Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Curvature of the energy per particle in neutron stars
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2311.13401.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T13:16:52.060473Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T11:19:50.476743Z
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 d0a1f96d-a68b-4958-b587-64183ec21daf · inbound
Observables and conformal properties of dark matter admixed isentropic neutron stars cites this paper.
Observables and conformal properties of dark matter admixed isentropic neutron stars Curvature of the energy per particle in neutron stars
Reference 66
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T11:19:50.478377Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 1bcb1503-0a72-48e8-9a8c-fdd4a22f4f62 · inbound
Can average speed of sound and thermodynamic response functions signal the exotic phases in neutron star cores? cites this paper.
Can average speed of sound and thermodynamic response functions signal the exotic phases in neutron star cores? Curvature of the energy per particle in neutron stars
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T05:52:28.674753Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dcc75ce4-9f15-45d2-8c0f-0cb05bd5ae9f · inbound
Quarkyonic Stars with Strangeness cites this paper.
Quarkyonic Stars with Strangeness Curvature of the energy per particle in neutron stars
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T13:16:52.060473Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.