A possible origin of gamma rays from the Fermi Bubbles
Satyendra Thoudam

TL;DR
This paper explores the hypothesis that the gamma rays from the Fermi Bubbles originate from Galactic cosmic-ray protons interacting with plasma, producing gamma rays and secondary emissions observed across multiple wavelengths.
Contribution
It proposes a model where cosmic-ray protons diffusing through the Galaxy produce the observed emissions via interactions within the bubbles, offering a potential explanation for their origin.
Findings
Cosmic-ray protons can produce gamma rays through $ ext{π}^0$ decay.
Secondary electrons/positrons generate radio and microwave synchrotron emissions.
The model aligns with observed correlations across gamma-ray, radio, and X-ray data.
Abstract
One of the most exciting discoveries of recent years is a pair of gigantic gamma-ray emission regions, the so-called Fermi bubbles, above and below the Galactic center. The bubbles, discovered by the Fermi space telescope, extend up to in Galactic latitude and are wide in Galactic longitude. The gamma-ray emission is also found to correlate with radio, microwave and X-rays emission. The origin of the bubbles and the associated non-thermal emissions are still not clearly understood. Possible explanations for the non-thermal emission include cosmic-ray injection from the Galactic center by high speed Galactic winds/jets, acceleration by multiple shocks or plasma turbulence present inside the bubbles, and acceleration by strong shock waves associated with the expansion of the bubbles. In this paper, I will discuss the possibility that the gamma-ray emission…
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