国际空间站α磁谱仪(AMS-02)的跃迁辐射探测器及宇宙射线正电子分数的精密测量

C. Chung
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引用次数: 3

摘要

2011年5月19日,AMS-02实验成功部署在绕地球轨道运行的国际空间站(ISS)上,此后一直在持续运行,没有中断。AMS是一个复杂的空间粒子探测器,通过精确测量带电宇宙粒子来研究加速、传播以及新粒子物理和天体物理源的贡献,从而进行天体粒子物理研究。这是由于AMS探测器的主要特点,即其广泛的接受度,国际空间站寿命限制的约20年的长时间任务,以及结合电磁量热计和过渡辐射探测器(TRD)独特的高质子排斥功率。TRD被设计用于以高效率从巨大的质子背景中分离正电子。提出了在0.5 ~ 350 GeV能量范围内精确测量正电子分数的方法。精确数据表明,正电子分数从10 ~ 250 GeV稳步增加,在20 ~ 250 GeV之间以一个数量级的斜率递减。正电子分数谱没有精细结构,也没有观察到各向异性。这些观测表明,不论是粒子物理学还是天体物理学的起源,都存在着新的物理现象。
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The transition radiation detector of the alpha magnetic spectrometer(AMS-02) on the International Space Station and the precision measurement of the cosmic ray positron fraction
On May 19th 2011, the AMS-02 experiment was successfully deployed on board the Earth-orbiting International Space Station (ISS) and is constantly operating since then without interruption. AMS is a complex particle detector in space and conducts research in astroparticle physics by precisely measuring charged cosmic particles to study acceleration, propagation and contributions from new particle physics and astrophysical sources. This is made possible by the main features of the AMS detector, namely its large acceptance, the long duration mission about 20 years limited by the ISS lifespan and the unique high proton rejection power by combining the electromagnetic calorimeter and the transition radiation detector (TRD). The TRD is designed to separate positrons from the huge proton background with a high efficiency. A precision measurement of the positron fraction in the energy range from 0.5 to 350 GeV is presented. The accurate data show that the positron fraction is steadily increasing from 10 to 250 GeV with a decreasing slope by an order of magnitude between 20 and 250 GeV. The positron fraction spectrum shows no fine structure and no observable anisotropy. These observations show the existence of new physical phenomena whether from a particle physics or an astrophysical origin.
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