Paper Citation Record · LEDGER

A global model of the magnetorotational instability in protoneutron stars

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2005.03567.

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

pith.paper-citation-record.v1
2005.03567 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:05:12.246961Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T03:55:54.251661Z

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 45ee6657-0a75-4883-9c8e-676da22030bf · inbound

Self-consistent scenario for jet and stellar explosion in collapsar: General relativistic magnetohydrodynamics simulation with dynamo cites this paper.

Self-consistent scenario for jet and stellar explosion in collapsar: General relativistic magnetohydrodynamics simulation with dynamo A global model of the magnetorotational instability in protoneutron stars

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-09T13:31:50.282363Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 92a04711-7a36-40ce-9ddb-979c32fbdfa5 · inbound

Magnetar field dynamics driven by chiral anomalies without magnetic helicity cites this paper.

Magnetar field dynamics driven by chiral anomalies without magnetic helicity A global model of the magnetorotational instability in protoneutron stars

Reference 14

Resolution: verified exact; arxiv_id, observed 2026-05-11T03:55:54.253570Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 67724d19-29a0-481d-a32e-16920901abc0 · inbound

Transport of angular momentum and chemical elements by the MRI dynamo in stellar radiative zones cites this paper.

Transport of angular momentum and chemical elements by the MRI dynamo in stellar radiative zones A global model of the magnetorotational instability in protoneutron stars

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-01T08:39:51.693582Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0fc42a11-41eb-49c7-aa38-31eea0f87f17 · inbound

Transport Properties of the MRI in Differentially Rotating Neutron Stars cites this paper.

Transport Properties of the MRI in Differentially Rotating Neutron Stars A global model of the magnetorotational instability in protoneutron stars

Reference 26

Resolution: unresolved; no resolver link, observed 2026-07-31T14:28:12.637204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7240c6d3-9dda-4e58-9921-9510c6196e58 · inbound

Structural quasi-universality in highly magnetized differentially rotating neutron stars cites this paper.

Structural quasi-universality in highly magnetized differentially rotating neutron stars A global model of the magnetorotational instability in protoneutron stars

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-15T15:05:12.246961Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dc77b0d3-8aab-4c6e-bb56-91411c38ef27 · inbound

3D simulations of a complete convective silicon shell burning phase cites this paper.

3D simulations of a complete convective silicon shell burning phase A global model of the magnetorotational instability in protoneutron stars

Reference 294

Resolution: unresolved; no resolver link, observed 2026-08-06T13:05:40.026691Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.