动量范围 ∼ 1 至 3 GeV/c 的宇宙射线μ介子的电荷比

IF 5.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Raj Shah, J.M. John, Suryanarayan Mondal, S. Pethuraj, G. Majumder and P. Shukla
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引用次数: 0

摘要

这项工作介绍了利用微型ICCAL探测器测量宇宙μ介子电荷比作为全方位角和动量在0.8至3.0 GeV/c范围内的函数。该探测器由10层RPC组成,自2018年8月起至近期,在印度马杜赖高能物理机构间中心(北纬9∘56',东经78∘00')海拔160米处收集宇宙μ介子数据。分析表明,宇宙μ介子电荷比 Rμ = Nμ+/Nμ- 在 1.1 到 1.2 之间,与天顶角的关系很小。在高达 50∘ 的天顶角范围内,对电荷比与动量和方位角的关系进行了深入研究。这些测量结果与 CORSIKA 大范围气雨模拟中不同强子模型组合的预测结果进行了比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Charge ratio of cosmic ray muons in momentum range ∼ 1 to 3 GeV/c
This work presents the measurements of the cosmic muon charge ratio as a function of full azimuthal angle and momentum within the range of 0.8 to 3.0 GeV/c, using the mini-ICAL detector. The detector, comprising 10 layers of RPCs, has collected cosmic muon data since August 2018 till recent time, at an altitude of 160 m above sea level at the Inter-Institutional Center for High Energy Physics in Madurai, India (9∘56' N, 78∘00' E). The muon charge identification is achieved through the use of a magnetic field of strength 1.4 T. The analysis shows that the cosmic muon charge ratio, Rμ = Nμ+/Nμ-, ranges from 1.1 to 1.2 and has small dependency on the zenith angle. The charge ratio's dependence on momentum and azimuthal angle is thoroughly examined for a wide range of zenith angle upto 50∘. These measurements are compared with the predictions from various combinations of different hadronic models in CORSIKA extensive air shower simulations.
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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