On the high-energy protons regular acceleration in the Fermi Bubbles
Istomin Ya. N., Gunya A. A

TL;DR
This paper models the electromagnetic fields in the Fermi bubbles, showing they can accelerate protons to ultra-high energies (~10^17 eV), explaining gamma-ray and neutrino emissions from the Galactic center.
Contribution
It introduces a model of electromagnetic fields in the Fermi bubbles that accounts for regular proton acceleration to ultra-high energies, linking to observed high-energy phenomena.
Findings
Protons can be accelerated up to ~10^17 eV in Fermi bubbles.
Electromagnetic field structure resembles that of AGN jets.
Model explains gamma-ray and neutrino emissions from the Galactic center.
Abstract
We propose the model of the global structure of the electromagnetic fields in the Fermi bubbles (FBs), which makes possible the proton regular acceleration up to ultra-high energies. The poloidal and the toroidal magnetic fields, as well as the radial electric field, turn to have a structure similar to fields that exist in jets ejected out from active galactic nuclei (AGN). A powerful source of relativistic particles observed in the centre of the Galaxy and associated with the rotating supermassive black hole (SMBH) Sgr A* can energize the FB and keeps its active for a long time. The absence of accretion onto a BH and thus the absence of a relativistic jet does not mean that there is no loss of rotational energy of BH. In the case of FB, the energy lost by BH can keep the FB activity. The regular FBs structure could be formed by inheritance from a relativistic jet that presumably…
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