空气阵雨模拟中的强子相互作用模型

M. Reininghaus, T. Sjostrand, M. Utheim
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引用次数: 3

摘要

强子相互作用模型是大范围风淋模拟的核心组成部分,也是风淋观测值预测不确定性的主要来源。最近,在基于加速器的高能物理中流行的强子相互作用模型Pythia 8也可用于空气淋室模拟。我们已经将Pythia 8及其新功能集成到空气淋室模拟框架CORSIKA 8中。第一个结果显示了明显较浅的星雨发展,我们将其归因于新的简化核模型更高的截面预测。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Pythia 8 as hadronic interaction model in air shower simulations
Hadronic interaction models are a core ingredient of simulations of extensive air showers and pose the major source of uncertainties of predictions of air shower observables. Recently, Pythia 8, a hadronic interaction model popular in accelerator-based high-energy physics, became usable in air shower simulations as well. We have integrated Pythia 8 with its new capabilities into the air shower simulation framework CORSIKA 8. First results show significantly shallower shower development, which we attribute to higher cross-section predictions by the new simplified nuclear model of Pythia.
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