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Search for magnetic monopoles with the ANTARES underwater neutrino telescope

机译:使用ANTARES水下中微子望远镜搜索磁性单极子

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The ANTARES underwater neutrino telescope, located in the Mediterranean Sea at a depth of 2475 m, 40kmoff the Provencal coast, is composed by an array of 885 photomultipliers distributed on 12 vertical lines. The detectoris fully operational since May 2008. Besides the detection of neutrino-induced muons, the telescope is more generallysensitive to particles which emit Cherenkov light, and, thanks to its large volume, offers new opportunities to improve thesensitivity to exotic particles, such as magnetic monopoles. Magnetic monopoles are stable magnetically charged particlesfirst introduced in quantum mechanics by Dirac in 1931, which showed that their existence would give an explanation tothe quantization of the electric charge. They would have been produced in the Early Universe, and would bring a firstproof to the existence of grand unified models. The paper introduces magnetic monopoles and their signal caracteristicsin a neutrino telescope, and then describes the analysis which uses a dedicated algorithm able to reconstruct the velocityof the incoming particles. A new upper limit on the upward going magnetic monopole flux, extracted from ANTARESdata taken in 2008, is presented. It is, at present, the best worldwide constraint in the velocity range = [0.625, 1], andprovides, for the first time with a neutrino telescope, a constraint for monopole velocities below the Cherenkov threshold.
机译:ANTARES水下中微子望远镜位于地中海,距普罗旺斯海岸40公里,深度2475 m,由分布在12条垂直线上的885个光电倍增管组成。该探测器自2008年5月开始全面运行。除了探测中微子引起的μ子外,该望远镜对发射切伦科夫光的粒子更敏感,并且由于其体积大,它提供了新的机会来提高对奇异粒子(如磁场)的敏感性单极子。磁单极子是稳定的带电粒子,最早是由狄拉克(Dirac)在1931年引入量子力学的,这表明它们的存在可以解释电荷的量子化。它们本来是在早期宇宙中生产的,这将为大统一模型的存在提供第一个证明。本文在中微子望远镜中介绍了磁单极子及其信号特性,然后描述了使用能够重构入射粒子速度的专用算法进行的分析。提出了从2008年获得的ANTARES数据中提取的单极磁通向上通量的新上限。目前,它是速度范围= [0.625,1]内的最佳全球约束,并且首次使用中微子望远镜为低于Cherenkov阈值的单极子速度提供了约束。

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