Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Neutron stars in $f(\mathcal{R,T})$ gravity using realistic equations of state in the light of massive pulsars and GW170817
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2009.04696.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T15:00:25.277943Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-12T07:37:10.906232Z
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 dbd53fe5-08f4-4249-83b1-15d33b5113fb · 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 Neutron stars in $f(\mathcal{R,T})$ gravity using realistic equations of state in the light of massive pulsars and GW170817
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:00:25.277943Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 01417350-f0cf-4562-8124-4e59e1fbc0c4 · inbound
Neutron stars in a conservative $f(R,T)$ gravity cites this paper.
Neutron stars in a conservative $f(R,T)$ gravity Neutron stars in $f(\mathcal{R,T})$ gravity using realistic equations of state in the light of massive pulsars and GW170817
Reference 49
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T07:37:10.970300Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.