BEGIN:VCALENDAR
VERSION:2.0
PRODID:www.dresden-science-calendar.de
METHOD:PUBLISH
CALSCALE:GREGORIAN
X-MICROSOFT-CALSCALE:GREGORIAN
X-WR-TIMEZONE:Europe/Berlin
BEGIN:VTIMEZONE
TZID:Europe/Berlin
X-LIC-LOCATION:Europe/Berlin
BEGIN:DAYLIGHT
TZNAME:CEST
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
DTSTART:19810329T030000
RRULE:FREQ=YEARLY;INTERVAL=1;BYMONTH=3;BYDAY=-1SU
END:DAYLIGHT
BEGIN:STANDARD
TZNAME:CET
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
DTSTART:19961027T030000
RRULE:FREQ=YEARLY;INTERVAL=1;BYMONTH=10;BYDAY=-1SU
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
UID:DSC-10939
DTSTART;TZID=Europe/Berlin:20160602T150000
SEQUENCE:1459252215
TRANSP:OPAQUE
DTEND;TZID=Europe/Berlin:20160602T160000
URL:https://dresden-science-calendar.de/calendar/de/detail/10939
LOCATION:Institut für Kern- und Teilchenphysik\, TU Dresden\, Zellescher W
 eg 1901069 Dresden
SUMMARY:Krikler: Muon-to-Electron Conversion at the COMET experiment
CLASS:PUBLIC
DESCRIPTION:Speaker: Benjamin Krikler\nInstitute of Speaker: Imperial Colle
 ge London\nTopics:\nPhysik\n Location:\n  Name: Institut für Kern- und Te
 ilchenphysik\, TU Dresden (ASB/E19)\n  Street: Zellescher Weg 19\n  City: 
 01069 Dresden\n  Phone: +49 351 463 37659\n  Fax: +49 351 463 33114\nDescr
 iption: Muon decay in the Standard Model requires the emission of two neut
 rinos thanks to the conservation of Lepton Flavour. Given neutrino oscilla
 tions\, however\, this conservation is known to be violated in the Standar
 d Model. The COMET experiment is one of a handful of projects hoping to de
 monstrate Charged Lepton Flavour Violation\, searching for COherent Muon t
 o Electron Transitions\, where a muon converts to an electron in the prese
 nce of an atomic nucleus\, without neutrino emission.    I present here an
  overview of muon-to-electron conversion and the COMET experiment itself. 
  Currently under construction to begin Phase-I data taking in JFY 2018\, t
 he first stage will see a factor 100 improvement on the current limit to a
 round 3x10^-15.  Phase-II will then go a further two orders of magnitude r
 unning early next decade. Setting such stringent limits comes with signifi
 cant design challenges.  These\, their solutions\, and recent developments
  in facility\, beam-line and detector construction will also be presented.
DTSTAMP:20260406T021312Z
CREATED:20160329T115015Z
LAST-MODIFIED:20160329T115015Z
END:VEVENT
END:VCALENDAR