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Paper Citation Record · LEDGER

Binary neutron star mergers as the source of the highest energy cosmic rays

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2405.12004.

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

pith.paper-citation-record.v1
2405.12004 v2

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 2026-08-09T06:31:02.800959+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T19:51:26.342186Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T11:39:46.736220Z

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 bdf2b9a6-0051-48bb-ae2e-e5e9c831257c · inbound

Ultraheavy Ultrahigh-Energy Cosmic Rays cites this paper.

Ultraheavy Ultrahigh-Energy Cosmic Rays Binary neutron star mergers as the source of the highest energy cosmic rays

Reference 97

Resolution
verified exact
arxiv_id, observed 2026-05-24T00:43:40.261577Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

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Observation daaf95dd-ac8a-4247-a655-4c2eff09c000 · inbound

The Global Cosmic Ray Observatory -- Challenging next-generation multi-messenger astronomy with interdisciplinary research cites this paper.

The Global Cosmic Ray Observatory -- Challenging next-generation multi-messenger astronomy with interdisciplinary research Binary neutron star mergers as the source of the highest energy cosmic rays

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-06T19:51:26.342186Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T19:51:26.342186Z digest=sha256:4645d5ac2e676db176c805e095fabf35fffd536cc2bb137b21be353909c0a535

Observation 685808a0-6f39-4659-a38a-10a087fe0d7d · inbound

Study of Flat Spectrum Radio Quasars and BL Lacertae Objects as Sources of Diffusive Ultra High-Energy Cosmic Rays cites this paper.

Study of Flat Spectrum Radio Quasars and BL Lacertae Objects as Sources of Diffusive Ultra High-Energy Cosmic Rays Binary neutron star mergers as the source of the highest energy cosmic rays

Reference 15

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verified exact
arxiv_id, observed 2026-05-17T23:55:31.191149Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-17T23:53:01.784343Z digest=sha256:69b6359bbfc6463cf758feb684a13bf457b175c191e975b6f1903abe200f92e5

Observation d75ccc90-b0f3-4cd2-af70-5c8480d45314 · inbound

A magnetar formation in binary neutron star merger cites this paper.

A magnetar formation in binary neutron star merger Binary neutron star mergers as the source of the highest energy cosmic rays

Reference 31

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verified exact
arxiv_id, observed 2026-07-03T07:37:45.132135Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-27T12:03:16.536504Z digest=sha256:c7a4fe4b792b686e6fd8e923269d50fc2e5ec944115b99952f23b2582b42a8ac

Observation b5b0684c-1379-4f15-a27d-9597e9347050 · inbound

Nuclei in high-energy neutrino sources: A multimessenger study of in-source propagation cites this paper.

Nuclei in high-energy neutrino sources: A multimessenger study of in-source propagation Binary neutron star mergers as the source of the highest energy cosmic rays

Reference 20

Resolution
verified exact
arxiv_id, observed 2026-07-04T11:39:46.737765Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-26T07:51:26.064246Z digest=sha256:e655d66ded8c9455f256c4a8b79ae9102b7b9b1d76abbc3c5f943eac6f79321f

Observation 4ee005d9-d533-47ee-8a33-a886b8a71de6 · inbound

Ultra-High-Energy Particle Production in Binary Mergers Endowed with Magnetic Fields cites this paper.

Ultra-High-Energy Particle Production in Binary Mergers Endowed with Magnetic Fields Binary neutron star mergers as the source of the highest energy cosmic rays

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-01T07:48:49.867444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T07:48:49.867444Z digest=sha256:1cf6acc7fac7594410f61114a7ad81d74304b77b8a47fcc995001ba1eb133fa1

Observation e85b41a1-8ff2-48c0-ae49-bd95fd313dbc · inbound

Proton-air interaction properties at $\sqrt{s} \simeq 100$ TeV from shower-depth measurements with the Pierre Auger Observatory and their connection to the Muon Puzzle cites this paper.

Proton-air interaction properties at $\sqrt{s} \simeq 100$ TeV from shower-depth measurements with the Pierre Auger Observatory and their connection to the Muon Puzzle Binary neutron star mergers as the source of the highest energy cosmic rays

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-01T05:12:26.591580Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T05:12:26.591580Z digest=sha256:ffac8f2894fcfc7a6b43fa3b0c8e1399049159b6bd232a4d28772979b14ba887