2019
DOI: 10.1063/1.5097440
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Double optimal density gradients for harmonic generation from relativistically oscillating plasma surfaces

Abstract: The influence of plasma density gradients on the harmonic generation process from relativistically oscillating mirror (ROM) is studied experimentally. It is observed that the harmonic intensities from orders of 21st to 24th first drop and then reach the maximum value with the increase of plasma scale length L. 2D particle-in-cell simulations are performed to investigate the intensities of high-order harmonics at different L values, which show that there are two optimal scale lengths L opt for efficient ROM har… Show more

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Cited by 11 publications
(10 citation statements)
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References 33 publications
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“…At the shortes gradients L − L 0 > λ 0 /50, the harmonic peaks are broad and their intensity quickly drops with increasing L, as expetected for CWE emission. At higher L, the harmonic peaks are remarkably narrower and their intensity goes through an optimum located at L − L 0 ≈ 0.06λ 0 , consistent with the theoretical expectations for relativistic SHHG emission as well as with earlier experimental observation with similar multi-cycle driver pulses [4,5,26,28]. We also remark that no harmonics are visible beyond the CWE-cutoff at 30 eV, even for softer gradients.…”
supporting
confidence: 91%
See 1 more Smart Citation
“…At the shortes gradients L − L 0 > λ 0 /50, the harmonic peaks are broad and their intensity quickly drops with increasing L, as expetected for CWE emission. At higher L, the harmonic peaks are remarkably narrower and their intensity goes through an optimum located at L − L 0 ≈ 0.06λ 0 , consistent with the theoretical expectations for relativistic SHHG emission as well as with earlier experimental observation with similar multi-cycle driver pulses [4,5,26,28]. We also remark that no harmonics are visible beyond the CWE-cutoff at 30 eV, even for softer gradients.…”
supporting
confidence: 91%
“…Furthermore, the intrinsic harmonic chirp and thus the spectral width of CWE-harmonic peaks increases with L [21,25]. In contrast, the optimal L for relativistic SHHG is longer and has been consistently found in single-shot experiments near a scale length L ≈ λ 0 /10 [4,5,26,28]. This can be shown to be consistent with particle-in-cell simulations, which often treat initially step-like plasma density profiles with variable peak density n. This adjusts the similarity parameter S = n/(n c a 0 ), which scales laser plasma-interaction in the relativistic regime [29].…”
mentioning
confidence: 90%
“…The different plasma emission characteristics can be explained as follows. Highest conversion efficiency for second harmonic generation on solid density targets is achieved for plasma density surface-scalelengths shorter than the pump laser wavelength 37 39 . Depending on the pre-pulse timing, the pre-pulses utilized here generate a scalelength of multiple pump laser wavelengths.…”
Section: Plasma Emission and Spectral Filteringmentioning
confidence: 99%
“…Here we propose a feasible scheme to realize the required pre-plasma truncation. The parameters of our scheme are based on the 200TW Ti:sapphire laser system at the Laboratory for Laser Plasmas of Shanghai Jiao Tong University [41]. As illustrated in Fig.…”
Section: Pre-plasma Truncation Realizationmentioning
confidence: 99%
“…The pre-plasma scale length is set to be L = 0.5λ 0 . This scale length is suitable for a fused silica glass irradiated by a laser with 10 −9 contrast [41], where the target surface would be preheated by the 10ps-ahead laser pedestal to a 10eV-level temperature. The 10 −9 contrast is currently a standard configuration for the commercial hundreds-of-terawatts laser chains.…”
Section: Pre-plasma Truncation Realizationmentioning
confidence: 99%