Ultra-relativistic nonthermal power-law ensembles: cosmic-ray electrons and positron fraction

DOI10.1016/J.PHYSA.2013.09.068zbMATH Open1395.81311OpenAlexW2033106634MaRDI QIDQ1782505

Roman Tomaschitz

Publication date: 20 September 2018

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

Full work available at URL: https://doi.org/10.1016/j.physa.2013.09.068

zbMATH Keywords

cosmic-ray electron/positron fluxhybrid quantum ensemblesnonthermal power-law distributionsquantization of stationary non-equilibrium ensemblesspectral Fitting of a two-component plasma with power-law densitiesstability and extensivity of entropyultra-relativistic electron-positron plasma

Mathematics Subject Classification ID

Atomic physics (81V45) Quantum dynamics and nonequilibrium statistical mechanics (general) (82C10)

Cites Work

• Tachyonic \(\gamma\)-ray spectra of active galactic nuclei: evidence for intrinsic spectral curvature
• Quantum statistics of superluminal radiation
• Bose-Einstein condensation in the three-sphere and in the infinite slab: analytical results

Related Items (4)

The stationary non-equilibrium plasma of cosmic-ray electrons and positrons ⋮ Weibull thermodynamics: subexponential decay in the energy spectrum of cosmic-ray nuclei ⋮ NATURE OF THE COSMIC RAY POWER LAW EXPONENTS ⋮ COOLING OF RELATIVISTIC ELECTRONS IN TEV BLAZARS: CLUES FROM MULTIWAVELENGTH SPECTRA

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