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
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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!. |
入库方式: OAI收割
来源:高能物理研究所
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