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Paper Citation Record · LEDGER

Rotating neutron stars: an invariant comparison of approximate and numerical spacetime models

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:gr-qc/0405146.

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

pith.paper-citation-record.v1
gr-qc/0405146 v2

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 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T11:32:34.755587Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-09T06:05:35.631453Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 0ad7c4c3-1fff-4ffe-b293-c384e3b286fc · inbound

Building Neutron Stars with the MUSES Calculation Engine cites this paper.

Building Neutron Stars with the MUSES Calculation Engine Rotating neutron stars: an invariant comparison of approximate and numerical spacetime models

Reference 151

Resolution
unresolved
no resolver link, observed 2026-08-08T11:32:34.755587Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation b537f4ed-c246-4788-8541-9da693d73bb8 · inbound

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation cites this paper.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Rotating neutron stars: an invariant comparison of approximate and numerical spacetime models

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:13.645287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:13.645287Z digest=sha256:2687ac03f041144014ae4cd42042b51332bba6773682d39368f94122c45edd72

Observation 29de0fba-443e-40f6-91d7-144921c645c1 · inbound

Unifying the Regge-Wheeler-Zerilli and Bardeen-Press-Teukolsky formalisms on spherical backgrounds cites this paper.

Unifying the Regge-Wheeler-Zerilli and Bardeen-Press-Teukolsky formalisms on spherical backgrounds Rotating neutron stars: an invariant comparison of approximate and numerical spacetime models

Reference 90

Resolution
verified exact
arxiv_id, observed 2026-07-04T17:48:02.477624Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-08T18:56:09.664711Z digest=sha256:a3a904dbc882a2eb5aa7aef499f561aeee110864a50e1b0152037f211c63a0d1