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Gravitational Waves from Inspiralling Compact Binaries: A Post-Newtonian Approach

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Clifford M. WILL

General Relativity and Quantum Cosmology · Submitted 17 Mar 1994

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim This paper discusses the foundations of this method, and provides a compendium of useful formulae and results.

how it is stated · asserted 0.98 read the record →

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arXiv IDgr-qc/9403033 (version 1)
Pith IDSNPBGPGZ, Pith's permanent record of this paper and its review
CitationClifford M. Will. "Gravitational Waves from Inspiralling Compact Binaries: A Post-Newtonian Approach." arXiv:gr-qc/9403033 (1994). https://pith.science/paper/SNPBGPGZ
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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,957 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.02 · states limitation 0.48 · human participants 0.02 · controlled comparison 0.01 · randomized assignment 0.01 · states quantitative result 0.04 · compares with prior results 0.05 · mentions code or data availability 0.15.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

Inspiralling binary systems of neutron stars or black holes are promising sources of gravitational radiation detectable by large-scale laser interferometric gravitational observatories, such as the US LIGO and Italian-French VIRGO projects. Accurate theoretical gravitational-waveform templates will be needed to carry out matched filtering data analysis of the detectors' output once they are on the air by the end of this decade. For all but the final, strongly general relativistic coalescence of the two bodies, high-order post-Newtonian methods are playing a major role in the theorists' efforts to develop the needed templates. This paper discusses the foundations of this method, and provides a compendium of useful formulae and results. Figures available upon request. (Invited talk given at the 8th Nishinomiya-Yukawa Memorial Symposium, October 28, 1993.)

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Inspiralling binary systems of neutron stars or black holes are promising sources of gravitational radiation detectable by large-scale laser interferometric gravitational observatories, such as the US LIGO and Italian-French VIRGO projects. background 1.00 0.05 0.05 asserted 0.59
s1 Accurate theoretical gravitational-waveform templates will be needed to carry out matched filtering data analysis of the detectors' output once they are on the air by the end of this decade. background 0.89 0.05 0.04 asserted 0.90
s2 For all but the final, strongly general relativistic coalescence of the two bodies, high-order post-Newtonian methods are playing a major role in the theorists' efforts to develop the needed templates. background 0.81 0.07 0.06 asserted 1.00
s3 This paper discusses the foundations of this method, and provides a compendium of useful formulae and results. contribution 1.00 0.76 0.14 asserted 0.98
s4 Figures available upon request. limitation 0.94 0.09 0.01 asserted 0.59
s5 (Invited talk given at the 8th Nishinomiya-Yukawa Memorial Symposium, October 28, 1993.) background 0.98 0.21 0.01 asserted 0.52

What kind of paper the classifier reports this is: review 0.92 · evidence from proof or derivation 0.79.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

Inspiralling binary systems of neutron stars or black holes are promising sources of gravitational radiation detectable by large-scale laser interferometric gravitational observatories, such as the US LIGO and Italian-French VIRGO projects. Accurate theoretical gravitational-waveform templates will be needed to carry out matched filtering data analysis of the detectors' output once they are on the air by the end of this decade. For all but the final, strongly general relativistic coalescence of the two bodies, high-order post-Newtonian methods are playing a major role in the theorists' efforts to develop the needed templates. This paper discusses the foundations of this method, and provides a compendium of useful formulae and results. Figures available upon request. (Invited talk given at the 8th Nishinomiya-Yukawa Memorial Symposium, October 28, 1993.)

Human review

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References
How the literature uses it

2 arXiv papers cite this in 2 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 1 sentence without a confident label

Cites it as background 1 paper
  • For reviews on analytic approximations and applications to the motion and the gravitational wave-generation see Refs. [ref] .

    Post-Newtonian Theory for Gravitational Waves · Analytic approximations and wave generation formalism · 0.98

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