Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Plausible presence of new state in neutron stars with masses above $0.98M_{\rm TOV}$
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2207.13613.
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 2026-08-10T23:31:06.085593Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T23:37:27.286484Z
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 c1f53236-44f9-4a8c-85f0-ec447acf4e3d · inbound
Stiffening of matter in quark-hadron continuity: a mini-review cites this paper.
Stiffening of matter in quark-hadron continuity: a mini-review Plausible presence of new state in neutron stars with masses above $0.98M_{\rm TOV}$
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T23:31:06.085593Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7b2b13b1-9305-4db1-9e27-649dd35968e1 · inbound
The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover cites this paper.
The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover Plausible presence of new state in neutron stars with masses above $0.98M_{\rm TOV}$
Reference 25
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T08:21:25.604374Z
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 0fef8ef6-9989-42fe-b5a9-0dd9fa9d659b · inbound
The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover cites this paper.
The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover Plausible presence of new state in neutron stars with masses above $0.98M_{\rm TOV}$
Reference 31
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T13:15:46.552654Z
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 e249f406-6e65-405b-a7a3-3270bacea2bf · inbound
Post-Merger Gravitational-Wave Uncertainties of Binary Neutron Stars under Multi-Messenger EOS Constraints cites this paper.
Post-Merger Gravitational-Wave Uncertainties of Binary Neutron Stars under Multi-Messenger EOS Constraints Plausible presence of new state in neutron stars with masses above $0.98M_{\rm TOV}$
Reference 24
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T23:37:27.287860Z
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 8a7e7750-232f-4b4e-8f83-773aba86b0ab · inbound
Post-Merger Gravitational-Wave Uncertainties of Binary Neutron Stars under Multi-Messenger EOS Constraints cites this paper.
Post-Merger Gravitational-Wave Uncertainties of Binary Neutron Stars under Multi-Messenger EOS Constraints Plausible presence of new state in neutron stars with masses above $0.98M_{\rm TOV}$
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T02:13:51.953642Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ed1575ee-b03d-4e7c-b749-6a897d21c9ff · inbound
Quarkyonic Stars with Strangeness cites this paper.
Quarkyonic Stars with Strangeness Plausible presence of new state in neutron stars with masses above $0.98M_{\rm TOV}$
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T13:16:51.826933Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.