首页|基于百太瓦级激光系统驱动的高能量13 nm波段高次谐波产生

基于百太瓦级激光系统驱动的高能量13 nm波段高次谐波产生

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利用百太瓦级激光系统在氖气(Ne)中得到基于高次谐波产生的极紫外脉冲.通过松聚焦结构在13 nm波段产生单级次单脉冲能量为13.5 nJ(13.1 nm波长)和11.1 nJ(13.5nm波长)的高次谐波辐射,转换效率为3.6 × 10-7和3.0× 10-7,谐波发散角的半高全宽为0.32 mrad和0.33 mrad.对含时薛定谔方程进行数值求解,得到单原子偶极发射谱,结合麦克斯韦方程组模拟传播效应,同时考虑气体对谐波的吸收效应,理论模拟得到的信号强度随气压和光强的变化趋势与实验结果基本符合.实现相位匹配的谐波光束质量很好,纵向空间分布为高斯型.结合相位匹配条件和空间分布的分析得到了目前激光参数下的最优相位匹配条件.这种基于高次谐波机制的高能量相干极紫外光源在作为自由电子激光的种子光源以及超快非线性实验和半导体工业检测等方面具有广阔的应用前景.
High-Energy High-Order Harmonic Generation Around 13 nm Wavelength Based on Hundred-Terawatt-Level Laser System
Objective With the rapid development of high-order harmonic extreme ultraviolet coherent light sources and attosecond pulses,they have caught widespread attention in free electron laser seed injection,time-resolved angular resolved photoelectron spectroscopy measurement,and nondestructive nanostructure detection.There are many ways to generate extreme ultraviolet light sources,including synchrotron radiation,laser produced plasma,and free electron lasers,which can also be employed to generate high-energy extreme ultraviolet light sources.Compared to other light sources,high-order harmonics feature good coherence,short pulse duration,and device miniaturization.Currently,the high-order harmonic mechanism has been widely adopted to generate coherent light sources in the extreme ultraviolet region.We utilize a self-developed 200 TW titanium sapphire laser system with a maximum single pulse energy that can reach 8 J,and a main pulse energy of 7.9 J after beam splitting is transported to the free electron laser experiment for generating an electron beam source based on the acceleration mechanism of laser wakefield.The second laser beam is leveraged for high-order harmonic generation experiments.Both experiments are conducted synchronously to facilitate the simultaneous injection of electron beams and extreme ultraviolet seed beams into the oscillators in the future.Methods As shown in Fig.1(a),the whole system is placed in a vacuum chamber to avoid strong absorption of extreme ultraviolet pulse,and the vacuum system maintains the background pressure of 10-3 Pa.The driving laser parameters include a center wavelength of 800 nm,repetition rate of 1 Hz,pulse width of 30 fs,and energy of 35 mJ.A plano-convex mirror with a focal length of 5000 mm and a focal spot diameter of about 400 μm is adopted.The length of the Ne-filled gas cell is 50 mm.The harmonic radiation propagates with the residual driving laser and then transmits through the iris to the measurement section.Two Mo mirrors and a 350 nm-thick Zr filter are placed behind the iris to attenuate the fundamental laser field.Then,the harmonic signals can be divided into two different paths via the moveable gold-coated spherical mirror.Absolute harmonic energy is measured with an XUV(extreme ultra violet)photodiode detector which is calibrated by the Beijing Synchrotron Radiation Facility to get the real spectrum response curve.When the spherical mirror moves into the beam path,the HHG(high-order harmonic generation)spectrum is detected by a home-built flat-filed grating spectrometer.The spatial harmonic distribution is obtained by calculating the longitudinal spectrum of the XUV charge-coupled device.Results and Discussions Figures 1(b)and 1(c)show the generated harmonic spectra.From the 41st to the 69th harmonics(19.5 nm to 11.6 nm wavelength),the total energy of HHG is about 78.7 nJ.According to the HHG spectral distribution,the single harmonic energy of the 61st harmonic(13.1 nm)and 59th harmonic(13.5 nm)is 13.5 nJ and 11.1 nJ,respectively.The conversion efficiency is 3.6 × 107 for 61st harmonic and 3 × 10-7 for 59th harmonic.The divergence of the output beam measured at 61st and 59th harmonics is about 0.32 mrad and 0.33 mrad(full width at half maxima,FWHM).To obtain the optimal HHG extreme ultraviolet source at the wavelength of 13 nm,we investigate the 61st and the 59th harmonic intensity generated in Ne as a function of the gas pressure and driving laser energy.Figures 2(a)and 2(e)present the optimal phase-matching conditions for driving laser energy with the position of gas cell.With the increasing laser energy,the optimal phase-matching position moves to the negative position.Then the optimal phase-matching conditions for the gas pressure at 9 × 1014 W/cm2 are studied.As shown in Figs.2(c)and 2(g),two optimal phase-matching conditions for 61st harmonic are 6.0 kPa at-100 mm position and 7.6 kPa at-160 mm position,respectively.The optimal gas pressure for the 59th and 61st harmonics is basically the same,but 59th harmonic matching range of gas pressure is wider,with the matching gas pressure slightly higher than that for the 61st harmonic.Figures 2(b),2(d),2(f),and 2(h)demonstrate the theoretical results in Ne that generates harmonics as a function of driving laser energy and gas pressure respectively.Based on the experimental and theoretical simulation results in Fig.2,the spectra of three different focal positions with maximum harmonic signals are selected for analysis in Fig.3,which shows the harmonic spectra at different focal positions.The beam divergence of the 61st and the 59th harmonics is about 0.30 mrad and 0.31 mrad at position of 0,0.32 mrad and 0.33 mrad at position of-100 mm,and 0.57 mrad and 0.65 mrad at position of-160 mm.The fitting results of harmonic distribution and curve at positions 0 and-100 mm are better than those at-160 mm.Additionally,the Gaussian-like distribution shows that the phase-matching conditions are well achieved.The simulated changes in gas pressure and driving laser energy in phase-matching conditions are basically the same as the experimental results.Finally,the optimal phase-matching conditions for the current laser parameters are obtained by combining the longitudinal distribution of the 13 nm spectra obtained at different focal positions.Combined with the experimental and simulation results,the relationship between phase-matching conditions and focal positions is realized by optimizing parameters such as driving laser energy and gas pressure.Meanwhile,the longitudinal spatial distribution of harmonic signals at different focal positions is measured,and numerical fitting proves that the spectrum has a good Gaussian distribution with a minimum divergence angle of 0.30 mrad.The results combining these two aspects verify that the optimal phase-matching conditions under the current laser parameters are achieved.Conclusions Extreme ultraviolet pulses with low divergence angle and high conversion efficiency are obtained by loosely focused beams,with a total energy of 78.7 nJ in the spectral wavelength range of 11.6 nm to 19.5 nm.We employ a 200 TW laser system homologous to free-electron lasing(FEL)and optimize the HHG extreme ultraviolet light source under this system platform to facilitate synchronous injection of FEL seed laser.In the future,wavefront correction technologies(such as deformable mirrors and wavefront sensors)will be adopted to further optimize beam quality,and higher repetition frequency lasers can be utilized to increase the average power of harmonics.This will have important application prospects in strong attosecond pulse generation,extreme ultraviolet pump-probe spectroscopy,and FEL seed source injection.

extreme ultraviolethigh-order harmonicphase matchingspatial distribution

高记星、娄智远、杨帆、杨晓骏、许毅、冷雨欣、郑颖辉、曾志男、李儒新

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中国科学院上海光学精密机械研究所强场激光物理国家重点实验室,上海 201800

中国科学院大学材料科学与光电工程中心,北京 100049

张江实验室,上海 201210

极紫外 高次谐波 相位匹配 空间分布

国家自然科学基金国家自然科学基金国家自然科学基金中国科学院战略性先导科技专项

111279019195020311874374XDB16

2024

光学学报
中国光学学会 中国科学院上海光学精密机械研究所

光学学报

CSTPCD北大核心
影响因子:1.931
ISSN:0253-2239
年,卷(期):2024.44(2)
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