论文标题
观察真空指数的光学诱导的变化的效果实验
The DeLLight experiment to observe an optically-induced change of the vacuum index
论文作者
论文摘要
量子电动力学预测,真空必须以非线性光学介质的形式行为:当真空通过强烈的电磁场压力时,应修改光速。尚未观察到这种光学现象。 Dellight(通过光的偏转)实验旨在观察真空的光学诱导的指数变化,这是从未探索过的非线性效应。该实验安装在IJClab的Laserix设施中,该设施可提供超短的激光脉冲(每脉冲2.5 j,每次30 fs持续时间,每个脉冲持续时间为10 Hz,重复率为10 Hz)。该建议是在横穿横向真空指数梯度时测量探针激光脉冲的折射,这是由非常强烈的泵脉冲产生的。折射诱导探针强度曲线的横向移动,该探针的信号被SAGNAC干涉仪扩增。在本文中,我们描述了实验方法和设置,并介绍了预期信号的完整理论计算。最小腰部为$ 5 \,μ$ m(对应于$ \ sim 3 \ times 10^{20} $ w/cm $ $^2 $)的最大强度,并且具有QED的非线性真空索引,预期的折射角度为0.13 prad。提出了干涉仪原型的第一个结果。结果表明,灭绝因子$ \ mathcal {f} = 0.4 \ times 10^{ - 5} $(对应于信号放大因子250)和空间分辨率$σ_y= 10 $ nm是可以实现的。然后,预期信号大约为15 pm,并且可以在5-秒置信度的水平下观察到约一个月的收集数据。
Quantum electrodynamics predicts that the vacuum must behave as a nonlinear optical medium: the speed of light should be modified when the vacuum is stressed by intense electromagnetic fields. This optical phenomenon has not yet been observed. The DeLLight (Deflection of Light by Light) experiment aims to observe the optically-induced index change of vacuum, a nonlinear effect which has never been explored. The experiment is installed in the LASERIX facility at IJCLab, which delivers ultra-short intense laser pulses (2.5 J per pulse, each of 30 fs duration, with a 10 Hz repetition rate). The proposal is to measure the refraction of a probe laser pulse when crossing a transverse vacuum index gradient, produced by a very intense pump pulse. The refraction induces a transverse shift in the intensity profile of the probe, whose signal is amplified by a Sagnac interferometer. In this article, we describe the experimental method and setup, and present the complete theoretical calculations for the expected signal. With a minimum waist at focus of $5 \,μ$m (corresponding to a maximum intensity of $\sim 3 \times 10^{20}$ W/cm$^2$), and with the nonlinear vacuum index derived from QED, the expected refraction angle is 0.13 prad. First results of the interferometer prototype are presented. It is shown that an extinction factor $\mathcal{F} = 0.4 \times 10^{-5}$ (corresponding to a signal amplification factor of 250) and a spatial resolution $σ_y = 10$ nm are achievable. The expected signal is then about 15 pm, and could be observed at a 5-sigma confidence level with about one month of collected data.