Paper Citation Record · LEDGER

Idealized Global Models of Accretion Disks with Strong Toroidal Magnetic Fields

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2505.12671.

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

pith.paper-citation-record.v1
2505.12671 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:44:34.610187Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-16T17:28:10.223062Z

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 1e563817-6855-4aa5-9eb8-cf6f66a6021e · inbound

Accretion of AGN Stars under Influence of Disk Geometry cites this paper.

Accretion of AGN Stars under Influence of Disk Geometry Idealized Global Models of Accretion Disks with Strong Toroidal Magnetic Fields

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T15:44:34.610187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7a27409b-2b43-4631-8d54-99e860496fc7 · inbound

Does magnetic field promote or suppress fragmentation in AGN disks? Results from local shearing box simulations with simple cooling cites this paper.

Does magnetic field promote or suppress fragmentation in AGN disks? Results from local shearing box simulations with simple cooling Idealized Global Models of Accretion Disks with Strong Toroidal Magnetic Fields

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-06T12:18:54.778870Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 354f7e74-9cc2-4c30-812f-b4ace4a6f18f · inbound

$\textit{BMAD}$-Circumbinary Magnetically Arrested Disks around Stellar or Black Hole Binaries: Hot Accretion Flows, Disk Properties, and Angular Momentum Transfer cites this paper.

$\textit{BMAD}$-Circumbinary Magnetically Arrested Disks around Stellar or Black Hole Binaries: Hot Accretion Flows, Disk Properties, and Angular Momentum Transfer Idealized Global Models of Accretion Disks with Strong Toroidal Magnetic Fields

Reference 172

Resolution: unresolved; no resolver link, observed 2026-08-05T17:13:12.005357Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ba484fb0-1dd0-4aa1-858c-8752a885c8d3 · inbound

Thick Disks, Thin Hopes: Suppressed Capture and Merger Rates in AGN cites this paper.

Thick Disks, Thin Hopes: Suppressed Capture and Merger Rates in AGN Idealized Global Models of Accretion Disks with Strong Toroidal Magnetic Fields

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-06-30T03:17:05.501251Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.