Attosecond Rabi Oscillations Revealed in EUV-Driven High Harmonic Spectroscopy

A. de las Heras, C. Hernández-García, J. Serrano, T. Popmintchev, L. Plaja
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引用次数: 0

Abstract

The prominent progress in the development of high-intensity extreme ultraviolet (EUV) coherent light sources enables the exploration of a novel regime of nonlinear optical interactions and attosecond metrology driven by short-wavelength pulses [1]–[3]. Here, we theoretically demonstrate the presence of ultrafast resonant two-state dynamics in EUV nonlinear optics phenomena, where the driving-laser photon energies are close to atomic transitions and the intense field induces ultrafast ionization. We observe, for the first time, a distinctive multi-peak harmonic signature of attosecond Rabi oscillations in the high-harmonic emission from helium driven by high-intensity EUV pulses. The periodic population exchange between the 1s and 2p orbitals of the helium atom triggers a temporal modulation of the dipole emission that leads to a multi-peak harmonic structure in the frequency domain. Interestingly, the period of such Rabi oscillations is of femtosecond-to-attosecond time scales. To the best of our knowledge, these are the fastest resonant dynamics ever reported.
在euv驱动的高谐波光谱中揭示的阿秒拉比振荡
高强度极紫外(EUV)相干光源的发展取得了显著进展,这使得探索由短波脉冲驱动的非线性光相互作用和阿秒计量的新体制成为可能[1]-[3]。在此,我们从理论上证明了在极紫外光非线性光学现象中存在超快共振双态动力学,其中驱动激光光子能量接近原子跃迁,强场诱导超快电离。我们首次观察到高强度极紫外光脉冲驱动氦的高次谐波发射中阿秒拉比振荡的明显多峰谐波特征。氦原子1s轨道和2p轨道之间的周期性能级交换触发偶极子发射的时间调制,导致频域的多峰谐波结构。有趣的是,这种拉比振荡的周期是飞秒到阿秒的时间尺度。据我们所知,这是有史以来最快的共振动力学。
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CiteScore
3.10
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