Table of Contents Author Guidelines Submit a Manuscript
Advances in High Energy Physics
Volume 2015, Article ID 541362, 8 pages
Research Article

The DarkSide Multiton Detector for the Direct Dark Matter Search

C. E. Aalseth,1 P. Agnes,2 A. Alton,3 K. Arisaka,4 D. M. Asner,1 H. O. Back,5 B. Baldin,6 K. Biery,6 G. Bonfini,7 M. Bossa,8 A. Brigatti,9 J. Brodsky,5 F. Budano,10 L. Cadonati,11 M. Cadoni,12 F. Calaprice,5 N. Canci,4 A. Candela,7 H. Cao,5 M. Cariello,13 P. Cavalcante,7 A. Chepurnov,14 A. G. Cocco,15 C. Condon,5 L. Crippa,9 D. D’Angelo,9 M. D’Incecco,7 S. Davini,16 M. De Deo,7 A. Derbin,17 A. Devoto,12 F. Di Eusanio,5 E. Edkins,18 A. Empl,16 A. Fan,4 G. Fiorillo,15 K. Fomenko,19 G. Forster,11 M. Foxe,1 D. Franco,2 F. Gabriele,7 C. Galbiati,5 A. Goretti,5 L. Grandi,20 M. Gromov,14 M. Y. Guan,21 Y. Guardincerri,6 B. Hackett,18 K. Herner,6 A. Hime,1 P. Humble,1 E. Hungerford,16 Al. Ianni,7 An. Ianni,5 D. E. Jaffe,22 C. Jollet,23 K. Keeter,24 C. Kendziora,6 S. Kidner,25 V. Kobychev,26 G. Koh,5 D. Korablev,19 G. Korga,16 A. Kurlej,11 P. X. Li,21 M. Lissia,12 P. Lombardi,9 L. Ludhova,9 S. Luitz,27 G. Lukyachenko,14 Y. Q. Ma,21 I. Machulin,28 A. Mandarano,10 S. M. Mari,10 J. Maricic,18 L. Marini,10 D. Markov,28 J. Martoff,29 A. Meregaglia,23 E. Meroni,9 P. D. Meyers,5 T. Miletic,29 R. Milincic,18 M. Montuschi,7 M. E. Monzani,27 P. Mosteiro,5 B. Mount,24 V. Muratova,17 P. Musico,13 D. Montanari,6 A. Nelson,5 S. Odrowski,7 A. Odrzywolek,30 J. L. Orrell,1 M. Orsini,7 F. Ortica,31 L. Pagani,13 M. Pallavicini,13 E. Pantic,4,32 S. Parmeggiano,9 B. Parsells,5 K. Pelczar,30 N. Pelliccia,31 S. Perasso,2 L. Perasso,13 A. Pocar,11 S. Pordes,6 D. Pugachev,28 H. Qian,5 K. Randle,11 G. Ranucci,9 A. Razeto,7 K. Recine,29 B. Reinhold,18 A. Renshaw,4 A. Romani,31 N. Rossi,7 B. Rossi,5,15 S. D. Rountree,25 D. Sablone,16 P. Saggese,9 R. Saldanha,20 W. Sands,5 S. Sangiorgio,33 E. Segreto,7 D. Semenov,17 E. Shields,5 M. Skorokhvatov,28 M. Smallcomb,3 O. Smirnov,19 A. Sotnikov,19 Y. Suvurov,4 R. Tartaglia,7 J. Tatarowicz,29 G. Testera,13 A. Tonazzo,2 E. Unzhakov,17 R. B. Vogelaar,25 M. Wada,5 S. E. Walker,15 H. Wang,4 Y. Wang,21 A. W. Watson,29 S. Westerdale,5 R. Williams,1 M. Wojcik,30 J. Xu,5 C. G. Yang,21 J. Yoo,6 B. Yu,22 S. Zavatarelli,13 W. L. Zhong,21 and G. Zuzel30

1Pacific Northwest National Laboratory, Richland, WA 99352, USA
2APC, Université Paris Diderot, Sorbonne Paris Cité, 75205 Paris, France
3Physics and Astronomy Department, Augustana College, Sioux Falls, SD 57197, USA
4Physics and Astronomy Department, University of California, Los Angeles, CA 90095, USA
5Physics Department, Princeton University, Princeton, NJ 08544, USA
6Fermi National Accelerator Laboratory, Batavia, IL 60510, USA
7Laboratori Nazionali del Gran Sasso, 67010 Assergi, Italy
8Gran Sasso Science Institute, 67100 L’Aquila, Italy
9Physics Department, Università degli Studi and INFN, 20133 Milano, Italy
10Physics Department, Università degli Studi Roma Tre and INFN, 00146 Roma, Italy
11Physics Department, University of Massachusetts, Amherst, MA 01003, USA
12Physics Department, Università degli Studi and INFN, 09042 Cagliari, Italy
13Physics Department, Università degli Studi and INFN, 16146 Genova, Italy
14Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow 119991, Russia
15Physics Department, Università degli Studi Federico II and INFN, 80126 Napoli, Italy
16Department of Physics, University of Houston, Houston, TX 77204, USA
17Saint Petersburg Nuclear Physics Institute, Gatchina 188350, Russia
18Department of Physics and Astronomy, University of Hawaii, Honolulu, HI 96822, USA
19Joint Institute for Nuclear Research, Dubna 141980, Russia
20Kavli Institute, Enrico Fermi Institute, and Department of Physics, University of Chicago, Chicago, IL 60637, USA
21Institute of High Energy Physics, Beijing 100049, China
22Brookhaven National Laboratory, Upton, NY 11973, USA
23IPHC, Université de Strasbourg, CNRS/IN2P3, 67037 Strasbourg, France
24School of Natural Sciences, Black Hills State University, Spearfish, SD 57799, USA
25Physics Department, Virginia Tech, Blacksburg, VA 24061, USA
26Institute for Nuclear Research, National Academy of Sciences of Ukraine, Kiev 03680, Ukraine
27SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA
28National Research Centre Kurchatov Institute, Moscow 123182, Russia
29Physics Department, Temple University, Philadelphia, PA 19122, USA
30Smoluchowski Institute of Physics, Jagiellonian University, 30059 Krakow, Poland
31Department of Chemistry, Biology and Biotechnology, Università degli Studi and INFN, 06123 Perugia, Italy
32Physics Department, University of California, Davis, CA 95616, USA
33Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, CA 94550, USA

Received 7 March 2014; Accepted 19 June 2014

Academic Editor: Marcello Messina

Copyright © 2015 C. E. Aalseth et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP3.


Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in principle be detected through their collisions with ordinary nuclei in a sensitive target, producing observable low-energy (<100 keV) nuclear recoils. The DarkSide program aims at the WIPMs detection using a liquid argon time projection chamber (LAr-TPC). In this paper we quickly review the DarkSide program focusing in particular on the next generation experiment DarkSide-G2, a 3.6-ton LAr-TPC. The different detector components are described as well as the improvements needed to scale the detector from DarkSide-50 (50 kg LAr-TPC) up to DarkSide-G2. Finally, the preliminary results on background suppression and expected sensitivity are presented.