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超短紫外和极紫外脉冲的共线产生。

Collinear generation of ultrashort UV and XUV pulses.

作者信息

Bothschafter E M, Schiffrin A, Yakovlev V S, Azzeer A M, Krausz F, Ernstorfer R, Kienberger R

机构信息

Max-Planck-Institut für Quantenoptik, Hans-Kopfermann-Str. 1, D-85748 Garching, Germany.

出版信息

Opt Express. 2010 Apr 26;18(9):9173-80. doi: 10.1364/OE.18.009173.

Abstract

We demonstrate the collinear generation of few-femtosecond ultraviolet and attosecond extreme ultraviolet pulses via a combination of third-harmonic and high harmonic generation in noble gases. The ultrashort coherent light bursts are produced by focusing a sub-1.5-cycle near-infrared/visible laser pulse in two subsequent quasi-static noble gas targets. This approach provides an inherently synchronized pair of UV and XUV pulses, where the UV radiation has a photon energy of approximately 5 eV and a pulse energy of up to 1 microJ and the XUV radiation contains up to 3.5 10(6) XUV photons per shot with a photon energy exceeding 100 eV. This source represents a novel tool for future UV pump/XUV probe experiments with unprecedented time-resolution.

摘要

我们通过在惰性气体中结合三次谐波产生和高次谐波产生,演示了飞秒级紫外光和阿秒级极紫外光脉冲的共线产生。超短相干光脉冲是通过将一个小于1.5周期的近红外/可见光激光脉冲聚焦在两个连续的准静态惰性气体靶中产生的。这种方法提供了一对本质上同步的紫外光和极紫外光脉冲,其中紫外辐射的光子能量约为5电子伏特,脉冲能量高达1微焦耳,而极紫外辐射每次脉冲包含多达3.5×10⁶个极紫外光子,光子能量超过100电子伏特。该光源代表了一种用于未来紫外泵浦/极紫外探测实验的新型工具,具有前所未有的时间分辨率。

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