超强激光:相对论非线性光学及其应用

Gérard A. Mourou
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引用次数: 1

摘要

传统光学和非线性光学都是研究激光与物质相互作用与eV特征能量的关系。超高强度的最新进展使得用相对论性能量驱动电子成为可能,开辟了相对论性非线性光学领域。近十年来,随着啁啾脉冲放大技术(CPA)的发明和飞秒技术的改进,激光的峰值功率发生了数量级的飞跃。现代CPA激光器可以产生大于1021 W/cm2的强度,比以前可能的大一百万倍。这些超强激光为研究人员提供了一种工具,可以产生前所未有的压力(太巴)、磁场(千兆赫)、温度(1010k)和加速度(1025g),并应用于核聚变能、核物理学(快速点火)、高能物理、天体物理学和宇宙学。它们将光学场从eV推进到GeV。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Ultraintense lasers: relativistic nonlinear optics and applications

Traditional optics and nonlinear optics are related to laser–matter interaction with eV characteristic energy. Recent progresses in ultrahigh intensity makes it possible to drive electrons with relativistic energy opening up the field of relativistic nonlinear optics. In the last decade, lasers have undergone orders-of-magnitude jumps in peak power, with the invention of the technique of chirped pulse amplification (CPA) and the refinements of femtosecond techniques. Modern CPA lasers can produce intensities greater than 1021 W/cm2, one million times greater than previously possible. These ultraintense lasers give researchers a tool to produce unprecedented pressures (terabars), magnetic fields (gigagauss), temperatures (1010 K), and accelerations (1025 g) with applications in fusion energy, nuclear physics (fast ignition), high-energy physics, astrophysics, and cosmology. They promote the optics field from the eV to the GeV.

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