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PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-1136
DTSTART:20080310T170000Z
DURATION:PT1H0M0S
DTSTAMP:20260423T041120Z
LAST-MODIFIED:20080310T173136Z
LOCATION:6515 Sterling
SUMMARY:Loose Ends in Cosmic Rays\, Galaxies Lunch!\, Pasquale Blasi\,
  Arcetri & Fermliab
DESCRIPTION:I will describe how cosmic rays must modify the environmen
 t in which they are accelerated and how this leads to predict that the
  the end of the galactic cosmic ray spectrum should be around 1017 eV 
 and be made of heavy nuclei. I will then describe how the galactic spe
 ctrum joins the emerging extragalactic cosmic ray spectrum\, and how t
 he global ultra high energy cosmic ray pectrum eventually ends. 
URL:https://www.physics.wisc.edu/events/?id=1136
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