Solar neutrino records: Gauss or non-Gauss is the question
A. Haubold, H. J. Haubold, D. Kumar

TL;DR
This paper investigates the variability of solar neutrino flux over time using statistical analysis, exploring whether the data follow Gaussian or non-Gaussian distributions, with implications for understanding underlying physical processes.
Contribution
It applies Standard Deviation Analysis and Diffusion Entropy Analysis to Super-Kamiokande-I data, revealing potential Levy-type distribution behavior and linking it to non-equilibrium statistical mechanics.
Findings
Data exhibit scaling behavior.
Possible Levy-type distribution.
Links to non-equilibrium statistical mechanics.
Abstract
This article discusses the possible variation of the solar neutrino flux over time in the records of Super-Kamiokande-I and the relation to non-equilibrium statistical mechanics and the entropic pathway model. The scaling behavior of the Super-Kamiokande-I time series is investigated utilizing Standard Deviation Analysis and Diffusion Entropy Analysis. The data set exhibit scaling behavior and may follow Levy-type probability distribution function.
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Taxonomy
TopicsStatistical Mechanics and Entropy · Complex Systems and Time Series Analysis · Climate variability and models
