重新审视电磁风淋室的纵向发展:对具有天顶角依赖性的格雷森形式论的分析改进

IF 2.9 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Sebastián Mendizabal , Nicolás Viaux M. , Sebastián Tapia , Raquel Pezoa R. , Barbara Gutiérrez , Constanza Valdivieso
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引用次数: 0

摘要

我们提出了一种新的电磁风淋室纵向发展的分析方法,对经典的格雷森形式主义进行了改进。我们引入了斜率函数λ1(s)的修改剖面,该剖面与原始λ1在0.3<s<;1.4之间的一致性小于0.75%,其中s表示淋浴发展阶段。我们的新形式提供了一个改进的阵雨演化的表示,特别是接近和超过阵雨最大值。此外,我们提出了一个修改过的格雷森剖面。我们的实现包括天顶角依赖于高海拔探测器水平的粒子数量,这使得它对高海拔天文台特别有用。该表达式适用于在各种能量和几何形状上实现风淋室模拟工具的装配程序。我们的分析表明,当我们将其与CORSIKA模拟进行比较时,与Greisen公式相比,改进的Greisen剖面与预期的粒子数演变更吻合。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Revisiting the longitudinal development of electromagnetic air showers: Analytical improvements to the Greisen formalism with zenith angle dependence
We present a new analytical approach to the longitudinal development of electromagnetic air showers, offering improvements to the classical Greisen formalism. We introduce a modified profile for the slope function λ1(s) that achieves an agreement less than 0.75% with the original λ1 for shower age parameter s between 0.3<s<1.4, where s represents the stage of shower development. Our new formalism provides an improved representation of shower evolution, particularly near and beyond the shower maximum. In addition, we propose a modified Greisen profile. Our implementation includes the zenith angle dependence on the number of particles at the detector level at high altitudes, making it particularly useful for high-altitude observatories. This expression is suitable for implementing air shower simulation tool fitting procedures over a wide range of energies and geometries. Our analysis shows that the modified Greisen profile provides better agreement with the expected evolution of particle numbers compared to the Greisen formulation when we compare it with CORSIKA simulations.
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来源期刊
Astroparticle Physics
Astroparticle Physics 地学天文-天文与天体物理
CiteScore
8.00
自引率
2.90%
发文量
41
审稿时长
79 days
期刊介绍: Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.
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