首页> 外文会议>2013 IEEE Nuclear Science Symposium and Medical Imaging Conference >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
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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

机译:国际空间站的α磁谱仪(AMS-02)的过渡辐射探测器和宇宙射线正电子分数的精确测量

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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.
机译:2011年5月19日,AMS-02实验成功部署在绕地球轨道的国际空间站(ISS)上,并自此一直持续运行。 AMS是太空中的复杂粒子探测器,通过精确测量带电的宇宙粒子来研究新粒子物理学和天体物理学来源的加速度,传播和贡献,从而在天体粒子物理学中进行研究。通过结合电磁热量计和过渡辐射探测器(TRD),AMS探测器的主要特征,即它的广泛接受,受ISS寿命限制的20年​​的长寿命任务以及独特的高质子排斥能力,使得这成为可能。 。 TRD旨在以高效率将正电子与巨大质子本底分开。提出了在0.5至350 GeV能量范围内对正电子分数的精确测量。准确的数据表明,正电子分数从10 GeV稳定增加,斜率在20 GeV和250 GeV之间减小一个数量级。正电子分数谱显示没有精细的结构并且没有可观察到的各向异性。这些观察结果表明,无论是从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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