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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-8177
DTSTART:20230131T200000Z
DURATION:PT1H0M0S
DTSTAMP:20260414T055037Z
LAST-MODIFIED:20230127T143819Z
LOCATION:Join Zoom Meeting https://berkeley.zoom.us/j/91230714547  Mee
 ting ID: 912 3071 4547
SUMMARY:High-Energy Multimesssenger Emission from Supermassive Black H
 oles\, Network in Neutrinos\, Nuclear Astrophysics\, and Symmetries (N
 3AS) Seminar\, Kohta Murase\, Penn State
DESCRIPTION:Supermassive black holes power disks\, coronae\, jets and 
 winds\, and a significant fraction of energy released by the black hol
 es may be carried by cosmic rays and associated high-energy non-therma
 l radiation. Recently\, the IceCube Collaboration reported association
 s of high-energy neutrinos with active galactic nuclei\, including a n
 earby Seyfert galaxy\, NGC 1068. We review the implications of the mul
 timessenger data for theoretical models and discuss their challenges. 
URL:https://www.physics.wisc.edu/events/?id=8177
END:VEVENT
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