Modeling the gamma-ray emission in the Galactic Center with a fading cosmic-ray accelerator
Ruo-Yu Liu, Xiang-Yu Wang, Anton Prosekin, Xiao-Chuan Chang

TL;DR
This paper proposes a model where a fading cosmic-ray accelerator, possibly a tidal disruption event near the supermassive black hole, explains gamma-ray emissions in the Galactic Center, matching observations of different regions.
Contribution
It introduces a self-consistent fading accelerator model, likely a TDE blast wave, to explain gamma-ray spectra and cosmic-ray profiles in the Galactic Center.
Findings
The model reproduces gamma-ray spectra of the CMZ and HESS J1745-290.
It matches the cosmic-ray energy density profile in the CMZ.
A fading accelerator can explain both recent and past cosmic-ray injections.
Abstract
Recent HESS observations of the ~200 pc scale diffuse gamma-ray emission from the central molecular zone (CMZ) suggest the presence of a PeV cosmic-ray accelerator (PeVatron) located in the inner 10 pc region of the Galactic Center. Interestingly, the gamma-ray spectrum of the point-like source (HESS J1745-290) in the Galactic Center shows a cutoff at ~10 TeV, implying a cutoff around 100 TeV in the cosmic-ray proton spectrum. Here we propose that the gamma-ray emission from the inner and the outer regions may be explained self-consistently by run-away protons from a single, yet fading accelerator. In this model, gamma rays from the CMZ region are produced by protons injected in the past, while gamma rays from the inner region are produced by protons injected more recently. We suggest that the blast wave formed in a tidal disruption event (TDE) caused by the supermassive black hole (Sgr…
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