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首页> 外文期刊>Advances in space research >Antiproton flux and properties of elementary particle fluxes in primary cosmic rays measured with the Alpha Magnetic Spectrometer on the International Space Station
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Antiproton flux and properties of elementary particle fluxes in primary cosmic rays measured with the Alpha Magnetic Spectrometer on the International Space Station

机译:用国际空间站α磁光谱仪测量初级宇宙射线中基本粒子通量的ANTIPROTON通量和性质

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Precision measurements by AMS of the antiproton flux and the antiproton-to-proton flux ratio in primary cosmic rays in the absolute rigidity range from 1 to 525 GV is presented, together with the fluxes and flux ratios of charged elementary particles in cosmic rays up to 1 TV. In the absolute rigidity range 60-500 GV, the antiproton (p) over bar, proton p and positron e(+) fluxes are found to have nearly identical rigidity dependence and the electron e(-) flux exhibits different rigidity dependence. From 60GV to 500 GV, the (p) over bar /p, (p) over bar /e(+) and p/e(+) flux ratios are rigidity independent. These AMS measurements continue to reveal important properties of cosmic ray elementary particle fluxes and provide invaluable input towards understanding the origin of many observed unexpected phenomena. (C) 2019 COSPAR. Published by Elsevier Ltd. All rights reserved.
机译:通过1至525GV的绝对刚度范围内的ANTIPORON通量的AMS的精度测量和初级辅助光线中的初级辅助光线的磁通比,以及宇宙光线中带电基本颗粒的助熔剂和通量比率。 1台电视。在绝对刚度范围内60-500gVV,发现对棒,质子P和正电子馈电通的反罗托(P)具有几乎相同的刚度依赖性,并且电子E( - )通量表现出不同的刚性依赖性。从60gV至500 gv,(p)上方的rel / p,(p)上方(+)和p / e(+)通量比是刚性的刚性。这些AMS测量继续揭示宇宙射线基本粒子通量的重要特性,并为了解许多观察到的意外现象的起源提供宝贵的输入。 (c)2019 Cospar。 elsevier有限公司出版。保留所有权利。

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