Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1905.00014.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T10:10:48.432957Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T14:28:12.473372Z
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 b6cf29a2-7a3e-4f89-a299-445662af1a5d · inbound
Constraints on maximum neutron star mass from proto-neutron star evolution cites this paper.
Constraints on maximum neutron star mass from proto-neutron star evolution Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities
Reference 34
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T14:28:12.534979Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 5f8bef76-1fa3-4920-b11e-6ba117b47181 · inbound
On the Nucleon Effective Mass in Neutron Stars Cooling cites this paper.
On the Nucleon Effective Mass in Neutron Stars Cooling Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:06:07.598968Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 859fb60d-e572-4906-a0a2-da85b3a3defa · inbound
Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects cites this paper.
Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T10:10:48.432957Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.