Paper Citation Record · LEDGER

Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2009.06669.

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

pith.paper-citation-record.v1
2009.06669 v1

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 2026-08-11T06:34:44.6726+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T15:52:56.828512Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T07:39:38.291026Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
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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 842ea84d-6107-49a7-93ae-3d8bdff65e42 · inbound

General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars cites this paper.

General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations

Reference 7

Resolution: verified exact; arxiv_id, observed 2026-05-09T04:41:38.011306Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 5ed4a085-3716-4dc0-8ff9-20d335041518 · inbound

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta cites this paper.

Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations

Reference 126

Resolution: unresolved; no resolver link, observed 2026-08-05T15:52:56.828512Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ee1550c6-ae70-48c6-9dc6-cd3be6da8c49 · inbound

Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field cites this paper.

Magnetic effects on fundamental modes in rotating neutron stars with a purely toroidal magnetic field Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-04T18:11:07.710084Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a023fee-c7f5-4e30-b945-a52397172477 · inbound

A magnetar formation in binary neutron star merger cites this paper.

A magnetar formation in binary neutron star merger Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations

Reference 137

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:37:45.166929Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation bc26cd18-c83f-4a01-bd5c-52396a3dbe4f · inbound

Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning cites this paper.

Subgrid Modelling for Relativistic Magnetohydrodynamics with Machine Learning Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations

Reference 94

Resolution: verified exact; arxiv_id, observed 2026-07-04T07:39:38.292704Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.