Searches for Lorentz-Violating Signals with Astrophysical Polarization Measurements

F. Kislat
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引用次数: 1

Abstract

Astrophysical observations are a powerful tool to constrain effects of Lorentz-invariance violation in the photon sector. Objects at high redshifts provide the longest possible baselines, and gamma-ray telescopes allow us to observe some of the highest energy photons. Observations include polarization measurements and time-of-flight measurements of transient or variable objects to constrain vacuum birefringence and dispersion. Observing multiple sources covering the entire sky allows the extraction of constraints on anisotropy. In this paper, I review methods and recent results on Lorentz- and CPT-invariance violation constraints derived from astrophysical polarization measurements in the framework of the Standard-Model Extension.
用天体物理偏振测量搜索违反洛伦兹的信号
天体物理观测是约束光子扇区中洛伦兹不变性破坏效应的有力工具。高红移的物体提供了最长的基线,而伽马射线望远镜使我们能够观察到一些最高能量的光子。观测包括偏振测量和瞬态或可变物体的飞行时间测量,以约束真空双折射和色散。观测覆盖整个天空的多个光源可以提取各向异性的约束条件。本文综述了在标准模型扩展框架下天体物理偏振测量得出的洛伦兹和cpt不变性违反约束的方法和最新结果。
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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