Stochastic Gyroresonant Acceleration for Hard Electron Spectra of Blazars: Effect of Damping of Cascading Turbulence

Abstract

Stochastic acceleration of nonthermal electrons is investigated in the context of hard photon spectra of blazars. It is well known that this acceleration mechanism can produce a hard electron spectrum of $m\equiv \partial \ln n_{\mathrm{e}}(\gamma )/\partial \ln \gamma =2$ with the high-energy cutoff, called an ultrarelativistic Maxwellian-like distribution, where $n_{\mathrm{e}}(\gamma )$ is an electron energy spectrum. We revisit the formation of this characteristic spectrum, considering a particular situation where the electrons are accelerated through gyroresonant interaction with magnetohydrodynamic wave turbulence driven by the turbulent cascade. By solving kinetic equations of the turbulent fields, electrons, and photons emitted via the synchrotron self-Compton (SSC) process, we demonstrate that in the non-test-particle treatment, the formation of a Maxwellian-like distribution is prevented by the damping effect on the turbulent fields due to the electron acceleration, at least unless an extreme parameter value is chosen. Instead, a softer electron spectrum with the index of $m\approx -1$ is produced if the Kolmogorov-type cascade is assumed. The SSC spectrum that originates from the resultant softer electron spectrum is still hard, but somewhat softer and broader than the case of $m=2$. This change of achievable hardness should be noted when this basic particle acceleration scenario is tested with observations of hard photon spectra accurately.

20 pages, 3 figures, 1 table, accepted version with minor midifications

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• Acceleration of ultra-high energy cosmic rays in the early afterglows of gamma-ray bursts: concurrence of jet's dynamics and wave-particle interactions
• Extreme TeV BL Lacs: a self-consistent stochastic acceleration model
• Stochastic acceleration in Extreme TeV BL Lacs through MCMC