Non-Thermal Radiation from the Inner Galaxy
Roland M. Crocker

TL;DR
This paper reviews the current understanding of non-thermal radiation from the Galactic Center and Inner Galaxy, discussing potential dark matter signals, energetic astrophysical phenomena, and recent discoveries like the Fermi Bubbles.
Contribution
It provides a comprehensive overview of non-thermal emissions in the Inner Galaxy, emphasizing the complexity of interpreting signals and highlighting recent findings such as the Fermi Bubbles.
Findings
Fermi Bubbles extend ~7 kpc from the Galactic nucleus.
Microwave emission coincides with the Fermi Bubbles.
Debate exists on whether the Bubbles result from black hole activity or star formation.
Abstract
I review our current state of knowledge about non-thermal radiation from the Galactic Centre (GC) and Inner Galaxy. Definitionally, the Galactic nucleus is at the bottom of the Galaxy's gravitational well, rendering it a promising region to seek the signatures of dark matter decay or annihilation. It also hosts, however, the Milky Way's resident supermassive black hole and up to 10% of current massive star formation in the Galaxy. Thus the Galactic nucleus is a dynamic and highly-energized environment implying that extreme caution must be exercised in interpreting any unusual or unexpected signal from (or emerging from) the region as evidence for dark matter-related processes. One spectacular example of an `unexpected' signal is the discovery within the last few years of the `Fermi Bubbles' and, subsequently, their polarised radio counterparts. These giant lobes extend ~7 kpc from the…
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