Lorentz-Violation Constraints with Astroparticle Physics

H. Mart'inez-Huerta
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引用次数: 3

Abstract

Astroparticle physics has recently reached a new status of precision due to the construction of new observatories, operating innovative technologies and the detection of large numbers of events and sources. The precise measurements of cosmic and gamma rays can be used as a test for fundamental physics, such as the Lorentz invariance violation (LV). Although LV signatures are expected to be small, the very high energies and long distances that astrophysical sources involve, lead to an unprecedented opportunity for this task. In this summary, exclusion limits results are presented from different types of astrophysical LV tests through the generic modification of the particle dispersion relation in the photon sector through the pair production threshold shifts and photon decay. Some perspectives for the next generations of gamma-ray telescopes are also addressed
天体粒子物理学中的洛伦兹违和约束
由于新天文台的建设、操作创新技术以及对大量事件和源的探测,天体粒子物理学最近达到了一个新的精度状态。对宇宙射线和伽马射线的精确测量可以用来测试基础物理学,比如洛伦兹不变性破坏(LV)。虽然LV信号预计很小,但天体物理源涉及的非常高的能量和长距离,为这项任务带来了前所未有的机会。本文通过对产生阈值位移和光子衰变对光子扇区粒子色散关系进行一般性修正,给出了不同类型的天体物理LV测试的排除极限结果。对下一代伽玛射线望远镜的一些展望也进行了讨论
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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