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SUMMARY:Cosmic Rays Antideuteron Sensitivity for AMS-02 Experiment
DTSTART;VALUE=DATE-TIME:20070709T194500Z
DTEND;VALUE=DATE-TIME:20070709T194500Z
DTSTAMP;VALUE=DATE-TIME:20260521T014229Z
UID:indico-contribution-1112@cern.ch
DESCRIPTION:Speakers: Dr. GIOVACCHINI\, Francesca (University and INFN Bol
 ogna)\nFor energies less than ~3 GeV/n\, the Cosmic Rays Antideuteron comp
 onent due \nto spallation becomes negligible for kinematic reasons and  th
 e detection of \neven a single antideuteron would strongly suggest the exi
 stence of new \nsources\, like neutralino Dark Matter.\nThe AMS-02 experim
 ent\, on board of ISS for a long duration mission (3 years)\, \nthanks to 
 its large acceptance (~ 0.5 m2 sr) and its good particle identification \n
 will be able to push down the current upper limit on the antideuteron flux
  into \nthe region where some new physics effects are expected.\nWe will r
 eport on the results of a detailed study\, using  Monte Carlo simulation\,
  \nwhere the  AMS-02 sensitivity  for antideuterons has been estimated as 
  of \n5X10^-7  (m^2 sr sec)^-1  in the kinetic energy range between 0.2 an
 d 1 \nGeV/n.\n\nhttps://indico.nucleares.unam.mx/event/4/session/40/contri
 bution/1112
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/40/contribution/1112
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