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Particle dark matter in the galactic halo: Recent results from DAMA/LIBRA

机译:银河晕中的暗物质粒子:DAMA / LIBRA的最新结果

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The DAMA/LIBRA experiment has a sensitive mass of about 250 kg highly radiopure NaI(Tl). It is running at the Gran Sasso National Laboratory of the INFN in Italy and is mainly devoted to the investigation of dark matter (DM) particles in the galactic halo by exploiting the model-independent DM annual modulation signature. The present DAMA/LIBRA and the former DAMA/NaI experiments (the first generation experiment having an exposed mass of about 100 kg) have thus far cumulatively released the results of data collected over 13 annual cycles (total exposure: 1.17 t year). They give model-independent evidence of the presence of DM particles in the galactic halo on the basis of the investigated DM signature at 8.9 π C.L. for the cumulative exposure. The main aspects of the obtained results are summarized and some comments are addressed.
机译:DAMA / LIBRA实验的敏感物质约为250 kg高纯NaI(Tl)。它在意大利INFN的Gran Sasso国家实验室运行,主要致力于通过利用与模型无关的DM年度调制特征来研究银河晕中的暗物质(DM)颗粒。迄今为止,目前的DAMA / LIBRA实验和以前的DAMA / NaI实验(第一代实验的暴露质量约为100千克)已经累积释放了13个年周期(总暴露量:1.17吨)收集的数据结果。根据研究的DM签名(在8.9πC.L下),他们提供了模型无关的证据,证明银河晕中存在DM颗粒。累积曝光。总结了所获得结果的主要方面,并提出了一些意见。

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