Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Can the post-Newtonian gravitational waveform of an inspiraling binary be improved by solving the energy balance equation numerically?
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:gr-qc/9912075.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T13:07:36.998643Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-19T05:52:07.222430Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 7cf512cd-9297-4cec-baa6-79ea5502f47b · inbound
Probing the existence of a minimal length through compact binary inspiral cites this paper.
Probing the existence of a minimal length through compact binary inspiral Can the post-Newtonian gravitational waveform of an inspiraling binary be improved by solving the energy balance equation numerically?
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T13:07:36.998643Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 19cfb63a-60f7-4488-ac43-675cf37c3072 · inbound
Tidal effects in the total flux and waveform in massless scalar-tensor theories to, respectively, relative 2PN and 1.5PN orders cites this paper.
Tidal effects in the total flux and waveform in massless scalar-tensor theories to, respectively, relative 2PN and 1.5PN orders Can the post-Newtonian gravitational waveform of an inspiraling binary be improved by solving the energy balance equation numerically?
Reference 34
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T05:52:07.225130Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.