Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Nuclear matter symmetry energy and the neutron skin thickness of heavy nuclei
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:nucl-th/0509009.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T17:11:13.158229Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T08:30:57.825532Z
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 2ff5b27d-e6c7-4600-bedb-29c610f9d3b4 · inbound
Extended Skyrme effective interactions with higher-order momentum-dependence for transport models and neutron stars cites this paper.
Extended Skyrme effective interactions with higher-order momentum-dependence for transport models and neutron stars Nuclear matter symmetry energy and the neutron skin thickness of heavy nuclei
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T17:11:13.158229Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d5600ce8-feaa-4a3b-b18d-ab46abe99879 · inbound
Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models cites this paper.
Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models Nuclear matter symmetry energy and the neutron skin thickness of heavy nuclei
Reference 51
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T16:56:58.962913Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.