Hard particle spectra from parallel shocks due to turbulence transmission

TL;DR

This paper explores how turbulence transmission through shock fronts affects particle acceleration, leading to harder energy spectra than traditional models predict, with implications for astrophysical sources like AGN and microquasars.

Contribution

It introduces the turbulence transmission scenario in parallel shocks, analyzing its impact on particle spectra and discussing its applicability in various astrophysical environments.

Findings

Turbulence transmission can significantly alter the effective compression ratio.

Harder particle energy spectra result from turbulence transmission.

Implications for particle acceleration in AGN and microquasar environments.

Abstract

If taken into account, the transmission of the particle-scattering turbulence --in addition to just the particles-- through the shock front can change the effective compression ratio felt by the accelerating particles significantly from the compression of the underlying plasma. This can lead to significantly harder energy spectra than what are traditionally predicted assuming frozen-in turbulence. I consider the applicability and limitations of turbulence transmission scenario in parallel shock waves of different thickness, its consequences in AGN and microquasar environments, and discuss the possible effects to the spectrum of the accelerated particles.