Evidence for a hadronic origin of the Fermi Bubbles and the Galactic Excess
Wim de Boer, Iris Gebauer, Simon Kunz, Alexander Neumann

TL;DR
This paper provides evidence that the Fermi Bubbles and the Galactic Center excess are of hadronic origin, linked to cosmic rays trapped in supernova remnants and dense molecular clouds, challenging dark matter explanations.
Contribution
It demonstrates a hadronic origin for the Fermi Bubbles and Galactic excess, connecting gamma-ray emission to cosmic rays in supernova remnants and molecular clouds, and refutes dark matter as the cause.
Findings
Bubble-like emission is present in the Galactic plane and halo.
The spectral shape matches cosmic rays trapped in sources.
The Galactic Center excess is an artifact of line-of-sight effects.
Abstract
The Fermi-LAT data revealed giant bubbles of emission above and below the Galactic plane with an energy spectrum significantly harder than seen from other directions. How the bubbles connect to the Galactic plane is unclear. We find that bubble-like emission is not only found in the halo, but it is strongly present in the Galactic plane as well with a morphology close to the spatial distribution of the 1.8 MeV gamma-ray line from 26Al, a radioactive nucleus synthesized in SNRs. In addition, the spectral shape of this hard component coincides with the predicted spectrum from cosmic rays trapped in sources. Hence, we propose that the bubble-like emission in the plane has a hadronic origin, which arises from SCRs. The bubbles in the halo have the same energy spectrum, which suggests that they are outflows from the plane with the gamma-rays arising from hadronic interactions of protons…
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