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Paper Citation Record · LEDGER

Spherically Symmetric Simulation with Boltzmann Neutrino Transport of Core Collapse and Post-Bounce Evolution of a 15 Solar Mass Star

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0005438.

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

pith.paper-citation-record.v1
astro-ph/0005438 v2

Coverage vector

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

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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T16:25:38.520777Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T12:45:44.448577Z

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 938b3ce7-a6fe-4254-9ff5-5914b24e0e1c · inbound

Individual Neutrino Masses From a Supernova cites this paper.

Individual Neutrino Masses From a Supernova Spherically Symmetric Simulation with Boltzmann Neutrino Transport of Core Collapse and Post-Bounce Evolution of a 15 Solar Mass Star

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-12T16:25:38.520777Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation c5e508d9-c877-4db1-bd87-70bfb9db941b · inbound

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves cites this paper.

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves Spherically Symmetric Simulation with Boltzmann Neutrino Transport of Core Collapse and Post-Bounce Evolution of a 15 Solar Mass Star

Reference 14

Resolution
unresolved
no resolver link, observed 2026-07-13T16:48:58.103396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T16:48:58.103396Z digest=sha256:5b2c804cd5eb70125eb9e96e1fe0a6163b37f2b71b2c5923a30b456c4ebe2817

Observation b9d85577-772d-46c3-a879-35dc4c674481 · inbound

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves cites this paper.

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves Spherically Symmetric Simulation with Boltzmann Neutrino Transport of Core Collapse and Post-Bounce Evolution of a 15 Solar Mass Star

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-04T05:43:24.184827Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T05:43:24.184827Z digest=sha256:ca2fbaf1c58e75b152755af7b08118d68988b82099fe1fa53ee1bd9dead87642

Observation 18e80ac5-9d34-44bd-94cd-065ecc00f63f · inbound

Parameterizing the Standing Accretion Shock Instability for Inference with Galactic Supernova Neutrino Signals at IceCube cites this paper.

Parameterizing the Standing Accretion Shock Instability for Inference with Galactic Supernova Neutrino Signals at IceCube Spherically Symmetric Simulation with Boltzmann Neutrino Transport of Core Collapse and Post-Bounce Evolution of a 15 Solar Mass Star

Reference 73

Resolution
verified exact
local_arxiv, observed 2026-07-01T12:45:44.449944Z

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=2026-07-01T01:47:53.424100Z digest=sha256:cd30ce725b9f11e8d6fdb3b55c1199094a8952d647df644cc9b9c7b5977266ce

Observation 88d5cb95-deeb-4d70-bc1f-1c1bb3a72487 · inbound

3D simulations of a complete convective silicon shell burning phase cites this paper.

3D simulations of a complete convective silicon shell burning phase Spherically Symmetric Simulation with Boltzmann Neutrino Transport of Core Collapse and Post-Bounce Evolution of a 15 Solar Mass Star

Reference 292

Resolution
unresolved
no resolver link, observed 2026-08-06T13:05:40.021611Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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