Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:hep-ph/9606387.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T21:34:30.337122Z
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
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
818
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 55ddf4f7-7d22-48e9-82ed-0ea48a3517f8 · inbound
On Legacy of Starobinsky Inflation cites this paper.
On Legacy of Starobinsky Inflation What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 76
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T05:37:36.209602Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 4b4395c4-bbb1-44b2-ad35-45904049bf03 · inbound
A Match Made in Heaven: Linking Observables in Inflationary Cosmology cites this paper.
A Match Made in Heaven: Linking Observables in Inflationary Cosmology What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 1
- Resolution
- verified exact
- local_arxiv, observed 2026-05-22T13:14:53.279680Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation d530f295-d04e-433d-8cf4-11755180a0d2 · inbound
Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data cites this paper.
Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:34:30.337122Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 84be32a7-a836-4737-bd07-42b6a1a23110 · inbound
Very-High-Frequency Gravitational Waves from Multi-Monodromy Inflation cites this paper.
Very-High-Frequency Gravitational Waves from Multi-Monodromy Inflation What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T10:38:17.067264Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 30a4428f-dade-44fe-9b1a-cc4b816d6851 · inbound
Wormholes and the imaginary distance bound cites this paper.
Wormholes and the imaginary distance bound What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 46
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T18:01:06.295110Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 950c36b0-5984-4d4e-9875-54fd937d1c2c · inbound
Wormholes and the imaginary distance bound cites this paper.
Wormholes and the imaginary distance bound What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T17:30:40.616474Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e978d396-48a5-4e87-a501-60a6ed5a7e16 · inbound
Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor cites this paper.
Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 71
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T04:28:59.153091Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation f25149f2-b5bd-43e9-b537-1d396ec54b49 · inbound
Massive Graviton Dark Matter from a Gapped Continuum cites this paper.
Massive Graviton Dark Matter from a Gapped Continuum What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 42
- Resolution
- verified exact
- local_arxiv, observed 2026-07-09T15:16:18.107869Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 7c750d85-ea61-4488-be9e-509435b54aaa · inbound
Massive Graviton Dark Matter from a Gapped Continuum cites this paper.
Massive Graviton Dark Matter from a Gapped Continuum What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T04:32:44.446870Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 83f88614-ed78-4cea-9c65-563f79333e94 · inbound
Searching for Folded Primordial Non-Gaussianity with Galaxy Surveys cites this paper.
Searching for Folded Primordial Non-Gaussianity with Galaxy Surveys What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:46:06.281235Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2cfe4bd0-75c0-4972-beb5-863244a503ea · inbound
Axion isocurvature and the model-building problem of low-scale inflation cites this paper.
Axion isocurvature and the model-building problem of low-scale inflation What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T04:30:48.843954Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ea646fa4-8ace-420a-9cbf-d1af35acb380 · inbound
Extra-dimensional Origins of Chemical Potentials at the Cosmological Collider cites this paper.
Extra-dimensional Origins of Chemical Potentials at the Cosmological Collider What would we learn by detecting a gravitational wave signal in the cosmic microwave background anisotropy?
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T01:19:16.137284Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.