Issue |
A&A
Volume 664, August 2022
|
|
---|---|---|
Article Number | L14 | |
Number of page(s) | 4 | |
Section | Letters to the Editor | |
DOI | https://doi.org/10.1051/0004-6361/202243915 | |
Published online | 25 August 2022 |
Letter to the Editor
Resonant energization of particles by radio AGN
1
Institute for Fusion Studies, The University of Texas at Austin, Austin, TX 78712, USA
e-mail: mahajan@mail.utexas.edu
2
School of Physics, Free University of Tbilisi, 0183 Tbilisi, Georgia
e-mail: z.osmanov@freeuni.edu.ge
3
E. Kharadze Georgian National Astrophysical Observatory, Abastumani 0301, Georgia
Received:
1
May
2022
Accepted:
9
June
2022
Aims. A new mechanism of particle acceleration, based on the resonant interaction of a classical electromagnetic wave (EM) with a quantum wave (associated with a relativistic particle), is explored.
Methods. In a model illustrative calculation, we study the fate of a Klein Gordon wave subjected to the intense radio frequency waves generated in the vicinity of an active galactic nuclei (AGN). In the framework of the paper, we examine a quantum wave associated with a relativistic particle, and it is shown that the group velocity of the wave approaches the speed of light, implying that the particles resonantly exchange energy with EM waves, eventually leading to acceleration of particles to very high energies.
Results. For typical parameters of under accreting Eddington radio AGN, it is shown that the resonant energization could catapult particles to extreme energies ∼1016−20 eV.
Key words: acceleration of particles / galaxies: active / plasmas / galaxies: jets
© S. M. Mahajan and Z. N. Osmanov 2022
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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