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VERSION:2.0
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PRODID:UW-Madison-Physics-Events
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SEQUENCE:2
UID:UW-Physics-Event-6348
DTSTART:20211026T190000Z
DTEND:20211026T200000Z
DTSTAMP:20260414T191921Z
LAST-MODIFIED:20211022T173357Z
LOCATION:https://berkeley.zoom.us/j/99464252867
SUMMARY:Comparing Supernova Models Using Past and Future Neutrino Data
  \, Network in Neutrinos\, Nuclear Astrophysics\, and Symmetries (N3AS
 ) Seminar\, Jackson Olsen \, University of Minnesota
DESCRIPTION:Recent advances in state-of-the-art core-collapse supernov
 a (CCSN) simulations have led to detailed predictions for the neutrino
  signal. These model predictions can be directly compared using observ
 ations. In this talk\, I describe a Bayesian comparison of three CCSN 
 neutrino emission models using the Kamiokande II data on SN 1987A. I t
 hen present an analysis of the capabilities of a water Cherenkov detec
 tor such as Super-Kamiokande to distinguish between these models in th
 e event of a future Galactic CCSN.
URL:https://www.physics.wisc.edu/events/?id=6348
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