The DarkSide Multiton Detector for the Direct Dark Matter Search

被引：24

作者：

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
,10
]}

Brodsky, J. ^{[5
]}

Budano, F. ^{[11
,12
]}

Cadonati, L. ^{[13
]}

Cadoni, M. ^{[14
,15
]}

Calaprice, F. ^{[5
]}

Canci, N. ^{[4
]}

Candela, A. ^{[7
]}

Cao, H. ^{[5
]}

Cariello, M. ^{[16
,17
]}

Cavalcante, P. ^{[7
]}

Chepurnov, A. ^{[18
]}

Cocco, A. G. ^{[19
,20
]}

Condon, C. ^{[5
]}

Crippa, L. ^{[9
,10
]}

D'Angelo, D. ^{[9
,10
]}

D'Incecco, M. ^{[7
]}

Davini, S. ^{[21
]}

De Deo, M. ^{[7
]}

Derbin, A. ^{[22
]}

Devoto, A. ^{[14
,15
]}

Di Eusanio, F. ^{[5
]}

Edkins, E. ^{[23
]}

Empl, A. ^{[21
]}

Fan, A. ^{[4
]}

Fiorillo, G. ^{[19
,20
]}

Fomenko, K. ^{[24
]}

Forster, G. ^{[13
]}

Foxe, M. ^{[1
]}

Franco, D. ^{[2
]}

Gabriele, F. ^{[7
]}

Galbiati, C. ^{[5
]}

Goretti, A. ^{[5
]}

Grandi, L. ^{[25
,26
]}

Gromov, M. ^{[18
]}

Guan, M. Y. ^{[27
]}

Guardincerri, Y. ^{[6
]}

Hackett, B. ^{[23
]}

Herner, K. ^{[6
]}

Hime, A. ^{[1
]}

机构：

[1] Pacific NW Natl Lab, Richland, WA 99352 USA

[2] Univ Paris Diderot, Sorbonne Paris Cite, APC, F-75205 Paris, France

[3] Augustana Coll, Dept Phys & Astron, Sioux Falls, SD 57197 USA

[4] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA

[5] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA

[6] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA

[7] Lab Nazl Gran Sasso, I-67010 Assergi, Italy

[8] Gran Sasso Sci Inst, I-67100 Laquila, Italy

[9] Univ Milan, Dept Phys, I-20133 Milan, Italy

[10] Ist Nazl Fis Nucl, I-20133 Milan, Italy

[11] Univ Rome Tre, Dept Phys, I-00146 Rome, Italy

[12] Ist Nazl Fis Nucl, I-00146 Rome, Italy

[13] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA

[14] Univ Cagliari, Dept Phys, I-09042 Cagliari, Italy

[15] Ist Nazl Fis Nucl, I-09042 Cagliari, Italy

[16] Univ Genoa, Dept Phys, I-16146 Genoa, Italy

[17] Ist Nazl Fis Nucl, I-16146 Genoa, Italy

[18] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119991, Russia

[19] Univ Naples Federico II, Dept Phys, I-80126 Naples, Italy

[20] Ist Nazl Fis Nucl, I-80126 Naples, Italy

[21] Univ Houston, Dept Phys, Houston, TX 77204 USA

[22] St Petersburg Nucl Phys Inst, Gatchina 188350, Russia

[23] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA

[24] Joint Inst Nucl Res, Dubna 141980, Russia

[25] Univ Chicago, Enrico Fermi Inst, Kavli Inst, Chicago, IL 60637 USA

[26] Univ Chicago, Dept Phys, Chicago, IL 60637 USA

[27] Inst High Energy Phys, Beijing 100049, Peoples R China

[28] Brookhaven Natl Lab, Upton, NY 11973 USA

[29] Univ Strasbourg, CNRS, IN2P3, IPHC, F-67037 Strasbourg, France

[30] Black Hills State Univ, Sch Nat Sci, Spearfish, SD 57799 USA

[31] Virginia Tech, Dept Phys, Blacksburg, VA 24061 USA

[32] Natl Acad Sci Ukraine, Inst Nucl Res, UA-03680 Kiev, Ukraine

[33] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[34] Natl Res Ctr, Kurchatov Inst, Moscow 123182, Russia

[35] Temple Univ, Dept Phys, Philadelphia, PA 19122 USA

[36] Jagiellonian Univ, Smoluchowski Inst Phys, PL-30059 Krakow, Poland

[37] Univ Perugia, Dept Chem Biol & Biotechnol, I-06123 Perugia, Italy

[38] Ist Nazl Fis Nucl, I-06123 Perugia, Italy

[39] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA

[40] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA

来源：

ADVANCES IN HIGH ENERGY PHYSICS | 2015年 / 2015卷

基金：

美国国家科学基金会;

关键词：

LIQUID ARGON;

D O I：

10.1155/2015/541362

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

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 DarkSide50 (50 kg LAr-TPC) up to DarkSide-G2. Finally, the preliminary results on background suppression and expected sensitivity are presented.

引用

页数：8

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