Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Mass-Radius relation for Neutron Stars in $f(R)$ gravity
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1509.04163.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T12:00:47.543625Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-20T04:23:03.757118Z
Reference resolution
0 of 0 outbound references displayed
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- malformed identifier0
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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 4184aba3-8604-428f-af6f-678ebc9c619d · inbound
An innovative black hole solution and thermodynamic properties in higher-order curvature gravity with a scalar field cites this paper.
An innovative black hole solution and thermodynamic properties in higher-order curvature gravity with a scalar field The Mass-Radius relation for Neutron Stars in $f(R)$ gravity
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T12:00:47.543625Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 162f3831-9ec6-4e3f-93b2-e19daff380e0 · inbound
Neutron stars in a conservative $f(R,T)$ gravity cites this paper.
Neutron stars in a conservative $f(R,T)$ gravity The Mass-Radius relation for Neutron Stars in $f(R)$ gravity
Reference 18
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T07:37:11.609778Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation a524ab32-2dc9-4fa2-8a96-d539c4813944 · inbound
Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability cites this paper.
Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability The Mass-Radius relation for Neutron Stars in $f(R)$ gravity
Reference 38
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T04:23:03.760269Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 23adb114-5a22-4c2b-9b56-869756a920de · inbound
Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability cites this paper.
Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability The Mass-Radius relation for Neutron Stars in $f(R)$ gravity
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T13:44:09.352267Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e39acd5c-4e49-488d-93df-60e7281f9290 · inbound
Gravitational wave echoes as probes of the maximum mass of strange stars in quadratic curvature-matter coupled gravity cites this paper.
Gravitational wave echoes as probes of the maximum mass of strange stars in quadratic curvature-matter coupled gravity The Mass-Radius relation for Neutron Stars in $f(R)$ gravity
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T12:55:54.524093Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.