Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Unifying the dark sector through a single matter fluid with non-zero pressure
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2308.15776.
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 2026-08-06T12:47:16.770021Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T12:47:16.883417Z
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 ce134b9a-bf46-4eba-b180-611bb93659ad · inbound
Bondi accretion disk luminosity around neutral and charged Simpson-Visser spacetimes cites this paper.
Bondi accretion disk luminosity around neutral and charged Simpson-Visser spacetimes Unifying the dark sector through a single matter fluid with non-zero pressure
Reference 76
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T12:47:16.886343Z
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.
Observation 3c864707-4c85-4e6e-93fe-96872063c592 · inbound
BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.
BAO miscalibration cannot rescue late-time solutions to the Hubble tension Unifying the dark sector through a single matter fluid with non-zero pressure
Reference 286
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T12:53:56.809036Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1ca13ffc-deb8-4f69-a0ed-62243e1eae7e · inbound
Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.
Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Unifying the dark sector through a single matter fluid with non-zero pressure
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T00:32:09.659215Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.