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Paper Citation Record · LEDGER

Evolution of neutron star magnetic fields

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2109.05584.

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

pith.paper-citation-record.v1
2109.05584 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 2026-08-17T06:30:58.91139+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T14:26:40.681527Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T20:55:04.837192Z

Reference resolution

0 of 0 outbound references displayed

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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 9674a105-74d0-4f5c-80e1-e6c14f67aa93 · inbound

Evidence for the spin-kick alignment of pulsars from the statistics of their magnetic inclinations cites this paper.

Evidence for the spin-kick alignment of pulsars from the statistics of their magnetic inclinations Evolution of neutron star magnetic fields

Reference 351

Resolution
unresolved
no resolver link, observed 2026-08-11T14:26:40.681527Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T14:26:40.681527Z digest=sha256:7ef247d2ca3563f200837c8f75fef96fdce94742212943c382b424f2b3991367

Observation 32295fef-0da5-4f81-be42-80d41720a526 · inbound

Transport coefficients of dense nucleon matter at low temperature cites this paper.

Transport coefficients of dense nucleon matter at low temperature Evolution of neutron star magnetic fields

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-10T23:33:52.940074Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:33:52.940074Z digest=sha256:bfba8e6325ce408c6ee45eaa2ca22e5d485b1227b76341c5ad60f1d31da91307

Observation cd1e4eff-a2f3-411c-963f-3b34263d9cbd · inbound

Screening rho-meson mass in the presence of strong magnetic fields cites this paper.

Screening rho-meson mass in the presence of strong magnetic fields Evolution of neutron star magnetic fields

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-08T11:06:14.399719Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T11:06:14.399719Z digest=sha256:c53126efd6a50867f84c080816e2f35662ec8921fe4ef7689235e74d4a1d655b

Observation 4f6b1bdf-1815-4221-a660-b92c725a374b · inbound

On Ultra-long Period (53.8 min) Pulsar ASKAP J1935+2148: Coherent Radio Emission Triggered by Local Superstrong Magnetic Reconnection cites this paper.

On Ultra-long Period (53.8 min) Pulsar ASKAP J1935+2148: Coherent Radio Emission Triggered by Local Superstrong Magnetic Reconnection Evolution of neutron star magnetic fields

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-05T15:37:35.654362Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T15:37:35.654362Z digest=sha256:49e9141d9187a695d4196e3e31c430dbecc244769d2813df7d3214f7e734e343

Observation 543ba09c-d293-49e6-9743-fd296902f44f · inbound

Complete one-loop self-energies of the linear sigma model coupled to quarks at finite temperature and in a magnetic field cites this paper.

Complete one-loop self-energies of the linear sigma model coupled to quarks at finite temperature and in a magnetic field Evolution of neutron star magnetic fields

Reference 17

Resolution
verified exact
arxiv_id, observed 2026-06-30T20:55:04.838766Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-06-30T20:46:17.090053Z digest=sha256:1fb03fc10a487f2d10189e7c6f915db5e2b6206ea9659ea92f0b0d2ff517480e