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

Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Martí i Franquès 1, E08028 Barcelona, Spain
Galaxies 2020, 8(4), 72; https://doi.org/10.3390/galaxies8040072
Received: 3 August 2020 / Revised: 16 September 2020 / Accepted: 22 September 2020 / Published: 1 October 2020
(This article belongs to the Special Issue Jet Physics of Accreting Super Massive Black Holes)
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. View Full-Text
Keywords: relativistic Jets; active galactic nuclei; theoretical emission models relativistic Jets; active galactic nuclei; theoretical emission models
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MDPI and ACS Style

Cerruti, M. Leptonic and Hadronic Radiative Processes in Supermassive-Black-Hole Jets. Galaxies 2020, 8, 72. https://doi.org/10.3390/galaxies8040072

AMA Style

Cerruti M. Leptonic and Hadronic Radiative Processes in Supermassive-Black-Hole Jets. Galaxies. 2020; 8(4):72. https://doi.org/10.3390/galaxies8040072

Chicago/Turabian Style

Cerruti, Matteo. 2020. "Leptonic and Hadronic Radiative Processes in Supermassive-Black-Hole Jets" Galaxies 8, no. 4: 72. https://doi.org/10.3390/galaxies8040072

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