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arxiv: 2603.19019 · v1 · submitted 2026-03-19 · 🌀 gr-qc · astro-ph.HE

Recognition: 2 theorem links

· Lean Theorem

GWTC-4.0: Tests of General Relativity. I. Overview and General Tests

The LIGO Scientific Collaboration , the Virgo Collaboration , the KAGRA Collaboration: A. G. Abac , I. Abouelfettouh , F. Acernese , K. Ackley , C. Adamcewicz , S. Adhicary
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Sharma Chaudhary P. Shawhan N. S. Shcheblanov E. Sheridan Z.-H. Shi M. Shikauchi R. Shimomura H. Shinkai S. Shirke D. H. Shoemaker D. M. Shoemaker R. W. Short S. ShyamSundar A. Sider H. Siegel D. Sigg L. Silenzi L. Silvestri M. Simmonds L. P. Singer Amitesh Singh Anika Singh D. Singh M. K. Singh N. Singh S. Singh A. M. Sintes V. Sipala V. Skliris B. J. J. Slagmolen D. A. Slater T. J. Slaven-Blair J. Smetana J. R. Smith L. Smith R. J. E. Smith W. J. Smith S. Soares de Albuquerque Filho M. Soares-Santos K. Somiya I. Song S. Soni V. Sordini F. Sorrentino H. Sotani F. Spada V. Spagnuolo A. P. Spencer P. Spinicelli A. K. Srivastava F. Stachurski C. J. Stark D. A. Steer J. Steinhoff N. Steinle J. Steinlechner S. Steinlechner N. Stergioulas P. Stevens M. StPierre M. D. Strong A. Strunk A. L. Stuver M. Suchenek S. Sudhagar Y. Sudo N. Sueltmann L. Suleiman K. D. Sullivan J. Sun L. Sun S. Sunil J. Suresh B. J. Sutton P. J. Sutton K. Suzuki M. Suzuki S. Swain B. L. Swinkels A. Syx M. J. 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H. Wang Y. F. Wang G. Waratkar J. Warner M. Was T. Washimi N. Y. Washington D. Watarai B. Weaver S. A. Webster N. L. Weickhardt M. Weinert A. J. Weinstein R. Weiss L. Wen K. Wette J. T. Whelan B. F. Whiting C. Whittle E. G. Wickens D. Wilken A. T. Wilkin B. M. Williams D. Williams M. J. Williams N. S. Williams J. L. Willis B. Willke M. Wils L. Wilson C. W. Winborn J. Winterflood C. C. Wipf G. Woan J. Woehler N. E. Wolfe H. T. Wong I. C. F. Wong K. Wong T. Wouters J. L. Wright M. Wright B. Wu C. Wu D. S. Wu H. Wu K. Wu Q. Wu Y. Wu Z. Wu E. Wuchner D. M. Wysocki V. A. Xu Y. Xu N. Yadav H. Yamamoto K. Yamamoto T. S. Yamamoto T. Yamamoto R. Yamazaki T. Yan K. Z. Yang Y. Yang Z. Yarbrough J. Yebana S.-W. Yeh A. B. Yelikar X. Yin J. Yokoyama T. Yokozawa S. Yuan H. Yuzurihara M. Zanolin M. Zeeshan T. Zelenova J.-P. Zendri M. Zeoli M. Zerrad M. Zevin L. Zhang N. Zhang R. Zhang T. Zhang C. Zhao J. Zhao Yue Zhao Yuhang Zhao Z.-C. Zhao Y. Zheng H. Zhong H. Zhou H. O. Zhu Z.-H. Zhu A. B. Zimmerman L. Zimmermann M. E. Zucker J. Zweizig
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Pith reviewed 2026-05-16 01:39 UTC · model grok-4.3

classification 🌀 gr-qc astro-ph.HE
keywords gravitational wavesgeneral relativity testsLIGOVirgoKAGRAbinary mergersGWTC-4.0
0
0 comments X

The pith

The 91 gravitational-wave events in GWTC-4.0 are consistent with general relativity.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This overview paper analyzes 91 confident signals from compact binary coalescences detected by the LIGO-Virgo-KAGRA network through the first part of O4. It conducts four general tests of consistency with general relativity on the waveforms. These include checking that the residuals after subtracting the best-fit GR waveform match the expected noise, that the final mass and spin parameters agree when estimated from the inspiral and ringdown portions separately, that the amplitudes of higher multipole moments follow GR predictions, and that the signals show no evidence of non-GR polarization states. No deviations are found in any of these tests for the selected events.

Core claim

For all 91 events, the gravitational-wave data are consistent with general relativity. The residuals match noise, low- and high-frequency inferences of final mass and spin agree, subdominant multipoles have the expected amplitudes, and polarization modes are consistent with GR expectations. Therefore, these observations remain compatible with vacuum general relativity without additional physics.

What carries the argument

A set of four consistency tests: residual analysis against noise, inspiral-merger-ringdown parameter consistency, subdominant multipole amplitude verification, and polarization mode checks.

If this is right

  • GR waveform models accurately describe the observed signals without systematic mismatches.
  • The catalog shows no signs of new physics in the strong-field regime for these binaries.
  • Similar tests on future events can continue to probe for deviations at higher precision.
  • The results guide the application of more specific tests in companion papers.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Any modifications to gravity beyond general relativity must produce effects too small to detect in these events or at scales not yet probed.
  • Independent waveform models could be used to cross-check the assumption that deviations would be visible.
  • Higher sensitivity in future runs might allow detection of subtle deviations if they exist.
  • These findings align with the idea that general relativity is sufficient for modeling current gravitational-wave observations.

Load-bearing premise

The models of general relativity waveforms are sufficiently accurate that any real deviation from general relativity would produce a detectable inconsistency in one of the tested quantities.

What would settle it

A clear mismatch between the low- and high-frequency estimates of final mass or spin in a single high-quality event, or a residual signal exceeding noise expectations, would falsify the claim of consistency.

read the original abstract

The worldwide LIGO-Virgo-KAGRA network of gravitational-wave (GW) detectors continues to increase in sensitivity, thus increasing the quantity and quality of the detected GW signals from compact binary coalescences. These signals allow us to perform ever-more sensitive tests of general relativity (GR) in the dynamical and strong-field regime of gravity. This paper is the first of three, where we present the results of a suite of tests of GR using the binary signals included in the fourth GW Transient Catalog (GWTC-4.0), i.e., up to and including the first part of the fourth observing run of the detectors (O4a). We restrict our analysis to the 91 confident signals, henceforth called events, that were measured by at least two detectors, and have false alarm rates $\le 10^{-3} \mathrm{yr}^{-1}$. These include 42 events from O4a. This first paper presents an overview of the methods, selection of events and GR tests, and serves as a guidemap for all three papers. Here we focus on the four general tests of consistency, where we find no evidence for deviations from our models. Specifically, for all the events considered, we find consistency of the residuals with noise. The final mass and final spin as inferred from the low- and high-frequency parts of the waveform are consistent with each other. We also find no evidence for deviations from the GR predictions for the amplitudes of subdominant GW multipole moments, or for non-GR modes of polarization. We thus find that GR, without new physics beyond it, is still consistent with these GW events. The results of the two additional papers in this trio also find overall consistency with vacuum GR, with more than 90% of the events being consistent with GR at the 90% credible level. While one of the ringdown analyses finds the GR value in the tails for its combined results, this may be due in part to catalog variance.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

1 major / 2 minor

Summary. The manuscript is the first of three papers presenting tests of general relativity (GR) with the 91 confident binary coalescence events in GWTC-4.0 (including 42 from O4a). It provides an overview of event selection, methods, and four general consistency tests: (i) residuals consistent with noise, (ii) final mass and spin inferred from low- versus high-frequency waveform segments, (iii) amplitudes of subdominant multipoles, and (iv) polarization content. The central claim is that all four tests show no evidence for deviations from GR, so that GR remains consistent with the catalog.

Significance. If the results hold after addressing model systematics, the work supplies a statistically powerful, multi-test consistency check of GR in the strong-field dynamical regime using the largest GW catalog to date. The explicit separation into general tests (this paper) and more targeted analyses (companion papers) is a clear organizational strength, and the use of a well-defined, multi-detector event set with FAR ≤ 10^{-3} yr^{-1} improves reproducibility.

major comments (1)
  1. [§4] §4 (General Tests): The four consistency tests are performed exclusively by comparing data to GR waveform templates. The manuscript does not quantify the magnitude of possible systematic errors in those templates (particularly in the merger-ringdown regime for the 42 O4a events) relative to the reported statistical uncertainties, leaving open whether a true deviation could be absorbed or a spurious inconsistency created.
minor comments (2)
  1. [Abstract] Abstract: The statement that 'more than 90% of the events [are] consistent with GR at the 90% credible level' refers to results in the companion papers; a single sentence directing readers to those papers would improve clarity.
  2. [§2] §2 (Event Selection): The precise definition of the 'confident signals' cut and any associated selection biases on the sensitivity of the four tests are only summarized; a short table or explicit list of the 91 events with their SNR and FAR values would aid readers.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for their careful and constructive review of our manuscript. We agree that a quantitative assessment of waveform model systematics is essential to strengthen the interpretation of the consistency tests. We will revise the manuscript to address this point directly.

read point-by-point responses
  1. Referee: [§4] §4 (General Tests): The four consistency tests are performed exclusively by comparing data to GR waveform templates. The manuscript does not quantify the magnitude of possible systematic errors in those templates (particularly in the merger-ringdown regime for the 42 O4a events) relative to the reported statistical uncertainties, leaving open whether a true deviation could be absorbed or a spurious inconsistency created.

    Authors: We thank the referee for raising this important issue. The four tests rely on comparisons to GR waveform models (primarily IMRPhenomXPHM and SEOBNRv4PHM), which have been validated against numerical relativity. Prior studies indicate that modeling errors are typically smaller than the statistical uncertainties for the GWTC-4.0 events. However, to directly address the concern, we will add a dedicated subsection to §4 that quantifies the impact of waveform systematics. This will include: (i) results from alternative waveform families, (ii) estimates of merger-ringdown modeling errors drawn from NR comparisons, and (iii) a direct comparison of these systematic magnitudes to the reported statistical uncertainties, with emphasis on the 42 O4a events. We expect this addition to confirm that the observed consistencies are robust and not artifacts of template inaccuracies. revision: yes

Circularity Check

0 steps flagged

No significant circularity; consistency tests are direct statistical comparisons to GR templates

full rationale

The paper reports four general tests (residuals vs noise, low/high-frequency final mass/spin consistency, subdominant multipole amplitudes, polarization content) performed by comparing observed GW data to standard GR waveform models. These are empirical mismatch statistics and parameter-consistency checks; the reported overall consistency with GR does not reduce by construction to quantities fitted from the same data, nor does it rely on self-citation chains, uniqueness theorems, or ansatzes smuggled from prior work. The central claim is a catalog-level statistical result whose validity rests on external waveform-model accuracy (an assumption, not a circular derivation). No load-bearing step equates a prediction to its own input.

Axiom & Free-Parameter Ledger

0 free parameters · 2 axioms · 0 invented entities

The central claim rests on standard assumptions of GR waveform modeling and detector noise characterization; no new free parameters or invented entities are introduced in the overview.

axioms (2)
  • domain assumption GR waveform models accurately represent the expected signals from compact binary coalescences.
    Invoked when subtracting best-fit waveforms to form residuals and when comparing inferred final mass and spin.
  • domain assumption Any deviation from GR would produce detectable mismatches in at least one of the four tested quantities.
    Underlies the interpretation that passing the tests supports GR.

pith-pipeline@v0.9.0 · 15754 in / 1332 out tokens · 181594 ms · 2026-05-16T01:39:04.038860+00:00 · methodology

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