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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:2
UID:UW-Physics-Event-8174
DTSTART:20230203T200000Z
DTEND:20230203T210000Z
DTSTAMP:20260414T054745Z
LAST-MODIFIED:20230203T190447Z
LOCATION:CH4274/https://uwmadison.zoom.us/j/94714568988?pwd=TnRuZFNQaF
 ErZDZ6V29DL0VpSC9rUT09
SUMMARY:Exploiting stellar explosion induced by the QCD phase transiti
 on in large-scale neutrino detectors\, NPAC (Nuclear/Particle/Astro/Co
 smo) Forum\, Anna Suliga\, UC Berkeley/UW Madison
DESCRIPTION:Core-collapse supernovae are one of the most complex pheno
 mena in the universe. Not only are they one of the sites of the produc
 tion of the heavy elements which enable the existence of life\, but th
 eir cores are also one of the densest environments we can indirectly p
 robe. At such densities\, the matter may no longer consist only of had
 ronic degrees of freedom but undergo a phase transition to quark matte
 r. In this talk\, I will discuss the implications of such a transition
  on the neutrino emission from core-collapse supernovae and how the de
 tection of such a signal on Earth can be used to point to the location
  of the supernova and set stringent limits on the absolute active neut
 rino mass.
URL:https://www.physics.wisc.edu/events/?id=8174
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