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Title:	GaisserCERN.pdf
Abstract:	Proceedings of UHECR-2012 with corrections from Chang Hyon and Spencer
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Handle:	Document-61645
Owner:	Site Administrator (User-2, admin:DocuShare)^DS
Create Date:	Thursday, July 19, 2012 08:13:48 AM CDT
Modified Date:	Thursday, July 19, 2012 08:13:48 AM CDT
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Abstract:	Depending on the environment of the acceleration processes for ultra-high energy cosmic rays, photons and neutrinos may be produced by interactions in the sources. This paper reviews some aspects of the search for photons and neutrinos from possible sources of ultra-high energy cosmic rays. It is therefore natural to select known sources of TeV gamma-rays as potential sources of neutrinos. 4 Neutrinos from unresolved sources Neutrinos are not absorbed therefore sources out to the Hubble radius will make roughly equal contributions from each spherical shell [24], so it is quite possible that many astrophysical neutrinos will be observed before a specific source is established. 5 ...
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Appears In:	Ultra high energy cosmic rays, CERN, February, 2012
Preferred Version:	GaisserCERN.pdf