First limits on nuclear recoil events from the ZEPLIN I galactic dark matter detector

被引:101
作者
Alner, GJ
Araujo, H
Arnison, GJ
Barton, JC
Bewick, A
Bungau, C
Camanzi, B
Carson, MJ
Davidge, D
Dawson, JV
Davies, GJ
Davies, JC
Durkin, T
Gamble, T
Hart, SP
Hollingworth, RJ
Homer, GJ
Howard, AS
Ivaniouchenkov, I
Jones, WG
Joshi, MK
Kudryavtsev, VA
Lawson, TB
Lebedenko, V
Lewin, JD
Lightfoot, PK
Liubarsky, I
Lehner, MJ
Lüscher, R
McMillan, JE
Morgan, B
Nicholls, A
Nicklin, G
Paling, SM
Preece, RM
Roberts, JW
Robinson, M
Quenby, JJ
Smith, NJT [1 ]
Smith, PF
Spooner, NJC
Sumner, TJ
Tovey, D
机构
[1] Rutherford Appleton Lab, Particles Phys Dept, Didcot OX11 0QX, Oxon, England
[2] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BZ, England
[3] Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England
[4] Queen Mary Univ London, Dept Phys, London E1 4NS, England
关键词
dark matter; WIMPs; scintillation detectors; liquid xenon; pulse shape analysis;
D O I
10.1016/j.astropartphys.2005.02.004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report first results from the ZEPLIN I dark matter detector, based on measurement of scintillation pulse shapes in a liquid xenon target of 3.2 kg fiducial mass. Neutron calibration shows nuclear recoil pulses to have a time constant congruent to 0.5 that of gamma and beta background events. The detector is located in the 2800 mwe depth UK Boulby Mine, and is surrounded by a liquid scintillator Compton veto and passive lead shielding. Three runs totaling 293 kg d fiducial exposure yielded data consistent with a single population of background pulses, with no significant low energy population of shorter pulses. From the 90% confidence limit on the latter a limit is derived on the spin-independent WIMP-nucleon cross-section versus particle mass with a minimum at 1.1 x 10(-6) ph. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:444 / 462
页数:19
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