Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Can the gravitational wave background feel wiggles in spacetime?
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2307.05455.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T20:02:43.313716Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-22T01:55:55.073227Z
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 1cf73bdd-30c9-4820-8404-1c403905755b · inbound
Bridge the Cosmological Tensions with Thawing Gravity cites this paper.
Bridge the Cosmological Tensions with Thawing Gravity Can the gravitational wave background feel wiggles in spacetime?
Reference 93
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T18:17:21.832631Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e2d8ae22-aab3-4ac0-8061-9a914de41d4c · inbound
Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order cites this paper.
Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order Can the gravitational wave background feel wiggles in spacetime?
Reference 267
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T01:55:55.075501Z
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 5c5a4acb-8cbb-493f-a9ca-71bc5b2ab550 · inbound
The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise cites this paper.
The power of SKA to Constrain cosmological gravitational-wave backgrounds below the astrophysical foreground noise Can the gravitational wave background feel wiggles in spacetime?
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T20:02:43.313716Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 66bb7496-0f02-43e2-8d49-c78210c27b2a · inbound
Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves cites this paper.
Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves Can the gravitational wave background feel wiggles in spacetime?
Reference 26
- Resolution
- verified exact
- arxiv_id, observed 2026-05-10T01:04:50.614172Z
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 eb9e6b5b-aaff-4997-9647-5d514bc0540c · inbound
Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves cites this paper.
Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves Can the gravitational wave background feel wiggles in spacetime?
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T15:56:58.079163Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.