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Paper Citation Record · LEDGER

A 3D Simulation of a Neutrino-Driven Supernova Explosion Aided By Convection and Magnetic Fields

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2007.04775.

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

pith.paper-citation-record.v1
2007.04775 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T13:05:34.480860Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-20T08:13:08.376618Z

Reference resolution

0 of 0 outbound references displayed

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

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 4c8dbf46-e7a6-4e9e-80da-2a0573e59432 · inbound

Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass cites this paper.

Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass A 3D Simulation of a Neutrino-Driven Supernova Explosion Aided By Convection and Magnetic Fields

Reference 93

Resolution
verified exact
arxiv_id, observed 2026-05-20T08:13:08.378029Z

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=2026-05-20T08:10:13.936279Z digest=sha256:da6a5d90acc0357b1aaebddcfd721f114e9642ee30156662aaf26fb4941e6c57

Observation b5ead0c8-0ddb-48c1-b3bd-14175ac74ff1 · inbound

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

3D simulations of a complete convective silicon shell burning phase A 3D Simulation of a Neutrino-Driven Supernova Explosion Aided By Convection and Magnetic Fields

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-06T13:05:34.480860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T13:05:34.480860Z digest=sha256:2759a1d08decb4081c52608aac8dccefdb4261b89ecf15025d8583241e0d7631