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• W2030793224 abstract "Context.In powerful cosmic nonthermal radiation sources with dominant magnetic-field self generation, the generation of magnetic fields at almost equipartition strength by relativistic plasma instabilities operates as fast as the acceleration or injection of ultra-high energy radiating electrons and hadrons in these sources. Consequently, the magnetic field strength becomes time-dependent and adjusts itself to the actual kinetic energy density of the radiating electrons in these sources. This coupling of the magnetic field and the magnetic field energy density to the kinetic energy of the radiating particles changes both the synchrotron emissivity and the intrinsic temporal evolution of the relativistic particle energy spectrum after injection." @default.
• W2030793224 created "2016-06-24" @default.
• W2030793224 creator A5012928335 @default.
• W2030793224 creator A5035724494 @default.
• W2030793224 date "2007-09-24" @default.
• W2030793224 modified "2023-10-16" @default.
• W2030793224 title "Nonlinear radiative cooling of relativistic particles under equipartition conditions" @default.
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• W2030793224 doi "https://doi.org/10.1051/0004-6361:20078088" @default.
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