Paper Citation Record · LEDGER

The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0612404.

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

pith.paper-citation-record.v1
astro-ph/0612404 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T05:11:41.979656Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 2ecd0449-507c-4153-b0f7-50ed7ef25978 · inbound

Neutrino oscillations in a neutrino-dominated accretion disk around a Kerr BH cites this paper.

Neutrino oscillations in a neutrino-dominated accretion disk around a Kerr BH The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-14T05:11:41.979656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7ce463db-2f85-42e8-97d1-802661f4384d · inbound

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

Transport Properties of the MRI in Differentially Rotating Neutron Stars The fundamental difference between shear alpha viscosity and turbulent magnetorotational stresses

Reference 54

Resolution: unresolved; no resolver link, observed 2026-07-31T14:28:12.783818Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.