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Paper Citation Record · LEDGER

High-energy neutrinos from fallback accretion of binary neutron star merger remnants

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1910.06578.

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

pith.paper-citation-record.v1
1910.06578 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T19:10:39.497964Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:37:45.085713Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 3ea3753d-bd12-42ce-a316-91941a47aa24 · inbound

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos cites this paper.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos High-energy neutrinos from fallback accretion of binary neutron star merger remnants

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-15T19:10:39.497964Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T19:10:39.497964Z digest=sha256:3e0ea6ef4eebcf98ce54b520d1ce9f8f3e92d0730bb40eb82e939ed1b8f0de1a

Observation 8bc96e1d-da6b-45a3-b7fb-fd5b05dae983 · inbound

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

A magnetar formation in binary neutron star merger High-energy neutrinos from fallback accretion of binary neutron star merger remnants

Reference 20

Resolution
verified exact
arxiv_id, observed 2026-07-03T07:37:45.087402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-06-27T12:03:16.536504Z digest=sha256:c94f1d048a6091ec97184a2a874dc3fa641cd6c3b34505a5a37000b67647e283