We present a generalization of the representation in plane waves of Dirac delta,ix ϵ e ix , x being any real number, for real values of q within the interval ͓1,2͓. Concomitantly, with the development of these new representations of Dirac delta, we also present two new families of representations of the transcendental number . Incidentally, we remark that the q-plane wave form which emerges, namely, e q ikx , is normalizable for 1 Ͻ q Ͻ 3, in contrast to the standard one, e ikx , which is not.
A wide class of physical distributions appears to follow the q-Gaussian form,
which plays the role of attractor according to a Central Limit Theorem
generalized in the presence of specific correlations between the relevant
random variables. In the realm of this theorem, a q-generalized Fourier
transform plays an important role. We introduce here a method which univocally
determines a distribution from the knowledge of its q-Fourier transform and
some supplementary information. This procedure involves a recently
q-generalized Dirac delta and the class of functions on which it acts. The
present method conveniently extends the inverse of the standard Fourier
transform, and is therefore expected to be very useful in the study of many
complex systems.Comment: 6 pages, 3 figures. To appear in Physics Letters
The search for patterns in time series is a very common task when dealing with complex systems. This is usually accomplished by employing a complexity measure such as entropies and fractal dimensions. However, such measures usually only capture a single aspect of the system dynamics. Here, we propose a family of complexity measures for time series based on a generalization of the complexity-entropy causality plane. By replacing the Shannon entropy by a monoparametric entropy (Tsallis q entropy) and after considering the proper generalization of the statistical complexity (q complexity), we build up a parametric curve (the q-complexity-entropy curve) that is used for characterizing and classifying time series. Based on simple exact results and numerical simulations of stochastic processes, we show that these curves can distinguish among different long-range, short-range, and oscillating correlated behaviors. Also, we verify that simulated chaotic and stochastic time series can be distinguished based on whether these curves are open or closed. We further test this technique in experimental scenarios related to chaotic laser intensity, stock price, sunspot, and geomagnetic dynamics, confirming its usefulness. Finally, we prove that these curves enhance the automatic classification of time series with long-range correlations and interbeat intervals of healthy subjects and patients with heart disease.
It was recently proven [Hilhorst, JSTAT, P10023 (2010)] that the q-generalization of the Fourier transform is not invertible in the full space of probability density functions for q > 1. It has also been recently shown that this complication disappears if we dispose of the q-Fourier transform not only of the function itself, but also of all of its shifts [Jauregui and Tsallis, Phys. Lett. A 375, 2085 (2011)]. Here we show that another road exists for completely removing the degeneracy associated with the inversion of the q-Fourier transform of a given probability density function. Indeed, it is possible to determine this density if we dispose of some extra information related to its q-moments.
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