2nd-order Fermi acceleration as the origin of the Fermi bubbles
Philipp Mertsch, Subir Sarkar (Oxford)

TL;DR
This paper proposes that stochastic 2nd-order Fermi acceleration by plasma wave turbulence inside the Fermi bubbles explains their gamma-ray emission, sharp edges, and surface brightness, offering an alternative to shock acceleration models.
Contribution
It introduces a novel model where plasma turbulence causes stochastic acceleration throughout the bubbles, accounting for observed gamma-ray features.
Findings
Almost constant gamma-ray surface brightness achieved
Reproduction of sharp bubble edges
Spatial variation of electron spectral index modeled
Abstract
Gamma-ray data from Fermi-LAT show a bi-lobular structure extending up to 50 degrees above and below the Galactic centre, coincident with a possibly related structure in the ROSAT X-ray map which presumably originated in some energy release close to the centre a few million years ago. It has been argued that the gamma-rays arise due to inverse Compton scattering of relativistic electrons accelerated at plasma shocks present in the bubbles. We explore the alternative possibility that the relativistic electrons undergo stochastic 2nd-order Fermi acceleration in the entire volume of the bubbles by plasma wave turbulence. This turbulence is generated behind the outer shock and propagates into the bubble volume, leading to a non-trivial spatial variation of the electron spectral index. Rather than a constant volume emissivity as predicted in other models we find an almost constant surface…
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