Speaker
Andrea Massari
(S)
Description
The Fermi γ-ray Space Telescope has observed the sky since 2008. Dark matter annihilations or decays contribute to the measured diffuse gamma-ray background flux. We present conservative bounds on annihilation cross section or decay lifetime. We consider DM annihilation/decay into 12 different Standard Model final states, 3 DM density profiles and 2 GeV < m_{DM} < 10 TeV , performing no astrophysical foreground modeling.
Authors
Andrea Massari
(S)
Eder Izaguirre
(Stanford University/SLAC)
Prof.
Elliott Bloom
(KIPAC-SLAC, Stanford University)
Rouven Essig
(S)
