BEGIN:VCALENDAR
VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-2991
DTSTART:20130319T210000Z
DURATION:PT1H0M0S
DTSTAMP:20260420T020637Z
LAST-MODIFIED:20130313T150111Z
LOCATION:5280 Chamberlin
SUMMARY:Ultra-high energy neutrino events at the IceCube and the Glash
 ow resonance\, WIPAC Seminar\, Atri Bhattacharya\, Harish-Chandra Rese
 arch Institute\, Allahabad\, India
DESCRIPTION:The Glashow resonance is a peak of enhanced cross-section 
 for an electron-anti-neutrino of 6.3 PeV energy interacting with an el
 ectron and producing a resonant W boson\, which further decays into el
 ectrons and hadrons producing cascades in a large volume (Km^3) neutri
 no detector such as the IceCube. We will explore the significance of t
 his narrow bin of energy\, generally with respect to ultra-high energy
  events in the IceCube\, and particularly\, in view of the two recentl
 y observed neutrino events at the PeV energies\; we will show that the
  observation of (or lack of) events at 6.3 PeV energies in the future 
 will allow us to understand several facets of the Ultra-high energy ne
 utrino flux coming\, possibly\, from extra-galactic sources.
URL:https://www.physics.wisc.edu/events/?id=2991
END:VEVENT
END:VCALENDAR