pith:2HXK5YCC
Are PTA measurements sensitive to gravitational wave non-Gaussianities?
PTA data after decorrelation cannot distinguish Gaussian from non-Gaussian gravitational wave backgrounds without strong assumptions.
arxiv:2605.05157 v2 · 2026-05-06 · astro-ph.CO · astro-ph.HE · gr-qc · hep-ph
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Claims
even in an idealized signal-dominated setup, after decorrelating data to avoid spurious detections, statistical tests applied to PTA data cannot distinguish between Gaussian and non-Gaussian GWBs in a model-agnostic way. In particular, without making strong assumptions on the GW spectrum or the properties of the population, the sensitivity to any distinctive non-Gaussian feature is washed out.
The conclusion depends on an idealized signal-dominated setup together with the assumption that decorrelation fully removes spurious correlations without erasing genuine non-Gaussian information; the result is stated to hold only in the absence of strong prior assumptions on spectrum or population.
PTA statistical tests lose sensitivity to non-Gaussian GW features after decorrelation and cannot distinguish them model-agnostically.
Receipt and verification
| First computed | 2026-06-19T16:10:38.368361Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/2HXK5YCCEBH2RGV3Z5MQUHAGX7 \
| jq -c '.canonical_record' \
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Canonical record JSON
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