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Paper Citation Record · LEDGER

Equation of state effects in the core collapse of a $20$-$M_\odot$ star

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1906.02009.

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

pith.paper-citation-record.v1
1906.02009 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T10:10:48.332913Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-20T08:13:08.424612Z

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 5715145e-04c2-4d83-8f66-83326ab08411 · inbound

Remnant properties of binary neutron star mergers undergoing prompt collapse cites this paper.

Remnant properties of binary neutron star mergers undergoing prompt collapse Equation of state effects in the core collapse of a $20$-$M_\odot$ star

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-06T14:25:05.995656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T14:25:05.995656Z digest=sha256:c0b288bdf3e24f519a1791393217086a0790dd9af024d487ddf4263189c9bf11

Observation 726997ae-3334-4b61-a62c-08db4d264a11 · inbound

The Gravitational-Wave Power Gap in Core-Collapse Supernovae: Insights from 60 Axisymmetric Simulations cites this paper.

The Gravitational-Wave Power Gap in Core-Collapse Supernovae: Insights from 60 Axisymmetric Simulations Equation of state effects in the core collapse of a $20$-$M_\odot$ star

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-04T05:44:58.849953Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T05:44:58.849953Z digest=sha256:ad6449223cd4ce348f5f8499b9922f964b5780cb1c4f23522157a39173122dbe

Observation 408a1a8a-d13b-463b-88c5-eb28d7834fe4 · inbound

Impact of Effective Nucleon Mass and Multineutron States on the Equation of State for Core-Collapse Supernovae cites this paper.

Impact of Effective Nucleon Mass and Multineutron States on the Equation of State for Core-Collapse Supernovae Equation of state effects in the core collapse of a $20$-$M_\odot$ star

Reference 8

Resolution
verified exact
arxiv_id, observed 2026-05-11T10:11:15.522124Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-10T15:34:47.069340Z digest=sha256:6f43d497bf61e3597131171eb5bf6f1d433a77e34119b7c646e9453e3166d18f

Observation 82d695d8-b5bd-4198-a13b-2267d7978dec · 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 Equation of state effects in the core collapse of a $20$-$M_\odot$ star

Reference 87

Resolution
verified exact
arxiv_id, observed 2026-05-20T08:13:08.426175Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-20T08:10:13.936279Z digest=sha256:3950ff5d57e2e910bf216e4e9bc474218e1df5facd3f2e8a1bc0d761e365744c

Observation f29922f7-3edf-4d44-9401-88096693f5b3 · inbound

On the Nucleon Effective Mass in Neutron Stars Cooling cites this paper.

On the Nucleon Effective Mass in Neutron Stars Cooling Equation of state effects in the core collapse of a $20$-$M_\odot$ star

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-01T00:06:07.415618Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T00:06:07.415618Z digest=sha256:6e45c49187d67e513e8368c1485ad4942980b22362f699b3f2d042d7cff7463c

Observation 85cb1bc0-da37-4ce1-8091-d6a1a75a6e27 · inbound

From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State cites this paper.

From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State Equation of state effects in the core collapse of a $20$-$M_\odot$ star

Reference 79

Resolution
malformed identifier
no resolver link, observed 2026-08-08T00:43:19.523537Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T00:43:19.523537Z digest=sha256:423effed3fb3500432cbdeab53d7686c563a0c0314812972008ed3f341d332e2

Observation da0cd4d4-93eb-4e4a-a9a2-62fbf1dce8ff · inbound

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects cites this paper.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Equation of state effects in the core collapse of a $20$-$M_\odot$ star

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-08T10:10:48.332913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T10:10:48.332913Z digest=sha256:29bb9b89830a3fc73fd5e0fac8d271d136908becc72c205c36af66af0c608600