Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
Pith reviewed 2026-05-18 10:03 UTC · model grok-4.3
The pith
A neural post-Einsteinian analysis of gravitational waves from GWTC-3 finds no significant deviation from general relativity.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
We report a test of general relativity (GR) with the third GW Transient Catalog (GWTC-3) plus a few O4 events using the recently developed neural post-Einsteinian framework, both on individual events and at the population level through hierarchical modeling. We find no significant violation of GR and place a constraint that, for the first time, efficiently covers non-GR theories characterized by not only post-Newtonian deviations but also those beyond under the same theory-agnostic framework.
What carries the argument
The neural post-Einsteinian framework, a method that uses neural networks to parameterize and map deviations from GR waveforms in a theory-agnostic manner.
If this is right
- Individual event analyses and population-level hierarchical modeling both support general relativity.
- Constraints are placed on non-GR theories that include both post-Newtonian and higher-order deviations.
- The framework provides efficient coverage of a broad class of alternative theories in one analysis.
- Data from additional O4 events can be incorporated into the same testing procedure.
Where Pith is reading between the lines
- This approach may enable more sensitive tests as gravitational wave catalogs grow with future detectors.
- Similar neural methods could be adapted to test other fundamental physics predictions in strong-field regimes.
- If deviations appear in larger datasets, the framework could help identify which modified gravity models are favored.
Load-bearing premise
The neural post-Einsteinian framework accurately maps the chosen set of deviation parameters onto the actual waveform morphology for the events in GWTC-3 without introducing uncontrolled systematics from the network architecture or training procedure.
What would settle it
A statistically significant non-zero value for the deviation parameters in a re-analysis of the same GWTC-3 events using an independent waveform model would falsify the no-violation conclusion.
Figures
read the original abstract
Gravitational waves (GWs) from compact binaries are excellent probes of gravity in the strong- and dynamical-field regimes. We report a test of general relativity (GR) with the third GW Transient Catalog (GWTC-3) plus a few O4 events using the recently developed neural post-Einsteinian framework, both on individual events and at the population level through hierarchical modeling. We find no significant violation of GR and place a constraint that, for the first time, efficiently covers non-GR theories characterized by not only post-Newtonian deviations but also those beyond under the same theory-agnostic framework.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper applies a neural post-Einsteinian framework to test general relativity using events from GWTC-3 together with a few O4 events. Analyses are performed both on individual events and at the population level via hierarchical modeling. The central claims are that no significant violation of GR is found and that the framework provides, for the first time, efficient joint constraints on non-GR theories that include both post-Newtonian deviations and those beyond the post-Newtonian regime under a single theory-agnostic setup.
Significance. If the neural mapping is shown to be free of uncontrolled systematics, the work would advance GW tests of gravity by enabling computationally efficient coverage of a wider range of deviations from GR, including beyond-PN effects, within one consistent analysis pipeline. The hierarchical population-level application is a notable strength if the underlying waveform mapping holds.
major comments (1)
- The headline result (no GR violation plus first efficient joint constraint on PN and beyond-PN deviations) requires that the neural network maps the chosen deviation parameters to actual waveform morphology for the GWTC-3 events without architecture- or training-induced systematics. This mapping is least secure for beyond-PN regimes. The manuscript does not demonstrate that recovered posteriors remain stable under changes to network depth, training distribution, or loss weighting, nor does it provide explicit cross-checks against known non-GR waveforms in the beyond-PN regime. This validation is load-bearing for the population constraints and the 'efficient coverage' claim in the abstract.
Simulated Author's Rebuttal
We thank the referee for their careful and constructive review. The major comment raises an important point about validation of the neural mapping, which we address directly below. We have revised the manuscript to incorporate additional robustness checks as suggested.
read point-by-point responses
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Referee: The headline result (no GR violation plus first efficient joint constraint on PN and beyond-PN deviations) requires that the neural network maps the chosen deviation parameters to actual waveform morphology for the GWTC-3 events without architecture- or training-induced systematics. This mapping is least secure for beyond-PN regimes. The manuscript does not demonstrate that recovered posteriors remain stable under changes to network depth, training distribution, or loss weighting, nor does it provide explicit cross-checks against known non-GR waveforms in the beyond-PN regime. This validation is load-bearing for the population constraints and the 'efficient coverage' claim in the abstract.
Authors: We agree that robust validation of the neural network mapping is essential, particularly in the beyond-PN regime where the mapping is less directly constrained by existing analytic results. The original manuscript included recovery tests on injected signals for a range of deviation parameters and demonstrated consistency with GR for the analyzed events. However, we acknowledge that explicit stability analyses under variations in network depth, training distribution, and loss weighting, together with direct cross-checks against known non-GR waveforms in the beyond-PN regime, were not presented in sufficient detail. We have added a new subsection in the methods and an appendix with these tests. The recovered posteriors remain stable within statistical uncertainties across the explored variations, and the cross-checks with beyond-PN injections confirm that the framework recovers the injected deviations without significant bias. These additions directly support the population-level constraints and the claim of efficient joint coverage. revision: yes
Circularity Check
No circularity: constraints derived from independent GW data analysis
full rationale
The paper applies the neural post-Einsteinian framework to GWTC-3 events for individual and hierarchical population inference, reporting no GR violation and joint constraints on PN and beyond-PN deviations. No load-bearing step reduces by construction to fitted inputs or self-citations; the framework is presented as a pre-developed tool whose mapping accuracy is taken as given for the analysis, with results driven by the catalog data rather than redefined within the derivation. The central claim remains falsifiable against the observed waveforms and does not rely on renaming or self-referential uniqueness theorems.
Axiom & Free-Parameter Ledger
axioms (1)
- domain assumption The neural post-Einsteinian parametrization spans the relevant space of non-GR theories for the events analyzed.
Lean theorems connected to this paper
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IndisputableMonolith/Foundation/RealityFromDistinction.leanreality_from_one_distinction unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
the npE dephasing model is constructed as δΨnpE(f; Ξ⃗ , ζ⃗ ) = ζb κ(Ξ⃗ , φ)ψ(Mf;φ)
What do these tags mean?
- matches
- The paper's claim is directly supported by a theorem in the formal canon.
- supports
- The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
- extends
- The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
- uses
- The paper appears to rely on the theorem as machinery.
- contradicts
- The paper's claim conflicts with a theorem or certificate in the canon.
- unclear
- Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.
Forward citations
Cited by 1 Pith paper
-
Beyond Three Terms: Continued Fractions for Rotating Black Holes in Modified Gravity
A reduction scheme transforms arbitrary N-term scalar and matrix recurrence relations from black hole perturbations in modified gravity into three-term relations solvable by continued fractions.
Reference graph
Works this paper leans on
-
[1]
C. M. Will, The Confrontation between General Rela- tivity and Experiment, Living Rev. Rel.17, 4 (2014), arXiv:1403.7377 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[2]
I. H. Stairs, Testing general relativity with pulsar timing, Living Rev. Rel.6, 5 (2003), arXiv:astro-ph/0307536
work page internal anchor Pith review Pith/arXiv arXiv 2003
-
[3]
Penrose, Gravitational collapse and space-time singu- larities, Phys
R. Penrose, Gravitational collapse and space-time singu- larities, Phys. Rev. Lett.14, 57 (1965)
work page 1965
-
[4]
J. M. M. Senovilla and D. Garfinkle, The 1965 Pen- rose singularity theorem, Class. Quant. Grav.32, 124008 (2015), arXiv:1410.5226 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 1965
-
[5]
A pedagogical explanation for the non-renormalizability of gravity
A. Shomer, A Pedagogical explanation for the non- renormalizability of gravity, (2007), arXiv:0709.3555 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv 2007
-
[6]
Rotation Curves of Spiral Galaxies
Y. Sofue and V. Rubin, Rotation curves of spiral galaxies, Ann. Rev. Astron. Astrophys.39, 137 (2001), arXiv:astro-ph/0010594
work page internal anchor Pith review Pith/arXiv arXiv 2001
-
[7]
G. Bertone and D. Hooper, History of dark matter, Rev. Mod. Phys.90, 045002 (2018), arXiv:1605.04909 [astro- ph.CO]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[8]
A. G. Riesset al.(Supernova Search Team), Observa- tional evidence from supernovae for an accelerating uni- verse and a cosmological constant, Astron. J.116, 1009 (1998), arXiv:astro-ph/9805201
work page internal anchor Pith review Pith/arXiv arXiv 1998
-
[9]
S. Perlmutteret al.(Supernova Cosmology Project), Measurements ofΩandΛfrom 42 High Redshift Su- pernovae, Astrophys. J.517, 565 (1999), arXiv:astro- ph/9812133
-
[10]
B. P. Abbottet al.(LIGO Scientific, Virgo), Observation of Gravitational Waves from a Binary Black Hole Merger, Phys. Rev. Lett.116, 061102 (2016), arXiv:1602.03837 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[11]
B.P.Abbottet al.(LIGOScientific, Virgo),BinaryBlack HoleMergersinthefirstAdvancedLIGOObservingRun, Phys. Rev. X6, 041015 (2016), [Erratum: Phys.Rev.X 8, 039903 (2018)], arXiv:1606.04856 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[12]
B. P. Abbottet al.(LIGO Scientific, Virgo), GWTC- 1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs, Phys. Rev. X9, 031040 (2019), arXiv:1811.12907 [astro-ph.HE]
work page internal anchor Pith review Pith/arXiv arXiv 2019
-
[13]
R. Abbottet al.(LIGO Scientific, Virgo), GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run, Phys. Rev. X11, 021053 (2021), arXiv:2010.14527 [gr- qc]
work page internal anchor Pith review Pith/arXiv arXiv 2021
-
[14]
R. Abbottet al.(LIGO Scientific, VIRGO), GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run, Phys. Rev. D109, 022001 (2024), arXiv:2108.01045 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2024
-
[15]
R. Abbottet al.(KAGRA, VIRGO, LIGO Scien- tific), GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run, Phys. Rev. X13, 041039 (2023), arXiv:2111.03606 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2023
- [16]
-
[17]
A. G. Abacet al.(LIGO Scientific, VIRGO, KA- GRA), GWTC-4.0: An Introduction to Version 4.0 of the Gravitational-Wave Transient Catalog, (2025), arXiv:2508.18080 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2025
-
[18]
A. G. Abacet al.(LIGO Scientific, VIRGO, KAGRA), GWTC-4.0: Updating the Gravitational-Wave Transient 6 Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run, (2025), arXiv:2508.18082 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2025
-
[19]
Extreme Gravity Tests with Gravitational Waves from Compact Binary Coalescences: (I) Inspiral-Merger
E. Berti, K. Yagi, and N. Yunes, Extreme Gravity Tests with Gravitational Waves from Compact Binary Coa- lescences: (I) Inspiral-Merger, Gen. Rel. Grav.50, 46 (2018), arXiv:1801.03208 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[20]
N.YunesandF.Pretorius,FundamentalTheoreticalBias in Gravitational Wave Astrophysics and the Parame- terized Post-Einsteinian Framework, Phys. Rev. D80, 122003 (2009), arXiv:0909.3328 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2009
-
[21]
Gravitational Wave Tests of General Relativity with the Parameterized Post-Einsteinian Framework
N. Cornish, L. Sampson, N. Yunes, and F. Pretorius, Gravitational Wave Tests of General Relativity with the Parameterized Post-Einsteinian Framework, Phys. Rev. D84, 062003 (2011), arXiv:1105.2088 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2011
-
[22]
K. Chatziioannou, N. Yunes, and N. Cornish, Model- Independent Test of General Relativity: An Extended post-Einsteinian Framework with Complete Polarization Content, Phys. Rev. D86, 022004 (2012), [Erratum: Phys.Rev.D 95, 129901 (2017)], arXiv:1204.2585 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2012
-
[23]
L. Sampson, N. Cornish, and N. Yunes, Gravita- tional Wave Tests of Strong Field General Relativity with Binary Inspirals: Realistic Injections and Opti- mal Model Selection, Phys. Rev. D87, 102001 (2013), arXiv:1303.1185 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2013
-
[24]
Theoretical Physics Implications of the Binary Black-Hole Mergers GW150914 and GW151226
N. Yunes, K. Yagi, and F. Pretorius, Theoretical Physics Implications of the Binary Black-Hole Mergers GW150914 and GW151226, Phys. Rev. D94, 084002 (2016), arXiv:1603.08955 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[25]
Parameterized Post- Einsteinian Gravitational Waveforms in Various Modified Theories of Gravity,
S. Tahura and K. Yagi, Parameterized Post-Einsteinian Gravitational Waveforms in Various Modified Theories of Gravity, Phys. Rev. D98, 084042 (2018), [Erratum: Phys.Rev.D 101, 109902 (2020)], arXiv:1809.00259 [gr- qc]
-
[26]
Gravitational-Radiation Damping of Compact Binary Systems to Second Post-Newtonian order
L.Blanchet, T.Damour, B.R.Iyer, C.M.Will,andA.G. Wiseman, Gravitational radiation damping of compact binary systems to second postNewtonian order, Phys. Rev. Lett.74, 3515 (1995), arXiv:gr-qc/9501027
work page internal anchor Pith review Pith/arXiv arXiv 1995
-
[27]
K. G. Arun, B. R. Iyer, M. S. S. Qusailah, and B. S. Sathyaprakash, Testing post-Newtonian theory with gravitational wave observations, Class. Quant. Grav.23, L37 (2006), arXiv:gr-qc/0604018
work page internal anchor Pith review Pith/arXiv arXiv 2006
-
[28]
C. K. Mishra, K. G. Arun, B. R. Iyer, and B. S. Sathyaprakash, Parametrized tests of post-Newtonian theory using Advanced LIGO and Einstein Telescope, Phys. Rev. D82, 064010 (2010), arXiv:1005.0304 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2010
-
[29]
T. G. F. Li, W. Del Pozzo, S. Vitale, C. Van Den Broeck, M. Agathos, J. Veitch, K. Grover, T. Sidery, R. Stu- rani, and A. Vecchio, Towards a generic test of the strong field dynamics of general relativity using com- pact binary coalescence, Phys. Rev. D85, 082003 (2012), arXiv:1110.0530 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2012
-
[30]
M. Agathos, W. Del Pozzo, T. G. F. Li, C. Van Den Broeck, J. Veitch, and S. Vitale, TIGER: A data analysis pipeline for testing the strong-field dynamics of general relativity with gravitational wave signals from coalescing compact binaries, Phys. Rev. D89, 082001 (2014), arXiv:1311.0420 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[31]
B. P. Abbottet al.(LIGO Scientific, Virgo), Tests of general relativity with GW150914, Phys. Rev. Lett.116, 221101 (2016), [Erratum: Phys.Rev.Lett. 121, 129902 (2018)], arXiv:1602.03841 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[32]
J. Meidamet al., Parametrized tests of the strong-field dynamics of general relativity using gravitational wave signalsfromcoalescingbinaryblackholes: Fastlikelihood calculations and sensitivity of the method, Phys. Rev. D 97, 044033 (2018), arXiv:1712.08772 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[33]
B.P.Abbottet al.(LIGOScientific, Virgo),TestsofGen- eral Relativity with GW170817, Phys. Rev. Lett.123, 011102 (2019), arXiv:1811.00364 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2019
-
[34]
B. P. Abbottet al.(LIGO Scientific, Virgo), Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1, Phys. Rev. D 100, 104036 (2019), arXiv:1903.04467 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2019
-
[35]
R.Abbottet al.(LIGOScientific, Virgo),Testsofgeneral relativity with binary black holes from the second LIGO- Virgo gravitational-wave transient catalog, Phys. Rev. D 103, 122002 (2021), arXiv:2010.14529 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2021
-
[36]
Tests of General Relativity with GWTC-3
R. Abbottet al.(LIGO Scientific, VIRGO, KAGRA), Tests of General Relativity with GWTC-3, (2021), arXiv:2112.06861 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2021
- [37]
- [38]
- [39]
- [40]
- [41]
-
[42]
R. R. Metsaev and A. A. Tseytlin, Curvature Cubed Terms in String Theory Effective Actions, Phys. Lett. B185, 52 (1987)
work page 1987
- [43]
-
[44]
Chern-Simons Modification of General Relativity
R. Jackiw and S. Y. Pi, Chern-Simons modification of general relativity, Phys. Rev. D68, 104012 (2003), arXiv:gr-qc/0308071
work page internal anchor Pith review Pith/arXiv arXiv 2003
-
[45]
Chern-Simons Modified General Relativity
S. Alexander and N. Yunes, Chern-Simons Modi- fied General Relativity, Phys. Rept.480, 1 (2009), arXiv:0907.2562 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv 2009
-
[46]
K. Schumacher, S. E. Perkins, A. Shaw, K. Yagi, and N. Yunes, Gravitational wave constraints on Einstein- æther theory with LIGO/Virgo data, Phys. Rev. D108, 104053 (2023), arXiv:2304.06801 [gr-qc]
- [47]
-
[48]
Gravitational radiation from compact binary systems in the massive Brans-Dicke theory of gravity
J. Alsing, E. Berti, C. M. Will, and H. Zaglauer, Grav- itational radiation from compact binary systems in the massive Brans-Dicke theory of gravity, Phys. Rev. D85, 064041 (2012), arXiv:1112.4903 [gr-qc]. 7
work page internal anchor Pith review Pith/arXiv arXiv 2012
-
[49]
Light scalar field constraints from gravitational-wave observations of compact binaries
E. Berti, L. Gualtieri, M. Horbatsch, and J. Alsing, Light scalar field constraints from gravitational-wave obser- vations of compact binaries, Phys. Rev. D85, 122005 (2012), arXiv:1204.4340 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2012
- [50]
- [51]
-
[52]
Hidden-Sector Modifications to Gravitational Waves From Binary Inspirals
S. Alexander, E. McDonough, R. Sims, and N. Yunes, Hidden-Sector Modifications to Gravitational Waves From Binary Inspirals, Class. Quant. Grav.35, 235012 (2018), arXiv:1808.05286 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2018
- [53]
-
[54]
Mis-Modelling in Gravitational Wave Astronomy: The Trouble With Templates
L. Sampson, N. Cornish, and N. Yunes, Mismodeling in gravitational-wave astronomy: The trouble with tem- plates, Phys. Rev. D89, 064037 (2014), arXiv:1311.4898 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2014
- [55]
-
[56]
D. P. Kingma and M. Welling, Auto-Encoding Varia- tional Bayes, (2013), arXiv:1312.6114 [stat.ML]
work page internal anchor Pith review Pith/arXiv arXiv 2013
-
[57]
Gravity with a dynamical preferred frame
T. Jacobson and D. Mattingly, Gravity with a dynam- ical preferred frame, Phys. Rev. D64, 024028 (2001), arXiv:gr-qc/0007031
work page internal anchor Pith review Pith/arXiv arXiv 2001
-
[58]
Einstein-aether gravity: a status report
T. Jacobson, Einstein-aether gravity: A Status report, PoSQG-PH, 020 (2007), arXiv:0801.1547 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2007
-
[59]
D. Blas, O. Pujolas, and S. Sibiryakov, Consistent Ex- tension of Horava Gravity, Phys. Rev. Lett.104, 181302 (2010), arXiv:0909.3525 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv 2010
-
[60]
D. Blas, O. Pujolas, and S. Sibiryakov, Models of non- relativistic quantum gravity: The Good, the bad and the healthy, JHEP04, 018, arXiv:1007.3503 [hep-th]
work page internal anchor Pith review Pith/arXiv arXiv
-
[61]
Constraining non-commutative space-time from GW150914
A. Kobakhidze, C. Lagger, and A. Manning, Constrain- ing noncommutative spacetime from GW150914, Phys. Rev. D94, 064033 (2016), arXiv:1607.03776 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[62]
P. A. M. Dirac, The Cosmological constants, Nature139, 323 (1937)
work page 1937
-
[63]
Constraining the evolutionary history of Newton's constant with gravitational wave observations
N. Yunes, F. Pretorius, and D. Spergel, Constraining the evolutionary history of Newton’s constant with grav- itational wave observations, Phys. Rev. D81, 064018 (2010), arXiv:0912.2724 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2010
- [64]
-
[65]
S. Mezzasoma and N. Yunes, Theory-agnostic frame- work for inspiral tests of general relativity with higher- harmonic gravitational waves, Phys. Rev. D106, 024026 (2022), arXiv:2203.15934 [gr-qc]
-
[66]
Projected Constraints on Scalarization with Gravitational Waves from Neutron Star Binaries
L. Sampson, N. Yunes, N. Cornish, M. Ponce, E. Ba- rausse, A. Klein, C. Palenzuela, and L. Lehner, Projected Constraints on Scalarization with Gravitational Waves from Neutron Star Binaries, Phys. Rev. D90, 124091 (2014), arXiv:1407.7038 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[67]
B. P. Abbottet al.(KAGRA, LIGO Scientific, Virgo), Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA, Living Rev. Rel.19, 1 (2016), arXiv:1304.0670 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[68]
Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo
R. Abbottet al.(LIGO Scientific, Virgo), Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo, SoftwareX13, 100658 (2021), arXiv:1912.11716 [gr-qc]
work page internal anchor Pith review arXiv 2021
-
[69]
Open data from the third observing run of LIGO, Virgo, KAGRA and GEO
R. Abbottet al.(KAGRA, VIRGO, LIGO Scientific), Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO, Astrophys. J. Suppl.267, 29 (2023), arXiv:2302.03676 [gr-qc]
work page internal anchor Pith review arXiv 2023
-
[70]
A simple model of complete precessing black-hole-binary gravitational waveforms
M. Hannam, P. Schmidt, A. Bohé, L. Haegel, S. Husa, F. Ohme, G. Pratten, and M. Pürrer, Simple Model of Complete Precessing Black-Hole-Binary Gravitational Waveforms, Phys. Rev. Lett.113, 151101 (2014), arXiv:1308.3271 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2014
-
[71]
S. Husa, S. Khan, M. Hannam, M. Pürrer, F. Ohme, X. Jiménez Forteza, and A. Bohé, Frequency-domain gravitational waves from nonprecessing black-hole bina- ries. I. New numerical waveforms and anatomy of the sig- nal, Phys. Rev. D93, 044006 (2016), arXiv:1508.07250 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[72]
S. Khan, S. Husa, M. Hannam, F. Ohme, M. Pür- rer, X. Jiménez Forteza, and A. Bohé, Frequency- domain gravitational waves from nonprecessing black- hole binaries. II. A phenomenological model for the ad- vanced detector era, Phys. Rev. D93, 044007 (2016), arXiv:1508.07253 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[73]
Abbottet al.(LIGO Scientific, Virgo), Phys
R. Abbottet al.(LIGO Scientific, Virgo), GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses, Phys. Rev. D102, 043015 (2020), arXiv:2004.08342 [astro-ph.HE]
-
[74]
G. Prattenet al., Computationally efficient models for the dominant and subdominant harmonic modes of pre- cessing binary black holes, Phys. Rev. D103, 104056 (2021), arXiv:2004.06503 [gr-qc]
work page internal anchor Pith review Pith/arXiv arXiv 2021
-
[75]
G. Pratten, S. Husa, C. Garcia-Quiros, M. Colleoni, A. Ramos-Buades, H. Estelles, and R. Jaume, Setting the cornerstone for a family of models for gravitational waves from compact binaries: The dominant harmonic for nonprecessing quasicircular black holes, Phys. Rev. D 102, 064001 (2020), arXiv:2001.11412 [gr-qc]
-
[76]
C. García-Quirós, M. Colleoni, S. Husa, H. Estel- lés, G. Pratten, A. Ramos-Buades, M. Mateu-Lucena, and R. Jaume, Multimode frequency-domain model for the gravitational wave signal from nonprecessing black-hole binaries, Phys. Rev. D102, 064002 (2020), arXiv:2001.10914 [gr-qc]
-
[77]
Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy
G. Ashtonet al., BILBY: A user-friendly Bayesian infer- encelibraryforgravitational-waveastronomy,Astrophys. J. Suppl.241, 27 (2019), arXiv:1811.02042 [astro-ph.IM]
work page internal anchor Pith review Pith/arXiv arXiv 2019
-
[78]
J. S. Speagle, dynesty: a dynamic nested sampling package for estimating Bayesian posteriors and evi- dences, Mon. Not. Roy. Astron. Soc.493, 3132 (2020), arXiv:1904.02180 [astro-ph.IM]
work page internal anchor Pith review Pith/arXiv arXiv 2020
-
[79]
P. A. R. Adeet al.(Planck), Planck 2015 results. XIII. Cosmological parameters, Astron. Astrophys.594, A13 (2016), arXiv:1502.01589 [astro-ph.CO]
work page internal anchor Pith review Pith/arXiv arXiv 2015
- [80]
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