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Multimessenger study of the Fermi bubbles: Very high energy gamma rays and neutrinos
2015
Physical Review D
The Fermi Bubbles have been imaged in sub-TeV gamma rays at Fermi-LAT, and, if their origin is hadronic, they might have been seen with low statistics in ∼ 0.1- 1 PeV neutrinos at IceCube. We discuss the detectability of these objects at the new High Altitude Water Cherenkov (HAWC) gamma ray detector. HAWC will view the North Bubble for ∼ 2-3 hours a day, and will map its spectrum at 0.1-100 TeV. For the hard primary proton spectrum required to explain five events at IceCube, a high
doi:10.1103/physrevd.92.021301
fatcat:sj24skbecbcllbcf4gt45muxh4