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Paper Citation Record · LEDGER

Determining cosmological growth parameter for stellar-mass black holes

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2311.09007.

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

pith.paper-citation-record.v1
2311.09007 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 1 of 1 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T03:35:52.655709Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

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  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

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Pith citing papers

Observation 35429171-6e4b-4488-9d39-b1731d7c59f6 · inbound

Evaporating cosmologically coupled black holes cites this paper.

Evaporating cosmologically coupled black holes Determining cosmological growth parameter for stellar-mass black holes

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-02T03:35:52.655709Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T03:35:52.655709Z digest=sha256:fed66767358bdd2a88106f6f0402ac8282b2e0996de577a3c0bf74e0bc695760