First search for a dark matter annual modulation signal with NaI(Tl) in the Southern Hemisphere by DM-Ice17

被引:43
|
作者
de Souza, E. Barbosa [1 ,2 ]
Cherwinka, J. [3 ]
Cole, A. [4 ,5 ]
Ezeribe, A. C. [4 ]
Grant, D. [6 ]
Halzen, F. [7 ,8 ]
Heeger, K. M. [1 ,2 ]
Hsu, L. [9 ]
Hubbard, A. J. F. [1 ,2 ,7 ,8 ,11 ]
Jo, J. H. [1 ,2 ]
Karle, A. [7 ,8 ]
Kauer, M. [1 ,2 ,7 ,8 ]
Kudryavtsev, V. A. [4 ]
Lim, K. E. [1 ,2 ]
Macdonald, C. [4 ]
Maruyama, R. H. [1 ,2 ]
Mouton, F. [4 ]
Paling, S. M. [5 ]
Pettus, W. [1 ,2 ,7 ,8 ,12 ,13 ]
Pierpoint, Z. P. [1 ,2 ,7 ,8 ]
Reilly, B. N. [1 ,2 ,7 ,8 ,14 ]
Robinson, M. [4 ]
Rogers, F. R. [1 ,2 ,15 ]
Sandstrom, P. [7 ,8 ]
Scarff, A. [4 ]
Spooner, N. J. C. [4 ]
Telfer, S. [4 ]
Yang, L. [10 ]
机构
[1] Yale Univ, Dept Phys, New Haven, CT 06520 USA
[2] Yale Univ, Wright Lab, New Haven, CT 06520 USA
[3] Univ Wisconsin, Phys Sci Lab, Stoughton, WI 53589 USA
[4] Univ Sheffield, Dept Phys & Astron, Sheffield S10 2TN, S Yorkshire, England
[5] STFC Boulby Underground Sci Facil, Boulby Mine TS13 4UZ, Cleveland, England
[6] Univ Alberta, Dept Phys, Edmonton, AB T6G 2E1, Canada
[7] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA
[8] Univ Wisconsin, Wisconsin IceCube Particle Astrophys Ctr, Madison, WI 53706 USA
[9] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA
[10] Univ Illinois, Dept Phys, Urbana, IL 61801 USA
[11] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA
[12] Univ Washington, CENPA, Seattle, WA 98195 USA
[13] Univ Washington, Dept Phys, Seattle, WA 98195 USA
[14] Univ Wisconsin Fox Valley, Dept Phys & Astron, Menasha, WI 54952 USA
[15] MIT, Nucl Sci Lab, Cambridge, MA 02139 USA
基金
加拿大自然科学与工程研究理事会; 美国国家科学基金会; 美国能源部;
关键词
BACKGROUNDS; CRYSTALS; MODEL;
D O I
10.1103/PhysRevD.95.032006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the first search for a dark matter annual modulation signal in the Southern Hemisphere conducted with NaI(Tl) detectors, performed by the DM-Ice17 experiment. Nuclear recoils from dark matter interactions are expected to yield an annually modulated signal independent of location within the Earth's hemispheres. DM-Ice17, the first step in the DM-Ice experimental program, consists of 17 kg of NaI (Tl) located at the South Pole under 2200 m.w.e. overburden of Antarctic glacial ice. Taken over 3.6 years for a total exposure of 60.8 kg yr, DM-Ice17 data are consistent with no modulation in the energy range of 4-20 keV, providing the strongest limits on weakly interacting massive particle dark matter from a direct detection experiment located in the Southern Hemisphere. The successful deployment and stable long-term operation of DM-Ice17 establishes the South Pole ice as a viable location for future dark matter searches and in particular for a high-sensitivity NaI(Tl) dark matter experiment to directly test the DAMA/LIBRA claim of the observation of dark matter.
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页数:6
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