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arXiv 2308.00935hep-phastro-ph.COastro-ph.HE
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类轴子粒子与高能伽马射线:相互转化的再探讨

Axion-like particles and high-energy gamma rays: interconversion revisited

Rafael Alves Batista, Cristina Viviente, Gaetano Di Marco, Miguel A. Sánchez-Conde

AI总结:

该研究针对类轴子粒子(ALPs)搜寻问题,通过Monte Carlo模拟磁化环境中TeV高能伽马射线与ALPs的相互转化,完整纳入星系际电磁级联效应,为当前及未来的ALP探测研究提供改进的传播过程分析。

摘要:

类轴子粒子(ALPs)是一种假想实体,常被用于解决粒子物理到宇宙学领域的各类问题,是解释难以探测的暗物质的最有潜力的候选者之一。搜寻ALPs的一种途径是研究其对光子的影响:在外部磁场存在时,ALPs与光子可相互转化,产生可测量的信号。本文展示了磁化环境中ALP-光子相互转化的Monte Carlo模拟结果,研究对象为在宇宙学距离上传播的TeV能段高能伽马射线,完整考虑了伽马射线引发的星系际电磁级联过程。最后讨论了这种改进的传播处理方式对当前及未来ALP搜寻工作的影响。

英文摘要:

Axion-like particles (ALPs) are hypothetical entities often invoked to solve various problems in particle physics to cosmology. They are one of the most promising candidates to explain the elusive dark matter. A way to search for ALPs is through their effects on photons. In the presence of external magnetic fields, ALPs and photons can convert into one another, leading to measurable signals. In this contribution we present results of Monte Carlo simulations of ALP-photon interconversion in magnetised environments. We focus on high-energy gamma rays with TeV energies travelling over cosmological distances. We include a full treatment of the intergalactic electromagnetic cascades triggered by the gamma rays. Finally, we discuss the impact of this improved treatment of the propagation for current and future ALP searches.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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