Paper Citation Record · LEDGER

Magnetar formation through a convective dynamo in protoneutron stars

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2003.06662.

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

pith.paper-citation-record.v1
2003.06662 v1

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 2026-08-07T06:34:17.273281+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T13:05:40.023970Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T03:55:54.287348Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 6b2ea1f1-26e2-43f2-aa82-21b901d7cf03 · inbound

Impact of rotation on the accretion of entropy perturbations in collapsing massive stars cites this paper.

Impact of rotation on the accretion of entropy perturbations in collapsing massive stars Magnetar formation through a convective dynamo in protoneutron stars

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-04T19:19:17.768192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42b42683-f6e2-4131-82da-2901d30bb242 · inbound

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves cites this paper.

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves Magnetar formation through a convective dynamo in protoneutron stars

Reference 98

Resolution: unresolved; no resolver link, observed 2026-07-13T16:48:58.103396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation abe7701f-c27a-4c24-832f-245094cb6bf5 · inbound

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves cites this paper.

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves Magnetar formation through a convective dynamo in protoneutron stars

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-04T05:43:33.144601Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 18aecf58-45bf-4113-97dd-15cfd216da68 · inbound

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

Magnetar field dynamics driven by chiral anomalies without magnetic helicity Magnetar formation through a convective dynamo in protoneutron stars

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-05-11T03:55:54.289190Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 057a14c7-9099-4e23-9742-e3c839df58dc · inbound

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

Transport Properties of the MRI in Differentially Rotating Neutron Stars Magnetar formation through a convective dynamo in protoneutron stars

Reference 27

Resolution: unresolved; no resolver link, observed 2026-07-31T14:28:12.643503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 347e518a-76d2-4d80-878e-a93ae0df623f · inbound

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

3D simulations of a complete convective silicon shell burning phase Magnetar formation through a convective dynamo in protoneutron stars

Reference 293

Resolution: unresolved; no resolver link, observed 2026-08-06T13:05:40.023970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.