Paper Citation Record · LEDGER

Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 inbound Pith citation observations for arXiv:2306.17239.

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

pith.paper-citation-record.v1
2306.17239 v4

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 17 of 17 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 17 of 17 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T13:07:10.848544Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T16:18:38.045763Z

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Outbound references

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Pith citing papers

Observation 0360b4a0-9092-4746-9bea-aebb3411ca5a · inbound

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

Pre-Big-Bang Cosmology Cannot Explain NANOGrav 15-year Signal Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-12T13:07:10.848544Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3814fe28-62bb-481c-a95c-e1644def8281 · inbound

Gravitational waves from supercooled phase transitions in conformal Majoron models of neutrino mass cites this paper.

Gravitational waves from supercooled phase transitions in conformal Majoron models of neutrino mass Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-11T23:21:32.210641Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a4c17587-77ea-4c7e-a1e4-ff3cf0177ff8 · inbound

PhaseTracer2: from the effective potential to gravitational waves cites this paper.

PhaseTracer2: from the effective potential to gravitational waves Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-11T21:15:41.989831Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09ca3e94-f746-4494-bc53-6f0279ae0f6e · inbound

Gravitational waves and dark matter with Witten effect cites this paper.

Gravitational waves and dark matter with Witten effect Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-10T20:03:21.569259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1a796917-6589-4c56-bcf5-b761be79b265 · inbound

Supercooled phase transitions in conformal dark sectors explain NANOGrav data cites this paper.

Supercooled phase transitions in conformal dark sectors explain NANOGrav data Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-10T18:16:28.585711Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ed2aa657-6b70-4bcb-97ed-8cdc45df30d2 · inbound

Supercooled Phase Transitions: Why Thermal History of Hidden Sector Matters in Analysis of Pulsar Timing Array Signals cites this paper.

Supercooled Phase Transitions: Why Thermal History of Hidden Sector Matters in Analysis of Pulsar Timing Array Signals Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T14:52:30.769729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 91fcf9b9-73c4-4663-a086-fa7e1d184d36 · inbound

Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison cites this paper.

Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-05T23:25:30.402157Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c52893f-c431-4ac9-ad7e-41dae80d295c · inbound

Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings cites this paper.

Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 6

Resolution: verified exact; arxiv_id, observed 2026-05-21T19:14:19.396224Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 99d4939d-9c29-4a1a-a47b-45d36126613b · inbound

Measuring gravitational wave spectrum from electroweak phase transition and Higgs self-couplings cites this paper.

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-04T00:32:11.225076Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6415b438-7a43-4100-8bdb-487a28f5961c · inbound

Beyond the Daisy Chain: Running and the 3D EFT View of Supercooled Phase Transitions cites this paper.

Beyond the Daisy Chain: Running and the 3D EFT View of Supercooled Phase Transitions Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-04T00:09:29.994163Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 78ca858e-ccf8-4e43-8c2c-32b151ead147 · inbound

Bayesian analysis of the complex singlet model with phase transition gravitational waves cites this paper.

Bayesian analysis of the complex singlet model with phase transition gravitational waves Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 6

Resolution: verified exact; arxiv_id, observed 2026-05-21T17:54:18.398047Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 4f50b21b-c59c-42bc-bc2d-55c649b3ca59 · inbound

Bayesian analysis of the complex singlet model with phase transition gravitational waves cites this paper.

Bayesian analysis of the complex singlet model with phase transition gravitational waves Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-03T20:05:41.978141Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 113f75b9-372c-49a5-a070-a6be214ac04b · inbound

Inflationary phase transitions in the early Universe: A Bayesian study with space-based gravitational-wave detectors cites this paper.

Inflationary phase transitions in the early Universe: A Bayesian study with space-based gravitational-wave detectors Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-02T17:45:17.064300Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cb34d17a-a929-4d48-82e3-74233415bc75 · inbound

Probing Dynamical Inverse Seesaw with Low-frequency Gravitational Waves cites this paper.

Probing Dynamical Inverse Seesaw with Low-frequency Gravitational Waves Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 100

Resolution: verified exact; arxiv_id, observed 2026-06-29T16:43:39.754452Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 55d625fe-7290-49da-9120-cef9345f257f · inbound

Search for High-Frequency Gravitational Waves via Geomagnetic Conversion with Radio Telescopes cites this paper.

Search for High-Frequency Gravitational Waves via Geomagnetic Conversion with Radio Telescopes Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 37

Resolution: verified exact; arxiv_id, observed 2026-07-03T16:18:38.047114Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation eda18067-08d9-4039-92da-b23c6e82cee6 · inbound

A critical look at low-scale cosmological phase transitions in the PTA era cites this paper.

A critical look at low-scale cosmological phase transitions in the PTA era Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 23

Resolution: verified exact; arxiv_id, observed 2026-07-03T09:27:48.890122Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation ddf1755b-1ac4-491b-882b-84e6e219fd89 · inbound

Cosmic string gravitational wave backgrounds at LISA: II. Reconstruction of conventional signals over astrophysical foregrounds cites this paper.

Cosmic string gravitational wave backgrounds at LISA: II. Reconstruction of conventional signals over astrophysical foregrounds Can supercooled phase transitions explain the gravitational wave background observed by pulsar timing arrays?

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-01T23:55:14.686679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.