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ELMAG: A Monte Carlo simulation of electromagnetic cascades on the extragalactic background light and in magnetic fields

机译:ELMAG:在银河外背景光和磁场中电磁级联的蒙特卡洛模拟

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摘要

A Monte Carlo program for the simulation of electromagnetic cascades initiated by high-energy photons and electrons interacting with extragalactic background light (EBL) is presented. Pair production and inverse Compton scattering on EBL photons as well as synchrotron losses and deflections of the charged component in extragalactic magnetic fields (EGMF) are included in the simulation. Weighted sampling of the cascade development is applied to reduce the number of secondary particles and to speed up computations. As final result, the simulation procedure provides the energy, the observation angle, and the time delay of secondary cascade particles at the present epoch. Possible applications are the study of TeV blazars and the influence of the EGMF on their spectra or the calculation of the contribution from ultrahigh energy cosmic rays or dark matter to the diffuse extragalactic gamma-ray background. As an illustration, we present results for deflections and time delays relevant for the derivation of limits on the EGMF.
机译:提出了用于模拟由高能光子和电子与河外背景光(EBL)相互作用引发的电磁级联的Monte Carlo程序。模拟包括EBL光子上的成对产生和Compton逆散射以及银河系外磁场(EGMF)中的同步加速器损耗和带电分量的偏转。级联展开的加权采样用于减少次级粒子的数量并加快计算速度。作为最终结果,模拟过程提供了当前时间段的二级叶栅粒子的能量,观察角度和时间延迟。可能的应用包括TeV blazar的研究以及EGMF对它们的光谱的影响,或者计算超高能宇宙射线或暗物质对弥漫性河外γ射线背景的贡献。作为说明,我们给出了与EGMF极限的推导有关的挠度和时间延迟的结果。

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