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Title:	Neutrino2012_UHENeutrino_Final.pdf
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Handle:	Document-61207
Owner:	Ishihara, Aya (User-239, aya:LDAP)^DS
Create Date:	Tuesday, June 5, 2012 03:32:43 AM CDT
Modified Date:	Sunday, June 17, 2012 09:20:13 PM CDT
Modified By:	Ishihara, Aya (User-239, aya:LDAP)^DS
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Abstract:	e ??n's Off-Source (<50Mpc) astrophysical neutrino production via GZK (Greisen-Zatsepin-Kuzmin) mechanism 3 Various GZK n models � Location of the cosmic-ray sources � Cosmological evolution of the cosmic-ray sources � Cosmic-ray spectra at sources � The highest energy of the cosmcrays � Composition of the cosmic-rays � Particle physics beyond the energies accelerators can reach Carries important physics Atmospheric neutrinos in PeV 4 Prompt Slope = 2.7 Conventional Slope = 3.7 Physics of heavy flavor ... n) Neutrino Energy Distributions (2010-2012) 10 � EM+hadronic (CC) or hadronic (NC) cascade energy ~ PeV � Most likely to be PeV to 10 PeV neutrinos � The highest energy neutrino events ...
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File name:	Neutrino2012_UHENeutrino_v3.pdf
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Appears In:	Neutrino 2012
Preferred Version:	Neutrino2012_UHENeutrino_v3.pdf