Paper Citation Record · LEDGER

Surface tension and curvature energy of quark matter in the NJL model

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1308.1452.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1308.1452 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:29:00.610565Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-05-25T01:55:12.623484Z

Reference resolution

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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 db028698-953d-4231-990b-c2e81262a818 · inbound

Phase transitions in neutron stars and their links to gravitational waves cites this paper.

Phase transitions in neutron stars and their links to gravitational waves Surface tension and curvature energy of quark matter in the NJL model

Reference 130

Resolution: verified exact; local_arxiv, observed 2026-05-25T01:55:12.625996Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 46e8a920-112a-4f0b-b6bc-923689a01104 · inbound

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity cites this paper.

Simulating Binary Neutron Stars with Hybrid Equation of States: Gravitational Waves, Electromagnetic Signatures, and Challenges for Numerical Relativity Surface tension and curvature energy of quark matter in the NJL model

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-14T14:29:00.610565Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b82ac27-c3da-46ce-9792-f0e09e951a0f · inbound

Probing up-down quark matter via gravitational waves cites this paper.

Probing up-down quark matter via gravitational waves Surface tension and curvature energy of quark matter in the NJL model

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-14T10:56:12.255312Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6f2e2de-3ea2-4a06-a175-62e997fc3456 · inbound

Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons cites this paper.

Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons Surface tension and curvature energy of quark matter in the NJL model

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-11T14:29:01.196733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5e69b3e2-cc1d-4007-a5dc-289b8afebc59 · inbound

The equation of state for neutron stars cites this paper.

The equation of state for neutron stars Surface tension and curvature energy of quark matter in the NJL model

Reference 115

Resolution: unresolved; no resolver link, observed 2026-08-01T19:22:14.813080Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.