Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Why the mean mass of primordial black hole distribution is close to 10$M_{\odot}$
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2004.11669.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-10T22:25:42.629865Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T22:27:36.785108Z
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 40990f19-0897-4338-a50c-c0b9f307a559 · inbound
Primordial black holes formation in inflationary $F(R)$ models with scalar fields cites this paper.
Primordial black holes formation in inflationary $F(R)$ models with scalar fields Why the mean mass of primordial black hole distribution is close to 10$M_{\odot}$
Reference 5
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T14:01:27.468340Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation aec34f20-180e-442c-9882-4b9e96a6e8ea · inbound
Effect of post-recombination accretion on primordial binary black hole mergers within virialized dark matter halos cites this paper.
Effect of post-recombination accretion on primordial binary black hole mergers within virialized dark matter halos Why the mean mass of primordial black hole distribution is close to 10$M_{\odot}$
Reference 33
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T22:27:36.807686Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.