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Paper Citation Record · LEDGER

Can stellar mass black holes be quark stars?

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0908.2672.

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

pith.paper-citation-record.v1
0908.2672 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T05:13:19.984609Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T15:59:48.141945Z

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 4c144bde-0abb-460e-aedd-d91f93f4d338 · inbound

Interacting quark matter and $f(Q)$ gravity: A new paradigm in exploring the properties of quark stars cites this paper.

Interacting quark matter and $f(Q)$ gravity: A new paradigm in exploring the properties of quark stars Can stellar mass black holes be quark stars?

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-12T05:13:19.984609Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T05:13:19.984609Z digest=sha256:d7610902cb849188937b4b89f090c780cdccd7ec8545ce9229715e7ede5861c1

Observation d7514da3-ac78-43fd-ab6d-cb27c1032929 · inbound

Properties of compact objects in quadratic non-metricity gravity cites this paper.

Properties of compact objects in quadratic non-metricity gravity Can stellar mass black holes be quark stars?

Reference 25

Resolution
verified exact
local_arxiv, observed 2026-08-06T15:59:48.207512Z

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=2026-08-06T15:59:42.289850Z digest=sha256:7f07876f68d932cb64996e6dd15aebc8a4c916076c34ee06c91d6e5414445e4a