The DarkSide Multiton Detector for the Direct Dark Matter Search

Author:

Aalseth C. E.1,Agnes P.2,Alton A.3,Arisaka K.4,Asner D. M.1,Back H. O.5,Baldin B.6,Biery K.6,Bonfini G.7,Bossa M.8,Brigatti A.9,Brodsky J.5,Budano F.10,Cadonati L.11,Cadoni M.12,Calaprice F.5,Canci N.4,Candela A.7,Cao H.5,Cariello M.13,Cavalcante P.7,Chepurnov A.14,Cocco A. G.15,Condon C.5,Crippa L.9,D’Angelo D.9,D’Incecco M.7,Davini S.16,De Deo M.7,Derbin A.17,Devoto A.12,Di Eusanio F.5,Edkins E.18,Empl A.16,Fan A.4,Fiorillo G.15,Fomenko K.19,Forster G.11,Foxe M.1,Franco D.2,Gabriele F.7,Galbiati C.5,Goretti A.5,Grandi L.20,Gromov M.14,Guan M. Y.21,Guardincerri Y.6,Hackett B.18,Herner K.6,Hime A.1,Humble P.1,Hungerford E.16,Ianni Al.7,Ianni An.5,Jaffe D. E.22,Jollet C.23,Keeter K.24,Kendziora C.6,Kidner S.25,Kobychev V.26,Koh G.5,Korablev D.19,Korga G.16,Kurlej A.11,Li P. X.21,Lissia M.12,Lombardi P.9,Ludhova L.9,Luitz S.27,Lukyachenko G.14,Ma Y. Q.21,Machulin I.28,Mandarano A.10,Mari S. M.10,Maricic J.18,Marini L.10,Markov D.28,Martoff J.29,Meregaglia A.23,Meroni E.9,Meyers P. D.5,Miletic T.29,Milincic R.18,Montuschi M.7,Monzani M. E.27,Mosteiro P.5,Mount B.24,Muratova V.17,Musico P.13,Montanari D.6,Nelson A.5,Odrowski S.7,Odrzywolek A.30,Orrell J. L.1,Orsini M.7,Ortica F.31,Pagani L.13,Pallavicini M.13,Pantic E.432,Parmeggiano S.9,Parsells B.5,Pelczar K.30,Pelliccia N.31,Perasso S.2,Perasso L.13,Pocar A.11,Pordes S.6,Pugachev D.28,Qian H.5,Randle K.11,Ranucci G.9,Razeto A.7,Recine K.29,Reinhold B.18,Renshaw A.4,Romani A.31,Rossi N.7,Rossi B.515,Rountree S. D.25,Sablone D.16,Saggese P.9,Saldanha R.20,Sands W.5,Sangiorgio S.33,Segreto E.7,Semenov D.17,Shields E.5,Skorokhvatov M.28,Smallcomb M.3,Smirnov O.19,Sotnikov A.19,Suvurov Y.4,Tartaglia R.7,Tatarowicz J.29,Testera G.13,Tonazzo A.2,Unzhakov E.17,Vogelaar R. B.25,Wada M.5,Walker S. E.15,Wang H.4,Wang Y.21,Watson A. W.29,Westerdale S.5,Williams R.1,Wojcik M.30,Xu J.5,Yang C. G.21,Yoo J.6,Yu B.22,Zavatarelli S.13,Zhong W. L.21,Zuzel G.30

Affiliation:

1. Pacific Northwest National Laboratory, Richland, WA 99352, USA

2. APC, Université Paris Diderot, Sorbonne Paris Cité, 75205 Paris, France

3. Physics and Astronomy Department, Augustana College, Sioux Falls, SD 57197, USA

4. Physics and Astronomy Department, University of California, Los Angeles, CA 90095, USA

5. Physics Department, Princeton University, Princeton, NJ 08544, USA

6. Fermi National Accelerator Laboratory, Batavia, IL 60510, USA

7. Laboratori Nazionali del Gran Sasso, 67010 Assergi, Italy

8. Gran Sasso Science Institute, 67100 L’Aquila, Italy

9. Physics Department, Università degli Studi and INFN, 20133 Milano, Italy

10. Physics Department, Università degli Studi Roma Tre and INFN, 00146 Roma, Italy

11. Physics Department, University of Massachusetts, Amherst, MA 01003, USA

12. Physics Department, Università degli Studi and INFN, 09042 Cagliari, Italy

13. Physics Department, Università degli Studi and INFN, 16146 Genova, Italy

14. Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow 119991, Russia

15. Physics Department, Università degli Studi Federico II and INFN, 80126 Napoli, Italy

16. Department of Physics, University of Houston, Houston, TX 77204, USA

17. Saint Petersburg Nuclear Physics Institute, Gatchina 188350, Russia

18. Department of Physics and Astronomy, University of Hawaii, Honolulu, HI 96822, USA

19. Joint Institute for Nuclear Research, Dubna 141980, Russia

20. Kavli Institute, Enrico Fermi Institute, and Department of Physics, University of Chicago, Chicago, IL 60637, USA

21. Institute of High Energy Physics, Beijing 100049, China

22. Brookhaven National Laboratory, Upton, NY 11973, USA

23. IPHC, Université de Strasbourg, CNRS/IN2P3, 67037 Strasbourg, France

24. School of Natural Sciences, Black Hills State University, Spearfish, SD 57799, USA

25. Physics Department, Virginia Tech, Blacksburg, VA 24061, USA

26. Institute for Nuclear Research, National Academy of Sciences of Ukraine, Kiev 03680, Ukraine

27. SLAC National Accelerator Laboratory, Menlo Park, CA 94025, USA

28. National Research Centre Kurchatov Institute, Moscow 123182, Russia

29. Physics Department, Temple University, Philadelphia, PA 19122, USA

30. Smoluchowski Institute of Physics, Jagiellonian University, 30059 Krakow, Poland

31. Department of Chemistry, Biology and Biotechnology, Università degli Studi and INFN, 06123 Perugia, Italy

32. Physics Department, University of California, Davis, CA 95616, USA

33. Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, CA 94550, USA

Abstract

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.

Publisher

Hindawi Limited

Subject

Nuclear and High Energy Physics

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