Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2407.18739.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T10:10:48.437906Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T10:11:15.575445Z
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 c4175281-6737-4521-8c32-1d403140bfc8 · inbound
Impact of Effective Nucleon Mass and Multineutron States on the Equation of State for Core-Collapse Supernovae cites this paper.
Impact of Effective Nucleon Mass and Multineutron States on the Equation of State for Core-Collapse Supernovae Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars
Reference 7
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T10:11:15.657376Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation e05915fa-0c24-493d-9dcc-3c18abe2b561 · inbound
On the Nucleon Effective Mass in Neutron Stars Cooling cites this paper.
On the Nucleon Effective Mass in Neutron Stars Cooling Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T00:06:07.708214Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 191392c5-bab0-42f7-9eb7-ee8cbb5288f8 · 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 Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T10:10:48.437906Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.