Superstatistics in the context of relativity

The statistical properties of space and astrophysical environments often exhibit heavy-tailed distributions, reflecting deviations from thermal equilibrium. These distributions can often be represented as a superposition of statistics, i.e., superstatistics. However, the heavy-tailed nature of these...

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Main Author: Kamel Ourabah
Format: Article
Language:English
Published: American Physical Society 2025-08-01
Series:Physical Review Research
Online Access:http://doi.org/10.1103/7j5q-hxm2
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author Kamel Ourabah
author_facet Kamel Ourabah
author_sort Kamel Ourabah
collection DOAJ
description The statistical properties of space and astrophysical environments often exhibit heavy-tailed distributions, reflecting deviations from thermal equilibrium. These distributions can often be represented as a superposition of statistics, i.e., superstatistics. However, the heavy-tailed nature of these distributions can lead to significant nonphysical contributions from unrealistic superluminal particles, thereby biasing thermodynamic properties and the overall dynamics. In this work, we first quantify these unphysical effects for key thermodynamic quantities, like pressure and entropy, within the three universality classes of superstatistics, and we discuss a regularized formulation that resolves the issue without requiring a fully relativistic treatment. We then develop a relativistic extension of superstatistics by generalizing the Maxwell-Jüttner distribution to nonequilibrium settings. We derive the thermodynamic properties of the resulting distributions and analyze their asymptotic behavior in the weakly relativistic and ultrarelativistic limits. Finally, we apply our model to observational data of solar energetic protons and show that it provides an excellent fit, demonstrating its relevance for describing the statistical properties of high-energy astrophysical systems.
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spelling doaj-art-e968d8c03694485d8a610d23a3d56afc2025-08-25T14:14:03ZengAmerican Physical SocietyPhysical Review Research2643-15642025-08-017303319010.1103/7j5q-hxm2Superstatistics in the context of relativityKamel OurabahThe statistical properties of space and astrophysical environments often exhibit heavy-tailed distributions, reflecting deviations from thermal equilibrium. These distributions can often be represented as a superposition of statistics, i.e., superstatistics. However, the heavy-tailed nature of these distributions can lead to significant nonphysical contributions from unrealistic superluminal particles, thereby biasing thermodynamic properties and the overall dynamics. In this work, we first quantify these unphysical effects for key thermodynamic quantities, like pressure and entropy, within the three universality classes of superstatistics, and we discuss a regularized formulation that resolves the issue without requiring a fully relativistic treatment. We then develop a relativistic extension of superstatistics by generalizing the Maxwell-Jüttner distribution to nonequilibrium settings. We derive the thermodynamic properties of the resulting distributions and analyze their asymptotic behavior in the weakly relativistic and ultrarelativistic limits. Finally, we apply our model to observational data of solar energetic protons and show that it provides an excellent fit, demonstrating its relevance for describing the statistical properties of high-energy astrophysical systems.http://doi.org/10.1103/7j5q-hxm2
spellingShingle Kamel Ourabah
Superstatistics in the context of relativity
Physical Review Research
title Superstatistics in the context of relativity
title_full Superstatistics in the context of relativity
title_fullStr Superstatistics in the context of relativity
title_full_unstemmed Superstatistics in the context of relativity
title_short Superstatistics in the context of relativity
title_sort superstatistics in the context of relativity
url http://doi.org/10.1103/7j5q-hxm2
work_keys_str_mv AT kamelourabah superstatisticsinthecontextofrelativity