Skip to content

Overtones and Mode Identifiability

Scrollable formula. Use Left and Right arrow keys to reveal hidden content.

Scrollable table. Use Left and Right arrow keys to reveal additional columns.

Scrollable figure. Use Left and Right arrow keys to inspect hidden content.

An overtone is a quasinormal mode with the same angular labels as another mode but a larger damping rate. Adding overtones can improve an early-time waveform fit; that is not yet evidence that detector data identify each added mode. Identification requires the extra component to be distinguishable from noise, prompt response, start-time shifts, and other flexible corrections under declared priors. This page develops the reusable decision protocol; dated event and catalog verdicts belong to Research rather than to a parallel evidence table here.

Helpful background. Ringdown Likelihoods and Start-Time Dependence supplies the finite-window likelihood and reference-time transformation used here. Ringdown Overtones develops waveform construction, and Completeness, Excitation, and Ringdown Content explains the spectral interpretation.

For one angular multipole, write

h(t)=Re⁡ ⁣[∑n=0NAn(t0)e−iωn(t−t0)],ωn=ωnR−iτn,t≥t0.h(t) = \operatorname{Re}\!\left[ \sum_{n=0}^{N} A_n(t_0)e^{-i\omega_n(t-t_0)} \right], \qquad \omega_n=\omega_n^R-\frac{i}{\tau_n}, \qquad t\geq t_0 .

With e−iωte^{-i\omega t}, higher nn generally means shorter τn\tau_n. An early reference time can therefore give an overtone a large amplitude even though it contributes little a few damping times later. The invariant comparison is not between raw amplitudes quoted at different t0t_0, but between waveforms or amplitudes transported to a common reference:

An(ta)=An(t0)e−iωn(ta−t0).A_n(t_a)=A_n(t_0)e^{-i\omega_n(t_a-t_0)}.

The Kerr label nn has physical content only when the inferred complex frequency agrees with the predicted spectral branch. A free damped sinusoid that absorbs modeling error is not automatically a quasinormal overtone.

Fit quality, necessity, and identification

Section titled “Fit quality, necessity, and identification”

Three questions must be separated.

  1. Reconstruction: Does a larger mode set reduce residuals or mismatch?
  2. Predictive necessity: Does it improve out-of-sample or posterior-predictive performance after the additional parameter volume is counted?
  3. Physical identification: Are its frequency, damping time, angular response, and start-time evolution consistent with one spectral mode and distinguishable from competitors?

A fixed-Kerr overtone model can win an evidence comparison because its frequencies are tied to a common (Mf,χf)(M_f,\chi_f). That is evidence for the constrained waveform family relative to the alternatives actually compared. It is weaker than measuring the overtone frequency independently. Conversely, freeing every ωn\omega_n may make physical identification impossible at available signal-to-noise ratio even if a Kerr-tied component is useful.

Near-degenerate exponentials make the problem ill-conditioned. Sample the complex basis functions qn(t)=e−iωn(t−t0)q_n(t)=e^{-i\omega_n(t-t_0)} in the chosen window and define a Hermitian noise-weighted Gram matrix

Gmn=⟨qm,qn⟩C≡qm†C−1qn.G_{mn}=\langle q_m,q_n\rangle_C \equiv q_m^\dagger C^{-1}q_n.

Equivalently, first whiten the vectors by C−1/2C^{-1/2} and use their ordinary Hermitian inner product. The exponentials themselves are not already whitened in colored noise. For real detector data, the actual amplitude Fisher matrix uses the corresponding sine and cosine quadratures; the complex matrix is a useful conditioning diagnostic. If its smallest eigenvalue approaches zero, compensating amplitude changes leave the waveform nearly unchanged. Normalize the basis before quoting a condition number so that a rescaling of amplitudes is not mistaken for a loss of information.

A credible overtone claim should survive all of the following:

  • scan t0t_0, the end time, and peak-time uncertainty, transporting amplitudes to one reference time;
  • compare Kerr-tied, freely damped, prompt-response, and reduced-mode models;
  • vary noise estimation, calibration, gating, and the detector network;
  • use amplitude priors whose transformation with t0t_0 is stated;
  • demonstrate frequency–damping localization rather than only a nonzero constrained amplitude;
  • recover injected overtones and measure the false-positive rate on fundamental-only injections and off-source data;
  • test whether the same conclusion follows from independent implementations.

Residual compatibility with the assumed noise is necessary but not sufficient: a flexible wrong model can leave noise-like residuals, and an imperfect whitening filter can leave correlations even for a correct signal. Bayes factors are conditional on prior volume and the model list. When many start times and mode sets were examined, significance must include that search. Held-out predictions in colored noise must use the conditional noise distribution or a genuinely independent realization; simply dividing correlated samples does not make a validation set independent.

An overtone claim should identify which evidentiary rung it reaches and which diagnostic supports that rung. Moving upward requires new information; a larger Bayes factor for the same constrained model comparison does not automatically supply a frequency measurement or rule out an omitted competitor.

Evidentiary rungMinimum diagnosticWhat the diagnostic cannot establish by itself
ReconstructionResidual, mismatch, or remnant recovery improves on a declared time windowPredictive necessity in noisy data
Predictive necessityHeld-out prediction, calibrated model comparison, or injection recovery favors the added component after parameter costA unique quasinormal-mode label
Physical identificationFrequency and damping localize on one Kerr branch and remain stable under admissible start-time, noise, and competitor changesUniversality across events or waveform families
RobustnessOvertone-present, overtone-absent, and off-source trials measure recovery, coverage, and false identificationImmunity to competitors that were never tested

Numerical-relativity reconstruction supplies a clean example of the first rung Giesler et al. 2019, Figs. 1–5 and remnant-recovery analysis. A detector-data reanalysis that varies start time, noise realization, and amplitude assumptions tests the higher rungs instead Cotesta et al. 2022, start-time scan and injection study. The finite-window likelihood explains why these tests answer different questions Isi and Farr 2021, §§V–VII. These papers are methodological case studies here, not a current evidence ranking.

  1. Let τ0=10 ms\tau_0=10\ {\rm ms} and τ1=3 ms\tau_1=3\ {\rm ms}. At t0t_0, ∣A1/A0∣=4\lvert A_1/A_0\rvert=4. Find the ratio 8 ms8\ {\rm ms} later.
Solution

Each magnitude decays as e−Δt/τne^{-\Delta t/\tau_n}, so

∣A1(t0+Δt)A0(t0+Δt)∣=4exp⁡ ⁣[−Δt(1τ1−1τ0)].\left\lvert\frac{A_1(t_0+\Delta t)}{A_0(t_0+\Delta t)}\right\rvert = 4\exp\!\left[ -\Delta t\left(\frac{1}{\tau_1}-\frac{1}{\tau_0}\right) \right].

For Δt=8 ms\Delta t=8\ {\rm ms} this is

4e−8(1/3−1/10)=4e−28/15≃0.62.4e^{-8(1/3-1/10)} = 4e^{-28/15} \simeq 0.62.

The apparently dominant overtone at the early reference is already subdominant, illustrating why raw amplitudes at different start times cannot be compared.

  1. Two normalized basis functions have overlap (q0∣q1)=r(q_0\mid q_1)=r, with real 0≤r<10\leq r<1. Find the eigenvalues and condition number of their Gram matrix.
Solution

Here

G=(1rr1),\boldsymbol G= \begin{pmatrix} 1&r\\ r&1 \end{pmatrix},

whose eigenvalues are 1+r1+r and 1−r1-r. The spectral condition number is

κ(G)=1+r1−r.\kappa(G)=\frac{1+r}{1-r}.

It diverges as r→1r\to1, so the two amplitudes become unidentifiable even though their sum may fit the waveform accurately.

  • Cotesta, R., Carullo, G., Berti, E., and Cardoso, V. (2022). “Analysis of Ringdown Overtones in GW150914.” Physical Review Letters 129, 111102. DOI.
  • Giesler, M., Isi, M., Scheel, M. A., and Teukolsky, S. A. (2019). “Black Hole Ringdown: The Importance of Overtones.” Physical Review X 9, 041060. DOI.
  • Isi, M., and Farr, W. M. (2021). “Analyzing black-hole ringdowns.” arXiv:2107.05609.