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Title:	Latest Results from IceCube (pdf)
Abstract:	Talk at 2011 SLAC Summer Institute
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Handle:	Document-58645
Owner:	Site Administrator (User-2, admin:DocuShare)^DS
Create Date:	Thursday, August 4, 2011 07:43:34 PM CDT
Modified Date:	Thursday, August 4, 2011 07:43:34 PM CDT
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Abstract:	Neutrino Astronomy at the South Pole Latest results from IceCube Kurt Woschnagg UC Berkeley SLAC Summer Institute August 3, 2011 Neutrinos as Cosmic Messengers Neutrinos and the Origin of Cosmic Rays Cosmic ray spectrum Greisen, Zatsepin, and Kuzmin (1966) ... or + �D� + � + +�+�+ g pn pn pn pp CMB Ep> 6 �1019eV GZK cutoff GZK neutrinos are �guaranteed� Galactic: SN remnants Extragalactic: AGNs / GRBs / Other We expect high-energy neutrinos from the same sources: Rate = Neutrino flux x Neutrino Effective Area = Neutrino flux x Neutrino Cross Section x Absorption in Earth x Size of detector x (Range of muon for nm) S . Klein, F. Halzen, Phys . D 84 (2011) 022004 Indirect Dark Matter ...
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File name:	KurtWoschnagg-IceCube-SSI-2011-asgiven.pdf
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Appears In:	SLAC Summer Institute 2011
Preferred Version:	Latest Results from IceCube (pdf)