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BEGIN:VEVENT
UID:DSC-360
DTSTART;TZID=Europe/Berlin:20110201T164000
SEQUENCE:1295458293
TRANSP:OPAQUE
DTEND;TZID=Europe/Berlin:20110201T181000
URL:https://dresden-science-calendar.de/calendar/de/detail/360
LOCATION:TUD Recknagel-Bau\, Haeckelstraße 1-501069 Dresden
SUMMARY:Baudis: Direct Detection of Dark Matter in the Milky Way
CLASS:PUBLIC
DESCRIPTION:Speaker: Laura Baudis\nInstitute of Speaker: Universität Züri
 ch\n\nTopics:\nPhysik\n Location:\n  Name: TUD Recknagel-Bau (C213)\n  Str
 eet: Haeckelstraße 1-5\n  City: 01069 Dresden\n  Phone: \n  Fax: \nDescri
 ption: We have strong evidence that about 95% of matter in our Universe is
  dark\, revealing its presence only by its gravitational attraction. In hi
 erarchical structure formation\, two macro-structures exist in the Milky W
 ay: the dark halo\, and the dark disk. If the dark matter in these structu
 res is made of Weakly Interacting Massive Particles (WIMPs)\, it can be di
 rectly detected via elastic scattering from nuclei in ultra-low background
 \, deep underground detectors. WIMPs arise naturally in many beyond standa
 rd model theories\, a popular example being the neutralino\, or the lighte
 st supersymmetric particle. After an introduction to the direct detection 
 method\, I will review the current techniques to search for these hypothet
 ical particles.  The focus will be on recent results\, and on the most pro
 mising techniques for the near future.
DTSTAMP:20260610T195619Z
CREATED:20110119T173133Z
LAST-MODIFIED:20110119T173133Z
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