Paper Citation Record · LEDGER

Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2208.01049.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2208.01049 v2

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measured 0 of 0 reference resolution

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measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:35:06.198582Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-07-02T10:06:51.850583Z

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Outbound references

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Pith citing papers

Observation 51daa0fc-5fe3-46a9-aa76-0982460168e0 · inbound

Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries cites this paper.

Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-23T23:18:35.882436Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 99df600c-ea3c-41f0-be70-1b0d411ca44a · inbound

Self-force framework for merger-ringdown waveforms cites this paper.

Self-force framework for merger-ringdown waveforms Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:06.198582Z

Source-reported events for the cited work

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Observation 35a60444-0e7b-43b0-ae0f-e0669e79d103 · inbound

Post-adiabatic dynamics and waveform generation in self-force theory: an invariant pseudo-Hamiltonian framework cites this paper.

Post-adiabatic dynamics and waveform generation in self-force theory: an invariant pseudo-Hamiltonian framework Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-06T18:34:53.383781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d05aadc-5d7c-4b5f-8f0f-cdf36b94396d · inbound

Perturbations of Plane Waves and Quadratic Quasinormal Modes on the Lightring cites this paper.

Perturbations of Plane Waves and Quadratic Quasinormal Modes on the Lightring Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-05T10:55:29.762216Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9446db49-2fca-4242-aa57-80bd7fa24059 · inbound

Black hole mergers beyond general relativity: a self-force approach cites this paper.

Black hole mergers beyond general relativity: a self-force approach Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 91

Resolution: verified exact; arxiv_id, observed 2026-05-18T07:16:02.267062Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation ca06c06a-fcd8-4278-a5f5-230deffd3166 · inbound

Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary cites this paper.

Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 40

Resolution: verified exact; arxiv_id, observed 2026-05-18T05:55:57.379329Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation d96d9d4a-aa7b-4224-94b5-6f2e3b017437 · inbound

From the confluent Heun equation to a new factorized and resummed gravitational waveform for circularized, nonspinning, compact binaries cites this paper.

From the confluent Heun equation to a new factorized and resummed gravitational waveform for circularized, nonspinning, compact binaries Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-03T03:14:27.548733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1eb8bd85-0d21-44bb-93fa-f684da34efae · inbound

Advancing the Effective-One-Body Framework in the Test-Mass Limit cites this paper.

Advancing the Effective-One-Body Framework in the Test-Mass Limit Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 109

Resolution: unresolved; no resolver link, observed 2026-07-15T14:26:35.666160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0279ca89-4b48-45b3-adb2-cfc18698bd66 · inbound

Secular evolution of orbital parameters for general bound orbits in Kerr spacetime cites this paper.

Secular evolution of orbital parameters for general bound orbits in Kerr spacetime Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-03T02:30:56.361932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 168c7376-3b9f-48c6-99df-661b4a8d60f5 · inbound

Self-force calculations with numerical relativity methods cites this paper.

Self-force calculations with numerical relativity methods Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 37

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:06:51.851926Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation e2a4b2da-6901-4c83-abd2-931ed5d5f345 · inbound

Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries cites this paper.

Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 104

Resolution: verified exact; arxiv_id, observed 2026-06-30T08:54:29.938151Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation ac3c9ac1-8217-4ab5-be99-255e9a7d26a9 · inbound

The significance of first post-adiabatic contributions for scalar charge measurements with intermediate and extreme mass ratio inspirals cites this paper.

The significance of first post-adiabatic contributions for scalar charge measurements with intermediate and extreme mass ratio inspirals Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries

Reference 56

Resolution: unresolved; no resolver link, observed 2026-07-13T03:59:32.375823Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.