Paper Citation Record · LEDGER

Confronting sound speed resonance with pulsar timing arrays

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2307.08687.

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

pith.paper-citation-record.v1
2307.08687 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T13:07:10.612242Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-22T01:55:55.414745Z

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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 c021538b-4f94-4f0e-a263-5415c08a9f9c · inbound

Pre-Big-Bang Cosmology Cannot Explain NANOGrav 15-year Signal cites this paper.

Pre-Big-Bang Cosmology Cannot Explain NANOGrav 15-year Signal Confronting sound speed resonance with pulsar timing arrays

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-12T13:07:10.612242Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 794ef448-fe2f-4013-aef7-c2a015243652 · inbound

Can tensor-scalar induced GWs dominate PTA observations ? cites this paper.

Can tensor-scalar induced GWs dominate PTA observations ? Confronting sound speed resonance with pulsar timing arrays

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-10T23:01:59.993655Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d2f7b81f-5356-48fc-b398-40420a41fee7 · 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 Confronting sound speed resonance with pulsar timing arrays

Reference 272

Resolution: verified exact; arxiv_id, observed 2026-05-22T01:55:55.417213Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 961bfc12-5baf-42fb-b049-ba108a6f6778 · inbound

Probing the scalar-induced gravitational waves with the Five-hundred-meter Aperture Spherical radio Telescope and the Square Kilometer Array cites this paper.

Probing the scalar-induced gravitational waves with the Five-hundred-meter Aperture Spherical radio Telescope and the Square Kilometer Array Confronting sound speed resonance with pulsar timing arrays

Reference 68

Resolution: verified exact; arxiv_id, observed 2026-05-19T05:22:59.691815Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 90a752b1-af6f-41a2-8b9a-29d739b8136e · inbound

Tensor induced gravitational waves cites this paper.

Tensor induced gravitational waves Confronting sound speed resonance with pulsar timing arrays

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-06T11:33:38.440462Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94538868-62b1-4364-9bbc-f483066aeb51 · 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 Confronting sound speed resonance with pulsar timing arrays

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-05-10T01:04:50.646810Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 6e8b7e16-6056-4f35-ac68-601c09cd01a5 · 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 Confronting sound speed resonance with pulsar timing arrays

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-02T15:56:58.470056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d4599b77-3f59-4e2a-9802-e5f0d90282b3 · 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 Confronting sound speed resonance with pulsar timing arrays

Reference 112

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.