Description
We discuss the possibility that the IceCube neutrino telescope might be observing the Fermi bubbles. If the bubbles discovered in gamma rays originate from accelerated protons, they should be strong emitters of high energy (≳ GeV) neutrinos. These neutrinos are detectable as showerlike or tracklike events at a Km3 neutrino observatory.
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- Lunardini, Cecilia (Author)
- Razzaque, Soebur (Author)
- Theodoseau, Kristopher (Author)
- Yang, Lili (Author)
- College of Liberal Arts and Sciences (Contributor)
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2014-07-21
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- Digital object identifier: 10.1103/PhysRevD.90.023016
- Identifier TypeInternational standard serial numberIdentifier Value2470-0029
- Identifier TypeInternational standard serial numberIdentifier Value2470-0010
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- Copyright 2014 by the American Physical Society. View the article as published at http://dx.doi.org/10.1103/PhysRevD.90.023016, opens in a new window
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Lunardini, Cecilia, Razzaque, Soebur, Theodoseau, Kristopher T., & Yang, Lili (2014). Neutrino events at IceCube and the Fermi bubbles. PHYSICAL REVIEW D, 90(2), 023016. http://dx.doi.org/10.1103/PhysRevD.90.023016