Paper Citation Record · LEDGER

What really makes an accretion disc MAD

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2111.02439.

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

pith.paper-citation-record.v1
2111.02439 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 2026-08-20T06:33:59.587034+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T21:41:37.506079Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-07T22:24:11.004806Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 1edbdef0-b426-4522-b9d8-0cd1cc67b912 · inbound

Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields cites this paper.

Quantum signatures in black hole accretion: Pair production in dynamical magnetic fields What really makes an accretion disc MAD

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-15T21:41:37.506079Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b64b7d4-8f48-4227-96c1-213c971b1513 · 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 What really makes an accretion disc MAD

Reference 120

Resolution: unresolved; no resolver link, observed 2026-08-05T17:13:11.758236Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a1ee7355-9c87-49c7-ac82-f1237833f607 · inbound

The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654 cites this paper.

The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654 What really makes an accretion disc MAD

Reference 1

Resolution: verified exact; local_arxiv, observed 2026-07-07T22:24:11.006043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation f6f0d0b3-84c7-4070-ac14-ec01bbfad43f · inbound

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer cites this paper.

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer What really makes an accretion disc MAD

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-01T13:29:31.626208Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e3ce9a07-b812-40b9-bee7-d0047ede3333 · inbound

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 cites this paper.

The physical mechanism for two rapid changing-look AGNs: SDSS J0225+0030 and SDSS J1723+5504 What really makes an accretion disc MAD

Reference 114

Resolution: unresolved; no resolver link, observed 2026-08-15T15:15:05.055393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c3d9b5a-095e-4fc3-a6bf-16e58aa6d2c1 · inbound

Signatures of Lorentz violation in bright ring for Sgr A* images by radiation ineffective accretion flows cites this paper.

Signatures of Lorentz violation in bright ring for Sgr A* images by radiation ineffective accretion flows What really makes an accretion disc MAD

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-06T00:18:32.657365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.