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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:3
UID:UW-Physics-Event-8104
DTSTART:20231103T203000Z
DTEND:20231103T220000Z
DTSTAMP:20260414T044957Z
LAST-MODIFIED:20231026T132413Z
LOCATION:Chamberlin 2241
SUMMARY:Multimessenger View of High-Energy Cosmic Neutrino Sources\, P
 hysics Department Colloquium\, Kohta Murase\, Penn State
DESCRIPTION:The discovery of high-energy cosmic neutrinos opened a new
  window of astroparticle physics. Revealing the sources is also releva
 nt for solving the long-standing puzzle about the origin of cosmic ray
 s. I will discuss theoretical implications of the latest results on hi
 gh-energy neutrino observations\, and demonstrate the power of multi-m
 essenger approaches. In particular\, I will highlight our recent devel
 opments about astrophysical neutrino emission from extragalactic gamma
 -ray dark sources and the Galactic plane. I will explore the potential
  of utilizing high-energy neutrinos as a probe of physics beyond the S
 tandard Model.
URL:https://www.physics.wisc.edu/events/?id=8104
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