Paper Citation Record · LEDGER

Stable dark energy stars

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:gr-qc/0508115.

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

pith.paper-citation-record.v1
gr-qc/0508115 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:39:39.751274Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T01:19:20.476421Z

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 98aa06fc-d444-4109-acd9-d285238c55c9 · inbound

Herrera Complexity and Shadows of Spherically Symmetric Compact Objects cites this paper.

Herrera Complexity and Shadows of Spherically Symmetric Compact Objects Stable dark energy stars

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-10T15:28:04.749817Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f4b546ce-5d4b-47e7-8980-b4bead308262 · inbound

Positive neutrino masses with DESI DR2 via matter conversion to dark energy cites this paper.

Positive neutrino masses with DESI DR2 via matter conversion to dark energy Stable dark energy stars

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-16T05:39:39.751274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f7fe6246-7bea-4ac4-917f-aa44964b563e · inbound

Rotating traversable wormholes and particle dynamics in $f(R,T)$ gravity cites this paper.

Rotating traversable wormholes and particle dynamics in $f(R,T)$ gravity Stable dark energy stars

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-07-01T21:36:15.188012Z

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.

Observation 7fd20a44-5227-4d46-89c0-3226f14e0de4 · inbound

Implications of Adler-Finch-Skea solution on charged dark energy star satisfying Karmarkar Condition cites this paper.

Implications of Adler-Finch-Skea solution on charged dark energy star satisfying Karmarkar Condition Stable dark energy stars

Reference 5

Resolution: verified exact; local_arxiv, observed 2026-07-04T01:19:20.478102Z

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.