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Paper Citation Record · LEDGER

Revealing the high-density equation of state through binary neutron star mergers

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1403.5301.

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

pith.paper-citation-record.v1
1403.5301 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:29:00.728049Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T15:27:05.841284Z

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 6e31b725-10b2-44d0-8b2a-8aaadf4e8421 · 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 Revealing the high-density equation of state through binary neutron star mergers

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-14T14:29:00.728049Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:29:00.728049Z digest=sha256:b8fdd0a7efcce6951519cc5c53962f9f77fe103a49dc5c906fd39a75f673daf9

Observation c2bff34b-8903-4f93-95ad-4f04cceffef3 · inbound

kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter cites this paper.

kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter Revealing the high-density equation of state through binary neutron star mergers

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-14T10:20:11.583037Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:20:11.583037Z digest=sha256:fa645d7ba07e2ee1496658592da72c621dfe9af980bd0f98366cff18ec10e929

Observation a1e66916-285d-4c70-be8e-4c237b97a8a6 · inbound

Radial Oscillations of Viscous Stars at Finite Temperature cites this paper.

Radial Oscillations of Viscous Stars at Finite Temperature Revealing the high-density equation of state through binary neutron star mergers

Reference 15

Resolution
verified exact
local_arxiv, observed 2026-07-02T15:27:05.843992Z

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.

source=pdf_text observed=2026-06-27T23:50:16.954566Z digest=sha256:54e7e986eff6a692608e66c388114392ea44d1cf59485a59e35f39ff1d1df864