Resonant energization of particles by radio AGN

Abstract

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. 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. For typical parameters of under accreting Eddington radio AGN, it is shown that the resonant energization could catapult particles to extreme energies $\sim 10^{16-20}$eV.

4 pages, 2 figures

References in corpus (5)

• Particle acceleration in strong MHD turbulence
• The Effect of Transient Accretion on the Spin-Up of Millisecond Pulsars
• On the efficiency of particle acceleration by rotating magnetospheres in AGN
• Relativistic Particle Transport and Acceleration in Structured Plasma Turbulence
• Extremely efficient Zevatron in rotating AGN magnetospheres