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SEQUENCE:2
UID:UW-Physics-Event-5309
DTSTART:20200128T213000Z
DURATION:PT1H0M0S
DTSTAMP:20260415T040936Z
LAST-MODIFIED:20200127T144852Z
LOCATION:Room 4274\, Chamberlin
SUMMARY:Multi-messenger astrophysics with high-energy neutrinos in the
  coming decade\, NPAC (Nuclear/Particle/Astro/Cosmo) Forum\, Marcos Sa
 ntander
DESCRIPTION:Neutrinos are unique messengers from the high-energy unive
 rse. They can escape dense astrophysical environments\, undeterred by 
 intervening matter and radiation fields. The detection of high-energy 
 astrophysical neutrinos in the TeV-PeV range by IceCube allows us to p
 robe extreme cosmic sources and understand their emission processes in
  ways what would not be possible with photons alone. Enabling neutrino
  astrophysics in the coming decade will rest not only on the construct
 ion of new\, more sensitive facilities\, but also on the combined oper
 ation of multiple observatories capable of identifying additional trac
 ers of hadronic emission. I will present a short overview of recent hi
 ghlights from the neutrino sky and introduce a vision for how the coor
 dinated operation of current and future multi-messenger observatories 
 will help us deliver answers to some of the most pressing questions in
  high-energy astrophysics.
URL:https://www.physics.wisc.edu/events/?id=5309
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