Synchrotron-limited particle acceleration in relativistic shearing flows

Fermi-type shear particle acceleration is a promising mechanism for sustaining ultrarelativistic particles along the kiloparsec scale jets in active galactic nuclei. We explore the possibility of synchrotron-limited electron acceleration in mildly relativistic shearing flows and present numerical so...

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Hauptverfasser: Rieger, Frank M. (VerfasserIn) , Duffy, Peter (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2025 July 29
In: The astrophysical journal
Year: 2025, Jahrgang: 988, Heft: 2, Pages: 1-5
ISSN:1538-4357
DOI:10.3847/1538-4357/adec67
Online-Zugang:Verlag, kostenfrei, Volltext: https://doi.org/10.3847/1538-4357/adec67
Verlag, kostenfrei, Volltext: https://iopscience.iop.org/article/10.3847/1538-4357/adec67
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Verfasserangaben:Frank M. Rieger and Peter Duffy
Beschreibung
Zusammenfassung:Fermi-type shear particle acceleration is a promising mechanism for sustaining ultrarelativistic particles along the kiloparsec scale jets in active galactic nuclei. We explore the possibility of synchrotron-limited electron acceleration in mildly relativistic shearing flows and present numerical solutions to the corresponding particle transport equation. We compare our findings with analytical calculations to infer an effective electron cutoff energy, and discuss the relationship to a simplified box model treatment. The results show that mildly relativistic large-scale jets offer a suitable environment for distributed electron acceleration beyond Lorentz factors of γe ∼ 108.
Beschreibung:Gesehen am 08.12.2025
Beschreibung:Online Resource
ISSN:1538-4357
DOI:10.3847/1538-4357/adec67