Paper Citation Record · LEDGER

Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45-65 in supernovae environment

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:nucl-th/0001018.

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pith.paper-citation-record.v1
nucl-th/0001018 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 5 of 5 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:50:44.353772Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T16:25:49.738345Z

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Outbound references

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Pith citing papers

Observation cd54a267-261b-4eb2-86b1-68d834b9c598 · inbound

Obtaining Precision Constraints on Modified Gravity with Helioseismology cites this paper.

Obtaining Precision Constraints on Modified Gravity with Helioseismology Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45-65 in supernovae environment

Reference 2000

Resolution: unresolved; no resolver link, observed 2026-08-14T04:50:44.353772Z

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Observation bc3034fe-f135-4571-8d9f-4027d5d5980e · inbound

Comparative Testing of Subgrid Models for Fast Neutrino Flavor Conversions in Core-collapse Supernova Simulations cites this paper.

Comparative Testing of Subgrid Models for Fast Neutrino Flavor Conversions in Core-collapse Supernova Simulations Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45-65 in supernovae environment

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-07T05:49:23.193245Z

Source-reported events for the cited work

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Observation 5854121d-5a60-4a8d-8e79-f2679eeb4e9f · inbound

Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics cites this paper.

Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45-65 in supernovae environment

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-05-16T15:31:04.260896Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 98ed81c3-75dc-4e41-8b0f-e7b112241eab · inbound

Temperature-resolved sensitivities of $^{56}{\rm Ni}$ production to helium-burning reactions in pair-instability supernovae cites this paper.

Temperature-resolved sensitivities of $^{56}{\rm Ni}$ production to helium-burning reactions in pair-instability supernovae Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45-65 in supernovae environment

Reference 37

Resolution: verified exact; local_arxiv, observed 2026-07-01T16:25:49.739567Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 9638735d-4a6c-48ae-aead-d8e76bccea03 · inbound

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures cites this paper.

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range A=45-65 in supernovae environment

Reference 137

Resolution: unresolved; no resolver link, observed 2026-08-01T09:55:49.299843Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.