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VERSION:2.0
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SUMMARY:Higgsino Dark Matter
DTSTART;VALUE=DATE-TIME:20191111T041500Z
DTEND;VALUE=DATE-TIME:20191111T044500Z
DTSTAMP;VALUE=DATE-TIME:20250110T182700Z
UID:indico-contribution-327-1526@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Takeo Moroi ()\nI will discuss phenomenology of Higg
 sino dark matter. First\, I will briefly overview theoretical issues relat
 ed to Higgsino dark matter.  Then\, I will summarize present status and fu
 ture prospects of Higgsino dark matter search using colliers and direct de
 tection experiments.\n\nhttps://indico.icrr.u-tokyo.ac.jp/event/259/contri
 butions/1526/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1526/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Overview on thermal DM models with emphasis on Electroweak charges
DTSTART;VALUE=DATE-TIME:20191111T034500Z
DTEND;VALUE=DATE-TIME:20191111T041500Z
DTSTAMP;VALUE=DATE-TIME:20250110T182700Z
UID:indico-contribution-327-1568@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Shigeki Matsumoto (Kavli IPMU)\nDark matter (DM) pro
 blem is now one of the most important problems in many fields of physics. 
 DM mass is\, however\, currently predicted to be in a range between 10^–
 55 g and 10^40 g\; uncertainty of a hundred orders of magnitude. A certain
  diversity of research is thus required to solve the DM problem and many D
 M candidates are now being proposed and discussed. Among various candidate
 s\, TeV-scale thermal DM candidates now attract attention as they are pred
 icted by new physics models intensively discussed after the Higgs discover
 y at LHC and they also have a certain reason why current DM search experim
 ents/observations do not detect their signals. I will summarize above inte
 resting discussions of the TeV scale thermal DM candidates in this talk.\n
 \nhttps://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1568/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1568/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Wino theory and future prospects
DTSTART;VALUE=DATE-TIME:20191111T044500Z
DTEND;VALUE=DATE-TIME:20191111T051500Z
DTSTAMP;VALUE=DATE-TIME:20250110T182700Z
UID:indico-contribution-327-1573@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Satoshi Shirai ()\nWino is one of the most attractiv
 e candidates of the dark matter.\nThe Wino is a natural prediction of SUSY
  models and provides very rich signatures in collider\, direct and indirec
 t search for the dark matter.\nI will talk about the current experimental 
 and theoretical status of the Wino dark matter and the future prospects.\n
 \nhttps://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1573/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1573/
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