Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Can Two Ultrarelativistic Objects Lose Almost All Their Energy to Gravitational Radiation?
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2212.03890.
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 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T13:07:29.308663Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-12T09:06:27.068177Z
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 d220fef2-63cd-4c72-a67d-da581951703d · inbound
QCD-Gravity double copy in Regge asymptotics: from $2\rightarrow n$ amplitudes to radiation in shockwave collisions cites this paper.
QCD-Gravity double copy in Regge asymptotics: from $2\rightarrow n$ amplitudes to radiation in shockwave collisions Can Two Ultrarelativistic Objects Lose Almost All Their Energy to Gravitational Radiation?
Reference 276
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T13:07:29.308663Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c6766afb-f919-4702-ae1c-449332a26751 · inbound
Trapping, Irregular Waveforms, and Efficient Radiation in Ultra-relativistic Black Hole Encounters cites this paper.
Trapping, Irregular Waveforms, and Efficient Radiation in Ultra-relativistic Black Hole Encounters Can Two Ultrarelativistic Objects Lose Almost All Their Energy to Gravitational Radiation?
Reference 13
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T09:06:27.071262Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.