Paper Citation Record · LEDGER

Comparing second-order gravitational self-force and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2406.04108.

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

pith.paper-citation-record.v1
2406.04108 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T10:52:51.063433Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T16:24:58.748180Z

Reference resolution

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 88626890-e2de-432d-9fdd-fe191c71010c · inbound

Comparing effective-one-body and Mathisson-Papapetrou-Dixon results for a spinning test particle on circular equatorial orbits around a Kerr black hole cites this paper.

Comparing effective-one-body and Mathisson-Papapetrou-Dixon results for a spinning test particle on circular equatorial orbits around a Kerr black hole Comparing second-order gravitational self-force and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-11T10:52:51.063433Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e8ab646-83a2-4095-9fcb-71ab1f6255f3 · inbound

The error budget of binary neutron star merger simulations for configurations with high spin cites this paper.

The error budget of binary neutron star merger simulations for configurations with high spin Comparing second-order gravitational self-force and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Reference 200

Resolution: unresolved; no resolver link, observed 2026-08-07T11:41:16.218123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd7c0fda-f563-4aa5-b2a9-3a195589faaf · 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 and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Reference 65

Resolution: verified exact; arxiv_id, observed 2026-05-18T05:55:56.972138Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 668c3415-5c1c-4287-a2e5-efba92d9cb61 · 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 and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-03T03:14:27.557026Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 22e57993-f47f-4983-9cdd-3e3c63124c37 · 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 and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Reference 114

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 ca9bf6fd-0763-4b4e-a2db-aeb3985aeffc · 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 and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-03T02:30:56.606126Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd33fcc9-91a8-4d8c-ae35-fdc06abfe1ec · 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 and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Reference 109

Resolution: verified exact; arxiv_id, observed 2026-06-30T09:04:32.395321Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation a38d76c7-20a4-40b0-883a-932252551017 · inbound

Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations cites this paper.

Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations Comparing second-order gravitational self-force and effective-one-body waveforms from inspiralling, quasi-circular black hole binaries with a non-spinning primary and a spinning secondary

Reference 162

Resolution: verified exact; arxiv_id, observed 2026-06-30T16:24:58.751530Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.