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Paper Citation Record · LEDGER

Simulating bulk viscosity in neutron stars. I. Formalism

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2204.11809.

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

pith.paper-citation-record.v1
2204.11809 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 2026-08-08T06:32:00.761636+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T00:03:47.131050Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T15:27:05.921189Z

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 a1e787f8-a6fe-49aa-9da7-ef59b3993532 · inbound

Causality constraints on radiative transfer cites this paper.

Causality constraints on radiative transfer Simulating bulk viscosity in neutron stars. I. Formalism

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-08T00:03:47.131050Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 06ecaaad-f4aa-4a3c-bd38-74aec81e5ef1 · inbound

Bulk viscosity from neutron decays to dark baryons in neutron star matter cites this paper.

Bulk viscosity from neutron decays to dark baryons in neutron star matter Simulating bulk viscosity in neutron stars. I. Formalism

Reference 95

Resolution
verified exact
arxiv_id, observed 2026-05-18T12:46:24.043387Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

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Observation c62febe8-1f0b-4f56-aef0-78b8851398b2 · inbound

TTE-CAM: Self-Explainable Class Activation Maps for Pretrained Black-Box CNNs cites this paper.

TTE-CAM: Self-Explainable Class Activation Maps for Pretrained Black-Box CNNs Simulating bulk viscosity in neutron stars. I. Formalism

Reference 75

Resolution
unresolved
no resolver link, observed 2026-07-13T17:23:25.842886Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T17:23:25.842886Z digest=sha256:99ba74a825ecde999132d78f830df26cf7da1fa29324d8b006ee6fe30c20747a

Observation 90073e24-303c-4eaf-8704-cf832b53d543 · inbound

Radial Oscillations of Viscous Stars at Finite Temperature cites this paper.

Radial Oscillations of Viscous Stars at Finite Temperature Simulating bulk viscosity in neutron stars. I. Formalism

Reference 23

Resolution
verified exact
arxiv_id, observed 2026-07-02T15:27:05.924010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-27T23:50:16.954566Z digest=sha256:d1b2f439b04ec63980d96ce3088e4832642f5af97bb5016bafaa137289d59cb0