BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//talks.cam.ac.uk//v3//EN
BEGIN:VTIMEZONE
TZID:Europe/London
BEGIN:DAYLIGHT
TZOFFSETFROM:+0000
TZOFFSETTO:+0100
TZNAME:BST
DTSTART:19700329T010000
RRULE:FREQ=YEARLY;BYMONTH=3;BYDAY=-1SU
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0100
TZOFFSETTO:+0000
TZNAME:GMT
DTSTART:19701025T020000
RRULE:FREQ=YEARLY;BYMONTH=10;BYDAY=-1SU
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
CATEGORIES:Cavendish HEP Seminars
SUMMARY:Dark Matter in the Galaxy and at the LHC -  making
  the connection - Dr. Malcolm Fairbairn (KCL)
DTSTART;TZID=Europe/London:20091117T150000
DTEND;TZID=Europe/London:20091117T160000
UID:TALK19449AThttp://talks.cam.ac.uk
URL:http://talks.cam.ac.uk/talk/index/19449
DESCRIPTION:There are three ways of detecting dark matter\, di
 rect detection where we look for the recoils of da
 rk matter from standard model particles\, indirect
  detection where we see the signals of dark matter
  annihilating with itself or decaying and finally 
 production at colliders.  If we are lucky enough t
 o detect what we think is dark matter in any of th
 ese ways we will enter a new era of research which
  involves trying to link the different observation
 s together to see if they fit -  making them fit i
 s a necessary step towards claiming a discovery\, 
 having them not fit is arguably more interesting. 
  Whichever situation may arise\, much work needs t
 o be done to prepare ourselves for the data which 
 will arrive from various sources over the next yea
 rs.  I will describe ongoing efforts in this direc
 tion.
LOCATION:Rutherford Seminar Room B
CONTACT:Steve Chun Hay Kom
END:VEVENT
END:VCALENDAR