Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Inspecting neutrino flavor instabilities during proto-neutron star cooling phase in supernova: I. Spherically symmetric model
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2407.20548.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T14:59:00.114909Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T14:59:04.147586Z
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 6e6a7e64-a6e3-4c74-a7ae-72782a287dfc · inbound
Predicting the outcome of collisional neutrino flavor conversion cites this paper.
Predicting the outcome of collisional neutrino flavor conversion Inspecting neutrino flavor instabilities during proto-neutron star cooling phase in supernova: I. Spherically symmetric model
Reference 57
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T14:59:04.273830Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.
Observation 58cafe47-f35d-4dff-92bc-b9ff911a633f · inbound
Approximate Energy-Integration Method for Identifying Collisional Neutrino Flavor Instabilities cites this paper.
Approximate Energy-Integration Method for Identifying Collisional Neutrino Flavor Instabilities Inspecting neutrino flavor instabilities during proto-neutron star cooling phase in supernova: I. Spherically symmetric model
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T14:38:02.703338Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.