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Paper Citation Record · LEDGER

Influence of three parameters on maximum mass and stability of strange star under linear $f(Q)-$action

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2309.10830.

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

pith.paper-citation-record.v1
2309.10830 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T05:13:20.107699Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T05:13:20.468244Z

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 0c8dc7d0-6be2-4f42-9d1f-0316ce8fe7e1 · 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 Influence of three parameters on maximum mass and stability of strange star under linear $f(Q)-$action

Reference 61

Resolution
verified exact
local_arxiv, observed 2026-08-12T05:13:20.471995Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-08-12T05:13:20.107699Z digest=sha256:51f4c50362f3c80635e042bfb8380d888cd9cb3f7e3cf7386ac8515e6363f8f0

Observation 68186dd2-fdde-4398-83e6-4f4b2aaaf067 · inbound

Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the impact on the $\sigma_8$ tension cites this paper.

Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the impact on the $\sigma_8$ tension Influence of three parameters on maximum mass and stability of strange star under linear $f(Q)-$action

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-03T15:39:59.736668Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T15:39:59.736668Z digest=sha256:aefd10ce484c34143afc5984b18a4bfcf756aef49b0b4148a68623202ee0fc42

Observation 37ba75d1-0b0a-42a4-9da8-f388861ae4c9 · inbound

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity cites this paper.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Influence of three parameters on maximum mass and stability of strange star under linear $f(Q)-$action

Reference 36

Resolution
unresolved
no resolver link, observed 2026-07-11T16:40:07.642828Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:b06fc0c5937ec7ea53627adee7c2fae0b39b7e6c02717bc2742a308578c8072a