Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-26T22:07:54.690Z Has data issue: false hasContentIssue false

Extremely powerful and frequency-tunable terahertz pulses from a table-top laser–plasma wiggler

Published online by Cambridge University Press:  26 September 2023

Jie Cai
Affiliation:
State Key Laboratory of Nuclear Physics and Technology, and Key Laboratory of HEDP of the Ministry of Education, CAPT, Peking University, Beijing, China
Yinren Shou
Affiliation:
Center for Relativistic Laser Science, Institute for Basic Science, Gwangju, Republic of Korea
Yixing Geng
Affiliation:
State Key Laboratory of Nuclear Physics and Technology, and Key Laboratory of HEDP of the Ministry of Education, CAPT, Peking University, Beijing, China
Liqi Han
Affiliation:
Hunan Provincial Key Laboratory of High-Energy Scale Physics and Applications, School of Physics and Electronics, Hunan University, Changsha, China
Xinlu Xu
Affiliation:
State Key Laboratory of Nuclear Physics and Technology, and Key Laboratory of HEDP of the Ministry of Education, CAPT, Peking University, Beijing, China
Shuangchun Wen
Affiliation:
Hunan Provincial Key Laboratory of High-Energy Scale Physics and Applications, School of Physics and Electronics, Hunan University, Changsha, China
Baifei Shen
Affiliation:
Shanghai Normal University, Shanghai, China
Jinqing Yu*
Affiliation:
Hunan Provincial Key Laboratory of High-Energy Scale Physics and Applications, School of Physics and Electronics, Hunan University, Changsha, China
Xueqing Yan*
Affiliation:
State Key Laboratory of Nuclear Physics and Technology, and Key Laboratory of HEDP of the Ministry of Education, CAPT, Peking University, Beijing, China Collaborative Innovation Center of Extreme Optics, Shanxi University, Taiyuan, China Guangdong Laser Plasma Institute, Guangzhou, China
*
Correspondence to: Jinqing Yu, Hunan Provincial Key Laboratory of High-Energy Scale Physics and Applications, School of Physics and Electronics, Hunan University, Changsha 410082, China. Email: jinqing.yu@hnu.edu.cn; Xueqing Yan, State Key Laboratory of Nuclear Physics and Technology, and Key Laboratory of HEDP of the Ministry of Education, CAPT, Peking University, Beijing 100871, China. Email: x.yan@pku.edu.cn
Correspondence to: Jinqing Yu, Hunan Provincial Key Laboratory of High-Energy Scale Physics and Applications, School of Physics and Electronics, Hunan University, Changsha 410082, China. Email: jinqing.yu@hnu.edu.cn; Xueqing Yan, State Key Laboratory of Nuclear Physics and Technology, and Key Laboratory of HEDP of the Ministry of Education, CAPT, Peking University, Beijing 100871, China. Email: x.yan@pku.edu.cn

Abstract

The production of broadband, terawatt terahertz (THz) pulses has been demonstrated by irradiating relativistic lasers on solid targets. However, the generation of extremely powerful, narrow-band and frequency-tunable THz pulses remains a challenge. Here, we present a novel approach for such THz pulses, in which a plasma wiggler is elaborated by a table-top laser and a near-critical density plasma. In such a wiggler, the laser-accelerated electrons emit THz radiations with a period closely related to the plasma thickness. The theoretical model and numerical simulations predict that a THz pulse with a laser–THz energy conversion of over 2.0%, an ultra-strong field exceeding 80 GV/m, a divergence angle of approximately 20° and a center frequency tunable from 4.4 to 1.5 THz can be generated from a laser of 430 mJ. Furthermore, we demonstrate that this method can work across a wide range of laser and plasma parameters, offering potential for future applications with extremely powerful THz pulses.

Type
Research Article
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2023. Published by Cambridge University Press in association with Chinese Laser Press

1 Introduction

Terahertz (THz) waves[ Reference Siegel 1 ], which are significantly less developed and utilized than microwaves and light waves, used to be regarded as the ‘THz gap’[ Reference Sirtori 2 ] in the electromagnetic spectrum due to the limitations of traditional electronic or optical methods in producing terahertz radiation during the early years. Such THz pulses have attracted significant interest for their potential applications in fields such as biology, medicine, material science, optical communication and the military[ Reference Ulbricht, Hendry, Shan, Heinz and Bonn 3 Reference Zhang, Shkurinov and Zhang 8 ]. To generate THz waves, several routine methods, such as cascade quantum laser[ Reference Kazarinov and Suris 9 , Reference Faist, Capasso, Sivco, Sirtori, Hutchinson and Cho 10 ], optical rectification[ Reference Yang, Richards and Shen 11 , Reference Auston, Cheung, Valdmanis and Kleinman 12 ], photoconductive[ Reference Auston, Cheung and Smith 13 ] and vacuum electronic[ Reference Maestrini, Ward, Gill, Javadi, Schlecht, Tripon-Canseliet, Chattopadhyay and Mehdi 14 , Reference Crowe, Mattauch, Roser, Bishop, Peatman and Liu 15 ] methods, have been widely demonstrated. Due to the material damage threshold, these methods are incapable of generating extremely powerful THz pulses. Such pulses can be used as a powerfully driven pulse for probing and controlling material properties[ Reference Kampfrath, Tanaka and Nelson 16 , Reference LaRue, Katayama, Lindenberg, Fisher, Öström, Nilsson and Ogasawara 17 ], biological macromolecules[ Reference Choi, Cheng, Huang, Zhang, Norris and Kotov 4 ], electron beam detection[ Reference Zhao, Wang, Tang, Wang, Cheng, Lu, Jiang, Zhu, Hu, Song, Wang, Qiu, Kostin, Jing, Antipov, Wang, Qi, Cheng, Xiang and Zhang 18 ] and charged particle acceleration[ Reference Hibberd, Healy, Lake, Georgiadis, Smith, Finlay, Pacey, Jones, Saveliev, Walsh, Snedden, Appleby, Burt, Graham and Jamison 19 , Reference Zhang, Fallahi, Hemmer, Wu, Fakhari, Hua, Cankaya, Calendron, Zapata, Matlis and Kärtner 20 ]. For instance, the mechanisms of four-wave mixing and photoionization become saturated in under-dense plasma just around the power of ${10}^{15}\;\mathrm{W}/{\mathrm{cm}}^2$ [ Reference Lu, He, Zhang, Zhang, Yao, Li and Zhang 21 Reference Bergé, Kaltenecker, Engelbrecht, Nguyen, Skupin, Merlat, Fischer, Zhou, Thiele and Jepsen 23 ]. As laser intensity continues to improve and nanotechnology develops, terahertz sources based on ultra-intense laser irradiation of dense plasma have started to emerge[ Reference Hamster, Sullivan, Gordon, White and Falcone 24 , Reference Gopal, Herzer, Schmidt, Singh, Reinhard, Ziegler, Brömmel, Karmakar, Gibbon, Dillner, May, Meyer and Paulus 25 ].

During the past two decades, the quick development of relativistic laser systems, whose peak intensity exceeds ${10}^{18}\;\mathrm{W}/{\mathrm{cm}}^2$ , has opened a new door to obtain extremely powerful THz pulses[ Reference Yi and Fülöp 26 ]. However, the existing terahertz sources based on relativistic lasers lack the ability to tune their spectra, which limits their versatility in applications[ Reference Zhang, Fallahi, Hemmer, Wu, Fakhari, Hua, Cankaya, Calendron, Zapata, Matlis and Kärtner 20 , Reference Vicario, Ruchert, Ardana-Lamas, Derlet, Tudu, Luning and Hauri 27 Reference Yuan and Bandrauk 30 ]. For example, two-color laser filaments can produce THz pulses with field amplitudes above 10 GV/m and a conversion efficiency of 2.36%[ Reference Koulouklidis, Gollner, Shumakova, Fedorov, Pugžlys, Baltuška and Tzortzakis 31 ], but such pulses have a non-tunable center frequency and a large bandwidth around hundreds of GHz. Another novel method, coherent transition radiation (CTR), occurs when an over-dense electron bunch, produced by irradiating a relativistic laser on a solid target, passes through the vacuum–plasma interface and can emit THz pulses with an energy of 55 mJ and a peak electron field at 4 GV/m[ Reference Liao, Li, Liu, Scott, Neely, Zhang, Zhu, Zhang, Armstrong, Zemaityte, Bradford, Huggard, Rusby, McKenna, Brenner, Woolsey, Wang, Sheng and Zhang 32 ]. Numerous efforts have been dedicated to achieving tunable strong-field terahertz radiation using various approaches, such as plasma oscillation[ Reference Pearson, Palastro and Antonsen 33 Reference Kwon, Kang, Song, Kim, Ersfeld, Jaroszynski and Hur 35 ] and plasma slab methods[ Reference Gupta, Jain, Kulagin, Hur and Suk 36 ]. However, most of these solutions have not been able to reach high field strengths. Miao et al.[ Reference Miao, Palastro and Antonsen 34 ] demonstrated frequency-tunable terahertz radiation with weak field strength by manipulating the frequency of plasma waves. Kwon et al.[ Reference Kwon, Kang, Song, Kim, Ersfeld, Jaroszynski and Hur 35 ] developed a terahertz source based on plasma dipole oscillation formed by two laser pulses. One of the challenges lies in accessing terahertz frequencies through radiation from plasma waves, as it requires extremely low densities, making it difficult to obtain strong-field terahertz radiation simultaneously. In a significant breakthrough, Liao et al.[ Reference Liao, Liu, Scott, Zhang, Zhu, Zhang, Li, Armstrong, Zemaityte, Bradford, Rusby, Neely, Huggard, McKenna, Brenner, Woolsey, Wang, Sheng and Zhang 37 ] achieved 0.1–1 THz tunable radiation by transforming the terahertz generation mechanism in laser-irradiated solid targets. However, it should be noted that the radiation derived from different mechanisms exhibits distinct characteristics. The center frequency of strong-field terahertz radiations above 1 THz from CTR is also non-adjustable[ Reference Liao and Li 38 ].

Here, we propose a novel plasma wiggler that uses a femtosecond (fs) laser pulse to produce frequency-tunable and extremely powerful terahertz radiations, improving the flexibility and accuracy of terahertz applications. Figure 1(a) draws the concept of the plasma wiggler. A laser pulse is used to irradiate a block-shaped near-critical density plasma, producing hot electrons[ Reference Wilks, Kruer, Tabak and Langdon 39 ]. The accelerated electrons move in two different trajectories. One kind of high-energy electrons gets rid of the potential barrier of the surface electric field and goes away from the plasma surface. The other group of electrons is trapped by the barrier acting as a wiggler. Figure 1(b) illustrates the laser–plasma interaction snapshot at around 273 fs. When this electron beam passes through the transverse interfaces of the plasma, THz radiation[ Reference Liao and Li 38 ] and sheath fields ${E}_{\mathrm{s}}$ [ Reference Daido, Nishiuchi and Pirozhkov 40 ] can be induced near the interfaces. Under the influence of ${E}_{\mathrm{s}}$ , the electrons are pulled back into the plasma and cross the transverse interface on the other side, exhibiting reciprocating motion along the plasma. The period of this motion is closely related to the plasma thickness and the size of ${E}_{\mathrm{s}}$ . As a result, the plasma with transverse sheath fields ${E}_{\mathrm{s}}$ can be used as a wiggler to manipulate the reciprocating motion of the electrons and regulate THz radiations. A theoretical model, which is verified by particle-in-cell (PIC) simulations, has been developed to describe the physical principles of the tunable THz pulse generation.

Figure 1 (a) Schematic for the generation of a high-power, collimated, narrow-band and center-frequency-tunable THz pulse. An intense femtosecond laser pulse irradiates on the left-hand side of a block-shaped near-critical density plasma. Hot electrons generated by laser ponderomotive force can be separated into two groups: the electrons in group A moving forward leaving the plasma and the electrons in group B reciprocating under the sheath fields ${E}_{\mathrm{s}}$ ; here the transverse sheath fields ${E}_{\mathrm{s}}$ are induced when electrons pass through the plasma transverse interfaces. Under the action of ${E}_{\mathrm{s}}$ , electrons in group B could be pulled back into the plasma and pass through the transverse interface on the other side. Such wiggler-like motions of these electrons can emit the desired THz pulse. (b) The electron accelerating in the plasma. (c) The trajectories of the two groups of electrons (blue and red) in the surface charge separation field.

Based on the theoretical model and PIC simulations, we find that the center frequency of the THz pulse can be regulated by changing the thickness of the plasma. In simulations using a laser pulse with energy of approximately 430 mJ, the generated THz pulse has a divergence angle of approximately 20°, an ultra-strong-field strength of over 80 GV/m, a laser–THz conversion efficiency of over 2.0% and a center frequency tunable from 4.4 to 1.5 THz by varying the plasma thickness from 20 to $80\;\mu \mathrm{m}$ . We also demonstrate that this plasma wiggler can work effectively over a wide range of plasma length, thickness, density and laser intensity. Therefore, this method could overcome significant scientific obstacles in the generation of high-quality THz sources and open up brand-new applications[ Reference Vicario, Ruchert, Ardana-Lamas, Derlet, Tudu, Luning and Hauri 27 Reference Koulouklidis, Gollner, Shumakova, Fedorov, Pugžlys, Baltuška and Tzortzakis 31 ].

2 Results

2.1 Theoretical model and simulation setup

When an intense laser pulse irradiates on a plasma, as shown in Figure 1(b), hot electrons whose beam length is close to the laser duration can be generated by laser ponderomotive force[ Reference Wilks, Kruer, Tabak and Langdon 39 ]. The electron beam transports in the plasma and passes through its transverse interfaces. As a result, transverse sheath fields ${E}_{\mathrm{s}}$ (more details in the Supplementary Material) can be generated and the maximum strength[ Reference Daido, Nishiuchi and Pirozhkov 40 ] on the plasma surfaces can be expressed as follows:

(1) $$\begin{align}{E}_{\mathrm{s}}=\sqrt{\frac{8\pi {n}_{\mathrm{e}}{T}_{\mathrm{e}}}{e}},\end{align}$$

where $e$ is the Euler’s number and ${n}_{\mathrm{e}}$ and ${T}_{\mathrm{e}}$ are the density and temperature of the hot electrons, respectively. Here, transverse sheath fields ${E}_{\mathrm{s}}$ higher than ${10}^{12}$ V/m can be induced near the plasma transverse interfaces[ Reference Tarkeshian, Vay, Lehe, Schroeder, Esarey, Feurer and Leemans 41 ], as shown in Figure 1(c). Under the action of ${E}_{\mathrm{s}}$ , electrons whose kinetic energy is less than ${\varepsilon}_{\mathrm{e}}$ could be pulled back into the plasma and pass through the transverse interface on the other side[ Reference Sentoku, Cowan, Kemp and Ruhl 42 ], where ${\varepsilon}_{\mathrm{e}}$ could be calculated by the following:

(2) $$\begin{align}{\varepsilon}_{\mathrm{e}}={\int}_0^{l_{\mathrm{e}}}\frac{E_{\mathrm{s}}}{\sin \phi } \mathrm{d}l.\end{align}$$

Here, $l$ is the transverse size of ${E}_{\mathrm{s}}$ , $\phi$ is the angle at which the electron enters the transverse sheath fields ${E}_{\mathrm{s}}$ and ${l}_{\mathrm{e}}$ is the transverse location where the electron could be pulled back into the plasma. An electron field derived from the simulation was used (more details in the Supplementary Material) for calculation, and then the relation between ${\varepsilon}_{\mathrm{e}}$ and ${l}_{\mathrm{e}}$ could be plotted in Figure 2 by employing ${E}_{\mathrm{s}}$ as shown in Figure 1(c). In the case that the electron perpendicularly penetrates ${E}_{\mathrm{s}}$ ( $\phi ={90}^{\circ }$ ), the threshold kinetic energy is about 6 MeV. Most of the electrons penetrate the transverse sheath fields with a much smaller $\phi$ , and the threshold kinetic energy could be much higher than 6 MeV. Some electrons, which are located in the forefront of the electron beam and experienced much weaker ${E}_{\mathrm{s}}$ , could not be pulled back to the plasma even with a much smaller kinetic energy[ Reference Mora 43 ]. According to the large difference in the dynamical behavior of the hot electrons, as shown in Figure 1(c) with red and blue colors, we could separate the hot electrons into two groups: the electrons in group A located in the front of the electron beam are marked with a red color and the electrons in group B located in the beam rear express are marked with a blue color.

Figure 2 In the case of the electron penetrating ${E}_{\mathrm{s}}$ with different $\phi$ (the angle at which the electron enters ${E}_{\mathrm{s}}$ ), the relation between the electron threshold kinetic energy ${\varepsilon}_{\mathrm{e}}$ and the transverse location ${l}_{\mathrm{e}}$ where the electron could be pulled back into the plasma.

Here, ${E}_{\mathrm{s}}$ , which propagates along the plasma surface[ Reference Li, Yuan, Xu, Zheng, Sheng, Chen, Ma, Liang, Yu, Zhang, Liu, Wang, Wei, Zhao, Jin and Zhang 44 ] at a velocity close to light speed, can guide the hot electrons in group B to oscillate transversely and propagate longitudinally, as shown in Figure 1(c). Every time the electron passes through the transverse interfaces of the plasma, THz radiation can be emitted. This behaves like a wiggler in traditional light sources[ Reference Bilderback, Elleaume and Weckert 45 ]. Therefore, the plasma with transverse sheath fields ${E}_{\mathrm{s}}$ can be considered as a wiggler for the electrons in group B. The reciprocating (wiggler) period of the electron can be expressed as follows:

(3) $$\begin{align}{\tau}_{\mathrm{r}}=\frac{4{l}_{\mathrm{s}}+2{l}_{\mathrm{t}}}{v_{\mathrm{t}}}.\end{align}$$

Here, ${l}_{\mathrm{s}}$ is the transverse distance between the plasma interface and the point where the electron turns around, ${l}_{\mathrm{t}}$ is the thickness of the plasma and ${v}_{\mathrm{t}}$ is the median transverse velocity of the electrons; ${l}_{\mathrm{s}}$ is determined by the transverse momentum of electrons and the strength of ${E}_{\mathrm{s}}$ . The radiation frequency $f$ is closely related to the wiggler frequency ${f}_{\mathrm{w}}=1/{\tau}_{\mathrm{r}}$ , and then we have the following:

(4) $$\begin{align}f=\frac{f_{\mathrm{w}}\left(2{\gamma}^2\right)}{1+{K}^2/2}=\frac{v_{\mathrm{t}}\left(2{\gamma}^2\right)}{\left(4{l}_{\mathrm{s}}+2{l}_{\mathrm{t}}\right)\left(1+{K}^2/2\right)},\end{align}$$

where $\gamma$ is the electron Lorentz factor and $K$ is the wiggle (undulator) parameter[ Reference Jackson 46 ]. Normally, ${l}_{\mathrm{s}}$ is several micro-meters[ Reference Mora 43 ]; while the changes in $\gamma$ , $K$ and ${v}_{\mathrm{t}}$ can be ignored for the same laser intensity and plasma density, then ${l}_{\mathrm{t}}$ is the only parameter that could be varied. Hence, one can regulate the frequency of the THz radiation by changing the plasma thickness ${l}_{\mathrm{t}}$ according to Equation (4). Since the length of the electron beam is close to the laser pulse duration, which is only 32 fs here, the radiation satisfies the time coherence condition at the THz frequencies[ Reference Liao, Li, Liu, Scott, Neely, Zhang, Zhu, Zhang, Armstrong, Zemaityte, Bradford, Huggard, Rusby, McKenna, Brenner, Woolsey, Wang, Sheng and Zhang 32 ].

2.2 Electron kinetics

To generate electrons in group B, one should use a plasma with limited transverse size to ensure the occurrence of reciprocating motion. Simulations, with plasma of different lengths ${l}_{\mathrm{p}}$ (fixing the plasma thickness ${l}_{\mathrm{t}}$ to $30\;\mu \mathrm{m}$ ), were performed to see the effect of plasma length on the electron dynamics. From the simulations with ${l}_{\mathrm{p}}\ge 50\;\mu \mathrm{m}$ , it was found that more than $75\%$ of the laser energy was converted to hot electrons (electron kinetic energy ${e}_{\mathrm{k}}\ge 0.5$ MeV). Meanwhile, in the case of ${l}_{\mathrm{p}}=10\;\mu \mathrm{m}$ , there were few electrons participating in reciprocating motion and most of the electrons could be classified into group A.

When ${l}_{\mathrm{p}}$ was increased to $50\;\mu \mathrm{m}$ , one could easily distinguish the electrons in group B from those in group A, as plotted in Figures 3(a) and 3(b). Figure 3(a) shows a typical angular-spectra distribution of the electrons, with a large divergence angle, accelerated by the laser ponderomotive force[ Reference Wilks, Kruer, Tabak and Langdon 39 ]. This figure is very similar to the result of ${{l}_{\mathrm{p}}=10\;\mu \mathrm{m}}$ . Under the action of ${E}_{\mathrm{s}}$ , the reciprocating motion of the electrons is facilitated and obvious changes in the angular-spectra distribution can be seen in Figure 3(b). In this case, the electron beam had a divergence angle of approximately ${60}^{\circ }$ , which indicates that most of the electrons penetrate the transverse sheath fields with an angle of ${\phi \approx {60}^{\circ }}$ . Hence, the threshold kinetic energy of the electron ${\varepsilon}_{\mathrm{e}}$ is about 8 MeV, which is consistent with the theoretical value predicted by Equation (2), as shown in Figure 2. If ${l}_{\mathrm{p}}$ is further increased, such as ${l}_{\mathrm{p}}=200\;\mu \mathrm{m}$ , more electrons of relatively low energy in group A come into group B, as shown in Figure 3(c), and the number of electrons in group B increases with ${l}_{\mathrm{p}}$ . As a result, the electron number shown in Figure 3(d) is larger than that in Figure 3(b). It is noted that the electrons in group B were manipulated and collimated into a smaller divergence angle by ${E}_{\mathrm{s}}$ , and the electron threshold kinetic energy ${\varepsilon}_{\mathrm{e}}$ could be much higher, as predicted by Equation (2).

Figure 3 The angular-spectra distribution of the hot electrons. The electrons from a plasma length of ${l}_{\mathrm{p}}=50\;\mu \mathrm{m}$ (a) collected by a screen with a radius of $55\;\mu \mathrm{m}$ in the first 270 fs of the simulation could be classified to group A, and (b) the electrons behind group A can be assigned to group B. The electrons from a plasma length of ${l}_{\mathrm{p}}=200\;\mu \mathrm{m}$ (c) in group A collected by a screen whose radius is $205\;\mu \mathrm{m}$ in the first 770 fs and (d) the electrons in group B.

We used a semicircular receiving screen, whose radius was 250 μm with the center locating at the midpoint of the plasma right-hand interface, to collect the radiation field. Then, the angular-spectra distribution of the THz source could be obtained from the radiation field through Fourier transform[ Reference Cai, Shou, Han, Huang, Wang, Song, Geng, Yu and Yan 47 ]. In this work, the angular spectrum method[ Reference Cai, Shou, Han, Huang, Wang, Song, Geng, Yu and Yan 47 Reference Ritter 49 ] was employed to remove the near-field radiation, and then all the results of the THz source could be recognized as far-field radiation.

In the simulation with ${l}_{\mathrm{p}}=150\;\mu \mathrm{m}$ , the median longitudinal (transverse) velocity ${v}_{\mathrm{l}}$ ( ${v}_{\mathrm{t}}$ ) of the electrons in group B was 0.94c (0.85c). The transverse size of ${E}_{\mathrm{s}}$ was about $2\;\mu \mathrm{m}$ (at full width at half maximum (FWHM)), and therefore we could assume ${l}_{\mathrm{s}}\approx 2\;\mu \mathrm{m}$ . According to Equation (3), one can get ${\tau}_{\mathrm{r}}=270$ fs and ${\lambda}_{\mathrm{w}}\approx {\tau}_{\mathrm{r}}\times {v}_{\mathrm{l}}=79.4\;\mu \mathrm{m}$ . The wiggler period ${\tau}_{\mathrm{w}}={\tau}_{\mathrm{r}}$ corresponds to a wiggle frequency ${f}_{\mathrm{w}}=3.7$ THz, and the Lorentz factor $\gamma$ for the longitudinal velocity ${v}_{\mathrm{l}}$ was 2.93. By tracking the electromagnetic fields exerting on the electrons in group B, we got an average value of $K\approx 6.0$ , which decreased to 5.5 when ${l}_{\mathrm{s}}$ increased to $80\;\mu \mathrm{m}$ . According to Equation (4), the radiation frequency was ${f=3.34}$  THz, which is also the same as the center frequency of 3.35 THz from the simulation. Hence, the theoretical model can accurately predict the terahertz frequency obtained from the simulations.

2.3 Spectrum of terahertz pulses

Figures 4(a)(c) show the angular-spectra distribution of the THz pulses from the plasma lengths ${l}_{\mathrm{p}}=50$ , 150 and $300\;\mu \mathrm{m}$ . In the condition of ${l}_{\mathrm{p}}$ being shorter than ${\lambda}_{\mathrm{w}}$ , the role of the electrons in group B could be ignored and the generation of the THz source is dominated by target rear CTR[ Reference Liao, Li, Liu, Scott, Neely, Zhang, Zhu, Zhang, Armstrong, Zemaityte, Bradford, Huggard, Rusby, McKenna, Brenner, Woolsey, Wang, Sheng and Zhang 32 , Reference Liao, Liu, Scott, Zhang, Zhu, Zhang, Li, Armstrong, Zemaityte, Bradford, Rusby, Neely, Huggard, McKenna, Brenner, Woolsey, Wang, Sheng and Zhang 37 , Reference Liao, Li, Li, Su, Zheng, Liu, Wang, Hu, Yan, Dunn, Nilsen, Hunter, Liu, Wang, Chen, Ma, Lu, Jin, Kodama, Sheng and Zhang 50 ] from the electrons in group A. Hence, the THz source had a large divergence angle (pointed at 88°) and a small energy conversion efficiency of 0.45%, as shown in Figure 4(a).

Figure 4 Simulation results from the plasma of different lengths ${l}_{\mathrm{p}}$ , while the thickness ${l}_{\mathrm{t}}$ was fixed to $30\;\mu \mathrm{m}$ . The angular-spectra distribution of the THz pulses from (a) ${l}_{\mathrm{p}}=50\;\mu \mathrm{m}$ , (b) ${l}_{\mathrm{p}}=150\;\mu \mathrm{m}$ and (c) ${l}_{\mathrm{p}}=300\;\mu \mathrm{m}$ . (d) The radiation field before filtering (blue line) and the field of the THz pulse (red line) collected at ${37}^{\circ }$ from the simulation of ${l}_{\mathrm{p}}=300\;\mu \mathrm{m}$ .

Every time the electron passes through the transverse interfaces of the plasma, THz radiation can be emitted and becomes stronger in the case of the electrons in group B oscillating for several periods. When ${l}_{\mathrm{p}}$ was enlarged to $150\;\mu \mathrm{m}$ , more than $1.3\%$ of the laser energy was converted to THz radiation and the characteristics of the narrow spectrum became obvious, as shown in Figure 4(b). The simulation results indicated that ${l}_{\mathrm{p}}\ge 150\;\mu \mathrm{m}$ was more conducive to obtain THz pulses of a narrow spectrum, as shown in Figures 4(b) and 4(c). As the electrons in group B are guided to oscillate along the plasma by ${E}_{\mathrm{s}}$ , the resulting THz pulse could be better collimated than the other intense laser–plasma-based THz sources[ Reference Yi and Fülöp 26 , Reference Liao, Liu, Scott, Zhang, Zhu, Zhang, Li, Armstrong, Zemaityte, Bradford, Rusby, Neely, Huggard, McKenna, Brenner, Woolsey, Wang, Sheng and Zhang 37 , Reference Liao, Li, Li, Su, Zheng, Liu, Wang, Hu, Yan, Dunn, Nilsen, Hunter, Liu, Wang, Chen, Ma, Lu, Jin, Kodama, Sheng and Zhang 50 ]. It was found that the THz pulse that pointed at $\theta ={37}^{\circ }$ could be collimated into a divergence angle of approximately ${20}^{\circ }$ , as shown in Figure 4(c). Since $\theta >1/\gamma$ , we call it a wiggler instead of an undulator. Then we collected the radiation field at ${37}^{\circ }$ from the simulation of ${l}_{\mathrm{p}}=300\;\mu \mathrm{m}$ , and filtered the THz signal (frequency range: 0.1–10 THz) from the radiation field, as shown in Figure 4(d). The THz field was higher than 80 GV/m, which was much greater than those from THz sources driven by similar laser parameters[ Reference Yi and Fülöp 26 , Reference Liao, Liu, Scott, Zhang, Zhu, Zhang, Li, Armstrong, Zemaityte, Bradford, Rusby, Neely, Huggard, McKenna, Brenner, Woolsey, Wang, Sheng and Zhang 37 ], after the THz pulse propagated $250\;\mu \mathrm{m}$ off the plasma. Because the THz radiation comes from the wiggler process, the THz electric field waveform of multi-cycles[ Reference Tian, Liu, Bai, Zhou, Sun, Liu, Zhao, Li and Xu 51 ] was completely different from the half-cycle THz sources driven by intense lasers and plasma[ Reference Yi and Fülöp 26 , Reference Liao, Liu, Scott, Zhang, Zhu, Zhang, Li, Armstrong, Zemaityte, Bradford, Rusby, Neely, Huggard, McKenna, Brenner, Woolsey, Wang, Sheng and Zhang 37 , Reference Liao, Li, Li, Su, Zheng, Liu, Wang, Hu, Yan, Dunn, Nilsen, Hunter, Liu, Wang, Chen, Ma, Lu, Jin, Kodama, Sheng and Zhang 50 ].

2.4 Tunable frequency

From Figures 3(a) and 3(c), one can see that the electrons in group A had a large divergence angle. The electron density ${n}_{\mathrm{e}}$ decreases with the increase of transmission distance, and ${E}_{\mathrm{s}}$ becomes weaker for the longer plasma according to Equation (1), in which case the electrons in group B are more difficult to pull back to the plasma. As a result of enhancing ${l}_{\mathrm{p}}$ , ${l}_{\mathrm{s}}$ becomes larger and more electrons no longer participate in the wiggler motion. Hence, the center frequency decreases and the growth of energy conversion efficiency gradually slows down with the enhancement of ${l}_{\mathrm{p}}$ . Simulations by varying ${l}_{\mathrm{p}}$ from 50 to $900\;\mu \mathrm{m}$ have demonstrated the effect on the center frequency, as shown in Figure 5(a). From the figure, one can see that the center frequency of the THz pulse was tunable from 3.5 to 2.6 THz by changing the plasma length ${l}_{\mathrm{p}}$ from 150 to $900\;\mu \mathrm{m}$ . On the other hand, the laser–THz energy conversion efficiency, which increased with ${l}_{\mathrm{p}}$ and became saturated after $600\;\mu \mathrm{m}$ , as shown in Figure 5(a), was 2.05%. The saturation length may be longer than $600\;\mu \mathrm{m}$ since a small portion of the THz source came out of the simulation window, in the case of longer ${l}_{\mathrm{p}}$ , due to the limitation of computational ability.

Figure 5 (a) The center frequency of the THz source and the laser–THz energy conversion efficiency from the simulations with plasmas of different lengths ${l}_{\mathrm{p}}$ from 50 to $900\;\mu \mathrm{m}$ , while ${l}_{\mathrm{t}}$ was fixed to $30\;\mu \mathrm{m}$ . (b) The center frequency of the THz source from the simulations (blue line) and the theoretical model of Equation (4) for the plasma thickness ${l}_{\mathrm{t}}$ changing from 20 to $80\;\mu \mathrm{m}$ (light black shadow).

Equation (4) indicates that we could regulate the center frequency of the THz pulse by changing the thickness of the plasma ${l}_{\mathrm{t}}$ . More simulations were performed by changing ${l}_{\mathrm{t}}$ from 20 to $80\;\mu \mathrm{m}$ (fixed ${l}_{\mathrm{p}}$ at $300\;\mu \mathrm{m}$ ). It was found that the laser–THz energy conversion efficiency was almost the same for different ${l}_{\mathrm{t}}$ , while the center frequency of the THz source decreased with the increase of ${l}_{\mathrm{t}}$ , as shown in Figure 5(b). For different ${l}_{\mathrm{t}}$ , ${v}_{\mathrm{t}}$ can be obtained from the corresponding simulations, and the simulation results also show ${l}_{\mathrm{s}}$ ranging from 0.5 to $5\;\mu \mathrm{m}$ . We assumed that $K$ decreased with the increase of ${l}_{\mathrm{s}}$ from 6.0 to 5.5 for the above cases, then we calculated the center frequencies of the THz pulse according to Equation (4) and plotted them in Figure 5(b). From the figure, one can see that the theoretical model developed here works very well in predicting the generation of center-frequency-tunable THz pulses with a laser-driven plasma wiggler.

3 Discussion

To validate the physical results, we conducted 3D PIC simulations using a box size of $1920\times 800\times 800$ and a resolution of $0.15\lambda \times 0.25\lambda \times 0.25\lambda$ (further details can be found in the Supplementary Material). The 3D simulation produced a spectrum in the cross-section that closely resembles that obtained from the 2D simulation. In addition, the spatial distribution exhibits a quasi-2D pattern, indicating similarities between the two simulations.

Parametric simulations were also carried out to see the effects of laser intensity, plasma density and density gradient at the boundary (more details in the Supplementary Material). It was found that the energy conversion efficiency was almost unchanged for the plasma of the same thickness under a relativistic intense laser ( ${a}_0\ge 1.0$ ), while the center frequency, which decreased from 3.35 to 1.7 THz, would further reduce under smaller ${a}_0$ due to the drop of electron ${v}_{\mathrm{t}}$ . Since a low-density plasma is more beneficial to improving the energy efficiency from the laser pulse to relativistic electrons, the laser–THz energy conversion efficiency was higher in the case of lower density plasma. However, the center frequency of the THz source was almost the same. In reality, the plasma has a density gradient at the boundaries. Simulations using a pre-expand plasma with a scale length varied from 0.1 to $1\;\mu \mathrm{m}$ showed that there were almost no changes in the THz angular-spectra distribution. The parametric scans demonstrated the validity of this novel laser-driven plasma wiggler for the generation of high-power and center-frequency-tunable THz pulses over a wide range of laser and plasma parameters. With this method, one could produce ultra-high-power THz pulses of approximately 200 mJ by using a laser pulse of approximately $10$  J. Such a state-of-the-art THz source would initiate future applications of high-power THz pulses based on a compact laser.

4 Conclusion

In summary, we propose a laser-driven plasma wiggler for efficiently generating a high-power, collimated, narrow-band and center-frequency-tunable THz pulse, by manipulating the electron reciprocating motion. A theoretical model is developed to describe the physical principle of realizing the center-frequency-tunable THz pulse. According to the model and PIC simulations, the center frequency of the THz pulse corresponds strictly to the reciprocating motion period of the electron beam. Simulations indicate that the center frequency of the THz pulses can be tuned from 4.4 to 1.5 THz as the plasma thickness changes from 20 to $80\;\mu \mathrm{m}$ . Meanwhile, the THz pulse is collimated into a divergence angle of approximately ${20}^{\circ }$ , enabling a laser–THz conversion efficiency of more than $2.0\%$ and an ultra-strong-field strength of over 80 GV/m, driven by a table-top laser of approximately $430$ mJ. This method could address a long-standing challenge in THz science and generate a state-of-the-art THz source over a wide range of laser and plasma parameters.

Appendix A. Particle-in-cell simulation setup

Numerical simulations were performed by using the 2D PIC codes EPOCH[ Reference Arber, Bennett, Brady, Lawrence-Douglas, Ramsay, Sircombe, Gillies, Evans, Schmitz, Bell and Ridgers 52 ] and SMILEI[ Reference Derouillat, Beck, Pérez, Vinci, Chiaramello, Grassi, Flé, Bouchard, Plotnikov, Aunai, Dargent, Riconda and Grech 53 ] to verify this scheme. The simulation window $X\times Y=600\;\mu \mathrm{m}\times 570\;\mu \mathrm{m}$ was divided into $12,500\times 7125$ cells. A laser pulse, with Gaussian spatial and ${\sin}^2$ temporal profiles, wavelength ${\lambda}_0=800$ nm, waist ${w}_0=7.2\;\mu \mathrm{m}$ , normalized intensity ${a}_0=3$ , polarized in the Y direction and with the duration of 32 fs at FWHM, was used as the driving source. Such a laser pulse can be produced by a compact laser[ Reference Danson, Haefner, Bromage, Butcher, Chanteloup, Chowdhury, Galvanauskas, Gizzi, Hein, Hillier, Hopps, Kato, Khazanov, Kodama, Korn, Li, Li, Limpert, Ma, Nam, Neely, Papadopoulos, Penman, Qian, Rocca, Shaykin, Siders, Spindloe, Szatmári, Trines, Zhu, Zhu and Zuegel 54 ]. We used a block-shaped near-critical density plasma (electron density ${n}_{\mathrm{e}}=0.2{n}_{\mathrm{c}}$ , where ${n}_{\mathrm{c}}$ is the critical density) whose length and thickness were adjustable. Such a plasma could be made of carbon nanotube foams[ Reference Ma, Song, Yang, Zhang, Zhao, Sun, Ren, Liu, Liu, Shen, Zhang, Xiang, Zhou and Xie 55 , Reference Shou, Wang, Lee, Rhee, Lee, Yoon, Sung, Lee, Pan, Kong, Mei, Liu, Xu, Deng, Zhou, Tajima, Choi, Yan, Nam and Ma 56 ]. Twenty-four (four) macro-electrons (C ${}^{6+}$ ) were initialized into each cell. The simulation time was varied with plasma length ${l}_{\mathrm{p}}$ to make sure that we had more than 1 picosecond to collect the THz signal, which should be enough to cover the whole interaction process for the generation of THz sources. Meanwhile, the zero padding method[ Reference Harris, Millman, Van Der Walt, Gommers, Virtanen, Cournapeau, Wieser, Taylor, Berg, Smith, Kern, Picus, Hoyer, van Kerkwijk, Brett, Haldane, del Río, Wiebe, Peterson, Gérard-Marchant, Sheppard, Reddy, Weckesser, Abbasi, Gohlke and Oliphant 57 ] was used to further improve the resolution of the THz signal.

Acknowledgements

This work was supported by the National Natural Science Foundation of China (Grant Nos. 11921006 and 12175058), Beijing Distinguished Young Scientist Program and National Grand Instrument Project (Grant No. SQ2019YFF01014400). The PIC code EPOCH was in part funded by UK EPSRC (Grant Nos. EP/G054950/1, EP/G056803/1, EP/G055165/1 and EP/M022463/1). We give thanks for the helpful discussions with Prof. Z. Najmudin from Imperial College London and Prof. Wenjun Ma from Peking University.

Supplementary Material

To view supplementary material for this article, please visit http://doi.org/10.1017/hpl.2023.78.

References

Siegel, P. H., IEEE Trans. Microwave Theory Techn. 50, 910 (2002).CrossRefGoogle Scholar
Sirtori, C., Nature 417, 132 (2002).CrossRefGoogle Scholar
Ulbricht, R., Hendry, E., Shan, J., Heinz, T. F, and Bonn, M., Rev. Mod. Phys. 83, 543 (2011).CrossRefGoogle Scholar
Choi, W. J., Cheng, G., Huang, Z., Zhang, S., Norris, T. B., and Kotov, N. A., Nat. Mater. 18, 820 (2019).CrossRefGoogle Scholar
Kleine-Ostmann, T. and Nagatsuma, T.. J. Infrared Millimeter Terahertz Waves 32, 143 (2011).CrossRefGoogle Scholar
Koenig, S., Lopez-Diaz, D., Antes, J., Boes, F., Henneberger, R., Leuther, A., Tessmann, A., Schmogrow, R., Hillerkuss, D., Palmer, R., Zwick, T., Koos, C., Freude, W., Ambacher, O., Leuthold, J., and Kallfass, I., Nat. Photonics 7, 977 (2013).CrossRefGoogle Scholar
Kalashnikov, D. A., Paterova, A. V., Kulik, S. P., and Krivitsky, L. A., Nat. Photonics 10, 98 (2016).CrossRefGoogle Scholar
Zhang, X. C., Shkurinov, A., and Zhang, Y., Nat. Photonics 11, 16 (2017).CrossRefGoogle Scholar
Kazarinov, R. F. and Suris, R. A., Fiz. Tekh. Poluprovodn. 5, 797 (1971).Google Scholar
Faist, J., Capasso, F., Sivco, D. L., Sirtori, C., Hutchinson, A. L., and Cho, A. Y., Science 264, 553 (1994).CrossRefGoogle Scholar
Yang, K. H., Richards, P. L., and Shen, Y. R., Appl. Phys. Lett. 19, 320 (1971).CrossRefGoogle Scholar
Auston, D. H., Cheung, K. P., Valdmanis, J. A., and Kleinman, D. A., Phys. Rev. Lett. 53, 1555 (1984).CrossRefGoogle Scholar
Auston, D. H., Cheung, K. P., and Smith, P. R., Appl. Phys. Lett. 45, 284 (1984).CrossRefGoogle Scholar
Maestrini, A., Ward, J. S., Gill, J. J., Javadi, H. S., Schlecht, E., Tripon-Canseliet, C., Chattopadhyay, G., and Mehdi, I., IEEE Trans. Microwave Theory Techn. 53, 2835 (2005).CrossRefGoogle Scholar
Crowe, T. W., Mattauch, R. J., Roser, H. P., Bishop, W. L., Peatman, W. C. B. and Liu, X., Proc. IEEE 80, 1827 (1992).CrossRefGoogle Scholar
Kampfrath, T., Tanaka, K., and Nelson, K. A., Nat. Photonics 7, 680 (2013).CrossRefGoogle Scholar
LaRue, J. L., Katayama, T., Lindenberg, A., Fisher, A. S., Öström, H., Nilsson, A., and Ogasawara, H., Phys. Rev. Lett. 115, 036103 (2015).CrossRefGoogle Scholar
Zhao, L., Wang, Z., Tang, H., Wang, R., Cheng, Y., Lu, C., Jiang, T., Zhu, P., Hu, L., Song, W., Wang, H., Qiu, J., Kostin, R., Jing, C., Antipov, S., Wang, P., Qi, J., Cheng, Y., Xiang, D., and Zhang, J., Phys. Rev. Lett. 122, 144801 (2019).CrossRefGoogle Scholar
Hibberd, M. T., Healy, A. L., Lake, D. S., Georgiadis, V., Smith, E. J. H., Finlay, O. J., Pacey, T. H., Jones, J. K., Saveliev, Y., Walsh, D. A., Snedden, E. W., Appleby, R. B., Burt, G., Graham, D. M., and Jamison, S. P., Nat. Photonics 14, 755 (2020).CrossRefGoogle Scholar
Zhang, D., Fallahi, A., Hemmer, M., Wu, X., Fakhari, M., Hua, Y., Cankaya, H., Calendron, A.-L., Zapata, L. E., Matlis, N. H., and Kärtner, F. X., Nat. Photonics 12, 336 (2018).CrossRefGoogle Scholar
Lu, C., He, T., Zhang, L., Zhang, H., Yao, Y., Li, S., and Zhang, S., Phys. Rev. A 92, 063850 (2015).CrossRefGoogle Scholar
Babushkin, I., Kuehn, W., Koehler, C., Skupin, S., Berge, L., Reimann, K., Woerner, M., Herrmann, J., and Elsaesser, T., Phys. Rev. Lett., 105, 053903 (2010).CrossRefGoogle Scholar
Bergé, L., Kaltenecker, K., Engelbrecht, S., Nguyen, A., Skupin, S., Merlat, L., Fischer, B., Zhou, B., Thiele, I., and Jepsen, P. U., Europhys. Lett. 126, 24001 (2019).CrossRefGoogle Scholar
Hamster, H., Sullivan, A., Gordon, S., White, W., and Falcone, R. W., Phys. Rev. Lett. 71, 2725 (1993).CrossRefGoogle Scholar
Gopal, A., Herzer, S., Schmidt, A., Singh, P., Reinhard, A., Ziegler, W., Brömmel, D., Karmakar, A., Gibbon, P., Dillner, U., May, T., Meyer, H.-G., and Paulus, G. G., Phys. Rev. Lett. 111, 074802 (2013).CrossRefGoogle Scholar
Yi, L. and Fülöp, T., Phys. Rev. Lett. 123, 094801 (2019).CrossRefGoogle Scholar
Vicario, C., Ruchert, C., Ardana-Lamas, F., Derlet, P. M., Tudu, B., Luning, J., and Hauri, C. P., Nat. Photonics 7, 720 (2013).CrossRefGoogle Scholar
Baierl, S., Hohenleutner, M., Kampfrath, T., Zvezdin, A. K., Kimel, A. V., Huber, R., and Mikhaylovskiy, R. V., Nat. Photonics 10, 715 (2016).CrossRefGoogle Scholar
Balogh, E., Kovacs, K., Dombi, P., Fulop, J. A., Farkas, G., Hebling, J., Tosa, V., and Varju, K., Phys. Rev. A 84, 023806 (2011).CrossRefGoogle Scholar
Yuan, K.-J. and Bandrauk, A. D., Phys. Rev. Lett. 110, 023003 (2013).CrossRefGoogle Scholar
Koulouklidis, A. D., Gollner, C., Shumakova, V., Fedorov, V. Y., Pugžlys, A., Baltuška, A., and Tzortzakis, S., Nat. Commun. 11, 292 (2020).CrossRefGoogle Scholar
Liao, G., Li, Y., Liu, H., Scott, G. G., Neely, D., Zhang, Y., Zhu, B., Zhang, Z., Armstrong, C., Zemaityte, E., Bradford, P., Huggard, P. G., Rusby, D. R., McKenna, P., Brenner, C. M., Woolsey, N. C., Wang, W., Sheng, Z., and Zhang, J., Proc. Natl. Acad. Sci. 116, 3994 (2019).CrossRefGoogle Scholar
Pearson, A. J., Palastro, J., and Antonsen, T. M., Phys. Rev. E 83, 056403 (2011).CrossRefGoogle Scholar
Miao, C., Palastro, J. P., and Antonsen, T. M., Phys. Plasmas 24, 043109 (2017).CrossRefGoogle Scholar
Kwon, K. B., Kang, T., Song, H. S., Kim, Y.-K., Ersfeld, B., Jaroszynski, D. A., and Hur, M. S., Sci. Rep. 8, 145 (2018).CrossRefGoogle Scholar
Gupta, D. N., Jain, A., Kulagin, V. V., Hur, M. S., and Suk, H., Appl. Phys. B 128, 50 (2022).CrossRefGoogle Scholar
Liao, G.-Q., Liu, H., Scott, G. G., Zhang, Y.-H., Zhu, B.-J., Zhang, Z., Li, Y.-T., Armstrong, C., Zemaityte, E., Bradford, P., Rusby, D. R., Neely, D., Huggard, P. G., McKenna, P., Brenner, C. M., Woolsey, N. C., Wang, W.-M., Sheng, Z.-M., and Zhang, J., Phys. Rev. X 10, 031062 (2020).Google Scholar
Liao, G.-Q. and Li, Y.-T., IEEE Trans. Plasma Sci. 47, 3002 (2019).CrossRefGoogle Scholar
Wilks, S. C., Kruer, W. L., Tabak, M., and Langdon, A. B., Phys. Rev. Lett. 69, 1383 (1992).CrossRefGoogle Scholar
Daido, H., Nishiuchi, M., and Pirozhkov, A. S., Rep. Progress Phys. 75, 056401 (2012).CrossRefGoogle Scholar
Tarkeshian, R., Vay, J. L., Lehe, R., Schroeder, C. B., Esarey, E. H., Feurer, T., and Leemans, W. P., Phys. Rev. X 8, 021039 (2018).Google Scholar
Sentoku, Y., Cowan, T. E., Kemp, A., and Ruhl, H., Phys. Plasmas 10, 2009 (2003).CrossRefGoogle Scholar
Mora, P., Phys. Rev. Lett. 90, 185002 (2003).CrossRefGoogle Scholar
Li, Y. T., Yuan, X. H., Xu, M. H., Zheng, Z. Y., Sheng, Z. M., Chen, M., Ma, Y. Y., Liang, W. X., Yu, Q. Z., Zhang, Y., Liu, F., Wang, Z. H., Wei, Z. Y., Zhao, W., Jin, Z., and Zhang, J., Phys. Rev. Lett. 96, 165003 (2006).CrossRefGoogle Scholar
Bilderback, D. H., Elleaume, P., and Weckert, E., J. Phys. B 38, S773 (2005).CrossRefGoogle Scholar
Jackson, J. D., Classical Electrodynamics (American Association of Physics Teachers, 1999).Google Scholar
Cai, J., Shou, Y. R., Han, L. Q., Huang, R. X., Wang, Y. X., Song, Z. H., Geng, Y. X., Yu, J. Q., and Yan, X. Q., Opt. Lett. 47, 1658 (2022).CrossRefGoogle Scholar
Lalor, É., J. Opt. Soc. Am. 58, 1235 (1968).CrossRefGoogle Scholar
Ritter, A., Opt. Express 22, 26265 (2014).CrossRefGoogle Scholar
Liao, G. Q., Li, Y. T., Li, C., Su, L. N., Zheng, Y., Liu, M., Wang, W. M., Hu, Z. D., Yan, W. C., Dunn, J., Nilsen, J., Hunter, J., Liu, Y., Wang, X., Chen, L. M., Ma, J. L., Lu, X., Jin, Z., Kodama, R., Sheng, Z. M., and Zhang, J., Phys. Rev. Lett. 114, 255001 (2015).CrossRefGoogle Scholar
Tian, Y., Liu, J., Bai, Y., Zhou, S., Sun, H., Liu, W., Zhao, J., Li, R., and Xu, Z., Nat. Photonics 11, 242 (2017).CrossRefGoogle Scholar
Arber, T. D., Bennett, K., Brady, C. S., Lawrence-Douglas, A., Ramsay, M. G., Sircombe, N. J., Gillies, P., Evans, R. G., Schmitz, H., Bell, A. R., and Ridgers, C. P., Plasma Phys. Controll. Fusion 57, 113001 (2015).CrossRefGoogle Scholar
Derouillat, J., Beck, A., Pérez, F., Vinci, T., Chiaramello, M., Grassi, A., Flé, M., Bouchard, G., Plotnikov, I., Aunai, N., Dargent, J., Riconda, C., and Grech, M., Comput. Phys. Commun. 222, 351 (2018).CrossRefGoogle Scholar
Danson, C. N., Haefner, C., Bromage, J., Butcher, T., Chanteloup, J.-C. F., Chowdhury, E. A., Galvanauskas, A., Gizzi, L. A., Hein, J., Hillier, D. I., Hopps, N. W., Kato, Y., Khazanov, E. A., Kodama, R., Korn, G., Li, R., Li, Y., Limpert, J., Ma, J., Nam, C. H., Neely, D., Papadopoulos, D., Penman, R. R., Qian, L., Rocca, J. J., Shaykin, A. A., Siders, C. W., Spindloe, C., Szatmári, S., Trines, R. M. G. M., Zhu, J., Zhu, P., and Zuegel, J. D., High Power Laser Sci. Eng. 7, e54 (2019).CrossRefGoogle Scholar
Ma, W., Song, L., Yang, R., Zhang, T., Zhao, Y., Sun, L., Ren, Y., Liu, D., Liu, L., Shen, J., Zhang, Z., Xiang, Y., Zhou, W., and Xie, S., Nano Lett. 7, 2307 (2007).CrossRefGoogle Scholar
Shou, Y., Wang, P., Lee, S. G., Rhee, Y. J., Lee, H. W., Yoon, J. W., Sung, J. H., Lee, S. K., Pan, Z., Kong, D., Mei, Z., Liu, J., Xu, S., Deng, Z., Zhou, W., Tajima, T., Choi, I. W., Yan, X., Nam, C. H., and Ma, W., Nat. Photonics 17, 137 (2023).CrossRefGoogle Scholar
Harris, C. R., Millman, K. J., Van Der Walt, S. J., Gommers, R., Virtanen, P., Cournapeau, D., Wieser, E., Taylor, J., Berg, S., Smith, N. J., Kern, R., Picus, M., Hoyer, S., van Kerkwijk, M. H., Brett, M., Haldane, A., del Río, J. F., Wiebe, M., Peterson, P., Gérard-Marchant, P., Sheppard, K., Reddy, T., Weckesser, W., Abbasi, H., Gohlke, C., and Oliphant, T. E., Nature 585, 357 (2020).CrossRefGoogle Scholar
Figure 0

Figure 1 (a) Schematic for the generation of a high-power, collimated, narrow-band and center-frequency-tunable THz pulse. An intense femtosecond laser pulse irradiates on the left-hand side of a block-shaped near-critical density plasma. Hot electrons generated by laser ponderomotive force can be separated into two groups: the electrons in group A moving forward leaving the plasma and the electrons in group B reciprocating under the sheath fields ${E}_{\mathrm{s}}$; here the transverse sheath fields ${E}_{\mathrm{s}}$ are induced when electrons pass through the plasma transverse interfaces. Under the action of ${E}_{\mathrm{s}}$, electrons in group B could be pulled back into the plasma and pass through the transverse interface on the other side. Such wiggler-like motions of these electrons can emit the desired THz pulse. (b) The electron accelerating in the plasma. (c) The trajectories of the two groups of electrons (blue and red) in the surface charge separation field.

Figure 1

Figure 2 In the case of the electron penetrating ${E}_{\mathrm{s}}$ with different $\phi$ (the angle at which the electron enters ${E}_{\mathrm{s}}$), the relation between the electron threshold kinetic energy ${\varepsilon}_{\mathrm{e}}$ and the transverse location ${l}_{\mathrm{e}}$ where the electron could be pulled back into the plasma.

Figure 2

Figure 3 The angular-spectra distribution of the hot electrons. The electrons from a plasma length of ${l}_{\mathrm{p}}=50\;\mu \mathrm{m}$ (a) collected by a screen with a radius of $55\;\mu \mathrm{m}$ in the first 270 fs of the simulation could be classified to group A, and (b) the electrons behind group A can be assigned to group B. The electrons from a plasma length of ${l}_{\mathrm{p}}=200\;\mu \mathrm{m}$ (c) in group A collected by a screen whose radius is $205\;\mu \mathrm{m}$ in the first 770 fs and (d) the electrons in group B.

Figure 3

Figure 4 Simulation results from the plasma of different lengths ${l}_{\mathrm{p}}$, while the thickness ${l}_{\mathrm{t}}$ was fixed to $30\;\mu \mathrm{m}$. The angular-spectra distribution of the THz pulses from (a) ${l}_{\mathrm{p}}=50\;\mu \mathrm{m}$, (b) ${l}_{\mathrm{p}}=150\;\mu \mathrm{m}$ and (c) ${l}_{\mathrm{p}}=300\;\mu \mathrm{m}$. (d) The radiation field before filtering (blue line) and the field of the THz pulse (red line) collected at ${37}^{\circ }$ from the simulation of ${l}_{\mathrm{p}}=300\;\mu \mathrm{m}$.

Figure 4

Figure 5 (a) The center frequency of the THz source and the laser–THz energy conversion efficiency from the simulations with plasmas of different lengths ${l}_{\mathrm{p}}$ from 50 to $900\;\mu \mathrm{m}$, while ${l}_{\mathrm{t}}$ was fixed to $30\;\mu \mathrm{m}$. (b) The center frequency of the THz source from the simulations (blue line) and the theoretical model of Equation (4) for the plasma thickness ${l}_{\mathrm{t}}$ changing from 20 to $80\;\mu \mathrm{m}$ (light black shadow).

Supplementary material: File

Cai et al. supplementary material
Download undefined(File)
File 607.9 KB