20.500.12556/RUNG-2836-d870809f-c377-ae9e-aa60-e9573d5e3aa7
Multi-messenger study of the Fermi Bubbles
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. I discuss the detectability of these objects at the new High Altitude Water Cherenkov (HAWC). 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 significance detection at HAWC will be achieved in less than 30 days. I will discuss how the combination of results at HAWC and IceCube will substantiate the hadronic model, or constrain its spectral parameters and how sensitive Cherenkov Telescope Array(CTA) is to the bubbles.
Fermi Bubbles
neutrinos
HAWC
true
true
false
Angleški jezik
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2016-12-06 09:30:05
2016-12-06 10:03:44
2023-06-13 14:24:35
0000-00-00 00:00:00
0
0
2016
Anton Pannekoek Instituut, University of Amsterdam, the Netherlands
0000-00-00
NiDoloceno
NiDoloceno
NiDoloceno
0000-00-00
0000-00-00
0000-00-00
4594939
URN:SI:UNG:REP:GJMX3VIO
Univerza v Novi Gorici
0
2
0