scholarly journals Perspective on dark matter annihilation limits from the LHAASO gamma-ray observation of dwarf Spheroidal galaxies

2019 ◽  
Author(s):  
Xiaojun Bi ◽  
Su-Jie Lin ◽  
Peng-Fei Yin
Galaxies ◽  
2018 ◽  
Vol 6 (3) ◽  
pp. 92
Author(s):  
Man Chan

Recently, many studies indicate that the GeV gamma ray excess signal from the central Milky Way can be best explained by ∼40–50 GeV dark matter annihilating via the b b ¯ channel. However, this model appears to be disfavored by the recent Fermi-LAT data for dwarf spheroidal galaxies and the constraint from synchrotron radiation. In this article, we describe a consistent picture to relieve the tensions between the dark matter annihilation model and the observations. We show that a baryonic feedback process is the key to alleviate the tensions and the ∼40–50 GeV dark matter model is still the best one to account for the GeV gamma ray excess in the Milky Way.


2015 ◽  
Vol 453 (1) ◽  
pp. 849-867 ◽  
Author(s):  
V. Bonnivard ◽  
C. Combet ◽  
M. Daniel ◽  
S. Funk ◽  
A. Geringer-Sameth ◽  
...  

2018 ◽  
Vol 853 (2) ◽  
pp. 154 ◽  
Author(s):  
A. Albert ◽  
R. Alfaro ◽  
C. Alvarez ◽  
J. D. Álvarez ◽  
R. Arceo ◽  
...  

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