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SUMMARY:A Monte Carlo detector response model for solar neutrino absorptio
 n on 40Ar in DEAP-3600
DTSTART;VALUE=DATE-TIME:20210915T160000Z
DTEND;VALUE=DATE-TIME:20210915T170000Z
DTSTAMP;VALUE=DATE-TIME:20260606T140623Z
UID:indico-contribution-73@indico.physics.ucsd.edu
DESCRIPTION:Speakers: Andrew Erlandson (Carleton University)\nDEAP-3600 is
  a liquid argon (LAr) scintillation detector designed to search for Weakly
  Interacting Massive Particles (WIMPs) at SNOLAB. Beyond the search for da
 rk matter\, the DEAP-3600 detector is also intrinsically sensitive to char
 ged current interactions on 40Ar from 8B solar neutrinos. Here we present 
 the expected detector response to high energy delayed coincidence events r
 esulting from neutrino absorption on the ~3.2 tonne target mass. We exploi
 t the Marley event generator in conjunction with a full optical simulation
  of the DEAP-3600 detector using the Reactor Analysis Tool (RAT). Through 
 the delayed coincidence channel\, we expect an event yield of (4.69 ± 0.4
 3) events in a 7.20 tonne-year exposure in DEAP-3600.\n\nhttps://indico.ph
 ysics.ucsd.edu/event/1/contributions/73/
LOCATION:
URL:https://indico.physics.ucsd.edu/event/1/contributions/73/
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