Paper Citation Record · LEDGER

Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2402.16781.

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pith.paper-citation-record.v1
2402.16781 v2

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measured 10 of 10 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T16:53:02.513896Z

measured 0 of 1 external citation measurements

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Source: arxiv_reference, observed 2026-05-22T01:55:55.406086Z

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Pith citing papers

Observation cf128056-4139-4103-894f-0f391c20a75e · inbound

Constraining inflation with nonminimal derivative coupling with the Parkes Pulsar Timing Array third data release cites this paper.

Constraining inflation with nonminimal derivative coupling with the Parkes Pulsar Timing Array third data release Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-11T16:53:02.513896Z

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Observation f614a0c0-fa1c-4b6e-95a3-822d1edd80b9 · inbound

Isotropic background and anisotropies of gravitational waves induced by cosmological soliton isocurvature perturbations cites this paper.

Isotropic background and anisotropies of gravitational waves induced by cosmological soliton isocurvature perturbations Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-10T22:07:19.969796Z

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Observation 607b56dd-9694-4b1a-8131-2301624310a7 · inbound

Infrared Behavior of Induced Gravitational Waves from Isocurvature Perturbations cites this paper.

Infrared Behavior of Induced Gravitational Waves from Isocurvature Perturbations Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-10T19:41:59.040184Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fadcfed8-a502-4e36-aa90-ce8a914fade7 · 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 we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

Reference 26

Resolution: verified exact; arxiv_id, observed 2026-05-22T01:55:55.408261Z

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Observation c7ce1831-30f1-42fe-a829-b2a3be040ab2 · inbound

Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer cites this paper.

Implications for Pulsar Timing Arrays of Sub-solar Black Hole Detections: From LVK to Einstein Telescope and Cosmic Explorer Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-05T15:54:09.228568Z

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Observation dc952e34-d09a-4f1c-b117-95ecba2d4eec · inbound

Isocurvature Induced Gravitational Waves at Pulsar Timing Arrays cites this paper.

Isocurvature Induced Gravitational Waves at Pulsar Timing Arrays Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-17T00:38:45.051954Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 594cd27c-ecc9-4431-81e5-a28990b05d2d · 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 we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-10T01:04:50.546833Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 2eea1877-1aea-46c4-a681-ae7a7eb564d6 · inbound

Purely quadratic non-Gaussianity from tachyonic instability: Primordial black holes and scalar-induced gravitational waves cites this paper.

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-02T15:56:59.809093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a113a660-e2ca-47f1-80f0-891d2672260c · inbound

Scalar-induced gravitational waves from a box-shaped curvature power spectrum cites this paper.

Scalar-induced gravitational waves from a box-shaped curvature power spectrum Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

Reference 126

Resolution: unresolved; no resolver link, observed 2026-07-14T09:40:09.826288Z

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Unavailable: canonical work link unavailable.

Observation cbda950a-f144-451d-8e83-38e7499a16d5 · inbound

Scalar-induced gravitational waves from inflation with symmetry breaking cites this paper.

Scalar-induced gravitational waves from inflation with symmetry breaking Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?

Reference 38

Resolution: unresolved; no resolver link, observed 2026-07-30T16:49:18.987380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.