Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Probing the nuclear equation of state from the existence of a $\sim 2.6~M_{\odot}$ neutron star: the GW190814 puzzle
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2012.09580.
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 2026-08-06T15:00:23.830215Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T08:37:46.398464Z
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 493451b6-7239-475d-9431-a0709c75d8b3 · inbound
Mass-Gap Neutron Stars from Vector \texorpdfstring{$f(R)$}{f(R)} Gravity Inflationary Deformations cites this paper.
Mass-Gap Neutron Stars from Vector \texorpdfstring{$f(R)$}{f(R)} Gravity Inflationary Deformations Probing the nuclear equation of state from the existence of a $\sim 2.6~M_{\odot}$ neutron star: the GW190814 puzzle
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:00:23.830215Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5ceecc7e-596e-4bf3-b243-dff93afe2f37 · inbound
General gravitational properties of neutron stars: curvature invariants, binding energy, and trace anomaly cites this paper.
General gravitational properties of neutron stars: curvature invariants, binding energy, and trace anomaly Probing the nuclear equation of state from the existence of a $\sim 2.6~M_{\odot}$ neutron star: the GW190814 puzzle
Reference 16
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T14:48:00.682827Z
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 1e8452b0-2992-4d3e-a4d8-0556905df83f · inbound
Neutron stars with primary scalar hair cites this paper.
Neutron stars with primary scalar hair Probing the nuclear equation of state from the existence of a $\sim 2.6~M_{\odot}$ neutron star: the GW190814 puzzle
Reference 6
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-03T08:37:46.399892Z
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.