The DarkSide Direct Dark Matter Search with Liquid Argon

被引：0

作者：

Edkins, E. ^{[1
]}

Agnes, P. ^{[2
]}

Alexander, T. ^{[39
]}

Alton, A. ^{[3
]}

Arisaka, K. ^{[38
]}

Back, H. O. ^{[31
]}

Baldin, B. ^{[10
]}

Biery, K. ^{[10
]}

Bonfini, G. ^{[20
]}

Bossa, M. ^{[13
]}

Brigatti, A. ^{[22
,23
]}

Brodsky, J. ^{[31
]}

Budano, F. ^{[32
,33
]}

Cadonati, L. ^{[39
]}

Calaprice, F. ^{[31
]}

Canci, N. ^{[38
]}

Candela, A. ^{[20
]}

Cao, H. ^{[31
]}

Cariello, M. ^{[11
,12
]}

Cavalcante, P. ^{[20
]}

Chavarria, A. ^{[6
,7
]}

Chepurnov, A. ^{[24
]}

Cocco, A. G. ^{[25
,26
]}

Crippa, L. ^{[22
,23
]}

D'Angelo, D. ^{[22
,23
]}

D'Incecco, M. ^{[20
]}

Davini, S. ^{[14
]}

De Deo, M. ^{[20
]}

Derbin, A. ^{[28
]}

Devoto, A. ^{[4
,5
]}

Di Eusanio, F. ^{[31
]}

Di Pietro, G. ^{[22
,23
]}

Empl, A. ^{[14
]}

Fan, A. ^{[38
]}

Fiorillo, G. ^{[25
,26
]}

Fomenko, K. ^{[9
]}

Forster, G. ^{[39
]}

Franco, D. ^{[2
]}

Gabriele, F. ^{[20
]}

Galbiati, C. ^{[31
]}

Goretti, A. ^{[31
]}

Grandi, L. ^{[6
,7
]}

Gromov, M. ^{[24
]}

Guan, M. Y. ^{[15
]}

Guardincerri, Y. ^{[10
]}

Hackett, B. ^{[1
]}

Herner, K. ^{[10
]}

Humble, P. ^{[27
]}

Hungerford, E. V. ^{[14
]}

Ianni, Al. ^{[20
]}

机构：

[1] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 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 Cagliari, Phys Dept, I-09042 Cagliari, Italy

[5] INFN, I-09042 Cagliari, Italy

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

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

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

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

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

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

[12] INFN, I-16146 Genoa, Italy

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

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

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

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

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

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

[19] Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA

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

[21] Nat Res Nucl Univ, Moscow Engn Phys Inst, Moscow 115409, Russia

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

[23] INFN, I-20133 Milan, Italy

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

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

[26] INFN, I-TESTERA10 Naples, Italy

[27] Pacific Northwest Natl Lab, Richland, WA 99352 USA

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

[29] Univ Perugia, Chem Dept, I-06123 Perugia, Italy

[30] INFN, I-06123 Perugia, Italy

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

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

[33] INFN, I-00146 Rome, Italy

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

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

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

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

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

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

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

来源：

WORKSHOP ON NEUTRINO PHYSICS AND UNIFICATION, NEAR DETECTOR PHYSICS AND DARK MATTER (CETUP* 2016) | 2017年 / 1900卷

关键词：

D O I：

10.1063/1.5010122

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

The DarkSide-50 direct dark matter detector is a liquid argon time projection chamber (TPC) surrounded by a liquid scintillator neutron veto (LSV) and a water Cerenkov muon veto (WCV). Located under 3800 m.w.e. at the Laboratori Nazionali del Gran Sasso, Italy, it is the only direct dark matter experiment currently operating background free. The atmospheric argon target was replaced with argon from underground sources in April, 2015. The level of Ar-39, a beta emitter present in atmospheric argon (AAr), has been shown to have been reduced by a factor of (1.4 +/- 0.2) x 10(3). The combined spin-independent WIMP exclusion limit of 2.0 x 10(-44) cm(2) (m(chi) = 100 GeV/c(2)) is currently the best limit on a liquid argon target.

引用

页数：6

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