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Paper Citation Record · LEDGER

Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2107.05094.

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

pith.paper-citation-record.v1
2107.05094 v1

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:32:16.805658Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T05:29:35.551405Z

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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 68e301c4-4f5c-4ba0-a4d7-009da68e577b · inbound

Superradiant amplification by rotating viscous compact objects cites this paper.

Superradiant amplification by rotating viscous compact objects Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-07T00:32:16.805658Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation d80b4dbd-bb7a-4b7f-b25a-04ed32f09e3b · 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 Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

Reference 96

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verified exact
arxiv_id, observed 2026-05-18T12:46:24.067695Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 0b32c8cb-1573-4426-849a-62da13f3ca7b · inbound

Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers cites this paper.

Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

Reference 15

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verified exact
arxiv_id, observed 2026-05-22T12:54:52.564425Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation c6074d52-b85b-41ec-a147-069f9a454eb6 · inbound

Radial Oscillations of Viscous Stars cites this paper.

Radial Oscillations of Viscous Stars Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

Reference 24

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unresolved
no resolver link, observed 2026-07-13T19:28:30.285139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 1b601354-dc1e-4563-8872-418a3cbf1a8c · 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 Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

Reference 67

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 1bebcf7c-23ba-4de9-b160-d52c58421b5a · inbound

Axial Oscillations of Viscous Neutron Stars cites this paper.

Axial Oscillations of Viscous Neutron Stars Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

Reference 26

Resolution
verified exact
arxiv_id, observed 2026-05-11T11:36:00.927820Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation b76ddec0-bd2c-4a57-a1d5-d9f81eb60c25 · inbound

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

Radial Oscillations of Viscous Stars at Finite Temperature Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

Reference 18

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verified exact
arxiv_id, observed 2026-07-02T15:27:05.933320Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-27T23:50:16.954566Z digest=sha256:f2094f8d0c27b13b9fe3c0068110b4e4cb904d770eb89e14e641e4f0ecebbed6

Observation df41ddd5-6b05-44a4-84d7-e54f392b4af4 · inbound

Out-of-Equilibrium Effects in Non-Radial Relativistic Stellar Perturbations: A Model-Agnostic Formulation and Mode Analysis cites this paper.

Out-of-Equilibrium Effects in Non-Radial Relativistic Stellar Perturbations: A Model-Agnostic Formulation and Mode Analysis Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

Reference 57

Resolution
verified exact
arxiv_id, observed 2026-07-04T05:29:35.552895Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation a93565a8-0a6d-43f7-9ea8-8644b5089686 · inbound

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity cites this paper.

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity Projecting the likely importance of weak-interaction-driven bulk viscosity in neutron star mergers

Reference 26

Resolution
unresolved
no resolver link, observed 2026-07-14T15:02:35.854356Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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