Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Do we need dense matter equation of state in curved spacetime for neutron stars?
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2206.02106.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T23:33:53.056304Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-16T19:28:20.564886Z
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 b6165d3b-4a8b-4874-a258-641209909da1 · inbound
Transport coefficients of dense nucleon matter at low temperature cites this paper.
Transport coefficients of dense nucleon matter at low temperature Do we need dense matter equation of state in curved spacetime for neutron stars?
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T23:33:53.056304Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 87428b75-93fe-406f-9768-174b2a5ca99f · inbound
Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis cites this paper.
Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Do we need dense matter equation of state in curved spacetime for neutron stars?
Reference 79
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T14:01:08.906947Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 41853132-75bd-4bec-b1cc-92793272712b · inbound
Fermi-liquid view of viscosity in cold and dense nucleon matter cites this paper.
Fermi-liquid view of viscosity in cold and dense nucleon matter Do we need dense matter equation of state in curved spacetime for neutron stars?
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T19:21:36.117528Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 06169756-a0e7-4f8c-a768-47fe78d595d6 · inbound
Impact of Anisotropy on Neutron Star Structure and Curvature cites this paper.
Impact of Anisotropy on Neutron Star Structure and Curvature Do we need dense matter equation of state in curved spacetime for neutron stars?
Reference 32
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T19:28:20.566776Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.