Paper Citation Record · LEDGER

Physical Acceptability of Isolated, Static, Spherically Symmetric, Perfect Fluid Solutions of Einstein's Equations

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:gr-qc/9809013.

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

pith.paper-citation-record.v1
gr-qc/9809013 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T10:33:30.809541Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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verified fuzzy0
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External citation measurements

631
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation bd2da32e-709c-47c2-8199-4b65cfca553d · inbound

The Kiselev black hole is neither perfect fluid, nor is it quintessence cites this paper.

The Kiselev black hole is neither perfect fluid, nor is it quintessence Physical Acceptability of Isolated, Static, Spherically Symmetric, Perfect Fluid Solutions of Einstein's Equations

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-14T10:33:30.809541Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e05af0ac-21db-44da-a579-24dfbf7ec116 · inbound

Perturbations of Black Holes Surrounded by Anisotropic Matter Field cites this paper.

Perturbations of Black Holes Surrounded by Anisotropic Matter Field Physical Acceptability of Isolated, Static, Spherically Symmetric, Perfect Fluid Solutions of Einstein's Equations

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-12T18:22:50.464632Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b34f8fd-3e35-4fe6-b024-54634664b06d · inbound

Rotating and non-linear magnetic-charged black hole with an anisotropic matter field cites this paper.

Rotating and non-linear magnetic-charged black hole with an anisotropic matter field Physical Acceptability of Isolated, Static, Spherically Symmetric, Perfect Fluid Solutions of Einstein's Equations

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-10T14:03:17.909688Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8b9f2431-4e7d-47df-8100-2fbadd50c46a · inbound

Energy conditions in static, spherically symmetric spacetimes and effective geometries cites this paper.

Energy conditions in static, spherically symmetric spacetimes and effective geometries Physical Acceptability of Isolated, Static, Spherically Symmetric, Perfect Fluid Solutions of Einstein's Equations

Reference 122

Resolution: verified exact; arxiv_id, observed 2026-05-10T08:32:51.935831Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 99f1b3e7-8369-4213-af0b-5ba945a8f301 · inbound

Revisiting Schwarzschild's constant density star in isotropic coordinates cites this paper.

Revisiting Schwarzschild's constant density star in isotropic coordinates Physical Acceptability of Isolated, Static, Spherically Symmetric, Perfect Fluid Solutions of Einstein's Equations

Reference 8

Resolution: metadata mismatch; local_arxiv, observed 2026-06-28T16:52:23.463487Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 0f0c3050-204f-4a41-ac85-9401fb016589 · 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 Physical Acceptability of Isolated, Static, Spherically Symmetric, Perfect Fluid Solutions of Einstein's Equations

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-07-04T01:19:20.504507Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.