中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Particle dark matter in the galactic halo

文献类型:期刊论文

作者Bernabei, R; Belli, P; Cappella, F; Cerulli, R; Dai, CJ; d'Angelo, A; He, HL; Incicchitti, A; Ma, XH; Montecchia, F
刊名PROGRESS IN PARTICLE AND NUCLEAR PHYSICS
出版日期2011
卷号66期号:2页码:#REF!
关键词Dark Matter Annual modulation Scintillators Rare processes
通讯作者Bernabei, R (reprint author), Univ Roma Tor Vergata, Dip Fis, Rome, Italy.
英文摘要The presence of Dark Matter (DM) particles in the galactic halo can be unambiguously pointed out in a model-independent way by exploiting the DM annual modulation signature with an apparatus of specific features placed deep underground. At present DAMA/LIBRA is running at the Gran Sasso National Laboratory of the I.N.F.N. and has presented so far the results obtained with the data collected in the first six annual cycles (exposure 0.87 ton x yr). When including the exposure of the former DAMA/Nal experiment (0.29 ton x yr), the total exposure is 1.17 ton x yr for 13 annual cycles, a value order of magnitude larger than those typically released in the field. These DAMA/LIBRA data have further confirmed the model-independent evidence of the presence of Dark Matter particles in the galactic halo on the basis of the exploited DM signature (8.9 sigma C.L for the cumulative exposure). (c) 2011 Elsevier BM. All rights reserved.
学科主题Physics
类目[WOS]Physics, Nuclear ; Physics, Particles & Fields
收录类别SCI
WOS记录号WOS:000289600900001
公开日期2016-05-03
源URL[http://ir.ihep.ac.cn/handle/311005/226656]  
专题高能物理研究所_粒子天体物理中心
推荐引用方式
GB/T 7714
Bernabei, R,Belli, P,Cappella, F,et al. Particle dark matter in the galactic halo[J]. PROGRESS IN PARTICLE AND NUCLEAR PHYSICS,2011,66(2):#REF!.
APA Bernabei, R.,Belli, P.,Cappella, F.,Cerulli, R.,Dai, CJ.,...&叶子飘.(2011).Particle dark matter in the galactic halo.PROGRESS IN PARTICLE AND NUCLEAR PHYSICS,66(2),#REF!.
MLA Bernabei, R,et al."Particle dark matter in the galactic halo".PROGRESS IN PARTICLE AND NUCLEAR PHYSICS 66.2(2011):#REF!.

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来源:高能物理研究所

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