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PRODID:UW-Madison-Physics-Events
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SEQUENCE:3
UID:UW-Physics-Event-8477
DTSTART:20240308T213000Z
DTEND:20240308T230000Z
DTSTAMP:20260413T223325Z
LAST-MODIFIED:20240305T180721Z
LOCATION:2241 Chamberlin Hall
SUMMARY:Using Radio Detectors to Discover the Highest Energy Astrophys
 ical Neutrinos\, Physics Department Colloquium\, Abigail Vieregg\, Uni
 versity of Chicago
DESCRIPTION:The detection of high energy astrophysical neutrinos is an
  important step toward understanding the most energetic cosmic acceler
 ators.  IceCube has observed the first astrophysical neutrinos and ide
 ntified the first potential sources.  However\, the best sensitivity a
 t the highest energies comes from detectors that look for coherent rad
 io Cherenkov emission from neutrino interactions.  I will give an over
 view of the state of current experimental efforts\, and then discuss t
 wo new experiments\, RNO-G and PUEO\, that are currently being constru
 cted to discover neutrinos at the highest energies and push the energy
  threshold for radio detection down to overlap with the energy range p
 robed by IceCube\, covering the full astrophysical energy range out to
  the highest energies\, and opening up new phase space for discovery. 
URL:https://www.physics.wisc.edu/events/?id=8477
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