Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2107.06804.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T00:09:05.593487Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T16:19:57.046774Z
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 3c358ca5-0c21-4d7e-b163-7e6cc1b706e1 · inbound
Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers cites this paper.
Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
Reference 113
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T21:29:52.897487Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8d329019-11d7-4840-8425-9dd965133093 · inbound
TTE-CAM: Self-Explainable Class Activation Maps for Pretrained Black-Box CNNs cites this paper.
TTE-CAM: Self-Explainable Class Activation Maps for Pretrained Black-Box CNNs Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
Reference 55
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T17:23:25.842886Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ac78cae1-2d3a-46d8-9343-2ea17bc5d98e · inbound
A magnetar formation in binary neutron star merger cites this paper.
A magnetar formation in binary neutron star merger Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
Reference 79
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T07:37:45.066155Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 55edaf14-e354-440c-b930-43ecb839fd5f · inbound
Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine cites this paper.
Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
Reference 80
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T16:19:57.048411Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation e2ef3e4d-8d56-4185-90bb-cf8aed0dadac · inbound
From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State cites this paper.
From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T00:43:19.441566Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ccdc7ea5-b051-45fe-94bb-252cc786ac52 · inbound
How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition cites this paper.
How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Impact of the nuclear symmetry energy on the post-merger phase of a binary neutron star coalescence
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:09:05.593487Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.