超高能量的天体粒子和粒子物理:皮埃尔·奥格天文台的结果

Antonella Castellina
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引用次数: 0

摘要

皮埃尔·奥格合作的科学成果涵盖了不同的和互补的研究领域。对超高能宇宙射线(uhecr)起源的研究是基于对原初能谱和质量组成的测量、对多信使的研究以及广泛的各向异性搜索。利用收集到的数据,还可以探索在人造加速器无法达到的能量下强子相互作用的特征,并评估非标准物理效应的存在。本文介绍了一些最新的研究结果,并讨论了新出现的情况。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Astroparticle and particle physics at ultra-high energy: Results from the Pierre Auger Observatory
The scientific achievements of the Pierre Auger Collaboration cover diverse and complementary fields of research. The search for the origin of ultra-high energy cosmic rays (UHECRs) is based on the measurement of the energy spectrum and mass composition of the primaries, on studies of multi-messengers, and on extensive anisotropy searches. With the collected data it is also possible to explore the characteristics of hadronic interactions at energies unreachable at human-made accelerators, and to assess the existence of non-standard physics effects. A selection of the latest results is presented and the emerging picture is discussed.
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