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Paper Citation Record · LEDGER

Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0008432.

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

pith.paper-citation-record.v1
astro-ph/0008432 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 2026-08-10T06:31:04.303077+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T14:43:37.249327Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

272
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 18ea3bf8-9742-4609-b6ae-f3a79ccf6388 · inbound

Time integration for neutrino radiation transport using minimally implicit Runge-Kutta methods cites this paper.

Time integration for neutrino radiation transport using minimally implicit Runge-Kutta methods Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae

Reference 21

Resolution
verified exact
local_arxiv, observed 2026-05-24T09:29:17.117530Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:1e641766a44f6617aa52f4de7df306b65ee0ae3dbe5f2ff162bc4dc50d675716

Observation c84f46a0-a1df-4436-b2e3-b8daad422f15 · inbound

Cooling the Shock: New Supernova Constraints on Dark Photons cites this paper.

Cooling the Shock: New Supernova Constraints on Dark Photons Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-09T14:43:37.249327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T14:43:37.249327Z digest=sha256:b9838fa672b12d5a81c47922d7539b08ebab2ace000e0386469180d958d74d8b

Observation f6392c10-3cad-4c31-8852-0b2ec0b62a01 · 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 Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae

Reference 12

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:e9d5a149eec9480a3627e63ebdff10aaf352ed01368268d7c2557abe4232b678

Observation 1e4aa790-0713-4460-b7e0-7272a6750742 · 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 Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-04T05:43:23.994894Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T05:43:23.994894Z digest=sha256:c9c945ab9b22c0984ab13114894836a6a297361d62fd9675c7510a4c663f4dbd

Observation 31e937ca-0a19-441d-8743-b886586119ca · inbound

Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors cites this paper.

Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors Conditions for Shock Revival by Neutrino Heating in Core-Collapse Supernovae

Reference 11

Resolution
verified exact
arxiv_id, observed 2026-05-11T18:26:11.742812Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-08T15:59:11.556246Z digest=sha256:4c6d65484afea0fa5497161a0dac99ffe88d31c41c737c608fe699ee88b414ac