海平面高能大气渺子通量和电荷比计算*

IF 1.1 4区物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS

Astronomy Letters-A Journal of Astronomy and Space Astrophysics Pub Date : 2024-03-17 DOI:10.1134/S1063773723340017

A. B. Bouasla, R. Attallah

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引用次数: 0

摘要

摘要高能大气μ介子是现代深大容积中微子望远镜的主要事件产率。研究它们在海平面上的特性对于准确破译观测到的信号至关重要。这项研究涉及计算海平面上能量超过 100 GeV 的大气μ介子的通量和电荷比。计算采用了蒙特卡洛代码 CORSIKA 和几种最先进的强子相互作用模型。所获得的结果与一组实验数据和其他最新的可比研究进行了比较。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Calculation of the Flux and Charge Ratio of High-Energy Atmospheric Muons at Sea Level*

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Calculation of the Flux and Charge Ratio of High-Energy Atmospheric Muons at Sea Level*

Atmospheric muons of high energy constitute the major event yield in modern deep large-volume neutrino telescopes. Examining their properties at sea level is crucial for accurately deciphering observed signals. This study involves the computation of the flux and charge ratio of the atmospheric muons with energies exceeding 100 GeV at sea level. The calculation employs the Monte Carlo code CORSIKA in conjunction with several state-of-the-art hadronic interaction models. The obtained results are compared with a set of experimental data and with other recent comparable studies.

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来源期刊

Astronomy Letters-A Journal of Astronomy and Space Astrophysics 地学天文-天文与天体物理

CiteScore

1.70

自引率

22.20%

发文量

审稿时长

6-12 weeks

期刊介绍： Astronomy Letters is an international peer reviewed journal that publishes the results of original research on all aspects of modern astronomy and astrophysics including high energy astrophysics, cosmology, space astronomy, theoretical astrophysics, radio astronomy, extragalactic astronomy, stellar astronomy, and investigation of the Solar system.