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Title:	Gaisser-Venice5.pdf
Abstract:	Revised after corrections from Albrecht
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Handle:	Document-58521
Owner:	Site Administrator (User-2, admin:DocuShare)^DS
Create Date:	Sunday, July 24, 2011 08:30:08 AM CDT
Modified Date:	Sunday, July 24, 2011 08:30:08 AM CDT
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Abstract:	Greisen wanted to search for high energy neutrinos of astrophysical origin above the background of the steeper atmospheric neutrino spectrum. Because interactions of atmospheric neutrinos are the main background for proton decay, both detectors measured those neutrinos in as much detail as possible, including contained interactions of muon and electron neutrinos as well as ??-induced muons, both through-going and stopping. The distributions of neutrino energy that give rise to the signal in the detector are shown for three parent neutrino spectra: conventional atmospheric, prompt atmospheric and E?2 astrophysical neutrinos. The strong angular dependence of the conventional atmospheric ...
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File name:	Gaisser-Venice5.pdf
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Appears In:	Venice Neutrino Telescopes 15-18 March 2011
Preferred Version:	Gaisser-Venice5.pdf