{"arxiv_id":"gr-qc/0604067","incoming":{"papers":55,"sentences":76,"groups":[{"kind":"extends","label":"Builds on it","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2408.14132","title":"Parametrized tests of general relativity using eccentric compact binaries","url":"/paper/2408.14132","section":"Summary and conclusions","sentence":"The first method is an extension of the standard null parametrized test of GR for quasicircular binaries [ref] .","intent_p":0.97,"contests_p":null}]},{"kind":"method_or_tool","label":"Uses its method or tool","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1302.2198","title":"Tests of General Relativity and Alternative theories of gravity using Gravitational Wave observations","url":"/paper/1302.2198","section":"Bayesian Inference and Tests of Gravity","sentence":"In these works they used the proposal of Ref. [ref] (described earlier) to test the PN coefficients of GR recasting it using Bayesian model selection.","intent_p":0.89,"contests_p":null},{"arxiv_id":"2311.08446","title":"Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves","url":"/paper/2311.08446","section":"Introduction","sentence":"For instance, here we deploy the parameterized tests of post-Newtonian (PN) coefficients which are designed to be sensitive to physical effects manifesting at different PN orders [ref] , and analytical phenomenological coefficients to model the intermediate and merger-ringdown regimes [ref] .","intent_p":0.92,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":27,"sentences":28,"quotes":[{"arxiv_id":"2402.15110","title":"A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits","url":"/paper/2402.15110","section":"Introduction","sentence":"* A model-agnostic residuals test, which subtracts out the best-matched GR-modeled CBC waveform from the data containing the GW signal, and checks if the statistical properties of the residual are consistent with noise [ref] * A test that probes the inspiral evolution of the CBC by searching for deviations in Post-Newtonian (PN) parameters of the GW signal [ref] * An inspiral-merger-ringdown consistency test (IMRCT) that compares and assesses the consistency between the low and high-frequency portions of the CBC signals [ref] * Propagation tests of GWs that compare their speed with respect to the speed of light [ref] as well as any modulations in the waveform due to finite-graviton-mass-driven velocity dispersion [ref] .","intent_p":0.94,"contests_p":null},{"arxiv_id":"2408.14132","title":"Parametrized tests of general relativity using eccentric compact binaries","url":"/paper/2408.14132","section":"Parametrized tests of GR for circular binaries","sentence":"In parametrized tests with circular binaries [ref] , the GR waveform is modified by adding phenomenological deviation parameters at each PN order that capture potential deviations from GR: $φ_i φ_i (1 + δφ̂_i)$.","intent_p":0.9,"contests_p":null},{"arxiv_id":"1207.4759","title":"Testing general relativity with gravitational waves: a reality check","url":"/paper/1207.4759","section":"Introduction and main results","sentence":"In the second class of tests, GR is tested for self-consistency by treating some of the coefficients in the post-Newtonian (PN) expansion of the phasing as free variables rather than deterministic functions of the source parameters, and verifying whether the recovered values are consistent with GR predictions [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"1410.8815","title":"Supermassive Black Hole Tests of General Relativity with eLISA","url":"/paper/1410.8815","section":"Introduction","sentence":"Among such are tests that introduce perturbations to the PN coefficients of the GR inspiral waveform [ref] ; similarly, the ringdown part of the waveform can be checked [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"2604.08680","title":"Prompt Response from Plunging Sources in Schwarzschild Spacetime","url":"/paper/2604.08680","section":"Introduction","sentence":"Over the past decades, post-Newtonian theory [ref] and black hole (BH) perturbation theory [ref] have been developed to describe the early inspiral [ref] and late ringdown [ref] stage, thereby forming the theoretical foundation for waveform modeling and for parameterizing deviations from General Relativity [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":45},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/gr-qc/0604067"}}