Weibull thermodynamics: subexponential decay in the energy spectrum of cosmic-ray nuclei

DOI10.1016/J.PHYSA.2017.03.034zbMath1499.81094OpenAlexW2604872779MaRDI QIDQ2147881

Roman Tomaschitz

Publication date: 20 June 2022

Published in: Physica A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.physa.2017.03.034

zbMATH Keywords

entropy of stationary non-equilibrium ensemblesheat capacities of a non-equilibrated gas mixturemultiply broken power-law densities with Weibull cutoffsubexponential spectral decaythermodynamics of cosmic-ray nucleiWeibull entropy and excess entropy

Mathematics Subject Classification ID

Nuclear physics (81V35)

Related Items (2)

Multiply broken power-law densities as survival functions: an alternative to Pareto and lognormal fits ⋮ Partially polarized black-body radiation

Cites Work

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• Tachyonic Cherenkov emission from Jupiter's radio electrons
• Tachyonic Cherenkov radiation in the absorptive aether
• Tachyonic \(\gamma\)-ray spectra of active galactic nuclei: evidence for intrinsic spectral curvature
• The stationary non-equilibrium plasma of cosmic-ray electrons and positrons
• Ultra-relativistic nonthermal power-law ensembles: cosmic-ray electrons and positron fraction

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