Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Thin accretion disk around a rotating Kerr-like black hole in Einstein-bumblebee gravity model
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1910.13259.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T20:10:46.017391Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T09:21:02.099363Z
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 b9f2b075-5eaa-4d9a-b522-93470cebbe8d · inbound
Spherical photon orbits around the Kerr-like black hole in Einstein-Bumblebee gravity cites this paper.
Spherical photon orbits around the Kerr-like black hole in Einstein-Bumblebee gravity Thin accretion disk around a rotating Kerr-like black hole in Einstein-bumblebee gravity model
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T20:10:46.017391Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5381b9af-3a39-4cbe-b320-e2dad5df951f · inbound
Boson Stars in Bumblebee Gravity and Their Gravitational Waveforms from Extreme-Mass-Ratio Inspirals cites this paper.
Boson Stars in Bumblebee Gravity and Their Gravitational Waveforms from Extreme-Mass-Ratio Inspirals Thin accretion disk around a rotating Kerr-like black hole in Einstein-bumblebee gravity model
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T14:50:41.004896Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9d5ecb0f-687c-47ff-ac42-7f9a636028f5 · inbound
Strong gravitational lensing and Quasiperiodic oscillations as a probe for an electrically charged Lorentz symmetry-violating black hole cites this paper.
Strong gravitational lensing and Quasiperiodic oscillations as a probe for an electrically charged Lorentz symmetry-violating black hole Thin accretion disk around a rotating Kerr-like black hole in Einstein-bumblebee gravity model
Reference 31
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T09:21:02.101463Z
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 b4b08aba-aa2e-4a9f-9eed-8dae2c3c944c · inbound
How does nonmetricity shape quantum emission from rotating bumblebee black holes? cites this paper.
How does nonmetricity shape quantum emission from rotating bumblebee black holes? Thin accretion disk around a rotating Kerr-like black hole in Einstein-bumblebee gravity model
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T00:19:46.452120Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 98485cdc-11b3-4ace-897c-4b703e4aa59b · inbound
Signatures of Lorentz violation in bright ring for Sgr A* images by radiation ineffective accretion flows cites this paper.
Signatures of Lorentz violation in bright ring for Sgr A* images by radiation ineffective accretion flows Thin accretion disk around a rotating Kerr-like black hole in Einstein-bumblebee gravity model
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T00:18:31.044900Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.