Leptonic and Hadronic Radiative Processes in Supermassive-Black-Hole Jets
Matteo Cerruti

TL;DR
This paper reviews the current understanding of radiative emission processes in jets launched by supermassive black holes, highlighting key mechanisms of particle acceleration and radiation in these astrophysical phenomena.
Contribution
It provides a comprehensive overview of the physical mechanisms behind radiative processes in supermassive-black-hole jets, summarizing recent advances and open questions.
Findings
Summarizes key radiative emission mechanisms in black-hole jets.
Highlights current challenges in understanding jet particle acceleration.
Reviews observational evidence supporting theoretical models.
Abstract
Supermassive black holes lying in the center of galaxies can launch relativistic jets of plasma along their polar axis. The physics of black-hole jets is a very active research topic in astrophysics, owing to the fact that many questions remain open on the physical mechanisms of jet launching, of particle acceleration in the jet, and on the radiative processes. In this work I focus on the last item, and present a review of the current understanding of radiative emission processes in supermassive-black-hole jets.
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