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Broadband laser driven near-forward scattering light of planar film target

Long Xin-Yu Xiong Jun An Hong-Hai Xie Zhi-Yong Wang Pei-Pei Fang Zhi-Heng Wang Wei Sun Jin-Ren Wang Chen

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Broadband laser driven near-forward scattering light of planar film target

Long Xin-Yu, Xiong Jun, An Hong-Hai, Xie Zhi-Yong, Wang Pei-Pei, Fang Zhi-Heng, Wang Wei, Sun Jin-Ren, Wang Chen
cstr: 32037.14.aps.73.20240823
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  • Laser-plasma instability (LPI) is one of the key problems in the ignition process of inertial confinement fusion (ICF), and has been extensively studied in theory, simulation, and experiment for many years. Broadband laser, due to its low temporal coherence, can reduce the effective electric field strength when interacting with plasma and disrupt the phase-matching conditions of LPI, thus an effective approach to solving LPI issues is considered. Current extensive simulation studies indicate that broadband laser can suppress the generation of phenomena such as stimulated Brillouin scattering (SBS), stimulated Raman scattering (SRS), and two-plasmon decay (TPD) to some extent. There are also a few backward scattering experimental studies, but more experimental researches, such as side-scattering, are still needed. Therefore, based on the broadband second harmonic laser facility “Kunwu”, the experiments are designed for studying the lateral scattering of critical density plasma driven by broadband laser and traditional narrowband laser, and the production of hot electrons as well in this work. The experimental results show that the side SBS spectra and side SRS spectra and portions at different angles excited by broadband lasers with a power density of 1×1015 W/cm2 are significantly different from those by narrowband lasers. Further analysis reveals that the overall portion of transverse hot electrons in broadband laser cases is higher than that in narrowband laser case. However, for broadband laser, the portion of SRS at small forward angle and backward angle are significantly lower than that for narrowband laser. Preliminary qualitative analysis suggests that SRS may not be the main mechanism for hot electron generation in this case, and that PDI might play a dominant role in generating hot electrons.
      Corresponding author: Sun Jin-Ren, sunjinren@263.net ; Wang Chen, wangch@mail.shcnc.ac.cn
    • Funds: Project supported by the National Natural Science Foundation of China (Grant Nos. 12074353, 12075227).
    [1]

    Lindl J D, Amendt P, Berger R L, Glendinning S G, Glenzer S H, Haan S W, Kauffman R L, Landen O L, Suter L J 2004 Phys. Plasmas 11 339Google Scholar

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    杨冬, 李志超, 李三伟, 郝亮, 李欣, 郭亮, 邹士阳, 蒋小华, 彭晓世, 徐涛, 理玉龙, 郑春阳, 蔡洪波, 刘占军, 郑坚, 龚韬, 王哲斌, 黎航, 况龙钰, 李琦, 王峰, 刘慎业, 杨家敏, 江少恩, 张保汉, 丁永坤 2018 中国科学: 物理学 力学 天文学 48 065203Google Scholar

    Yang D, Li Z C, Li S W, Hao L, Li X, Guo L, Zou S Y, Jiang X H, Peng X S, Xu T, Li Y L, Zheng C Y, Cai H B, Liu Z J, Zheng J, Long T, Wang Z B, Li H, Kuang L Y, Li Q, Wang F, Liu S Y, Yang J M, Jiang S E, Zhang B H, Ding Y K 2018 Sci. Sin-Phys. Mech. Astron. 48 065203Google Scholar

    [3]

    MacGowan B J, Afeyan B B, Back C A, Berger R L, Bonnaud G, Casanova M, Cohen B I, Desenne D E, DuBois D F, Dulieu A G, Estabrook K G, Fernandez J C, Glenzer S H, Hinkel D E, Kaiser T B, Kalantar D H, Kauffman R L, Kirkwood R K, Kruer W L, Langdon A B, Lasinski B F, Montgomery D S, Moody J D, Munro D H, Powers L V, Rose H A, Rousseaux C, Turner R E, Wilde B H, Wilks S C, Williams E A 1996 Phys. Plasmas 3 2029Google Scholar

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    Montgomery D S, Afeyan B B, Cobble J A, Fernandez J C, Wilke M D, Glenzer S H, Kirkwood R K, MacGowan B J, Moody J D, Lindman E L, Munro D H, Wilde B H, Rose H A, Dubois D F, Bezzerides B, Vu H X 1998 Phys. Plasmas 5 1973Google Scholar

    [5]

    Li C X, Dong L F, Feng J Y, Huang Y P, Sun H Y 2020 Rev. Sci Instrum. 91 026105Google Scholar

    [6]

    Niemann C, Berger R, Divol L, Kirkwood R, Moody J, Sorce C, Glenzer S 2011 J. Instrum. 6 P10008Google Scholar

    [7]

    Froula D, Divol L, London R, Berger R, Döppner T, Meezan N, Ross J, Suter L, Sorce C, Glenzer S 2009 Phys. Rev. Lett. 103 045006Google Scholar

    [8]

    Follett R K, Shaw J G, Myatt J F, Palastro J P, Short R W, Froula D H 2018 Phys. Rev. Lett. 120 135005Google Scholar

    [9]

    Bibeau C, Speck D R, Ehrlich R B, Laumann C W, Kyrazis D T, Henesian M A, Lawson J K, Perry M D, Wegner P J, Weiland T L 1992 Appl. Opt 31 5799Google Scholar

    [10]

    Dixit S N, Feit M D, Perry M D, Powell H T 1996 Opt. Lett 21 1715Google Scholar

    [11]

    Grun J, Emery M E, Manka C K, Lee T N, McLean E A, Mostovych A, Stamper J, Bodner S, Obenschain S P, Ripin B H 1987 Phys. Rev. Lett. 58 2672Google Scholar

    [12]

    Duluc M, Penninckx D, Loiseau P, Riazuelo G, Bourgeade A, Chatagnier A, D’Humières E 2019 Phys. Plasmas 26 42707Google Scholar

    [13]

    Albright B, Yin L, Afeyan B 2014 Phys. Rev. Lett. 113 045002Google Scholar

    [14]

    Feng Q S, Liu Z J, Cao L H, Xiao C Z, Hao L, Zheng C Y, Ning C, He X T 2020 Nucl. Fusion 60 066012Google Scholar

    [15]

    Zhong Z Q, Li B, Xiong H, Li J W, Qiu J, Hao L, Zhang B 2021 Opt. Express 29 1304Google Scholar

    [16]

    Follett R K, Shaw J G, Myatt J F, Dorrer C, Froula D H, Palastro J P 2019 Phys. Plasmas 26 062111Google Scholar

    [17]

    Thomson J J, Karush J I 1974 Phys. Fluids 17 1608Google Scholar

    [18]

    Gao Y Q, Cui Y, Ji L L, Rao D X, Zhao X H, Li F J, Liu D, Feng W, Xia L, Liu J N, Shi H T, Du P Y, Liu J, Li X L, Wang T, Zhang T X, Shan C, Hua Y L, Ma W X, Sun X, Chen X F, Huang X G, Zhu J A, Pei W B, Sui Z, Fu S Z 2020 Matter Radiat. Extrem. 5 065201Google Scholar

    [19]

    Lei A L, Kang N, Zhao Y, Liu H Y, An H H, Xiong J, Wang R R, Xie Z Y, Tu Y C, Xu G X, Zhou X C, Fang Z H, Wang W, Xia L, Feng W, Zhao X H, Ji L L, Cui Y, Zhou S L, Liu Z J, Zheng C Y, Wang L F, Gao Y Q, Huang X G, Fu S Z 2024 Phys. Rev. Lett. 132 035102Google Scholar

    [20]

    Wang P P, An H H, Fang Z H, Xiong J, Xie Z Y, Wang C, He Z Y, Jia G, Wang R R, Zheng S, Xia L, Feng W, Shi H T, Wang W, Sun J R, Gao Y Q, Fu S Z 2024 Matter Radiat. Extrem. 9 015602Google Scholar

    [21]

    Moody J, MacGowan B, Glenzer S, Kirkwood R, Kruer W, Montgomery D, Schmitt A, Williams E, Stone G 2000 Phys. Plasmas 7 2114Google Scholar

    [22]

    Yao C, Li J, Hao L, Yan R, Wang C, Lei A L, Ding Y K, Zheng J 2024 Nucl. Fusion 64 106013Google Scholar

  • 图 1  实验方案示意图

    Figure 1.  Sketch of the experimental setup.

    图 2  实验用靶示意图

    Figure 2.  Schematic diagram of the target.

    图 3  宽带激光与窄带激光驱动平面厚靶的25°近背向散射典型光谱

    Figure 3.  25° near back-scatter typical spectra driven by broadband laser and narrowband laser.

    图 4  宽带与窄带驱动平面厚靶的85°侧向散射典型光谱

    Figure 4.  85° side-scatter typical spectra driven by broadband laser and narrowband laser.

    图 5  宽带与窄带驱动平面厚靶的140°近前向散射典型光谱

    Figure 5.  140° near forward-scatter typical spectra driven by broadband laser and narrowband laser.

    图 6  不同角度的散射光能量份额 (a) SBS; (b) SRS

    Figure 6.  Energy information at different scattering measurement angles: (a) SBS; (b) SRS.

    图 7  不同角度的超热电子产生情况 (a)能谱图; (b) 份额图

    Figure 7.  Hot electrons at different scattering measurement angles: (a) Energy spectrum; (b) share chart.

  • [1]

    Lindl J D, Amendt P, Berger R L, Glendinning S G, Glenzer S H, Haan S W, Kauffman R L, Landen O L, Suter L J 2004 Phys. Plasmas 11 339Google Scholar

    [2]

    杨冬, 李志超, 李三伟, 郝亮, 李欣, 郭亮, 邹士阳, 蒋小华, 彭晓世, 徐涛, 理玉龙, 郑春阳, 蔡洪波, 刘占军, 郑坚, 龚韬, 王哲斌, 黎航, 况龙钰, 李琦, 王峰, 刘慎业, 杨家敏, 江少恩, 张保汉, 丁永坤 2018 中国科学: 物理学 力学 天文学 48 065203Google Scholar

    Yang D, Li Z C, Li S W, Hao L, Li X, Guo L, Zou S Y, Jiang X H, Peng X S, Xu T, Li Y L, Zheng C Y, Cai H B, Liu Z J, Zheng J, Long T, Wang Z B, Li H, Kuang L Y, Li Q, Wang F, Liu S Y, Yang J M, Jiang S E, Zhang B H, Ding Y K 2018 Sci. Sin-Phys. Mech. Astron. 48 065203Google Scholar

    [3]

    MacGowan B J, Afeyan B B, Back C A, Berger R L, Bonnaud G, Casanova M, Cohen B I, Desenne D E, DuBois D F, Dulieu A G, Estabrook K G, Fernandez J C, Glenzer S H, Hinkel D E, Kaiser T B, Kalantar D H, Kauffman R L, Kirkwood R K, Kruer W L, Langdon A B, Lasinski B F, Montgomery D S, Moody J D, Munro D H, Powers L V, Rose H A, Rousseaux C, Turner R E, Wilde B H, Wilks S C, Williams E A 1996 Phys. Plasmas 3 2029Google Scholar

    [4]

    Montgomery D S, Afeyan B B, Cobble J A, Fernandez J C, Wilke M D, Glenzer S H, Kirkwood R K, MacGowan B J, Moody J D, Lindman E L, Munro D H, Wilde B H, Rose H A, Dubois D F, Bezzerides B, Vu H X 1998 Phys. Plasmas 5 1973Google Scholar

    [5]

    Li C X, Dong L F, Feng J Y, Huang Y P, Sun H Y 2020 Rev. Sci Instrum. 91 026105Google Scholar

    [6]

    Niemann C, Berger R, Divol L, Kirkwood R, Moody J, Sorce C, Glenzer S 2011 J. Instrum. 6 P10008Google Scholar

    [7]

    Froula D, Divol L, London R, Berger R, Döppner T, Meezan N, Ross J, Suter L, Sorce C, Glenzer S 2009 Phys. Rev. Lett. 103 045006Google Scholar

    [8]

    Follett R K, Shaw J G, Myatt J F, Palastro J P, Short R W, Froula D H 2018 Phys. Rev. Lett. 120 135005Google Scholar

    [9]

    Bibeau C, Speck D R, Ehrlich R B, Laumann C W, Kyrazis D T, Henesian M A, Lawson J K, Perry M D, Wegner P J, Weiland T L 1992 Appl. Opt 31 5799Google Scholar

    [10]

    Dixit S N, Feit M D, Perry M D, Powell H T 1996 Opt. Lett 21 1715Google Scholar

    [11]

    Grun J, Emery M E, Manka C K, Lee T N, McLean E A, Mostovych A, Stamper J, Bodner S, Obenschain S P, Ripin B H 1987 Phys. Rev. Lett. 58 2672Google Scholar

    [12]

    Duluc M, Penninckx D, Loiseau P, Riazuelo G, Bourgeade A, Chatagnier A, D’Humières E 2019 Phys. Plasmas 26 42707Google Scholar

    [13]

    Albright B, Yin L, Afeyan B 2014 Phys. Rev. Lett. 113 045002Google Scholar

    [14]

    Feng Q S, Liu Z J, Cao L H, Xiao C Z, Hao L, Zheng C Y, Ning C, He X T 2020 Nucl. Fusion 60 066012Google Scholar

    [15]

    Zhong Z Q, Li B, Xiong H, Li J W, Qiu J, Hao L, Zhang B 2021 Opt. Express 29 1304Google Scholar

    [16]

    Follett R K, Shaw J G, Myatt J F, Dorrer C, Froula D H, Palastro J P 2019 Phys. Plasmas 26 062111Google Scholar

    [17]

    Thomson J J, Karush J I 1974 Phys. Fluids 17 1608Google Scholar

    [18]

    Gao Y Q, Cui Y, Ji L L, Rao D X, Zhao X H, Li F J, Liu D, Feng W, Xia L, Liu J N, Shi H T, Du P Y, Liu J, Li X L, Wang T, Zhang T X, Shan C, Hua Y L, Ma W X, Sun X, Chen X F, Huang X G, Zhu J A, Pei W B, Sui Z, Fu S Z 2020 Matter Radiat. Extrem. 5 065201Google Scholar

    [19]

    Lei A L, Kang N, Zhao Y, Liu H Y, An H H, Xiong J, Wang R R, Xie Z Y, Tu Y C, Xu G X, Zhou X C, Fang Z H, Wang W, Xia L, Feng W, Zhao X H, Ji L L, Cui Y, Zhou S L, Liu Z J, Zheng C Y, Wang L F, Gao Y Q, Huang X G, Fu S Z 2024 Phys. Rev. Lett. 132 035102Google Scholar

    [20]

    Wang P P, An H H, Fang Z H, Xiong J, Xie Z Y, Wang C, He Z Y, Jia G, Wang R R, Zheng S, Xia L, Feng W, Shi H T, Wang W, Sun J R, Gao Y Q, Fu S Z 2024 Matter Radiat. Extrem. 9 015602Google Scholar

    [21]

    Moody J, MacGowan B, Glenzer S, Kirkwood R, Kruer W, Montgomery D, Schmitt A, Williams E, Stone G 2000 Phys. Plasmas 7 2114Google Scholar

    [22]

    Yao C, Li J, Hao L, Yan R, Wang C, Lei A L, Ding Y K, Zheng J 2024 Nucl. Fusion 64 106013Google Scholar

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Publishing process
  • Received Date:  11 June 2024
  • Accepted Date:  09 October 2024
  • Available Online:  28 October 2024
  • Published Online:  20 November 2024

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