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UID:MEC-f26dab9bf6a137c3b6782e562794c2f2@community.kavlimeetings.org
DTSTART:20220106T190000Z
DTEND:20220106T200000Z
DTSTAMP:20220101T054700Z
CREATED:20211231
LAST-MODIFIED:20211231
PRIORITY:5
TRANSP:OPAQUE
SUMMARY:Discovering the Highest Energy Neutrinos With Radio Detectors
DESCRIPTION:Astrophysics Colloquium Abigail Vieregg (University of Chicago)\nJan 06, 2022\n11:00 am – 12:00 pm PST\nDiscovering the Highest Energy Neutrinos With Radio Detectors\nThe detection of high energy astrophysical neutrinos is an important step toward understanding the most energetic cosmic accelerators.  IceCube, a large optical detector at the South Pole, has observed the first astrophysical neutrinos and identified at least one potential source.  However, the best sensitivity at the highest energies comes from detectors that look for coherent radio Cherenkov emission from neutrino interactions.  I will give an overview of the state of current experimental efforts, including recent results, and then discuss a suite of new experiments designed to discover neutrinos at the highest energies and push the energy threshold for radio detection down to overlap with the energy range probed by IceCube, thus covering the full astrophysical energy range out to the highest energies, and opening up new phase space for discovery.  These include ground-based experiments such as RNO-G and IceCube-Gen2, as well as the balloon-borne experiment PUEO.\nIn Person and zoom\nZoom Info: https://stanford.zoom.us/j/423773826 ( https://stanford.zoom.us/j/423773826 ),\nplease contact KIPAC Managing Director Barbara Beebe bmbeebe@stanford.edu  ( mailto:bmbeebe@stanford.edu )for permission to attend and zoom password.\n
URL:https://community.kavlimeetings.org/calendar-archive/discovering-the-highest-energy-neutrinos-with-radio-detectors/
ORGANIZER;CN=(KIPAC) The Kavli Institute for Particle Astrophysics and Cosmology at Stanford University:MAILTO:
CATEGORIES:Astrophysics
LOCATION:Virtual
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