To illustrate the method, we perform a study with simulated events targeting the l=m=3 ringdown mode of the remnant black holes. We show that this method can significantly boost the signal-to-noise ratio of the collective target mode compared to that of the single loudest event. Using current estimates of merger rates we show that it is likely that advanced-era detectors can measure this collective ringdown mode with one year of coincident data gathered at design sensitivity.

fields

gr-qc 3

verdicts

UNVERDICTED 3

representative citing papers

Detectability of avoided crossings in black hole ringdowns

gr-qc · 2026-05-15 · unverdicted · novelty 6.0

Bayesian analysis finds individual QNM frequencies near avoided crossings hard to resolve even under optimistic conditions, though collective AC waveform signatures may remain detectable if those modes dominate and slower-mode contamination is minimal.

Plunge spectra as discriminators of black hole mimickers

gr-qc · 2025-09-12 · unverdicted · novelty 5.0

Plunge spectra of extreme mass ratio events onto black hole mimickers show a low-frequency resonance comb and a high-frequency deviation from black hole behavior above Mω_th ≈ 0.39.

Science with the Einstein Telescope: a comparison of different designs

gr-qc · 2023-03-28 · unverdicted · novelty 3.0

The paper evaluates how triangular versus two-L-shaped geometries, arm lengths, and presence of low-frequency instruments affect the science reach of the Einstein Telescope for compact binaries, multi-messenger events, and stochastic backgrounds.

citing papers explorer

Showing 3 of 3 citing papers.

  • Detectability of avoided crossings in black hole ringdowns gr-qc · 2026-05-15 · unverdicted · none · ref 60 · internal anchor

    Bayesian analysis finds individual QNM frequencies near avoided crossings hard to resolve even under optimistic conditions, though collective AC waveform signatures may remain detectable if those modes dominate and slower-mode contamination is minimal.

  • Plunge spectra as discriminators of black hole mimickers gr-qc · 2025-09-12 · unverdicted · none · ref 62 · internal anchor

    Plunge spectra of extreme mass ratio events onto black hole mimickers show a low-frequency resonance comb and a high-frequency deviation from black hole behavior above Mω_th ≈ 0.39.

  • Science with the Einstein Telescope: a comparison of different designs gr-qc · 2023-03-28 · unverdicted · none · ref 185 · internal anchor

    The paper evaluates how triangular versus two-L-shaped geometries, arm lengths, and presence of low-frequency instruments affect the science reach of the Einstein Telescope for compact binaries, multi-messenger events, and stochastic backgrounds.