Pith. sign in

Paper Citation Record · LEDGER

Modeling general-relativistic plasmas with collisionless moments and dissipative two-fluid magnetohydrodynamics

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2111.05752.

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

pith.paper-citation-record.v1
2111.05752 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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T11:18:58.798426Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-16T11:18:59.610448Z

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 2877bf88-9bad-4eb1-9f5e-9508a28e4ac9 · inbound

Unveiling the electrodynamic nature of spacetime collisions cites this paper.

Unveiling the electrodynamic nature of spacetime collisions Modeling general-relativistic plasmas with collisionless moments and dissipative two-fluid magnetohydrodynamics

Reference 37

Resolution
verified exact
local_arxiv, observed 2026-08-16T11:18:59.615727Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-08-16T11:18:58.798426Z digest=sha256:0703236aa9c66afbfc8a0083bb34853d89aa5429b793a67915760abf7d10a441

Observation 57dc658a-7470-4c8c-95e0-be1e58de01a2 · 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 Modeling general-relativistic plasmas with collisionless moments and dissipative two-fluid magnetohydrodynamics

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-05T17:13:11.355459Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T17:13:11.355459Z digest=sha256:cfa0baea152588a778642a8b7d677c5d08cfd32c871dd184a9a20e3ff07b7777