Amaudruz, P-A; Baldwin, M; Batygov, M; Beltran, B; Bina, CE; Bishop, D; Bonatt, J; Boorman, G; Boulay, MG; Broerman, B; Bromwich, T; Bueno, JF; Burghardt, PM; Butcher, A; Cai, B; Chan, S; Chen, M; Chouinard, R; Churchwell, S; Cleveland, BT; Cranshaw, D; Dering, K; DiGioseffo, J; Dittmeier, S; Duncan, FA; Dunford, M; Erlandson, A; Fatemighomi, N; Florian, S; Flower, A; Ford, RJ; Gagnon, R; Giampa, P; Golovko, VV; Gorel, P; Gornea, R; Grace, E; Graham, K; Grant, DR; Gulyev, E; Hall, A; Hallin, AL; Hamstra, M; Harvey, PJ; Hearns, C; Jillings, CJ; Kamaev, O; Kemp, A; Kuźniak, M; Langrock, S; La Zia, F; Lehnert, B; Li, O; Lidgard, JJ; Liimatainen, P; Lim, C; Lindner, T; Linn, Y; Liu, S; Majewski, P; Mathew, R; McDonald, AB; McElroy, T; McFarlane, K; McGinn, T; McLaughlin, JB; Mead, S; Mehdiyev, R; Mielnichuk, C; Monroe, J; Muir, A; Nadeau, P; Nantais, C; Ng, C; Noble, AJ; O’Dwyer, E; Ohlmann, C; Olchanski, K; Olsen, KS; Ouellet, C; Pasuthip, P; Peeters, SJM; Pollmann, TR; Rand, ET; Rau, W

doi:10.1016/j.astropartphys.2018.09.006

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Design and construction of the DEAP-3600 dark matter detector

2019

Amaudruz, P-A;
Baldwin, M;
Batygov, M;
Beltran, B;
Bina, CE;
Bishop, D;
Bonatt, J;
Boorman, G;
Boulay, MG;
Broerman, B;
Bromwich, T;
Bueno, JF;
Burghardt, PM;
Butcher, A;
Cai, B;
Chan, S;
Chen, M;
Chouinard, R;
Churchwell, S;
Cleveland, BT;
Cranshaw, D;
Dering, K;
DiGioseffo, J;
Dittmeier, S;
Duncan, FA;
Dunford, M;
Erlandson, A;
Fatemighomi, N;
Florian, S;
Flower, A;
Ford, RJ;
Gagnon, R;
Giampa, P;
Golovko, VV;
Gorel, P;
Gornea, R;
Grace, E;
Graham, K;
Grant, DR;
Gulyev, E;
Hall, A;
Hallin, AL;
Hamstra, M;
Harvey, PJ;
Hearns, C;
Jillings, CJ;
Kamaev, O;
Kemp, A;
Kuźniak, M;
Langrock, S;
La Zia, F;
Lehnert, B;
Li, O;
Lidgard, JJ;
Liimatainen, P;
Lim, C;
Lindner, T;
Linn, Y;
Liu, S;
Majewski, P;
Mathew, R;
McDonald, AB;
McElroy, T;
McFarlane, K;
McGinn, T;
McLaughlin, JB;
Mead, S;
Mehdiyev, R;
Mielnichuk, C;
Monroe, J;
Muir, A;
Nadeau, P;
Nantais, C;
Ng, C;
Noble, AJ;
O’Dwyer, E;
Ohlmann, C;
Olchanski, K;
Olsen, KS;
Ouellet, C;
Pasuthip, P;
Peeters, SJM;
Pollmann, TR;
Rand, ET;
Rau, W;
Rethmeier, C;
Retière, F;
Seeburn, N;
Shaw, B;
Singhrao, K;
Skensved, P;
Smith, B;
Smith, NJT;
Sonley, T;
Soukup, J;
Stainforth, R;
Stone, C;
Strickland, V;
Sur, B;
Tang, J;
Taylor, J;
Veloce, L;
Vázquez-Jáuregui, E;
Walding, J;
Ward, M;
Westerdale, S;
White, R;
Woolsey, E;
Zielinski, J
et al.

Published Web Location

https://doi.org/10.1016/j.astropartphys.2018.09.006

Abstract

The Dark matter Experiment using Argon Pulse-shape discrimination (DEAP) has been designed for a direct detection search for particle dark matter using a single-phase liquid argon target. The projected cross section sensitivity for DEAP-3600 to the spin-independent scattering of Weakly Interacting Massive Particles (WIMPs) on nucleons is 10−46cm2 for a 100 GeV/c2 WIMP mass with a fiducial exposure of 3 tonne-years. This paper describes the physical properties and construction of the DEAP-3600 detector.

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Lawrence Berkeley National Laboratory

Design and construction of the DEAP-3600 dark matter detector

Published Web Location