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Paper Citation Record · LEDGER

Numerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2111.05183.

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

pith.paper-citation-record.v1
2111.05183 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T14:25:05.950968Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T05:56:01.619774Z

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 58579b16-5650-4ba7-9990-6ec826506371 · inbound

Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors cites this paper.

Exploring the Potential for Detecting Rotational Instabilities in Binary Neutron Star Merger Remnants with Gravitational Wave Detectors Numerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817

Reference 40

Resolution
verified exact
arxiv_id, observed 2026-05-24T05:56:01.623273Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-24T05:55:32.580041Z digest=sha256:6562f95a020d7e102a5d47d98121700d1eed9d2f9a3695d2a09987f7208b6c35

Observation ca5c03fd-c7f7-42ee-b12f-b5559adb5e3f · inbound

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

Remnant properties of binary neutron star mergers undergoing prompt collapse Numerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-06T14:25:05.950968Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T14:25:05.950968Z digest=sha256:2d4bd5e0239fa925907b662f15d057b3a1ebffa358745916af38f920b226266d

Observation fdc01ee2-4183-49c3-933a-d0d4c6b77cdc · inbound

Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology cites this paper.

Binary neutron stars in the next-generation era: Multi-messenger detection prospects and constraints on the equation of state, mass distribution, and cosmology Numerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817

Reference 131

Resolution
unresolved
no resolver link, observed 2026-07-31T07:22:45.794825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T07:22:45.794825Z digest=sha256:0508c75073d29a5708730b63da1f969cfdaf45f4de48ceb0476b37717e77b5ec