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PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-1220
DTSTART:20081120T220000Z
DTEND:20081120T230000Z
DTSTAMP:20260429T222608Z
LAST-MODIFIED:20080818T143802Z
LOCATION:4274 Chamberlin
SUMMARY:Prospects for High-Energy Cosmic Rays and Neutrinos from Gamma
 -Ray Bursts in the Swift/GLAST Era\, NPAC (Nuclear/Particle/Astro/Cosm
 o) Forum\, Kohta Murase\, Kyoto University\, Yukawa Institute
DESCRIPTION:Gamma-ray burst (GRB) is one of the cosmic-ray acceleratio
 n sites\,  <br>
\nand high-energy neutrino emission from GRBs has been
  expected in <br>
\nvarious scenarios. Many predictions for prompt and
  afterglow emission were done in the pre-Swift era. Recently\, Swift h
 as shown several novel phenomena\, which allows us to expect new possi
 bilities for cosmic-ray acceleration and associated secondary particle
  emission. I will discuss cosmic-ray acceleration and neutrino emissio
 n in various scenarios of GRBs\, motivated by recent observations and 
 theoretical developments. The possible connection between ultra-high-e
 nergy cosmic rays (UHECRs) and GRBs will also be discussed.
URL:https://www.physics.wisc.edu/events/?id=1220
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