Improved dark matter limits from pulse shape discrimination in a low background sodium iodide detector at the Boulby mine

被引:149
作者
Smith, PF
Arnison, GTJ
Homer, GJ
Lewin, JD
Alner, GJ
Spooner, NJC
Quenby, JJ
Sumner, TJ
Bewick, A
Li, JP
Shaul, D
Ali, T
Jones, WG
Smith, NJT
Davies, GJ
Lally, CH
vandenPutte, MJ
Barton, JC
Blake, PR
机构
[1] UNIV SHEFFIELD, DEPT PHYS, SHEFFIELD S3 7RH, S YORKSHIRE, ENGLAND
[2] UNIV LONDON IMPERIAL COLL SCI TECHNOL & MED, BLACKETT LAB, LONDON SW7 2BZ, ENGLAND
[3] UNIV LONDON BIRKBECK COLL, DEPT PHYS, LONDON WC1E 7HX, ENGLAND
[4] UNIV NOTTINGHAM, DEPT PHYS, NOTTINGHAM NG7 2RD, ENGLAND
关键词
D O I
10.1016/0370-2693(96)00350-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report new limits on nuclear scattering events resulting from Galactic dark matter in the form of hypothetical weakly interacting massive particles. By pulse shape analysis of 6 months' underground data from a 6 kg sodium iodide crystal, over the gamma-equivalent energy range 4-25 keV, we achieve a sensitivity to nuclear recoil events a factor 10-40 below the gamma and beta background. Limits obtained for spin-dependent dark matter interactions improve on Ge detectors by a factor 50. Limits for coherent interactions improve marginally on Ge for masses > 50 GeV, with foreseeable improvements offering further gains of 1-2 orders of magnitude.
引用
收藏
页码:299 / 308
页数:10
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