Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Turbulence modelling in neutron star merger simulations
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2402.03224.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T01:02:19.972782Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T18:50:04.506602Z
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 ad11e7f1-0fbc-4cda-a81b-e228b49fc1f3 · inbound
Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning cites this paper.
Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning Turbulence modelling in neutron star merger simulations
Reference 17
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T07:29:39.507727Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation b1500020-d80e-45be-ae0b-62071b258af5 · inbound
Beyond the Tayler instability: A new global instability of toroidal magnetic fields in stars cites this paper.
Beyond the Tayler instability: A new global instability of toroidal magnetic fields in stars Turbulence modelling in neutron star merger simulations
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T18:50:04.507897Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 9308a066-6b6d-4c55-b51b-ab730fe003c1 · inbound
SPH methods in the modelling of compact objects cites this paper.
SPH methods in the modelling of compact objects Turbulence modelling in neutron star merger simulations
Reference 153
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T01:02:19.972782Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c83d5ddc-aa2a-4636-b077-ba279d852ace · inbound
Transport Properties of the MRI in Differentially Rotating Neutron Stars cites this paper.
Transport Properties of the MRI in Differentially Rotating Neutron Stars Turbulence modelling in neutron star merger simulations
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T14:28:12.811823Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.