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Paper Citation Record · LEDGER

Density dependent quark mass model revisited: Thermodynamic consistency, stability windows and stellar properties

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2007.04494.

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

pith.paper-citation-record.v1
2007.04494 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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T09:30:11.011428Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-17T04:29:02.100153Z

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 045fe54d-f116-4e9c-a88d-1644531dff2b · inbound

Rotational effects in quark stars: comparing different models cites this paper.

Rotational effects in quark stars: comparing different models Density dependent quark mass model revisited: Thermodynamic consistency, stability windows and stellar properties

Reference 40

Resolution
verified exact
arxiv_id, observed 2026-05-17T04:29:02.102063Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-17T04:24:27.138790Z digest=sha256:28413c13f074596a3a3862cddf350a1d4bbe051a7368777689261715c3881229

Observation 677bc6a5-a138-4e72-9139-13ad5b1511ca · inbound

Rotational enhancement and stability of protoquark stars during thermal evolution cites this paper.

Rotational enhancement and stability of protoquark stars during thermal evolution Density dependent quark mass model revisited: Thermodynamic consistency, stability windows and stellar properties

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-03T09:30:11.011428Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T09:30:11.011428Z digest=sha256:377852f3eb9e9a189cbe376585ab40237fb1f0651cfbf16e5216291c8bfdc13b