***ATTENTION Indico Users***

Notice: LaTeX services are temporarily disabled and will be reintroduced in 3.3.12 which is currently being planned

Please see the News section for more information.

13–17 Aug 2013
University of California, Santa Cruz
US/Pacific timezone

Observation of High-Energy Neutrinos with IceCube

16 Aug 2013, 08:30
30m
ISB 221 (University of California, Santa Cruz)

ISB 221

University of California, Santa Cruz

oral presentation Neutrino Physics Neutrino Physics

Speaker

Dr Nathan Whitehorn (University of Wisconsin - Madison)

Description

The origin of high-energy cosmic rays is one one of the most persistent mysteries in physics. Neutrinos, as neutral tracers of hadronic acceleration, may offer a new and unique window into this problem and others in high-energy astrophysics. This talk will discuss recent results from the antarctic IceCube neutrino observatory, the first operating gigaton-scale neutrino detector, showing first evidence for a population of extremely high energy neutrinos (100+ TeV) that cannot easily be explained by processes occurring in cosmic ray showers in the Earth's atmosphere and may represent the first evidence for a population of high-energy neutrinos of extraterrestrial origin.
APS member ID 61121482

Author

Dr Nathan Whitehorn (University of Wisconsin - Madison)

Presentation materials