用日晷观测轴子和轴子（类）粒子的天体物理特征
Axion Searches with Helioscopes and astrophysical signatures for axion(-like) particles
摘要：
第一部分回顾了轴子太阳镜的工作机制、性能和性能，包括迄今为止所取得的成果。第二部分是观察驱动。用Geant 4代码获得的新模拟结果重建了太阳X射线光谱的光谱形状，以及它们的各向同性发射和横向尺寸。导出的类轴子粒子的初始质量约为10meV。轴子与磁场梯度的相互作用是一个通用的理论建议，可以调和目前的限制与相关的太阳X射线活动。本文对实验上的太阳轴子场的扩展作了简要的展望。
英文摘要：
The first part reviews the working mechanisms, capabilities and performance of axion helioscopes, including the achieved results so far. The 2nd part is observationally driven. New simulation results obtained with the Geant4 code reconstruct spectral shape of solar X-ray spectra, and their isotropic emission and lateral size. The derived rst mass of the axion(-like) particles is ~10meV. The axion interaction with magnetic field gradient is a generic theoretical suggestion that could reconcile present limits with relevant solar X-ray activity. A short outlook of the experimentally expanding solar axion field is given.
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。
