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Paper Citation Record · LEDGER

Neutron Star Collapse From Accretion: a Probe of Massive Dark Matter Particles

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2408.00594.

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

pith.paper-citation-record.v1
2408.00594 v1

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 2026-08-06T19:18:39.075755Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-19T03:47:01.793579Z

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 e57e35df-9f73-4aa8-953e-6670d4eaae7a · inbound

Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter? cites this paper.

Can Orbital Decay of Accreting Binary Pulsars Probe Dark Matter? Neutron Star Collapse From Accretion: a Probe of Massive Dark Matter Particles

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-06T19:18:39.075755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T19:18:39.075755Z digest=sha256:172aba77145585306cfadffbd9830e88d1b6339cf163ee89414c0a0743616a90

Observation 77ccede0-67d4-43cc-8b18-ab282417235e · inbound

Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter cites this paper.

Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Late Inspiral & Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter Neutron Star Collapse From Accretion: a Probe of Massive Dark Matter Particles

Reference 34

Resolution
verified exact
arxiv_id, observed 2026-05-19T03:47:01.796276Z

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=2026-05-19T03:44:07.472458Z digest=sha256:8513ddb9bfffce1cbd4b27db79fae6523803ff4a765eed31791acfe58cd810dc