Diffraction of return time measures
Abstract
Letting denote an ergodic transformation of the unit interval and letting denote an observable, we construct the -weighted return time measure for a reference point as the weighted Dirac comb with support in and weights at , and if is non-invertible, then we set the weights equal to zero for all . Given such a Dirac comb, we are interested in its diffraction spectrum which emerges from the Fourier transform of its autocorrelation and analyse it for the dependence on the underlying transformation. For certain rapidly mixing transformations and observables of bounded variation, we show that the diffraction of consists of a trivial atom and an absolutely continuous part, almost surely with respect to . This contrasts what occurs in the setting of regular model sets arising from cut and project schemes and deterministic incommensurate structures. As a prominent example of non-mixing transformations, we consider the family of rigid rotations with rotation number . In contrast to when is mixing, we observe that the diffraction of is pure point, almost surely with respect to . Moreover, if is irrational and the observable is Riemann integrable, then the diffraction of is independent of . Finally, for a converging sequence of rotation numbers, we provide new results concerning the limiting behaviour of the associated diffractions.
Cite
@article{arxiv.1801.07608,
title = {Diffraction of return time measures},
author = {Marc Kesseböhmer and Arne Mosbach and Tony Samuel and Malte Steffens},
journal= {arXiv preprint arXiv:1801.07608},
year = {2019}
}
Comments
11 pages, 2 figures