A multi-messenger study of the Fermi Bubbles: very high energy gamma rays and neutrinos
arXiv:1504.07033 · doi:10.1103/PhysRevD.92.021301
Abstract
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 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 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. The combination of results at HAWC and IceCube will substantiate the hadronic model, or constrain its spectral parameters.
5 pages, 4 figures, references added, accepted for publication in PRD Rapid Communication
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Cited by in corpus (10)
- Galactic Neutrinos in the TeV to PeV Range
- Gamma-ray bounds from EAS detectors and heavy decaying dark matter constraints
- Search for Very High Energy Gamma Rays from the Northern Bubble Region with HAWC
- IceCube and HAWC constraints on very-high-energy emission from the Fermi bubbles
- Constraints on very high energy gamma-ray emission from the Fermi Bubbles with future ground-based experiments
- How Unequal Fluxes of High Energy Astrophysical Neutrinos and Antineutrinos can Fake New Physics
- A lepto-hadronic model of gamma rays from the Eta Carinae and prospects for neutrino telescopes
- Emission from hadronic and leptonic processes in galactic jet-driven bubbles
- The Dawn of Multi-Messenger Astronomy
- Results from the ANTARES Neutrino Telescope