Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Non-trivial, static, geodesically complete space-times with a negative cosmological constant II. $n\ge 5$
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:gr-qc/0401081.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T05:27:08.747599Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T08:50:58.160897Z
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 06e58853-d7ca-499b-a93b-73b7a24b2a9f · inbound
Holographic is Hamiltonian, relatively cites this paper.
Holographic is Hamiltonian, relatively Non-trivial, static, geodesically complete space-times with a negative cosmological constant II. $n\ge 5$
Reference 1
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T18:11:18.579131Z
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 c89305c0-170c-4848-af23-17833ff712f5 · inbound
Static vacuum metrics in (4 + 1) dimensions with {\Lambda} < 0 and squashed conformal infinity cites this paper.
Static vacuum metrics in (4 + 1) dimensions with {\Lambda} < 0 and squashed conformal infinity Non-trivial, static, geodesically complete space-times with a negative cosmological constant II. $n\ge 5$
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T05:27:08.747599Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.