Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Confronting sound speed resonance with pulsar timing arrays
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2307.08687.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T20:02:43.338621Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-22T01:55:55.414745Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 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 2026-08-18T06:34:40.430872+00:00.
Observation 37c9c4c7-8a66-4f90-b4a6-2576692093d4 · 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 Confronting sound speed resonance with pulsar timing arrays
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T20:02:43.338621Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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 2026-08-18T06:34:40.430872+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 2026-08-18T06:34:40.430872+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.