2020
DOI: 10.1007/s00023-020-00985-3
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On the Correlation Between Nodal and Nonzero Level Sets for Random Spherical Harmonics

Abstract: We study the correlation between the nodal length of random spherical harmonics and the length of a nonzero level set. We show that the correlation is asymptotically zero, while the partial correlation after removing the effect of the random $$L^2$$ L 2 -norm of the eigenfunctions is asymptotically one.

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Cited by 9 publications
(8 citation statements)
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“…Canzani and Hanin (2020) studied the universality phenomenon in general Riemannian manifolds. The reader can find results on arithmetic random waves defined on the flat torus (Cammarota, 2019;Dalmao et al, 2019) and on random spherical harmonics in Cammarota and Marinucci (2019); Fantaye et al (2019); Marinucci and Rossi (2021) and references therein, see also Rossi (2019) for a survey on both subjects. The nodal sets of Berry's planar random waves, i.e.…”
Section: Introductionmentioning
confidence: 99%
“…Canzani and Hanin (2020) studied the universality phenomenon in general Riemannian manifolds. The reader can find results on arithmetic random waves defined on the flat torus (Cammarota, 2019;Dalmao et al, 2019) and on random spherical harmonics in Cammarota and Marinucci (2019); Fantaye et al (2019); Marinucci and Rossi (2021) and references therein, see also Rossi (2019) for a survey on both subjects. The nodal sets of Berry's planar random waves, i.e.…”
Section: Introductionmentioning
confidence: 99%
“…While it is easy to check that fact via the cross-correlation route, it is intuitively clear from the corresponding result for the excursion sets [42]. Because of that it was also later observed [41] that the projection of the non-nodal length at level t = 0 to the 2nd Wiener chaos, dominating the fluctuations of the level curve length, is, up to the factor √ ce −t 2 /2 t 2 , equal to the squared norm of T ℓ . This is in contrast to the nodal case, that is invariant to products by a constant, hence the projection onto the 2nd Wiener chaos vanishes precisely, and the fluctuations of the nodal length are dominated by its projection onto the 4th Wiener chaos.…”
Section: Nodal Volumementioning
confidence: 79%
“…Part (ii) contains a general version of the chaos cancellation phenomenon observed e.g. in Wigman (2010); Marinucci and Rossi (2021); Krishnapur et al (2013); Dalmao et al (2019); Marinucci et al (2016); Nourdin et al (2019); Cammarota (2019). Its proof is deferred to Appendix A.…”
Section: Wiener Chaos and Abstract Cancellation Phenomenamentioning
confidence: 99%
“…where g 2 L 2 (Z) := Z g(z) 2 µ(dz), (see also Rossi, 2021 andCammarota et al, 2020). In particular, the second order chaotic projection of J is a linear combination of the centred square (random) norms of the fields X…”
Section: Wiener Chaos and Abstract Cancellation Phenomenamentioning
confidence: 99%