Physics
Scientific paper
Mar 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jphcs..60...26w&link_type=abstract
Journal of Physics: Conference Series, Volume 60, Issue 1, pp. 26-33 (2007).
Physics
Scientific paper
Theoretical and experimental constructions together make a compelling case that the discovery of high-energy (gtrsim1015eV) astrophysical neutrinos is imminent. In this talk, we investigate some of the reasons for excitement. We focus on the larger cosmic neutrino flux expected due to the recently-argued lower-energy cosmic-ray crossover from galactic to extragalactic origin; and on various aspects of source dynamics that can be probed by neutrino flavor physics. We conclude with a brief overview of the information contained in the fluctuations and correlations expected in neutrino flavor data.
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