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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-1834
DTSTART:20100421T210000Z
DURATION:PT1H0M0S
DTSTAMP:20260506T161527Z
LAST-MODIFIED:20100405T134917Z
LOCATION:4274 Chamberlin
SUMMARY:Core Collapse Supernova Neutrino Detection\, NPAC (Nuclear/Par
 ticle/Astro/Cosmo) Forum\, Kate Scholberg\, Duke University
DESCRIPTION: When a massive star collapses at the end of its life\, ne
 arly all of  the gravitational binding energy of the resulting remnant
  is released in the form of neutrinos.  I will discuss the nature of t
 he core collapse neutrino burst and what we can learn from its detecti
 on.  I will cover supernova neutrino detection techniques\, and prospe
 cts for future supernova-neutrino-sensitive experiments.
URL:https://www.physics.wisc.edu/events/?id=1834
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