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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-4226
DTSTART:20161122T213000Z
DURATION:PT1H0M0S
DTSTAMP:20260419T060355Z
LAST-MODIFIED:20161121T205319Z
LOCATION:5280 Chamberlin
SUMMARY:Neutrino Masses: First Signal From SUSY!\, Theory Seminar (Hig
 h Energy/Cosmology)\, Seyda Ipek\, Fermilab
DESCRIPTION:We know neutrinos have mass\, but we don't know how they g
 et their masses. Many models augment the Standard Model with right-han
 ded neutrinos\, either Dirac or Majorana\, to generate the neutrino ma
 sses. I will show that in R-symmetric supersymmetric models\, the bino
  and its Dirac partner the singlino can play the role of right-handed 
 neutrinos. In this mechanism the neutrino masses are generated in a ve
 ry simple fashion. I will also discuss low and high energy constraints
 /signatures in this framework.
URL:https://www.physics.wisc.edu/events/?id=4226
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