Paper Citation Record · LEDGER

Gravitational-wave energy flux for compact binaries through second order in the mass ratio

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 20 inbound Pith citation observations for arXiv:2107.01298.

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

pith.paper-citation-record.v1
2107.01298 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 20 of 20 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 20 of 20 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T20:30:53.741061Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T18:50:05.316238Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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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 0c39f4d4-bda7-464e-b4e3-4e0262e2908d · 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 Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 5

Resolution: verified exact; arxiv_id, observed 2026-05-23T23:18:35.924622Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 3dfd5a8b-4214-4124-9a2d-676c4fc14b13 · inbound

Actions of spinning compact binaries: Spinning particle in Kerr matched to dynamics at 1.5 post-Newtonian order cites this paper.

Actions of spinning compact binaries: Spinning particle in Kerr matched to dynamics at 1.5 post-Newtonian order Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-12T20:30:53.741061Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8493e0a2-2bd3-4db9-88c4-8b77ec1621bd · inbound

Environmental effects in extreme mass ratio inspirals: perturbations to the environment in Kerr cites this paper.

Environmental effects in extreme mass ratio inspirals: perturbations to the environment in Kerr Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 123

Resolution: unresolved; no resolver link, observed 2026-08-10T19:46:47.734272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8111bd5-8997-4357-89c6-f105cdf7a868 · inbound

Extreme mass-ratio inspiral within an ultralight scalar cloud I. Scalar radiation cites this paper.

Extreme mass-ratio inspiral within an ultralight scalar cloud I. Scalar radiation Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-06T21:02:47.610740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0750c5a4-07d5-4b6d-bc3e-3e2d84307fa1 · inbound

A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments cites this paper.

A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 42

Resolution: verified exact; arxiv_id, observed 2026-05-19T05:52:59.429285Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation fb74a2c0-2606-4b89-ad6b-e7583dc87bd2 · 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 Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 108

Resolution: unresolved; no resolver link, observed 2026-08-06T18:34:53.453983Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2314d8dd-689c-4bd7-9533-d3c341ec21d8 · inbound

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

Black hole mergers beyond general relativity: a self-force approach Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 87

Resolution: verified exact; arxiv_id, observed 2026-05-18T07:16:02.577629Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation ab020343-2ff8-46f7-949d-118eb835f93b · 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 Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-18T05:55:57.330550Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 5ab0c754-28b0-4e23-8120-e48d3c31e3ea · 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 Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-03T03:14:27.543238Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c7de917-9f37-4d96-975d-ed34c3da9e87 · 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 Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-03T02:30:55.879296Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 35e03653-1cb3-49c1-91a5-3231f654b05c · inbound

All-order structure of static gravitational interactions and the seventh post-Newtonian potential cites this paper.

All-order structure of static gravitational interactions and the seventh post-Newtonian potential Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 78

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T11:41:02.862926Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 5ea32bd2-0aef-4e7f-9317-645cbc4dfcef · inbound

Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework cites this paper.

Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-12T03:06:19.091708Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 6ce25d76-7bf8-4c8c-a7fc-29b800370bf3 · inbound

Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework cites this paper.

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-13T07:47:32.114617Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation b72a1ea5-293c-4bfb-af3c-51836d4366a1 · inbound

Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework cites this paper.

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-07-01T13:35:45.519814Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 1aaf3493-c768-4e57-979b-c7eb079e8f47 · inbound

Eccentric and unbound compact binaries in the LIGO-Virgo-KAGRA catalog: parameter estimation and waveform systematics with SEOBNRv6EHM cites this paper.

Eccentric and unbound compact binaries in the LIGO-Virgo-KAGRA catalog: parameter estimation and waveform systematics with SEOBNRv6EHM Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 115

Resolution: verified exact; arxiv_id, observed 2026-06-29T11:13:21.902604Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 8ee47353-f740-41d8-9563-d43e539b8fe9 · inbound

Weak-field waveforms for generic relativistic orbits cites this paper.

Weak-field waveforms for generic relativistic orbits Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 72

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:27:44.793012Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 85f961c3-c136-440b-81d9-68864391b664 · inbound

The Bondi--Sachs gauge, BMS frames, and memory in black hole perturbation theory cites this paper.

The Bondi--Sachs gauge, BMS frames, and memory in black hole perturbation theory Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 57

Resolution: verified exact; arxiv_id, observed 2026-07-04T18:50:05.318089Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation ee578098-54a0-4ed1-b624-8623bdd96ca1 · 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 Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 53

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b467ea53-7797-4f28-aa03-653b01956168 · inbound

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-04T21:28:07.693883Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation edd17185-d7d3-41df-a14b-d3384f7c026d · inbound

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms cites this paper.

High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms Gravitational-wave energy flux for compact binaries through second order in the mass ratio

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-07T00:15:14.372058Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.