搜索

x

留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码

二维激子-极化子凝聚体中冲击波的产生与调控

王金玲 张昆 林机 李慧军

引用本文:
Citation:

二维激子-极化子凝聚体中冲击波的产生与调控

王金玲, 张昆, 林机, 李慧军

Generation and modulation of shock waves in two-dimensional polariton condensates

Wang Jin-Ling, Zhang Kun, Lin Ji, Li Hui-Jun
PDF
HTML
导出引用
  • 由于半导体微腔中形成的激子-极化子凝聚体能在室温实现, 且具有非平衡、强相互作用等特性, 其成为研究非平衡量子系统非线性特性的一个理想平台. 本文采用谱方法与四阶龙格库塔法, 探究二维极化子凝聚体中产生和调控冲击波的方案. 发现, 若在高凝聚率时淬火凝聚体与热库之间的交叉相互作用, 可将初始制备的亮孤子调制成两种波速不同的旋转对称型冲击波, 而初始的类暗孤子只能转变成单一波速的旋转对称型冲击波; 若淬火外势, 则可将类暗孤子转化成各向异性的超声速冲击波, 并给出冲击波对外势宽度的依赖关系. 若在低凝聚率时调控外势和非相干泵浦, 可在均匀凝聚体中激发出多种各向异性冲击波, 还可通过它们的振幅调控冲击波的波数和振幅, 并展示了激发冲击波所需外势或非相干泵浦的宽度范围. 文中方案不仅为激子-极化子凝聚体中产生和调控冲击波提供理论指导, 找到了与实验相似的对称型冲击波, 而且为非平衡或不可积系统中激发冲击波开辟了一条普适捷径, 可能成为调控孤子向冲击波转变的一种范式.
    Due to the ability of exciton-polariton condensates formed in semiconductor microcavities to be achieved at room temperature and their characteristics such as non-equilibrium and strong interactions, they have become an ideal platform for studying the nonlinear properties of non-equilibrium quantum systems. In 2013, the research group led by L. Dominici observed two-dimensional symmetric shock waves in the polariton condensate driven by coherent pump. However, owing to the characteristics of this system, theoretical researches have lagged behind. In one-dimensional polariton condensates, disregarding cross-interaction of the system, a type of asymmetric shock wave was respectively discovered by A. M. Kamchatnov in 2012 and A. M. Belounis in 2017. In 2023, utilizing the adiabatic approximation, our research team not only uncovered sparse wave, symmetric, and asymmetric shock waves in the system, but also revealed that the symmetric shock waves are triggered by cross-interaction. At present, there is no theoretical research on shock waves in two-dimensional polariton condensate. In this paper, spectral methods and fourth-order Runge-Kutta methods are used to explore the generation and control of shock waves in two-dimensional polariton condensates. It is found that when the cross-interaction between the condensate and the polariton thermal reservoir is quenched at high condensation rates, the initially prepared bright solitons can be modulated into two types of rotationally symmetric shock waves with different velocities, while the initial dark-like solitons can only transform into a single velocity rotationally symmetric shock wave. If quenching the external potential, the dark-like solitons can be transformed into anisotropic supersonic shock waves, and the dependence of shock wave on the width of the external potential is also shown. When the external potential and incoherent pumping are controlled at low condensation rates, multiple anisotropic shock waves can be excited in a uniform condensate, and their amplitudes can be used to control the wave number and amplitude of the shock waves and the range of widths for the external potential or incoherent pumping to excite shock waves is also demonstrated. The proposed methods in this paper not only provide theoretical guidance for the generation and control of shock waves in exciton-polariton condensates, but also find symmetric shock waves similar to experiments (Nat. Commun. 6 , 8993) without adopting any approximation, and open up a universal pathway for exciting shock waves in non-equilibrium or non-integrable systems, which may become a paradigm for transforming solitons into shock waves and significantly propel the rapid development of shock wave theory in different domains.
      通信作者: 林机, linji@zjnu.edu.cn ; 李慧军, hjli@zjnu.cn
    • 基金项目: 国家自然科学基金(批准号: 12074343, 12375006)和浙江省自然科学基金重点项目(批准号: LZ22A050002) 资助的课题.
      Corresponding author: Lin Ji, linji@zjnu.edu.cn ; Li Hui-Jun, hjli@zjnu.cn
    • Funds: Project supported by the National Natural Science Foundation of China (Grant Nos. 12074343, 12375006) and the Natural Science Foundation of Zhejiang Province, China (Grant No. LZ22A050002).
    [1]

    Zhang S, Zhu Z, Du W, Wu X, Ghosh S, Zhang Q, Xiong Q, Liu X 2023 ACS Photonics 10 2414Google Scholar

    [2]

    Kottilil D, Gupta M, Lu S, Babusenan A, Ji W 2023 Adv. Mater. 35 2209094Google Scholar

    [3]

    Deng H, Weihs G, Santori C, Bloch J, Yamamoto Y 2002 Science 298 199Google Scholar

    [4]

    Baumberg J J, Kavokin A V, Christopoulos S, Grundy A J D, Butté R, Christmann G, Solnyshkov D D, Malpuech G, Baldassarri Höger von Högersthal G, Feltin E, Carlin J F, Grandjean N 2008 Phys. Rev. Lett. 101 136409Google Scholar

    [5]

    Zhang Y, Jia C, Liang Z 2022 Chin. Phys. Lett. 39 020501Google Scholar

    [6]

    Qi W, Guo X G, Dong L W, Zhang X F 2023 Chin. Phys. B 32 030502Google Scholar

    [7]

    黄轶凡, 梁兆新 2023 物理学报 72 100505Google Scholar

    Huang Y F, Liang Z X 2023 Acta Phys. Sin. 72 100505Google Scholar

    [8]

    陈礼元, 高超, 林机, 李慧军 2022 物理学报 71 181101Google Scholar

    Chen L Y, Gao C, Lin J, Li H J 2022 Acta Phys. Sin. 71 181101Google Scholar

    [9]

    Weisbuch C, Nishioka M, Ishikawa A, Arakawa Y 1992 Phys. Rev. Lett. 69 3314Google Scholar

    [10]

    Kasprzak J, Richard M, Kundermann S, Baas A, Jeambrun P, Keeling J M J, Marchetti F M, Szymańska M H, André R, Staehli J L, Savona V, Littlewood P B, Deveaud B, Dang L S 2006 Nature 443 409Google Scholar

    [11]

    Jia C Y, Liang Z X 2020 Chin. Phys. Lett. 37 040502Google Scholar

    [12]

    Ye Z, Chen F, Zhou H, Luo S, Sun Z, Xu H, Xu H, Li H, Chen Z, Wu J 2023 Phys. Rev. B 107 L060303Google Scholar

    [13]

    Balili R, Hartwell V, Snoke D, Pfeiffer L, West K 2007 Science 316 1007Google Scholar

    [14]

    Szymańska M H, Keeling J, Littlewood P B 2006 Phys. Rev. Lett. 96 230602Google Scholar

    [15]

    Byrnes T, Kim N Y, Yamamoto Y 2014 Nat. Phys. 10 803Google Scholar

    [16]

    Zhang K, Wen W, Lin J, Li H J 2021 New J. Phys. 23 033011Google Scholar

    [17]

    Zhang K, Wen W, Lin J, Li H J 2022 Front. Phys. 10 798562Google Scholar

    [18]

    Tanese D, Flayac H, Solnyshkov D, Amo A, Lemaître A, Galopin E, Braive R, Senellart P, Sagnes I, Malpuech G, Bloch J 2013 Nat. Commun. 4 1749Google Scholar

    [19]

    Chen H J, Ren Y, Wang H 2022 Acta Phys. Sin. 71 056701Google Scholar

    [20]

    Ostrovskaya E A, Abdullaev J, Fraser M D, Desyatnikov A S, Kivshar Y S 2013 Phys. Rev. Lett. 110 170407Google Scholar

    [21]

    Pinsker F, Flayac H 2014 Phys. Rev. Lett. 112 140405Google Scholar

    [22]

    El G A, Geogjaev V V, Gurevich A V, Krylov A L 1995 Phys. D 87 186Google Scholar

    [23]

    El G A, Hoefer M A 2016 Phys. D 333 11Google Scholar

    [24]

    El G A, Gammal A, Khamis E G, Kraenkel R A, Kamchatnov A M 2007 Phys. Rev. A 76 053813Google Scholar

    [25]

    公睿智, 王灯山 2023 物理学报 72 100503Google Scholar

    Gong R Z, Wang D S 2023 Acta Phys. Sin. 72 100503Google Scholar

    [26]

    Kamchatnov A M 2021 Phys.-Usp. 64 48Google Scholar

    [27]

    Bikbaev R, Kudashev V 1994 Phys. Rev. A 190 255Google Scholar

    [28]

    Wang D S, Xu L, Xuan Z 2022 J. Nonlinear Sci. 32 3Google Scholar

    [29]

    Kamchatnov A M 2019 Phys. Rev. E 99 012203Google Scholar

    [30]

    Gong R, Wang D S 2022 Physica D 439 133398Google Scholar

    [31]

    Gong R, Wang D S 2022 Appl. Math. Lett. 126 107795Google Scholar

    [32]

    Sagdeev R Z 1962 Sov. Phys. Tech. Phys. 6 867

    [33]

    Wan W, Jia S, Fleischer J 2007 Nat. Phys. 3 46Google Scholar

    [34]

    Chanson H 2009 Eur. J. Mech. B 28 191Google Scholar

    [35]

    Hang C, Bai Z, Li W, Kamchatnov A, Huang G 2023 Phys. Rev. A 107 033503Google Scholar

    [36]

    贾瑞煜, 方乒乒, 高超, 林机 2021 物理学报 70 180303Google Scholar

    Jia R Y, Fang P P, Gao C, Lin J 2021 Acta Phys. Sin. 70 180303Google Scholar

    [37]

    Simplicio C, Purita J, Murrell W, Santos G, Dos Santos R, Lana J 2020 J. Clin. Orthop. Trauma 11 S309Google Scholar

    [38]

    Takayama K, Saito T 2004 Annu. Rev. Fluid Mech. 36 347Google Scholar

    [39]

    Yang Z, Zhang B 2023 Combust. Flame 251 112691Google Scholar

    [40]

    Hu Q, Shen X, Huang Z, Qian X, Jiang J, Yuan M, Pang L 2023 Int. J. Hydrog. Energy 51 830Google Scholar

    [41]

    Mayilswamy N, Krishnan A, Mundhada M, Deodhar H, Joshi G, Kandasubramanian B 2023 Ind. Eng. Chem. Res. 62 6584Google Scholar

    [42]

    Ciccarelli G, Johansen C, Parravani M 2010 Combust. Flame 157 2125Google Scholar

    [43]

    Dominici L, De Giorgi M, Ballarini D, Cancellieri E, Laussy F, Giacobino E, Bramati A, Gigli G, Sanvitto D 2013 IEEE Conference on Lasers and Electro-Optics (CLEO: 2013), June 9–14 2013, San Jose, California, USA, pp1–2

    [44]

    Dominici L, Petrov M, Matuszewski M, Ballarini D, De Giorgi M, Colas D, Cancellieri E, Silva Fernández B, Bramati A, Gigli G, Kavokin A, Laussy F, Sanvitto D 2015 Nat. Commun. 6 8993Google Scholar

    [45]

    Kamchatnov A M, Kartashov Y V 2012 Europhys. Lett. 97 10006Google Scholar

    [46]

    Belounis A M, Kessal S 2017 Can. J. Phys. 95 1234Google Scholar

    [47]

    Wang J L, Wen W, Lin J, Li H J 2023 Chin. Phys. Lett. 40 070302Google Scholar

    [48]

    Wang Q W, Wang J L, Wen W, Lin J, Li H J 2023 Commun. Theor. Phys. 75 065001Google Scholar

    [49]

    Yang J 2011 Nonlinear Waves in Integrable and Nonintegrable Systems (1st Ed.) (SIAM: Philadephia

  • 图 1  取亮孤子为初态, 淬火交叉相互作用$ \sigma_{2} $产生的冲击波 (a)参数取$ \sigma_{2}=1 $时, 亮孤子的轮廓图; (b)冲击波波速$ v_{\eta} $与声速$ C_{\eta} $随交叉相互作用强度$ \sigma_{2} $的变化曲线; (c)和(d)分别为$ \sigma_{2}=4,\; s=18 $和$ \sigma_{2}=5.8, \;s=16.5 $时冲击波的轮廓图, 二者波速分别为$ v_{\eta}=1.57 $和$ v_{\eta}=1.63 $, 此时选取(b)图中黑点对应的参数. 图中的插图均是取$ \xi=0 $的截面图

    Fig. 1.  A bright soliton is chosen as the initial incident wave, shock waves are generated through quenching the cross-interaction strength $ \sigma_{2} $: (a) Profile of the bright soliton with $ \sigma_{2}=1 $; (b) curves illustrating the variation of shock wave velocity and sound speed as a function of $ \sigma_{2} $; (c) and (d) represent the profiles of shock waves at $ \sigma_{2}=4,\; s = 18,\; v_{\eta}=1.57 $ and $ \sigma_{2}=5.8,\; s = 16.5,\; v_{\eta}=1.63 $, respectively, with corresponding parameters marked by the black dots in panel (b). The insets are cross-sections of the bright soliton and shock waves at $ \xi=0 $.

    图 2  取类暗孤子为初态, 淬火交叉相互作用强度$ \sigma_{2} $产生的冲击波 (a)参数取$ \sigma_{2}=1 $时, 类暗孤子的轮廓图; (b)冲击波波速$ v_{\eta} $与声速$ C_{\eta} $随交叉相互作用强度$ \sigma_{2} $的变化曲线; (c)和(d)分别为$ \sigma_{2}=4.5,\; s=18,\;v_{\eta}=1.5 $和$ \sigma_{2}=6.5,\; s=18,\; v_{\eta}= $$ 1.5 $时冲击波的轮廓图, 此时选取(b)图中黑点对应的参数. 图中的插图均是取$ \xi=0 $的截面图

    Fig. 2.  A dark-like soliton is chosen as the initial incident wave, shock waves are generated through quenching the cross-interaction strength $ \sigma_{2} $: (a) Profile of the dark-like soliton with $ \sigma_{2}=1 $; (b) curves illustrating the variation of shock wave velocity and sound speed as a function of $ \sigma_{2} $; (c) and (d) represent the profiles of shock waves at $ \sigma_{2}=4.5,\; s=18,\; v_{\eta}=1.5 $ and $ \sigma_{2}=6.5,\; s=18,\; v_{\eta}=1.5 $, respectively, with corresponding parameters marked by the black dots in panel (b). The insets are cross-sections of the dark-like soliton and shock waves at $ \xi=0 $.

    图 3  以类暗孤子为初态, 淬火外势产生的冲击波 (a) 冲击波的存在区域图. (b)—(c) 分别为 $ \sigma_{11}=3,\; v_{\eta}=1.42,\; s=11 $ 和$ \sigma_{11}=7,\; v_{\eta}=1.42,\; s=11 $的冲击波轮廓图, 其中 $ d_{\xi}=8, d_{\eta}=1 $. 右上插图给出冲击波的投影图, 右下插图给出$ \xi=0 $ ($ \eta=0 $) 时的截面图, 用蓝色实线 (红色虚线) 表示. (d) $ \sigma_{11}=3 $, $ d_{\xi}=\infty $, $ d_{\eta}=1, \; s=8 $ 时冲击波的投影图, 此时, 冲击波速度为$ v_{\eta}=1.42 $, 图3(e)3(f) 分别给出 3(d) 中 $ \xi=-16.16 $ 与$ \xi=0 $ 处两条黑色虚线对应的截面图

    Fig. 3.  A dark-like soliton is chosen as the initial incident wave, shock waves are produced by quenching the external potential. (a) Existence interval of the shock wave as a function of $ d_{\eta} $ and $ \sigma_{12} $; (b)–(c) Profiles of shock waves with $ \sigma_{11}=3, \, 7,\; s=11 $, here, $ d_{\xi}=8,\; d_{\eta}=1,\; v_{\eta}=1.42 $, projections and cross-sections along the η (blue solid line)and ξ (red dashed line)directions are displayed on the right side of (b) and (c); (d) Projection of the shock wave, here, $ \sigma_{11}=3,\; d_{\xi}=\infty, \; d_{\eta}=1,\; s=8,\; v_{\eta}=1.42 $; The cross-sections corresponding to the two black dashed lines for $ \xi=-16.16 $ and $ \xi=0 $ are illustrated in (e) and (f), respectively.

    图 4  通过调控外势在均匀凝聚体中激发的冲击波 (a) 冲击波的存在区域图. (b)—(c) $ \sigma_{11}= 3$和$ \sigma_{11}= 7 $时对应的冲击波轮廓图, 其中 $ d_{\xi}=8, \; d_{\eta}=1,\; v_{\eta}=1.72, s=11 $. 右上插图给出冲击波的投影图, 右下插图给出$ \xi=0 $ ($ \eta=0 $) 时的截面图, 用蓝色实线 (红色虚线) 表示

    Fig. 4.  Shock waves induced by potential in a homogeneous condensate. (a) Existence interval of the shock wave as a function of $ d_{\eta} $ and $ \sigma_{12} $; (b)–(c) Profiles of shock waves with $ \sigma_{11}=3, \, 7 $, here, $ d_{\xi}=8, \;d_{\eta}=1,\; v_{\eta}=1.72,\; s=11 $, projections and cross-sections along the η (blue solid line)and ξ (red dashed line) directions are displayed on the right side of (b) and (c).

    图 5  通过调控泵浦在均匀凝聚体中激发的冲击波 (a) 冲击波的存在区域图. (b)—(c) $ \sigma_{10}=3 $ 和$ \sigma_{10}=7 $时对应的冲击波轮廓图, 其中 $ d_{\xi}=10,\; d_{\eta}=2, \; v_{\eta}=1.57, \; s=17 $. 右上插图给出冲击波的投影图, 右下插图给出$ \xi=0 $ ($ \eta=0 $) 时的截面图, 用蓝色实线 (红色虚线) 表示.

    Fig. 5.  Shock waves induced by incoherent pump in a homogeneous condensate. (a) Existence interval of the shock wave as a function of $ d_{\eta} $ and $ \sigma_{12} $; (b)–(c) Profiles of shock waves with $ \sigma_{10}=3, \, 7 $, here, $ d_{\xi}=10, \; d_{\eta}=2, \; v_{\eta}=1.57, \; s=17 $, projections and cross-sections along the η (blue solid line)and ξ (red dashed line) directions are displayed on the right side of (b) and (c).

  • [1]

    Zhang S, Zhu Z, Du W, Wu X, Ghosh S, Zhang Q, Xiong Q, Liu X 2023 ACS Photonics 10 2414Google Scholar

    [2]

    Kottilil D, Gupta M, Lu S, Babusenan A, Ji W 2023 Adv. Mater. 35 2209094Google Scholar

    [3]

    Deng H, Weihs G, Santori C, Bloch J, Yamamoto Y 2002 Science 298 199Google Scholar

    [4]

    Baumberg J J, Kavokin A V, Christopoulos S, Grundy A J D, Butté R, Christmann G, Solnyshkov D D, Malpuech G, Baldassarri Höger von Högersthal G, Feltin E, Carlin J F, Grandjean N 2008 Phys. Rev. Lett. 101 136409Google Scholar

    [5]

    Zhang Y, Jia C, Liang Z 2022 Chin. Phys. Lett. 39 020501Google Scholar

    [6]

    Qi W, Guo X G, Dong L W, Zhang X F 2023 Chin. Phys. B 32 030502Google Scholar

    [7]

    黄轶凡, 梁兆新 2023 物理学报 72 100505Google Scholar

    Huang Y F, Liang Z X 2023 Acta Phys. Sin. 72 100505Google Scholar

    [8]

    陈礼元, 高超, 林机, 李慧军 2022 物理学报 71 181101Google Scholar

    Chen L Y, Gao C, Lin J, Li H J 2022 Acta Phys. Sin. 71 181101Google Scholar

    [9]

    Weisbuch C, Nishioka M, Ishikawa A, Arakawa Y 1992 Phys. Rev. Lett. 69 3314Google Scholar

    [10]

    Kasprzak J, Richard M, Kundermann S, Baas A, Jeambrun P, Keeling J M J, Marchetti F M, Szymańska M H, André R, Staehli J L, Savona V, Littlewood P B, Deveaud B, Dang L S 2006 Nature 443 409Google Scholar

    [11]

    Jia C Y, Liang Z X 2020 Chin. Phys. Lett. 37 040502Google Scholar

    [12]

    Ye Z, Chen F, Zhou H, Luo S, Sun Z, Xu H, Xu H, Li H, Chen Z, Wu J 2023 Phys. Rev. B 107 L060303Google Scholar

    [13]

    Balili R, Hartwell V, Snoke D, Pfeiffer L, West K 2007 Science 316 1007Google Scholar

    [14]

    Szymańska M H, Keeling J, Littlewood P B 2006 Phys. Rev. Lett. 96 230602Google Scholar

    [15]

    Byrnes T, Kim N Y, Yamamoto Y 2014 Nat. Phys. 10 803Google Scholar

    [16]

    Zhang K, Wen W, Lin J, Li H J 2021 New J. Phys. 23 033011Google Scholar

    [17]

    Zhang K, Wen W, Lin J, Li H J 2022 Front. Phys. 10 798562Google Scholar

    [18]

    Tanese D, Flayac H, Solnyshkov D, Amo A, Lemaître A, Galopin E, Braive R, Senellart P, Sagnes I, Malpuech G, Bloch J 2013 Nat. Commun. 4 1749Google Scholar

    [19]

    Chen H J, Ren Y, Wang H 2022 Acta Phys. Sin. 71 056701Google Scholar

    [20]

    Ostrovskaya E A, Abdullaev J, Fraser M D, Desyatnikov A S, Kivshar Y S 2013 Phys. Rev. Lett. 110 170407Google Scholar

    [21]

    Pinsker F, Flayac H 2014 Phys. Rev. Lett. 112 140405Google Scholar

    [22]

    El G A, Geogjaev V V, Gurevich A V, Krylov A L 1995 Phys. D 87 186Google Scholar

    [23]

    El G A, Hoefer M A 2016 Phys. D 333 11Google Scholar

    [24]

    El G A, Gammal A, Khamis E G, Kraenkel R A, Kamchatnov A M 2007 Phys. Rev. A 76 053813Google Scholar

    [25]

    公睿智, 王灯山 2023 物理学报 72 100503Google Scholar

    Gong R Z, Wang D S 2023 Acta Phys. Sin. 72 100503Google Scholar

    [26]

    Kamchatnov A M 2021 Phys.-Usp. 64 48Google Scholar

    [27]

    Bikbaev R, Kudashev V 1994 Phys. Rev. A 190 255Google Scholar

    [28]

    Wang D S, Xu L, Xuan Z 2022 J. Nonlinear Sci. 32 3Google Scholar

    [29]

    Kamchatnov A M 2019 Phys. Rev. E 99 012203Google Scholar

    [30]

    Gong R, Wang D S 2022 Physica D 439 133398Google Scholar

    [31]

    Gong R, Wang D S 2022 Appl. Math. Lett. 126 107795Google Scholar

    [32]

    Sagdeev R Z 1962 Sov. Phys. Tech. Phys. 6 867

    [33]

    Wan W, Jia S, Fleischer J 2007 Nat. Phys. 3 46Google Scholar

    [34]

    Chanson H 2009 Eur. J. Mech. B 28 191Google Scholar

    [35]

    Hang C, Bai Z, Li W, Kamchatnov A, Huang G 2023 Phys. Rev. A 107 033503Google Scholar

    [36]

    贾瑞煜, 方乒乒, 高超, 林机 2021 物理学报 70 180303Google Scholar

    Jia R Y, Fang P P, Gao C, Lin J 2021 Acta Phys. Sin. 70 180303Google Scholar

    [37]

    Simplicio C, Purita J, Murrell W, Santos G, Dos Santos R, Lana J 2020 J. Clin. Orthop. Trauma 11 S309Google Scholar

    [38]

    Takayama K, Saito T 2004 Annu. Rev. Fluid Mech. 36 347Google Scholar

    [39]

    Yang Z, Zhang B 2023 Combust. Flame 251 112691Google Scholar

    [40]

    Hu Q, Shen X, Huang Z, Qian X, Jiang J, Yuan M, Pang L 2023 Int. J. Hydrog. Energy 51 830Google Scholar

    [41]

    Mayilswamy N, Krishnan A, Mundhada M, Deodhar H, Joshi G, Kandasubramanian B 2023 Ind. Eng. Chem. Res. 62 6584Google Scholar

    [42]

    Ciccarelli G, Johansen C, Parravani M 2010 Combust. Flame 157 2125Google Scholar

    [43]

    Dominici L, De Giorgi M, Ballarini D, Cancellieri E, Laussy F, Giacobino E, Bramati A, Gigli G, Sanvitto D 2013 IEEE Conference on Lasers and Electro-Optics (CLEO: 2013), June 9–14 2013, San Jose, California, USA, pp1–2

    [44]

    Dominici L, Petrov M, Matuszewski M, Ballarini D, De Giorgi M, Colas D, Cancellieri E, Silva Fernández B, Bramati A, Gigli G, Kavokin A, Laussy F, Sanvitto D 2015 Nat. Commun. 6 8993Google Scholar

    [45]

    Kamchatnov A M, Kartashov Y V 2012 Europhys. Lett. 97 10006Google Scholar

    [46]

    Belounis A M, Kessal S 2017 Can. J. Phys. 95 1234Google Scholar

    [47]

    Wang J L, Wen W, Lin J, Li H J 2023 Chin. Phys. Lett. 40 070302Google Scholar

    [48]

    Wang Q W, Wang J L, Wen W, Lin J, Li H J 2023 Commun. Theor. Phys. 75 065001Google Scholar

    [49]

    Yang J 2011 Nonlinear Waves in Integrable and Nonintegrable Systems (1st Ed.) (SIAM: Philadephia

  • [1] 李新月, 祁娟娟, 赵敦, 刘伍明. 自旋-轨道耦合二分量玻色-爱因斯坦凝聚系统的孤子解. 物理学报, 2023, 72(10): 106701. doi: 10.7498/aps.72.20222319
    [2] 陈礼元, 高超, 林机, 李慧军. $ {\cal{PT}}$对称极化子凝聚体系统中的稳定孤子及其调控. 物理学报, 2022, 71(18): 181101. doi: 10.7498/aps.71.20220475
    [3] 王小峰, 陶钢, 徐宁, 王鹏, 李召, 闻鹏. 冲击波诱导水中纳米气泡塌陷的分子动力学分析. 物理学报, 2021, 70(13): 134702. doi: 10.7498/aps.70.20210058
    [4] 贾瑞煜, 方乒乒, 高超, 林机. 玻色-爱因斯坦凝聚体中的淬火孤子与冲击波. 物理学报, 2021, 70(18): 180303. doi: 10.7498/aps.70.20210564
    [5] 文林, 梁毅, 周晶, 余鹏, 夏雷, 牛连斌, 张晓斐. 线性塞曼劈裂对自旋-轨道耦合玻色-爱因斯坦凝聚体中亮孤子动力学的影响. 物理学报, 2019, 68(8): 080301. doi: 10.7498/aps.68.20182013
    [6] 伍友成, 刘高旻, 戴文峰, 高志鹏, 贺红亮, 郝世荣, 邓建军. 冲击波作用下Pb(Zr0.95Ti0.05)O3铁电陶瓷去极化后电阻率动态特性. 物理学报, 2017, 66(4): 047201. doi: 10.7498/aps.66.047201
    [7] 何章明, 张志强. 玻色-爱因斯坦凝聚体中的双孤子相互作用操控. 物理学报, 2016, 65(11): 110502. doi: 10.7498/aps.65.110502
    [8] 张恒, 段文山. 二维玻色-爱因斯坦凝聚中孤立波的调制不稳定性. 物理学报, 2013, 62(4): 044703. doi: 10.7498/aps.62.044703
    [9] 张波, 王登龙, 佘彦超, 张蔚曦. 方势阱中凝聚体的孤子动力学行为. 物理学报, 2013, 62(11): 110501. doi: 10.7498/aps.62.110501
    [10] 喻寅, 王文强, 杨佳, 张友君, 蒋冬冬, 贺红亮. 多孔脆性介质冲击波压缩破坏的细观机理和图像. 物理学报, 2012, 61(4): 048103. doi: 10.7498/aps.61.048103
    [11] 王峰, 彭晓世, 梅鲁生, 刘慎业, 蒋小华, 丁永坤. 基于速度干涉仪的冲击波精密调速实验技术研究. 物理学报, 2012, 61(13): 135201. doi: 10.7498/aps.61.135201
    [12] 王峰, 彭晓世, 刘慎业, 蒋小华, 徐涛, 丁永坤, 张保汉. 三明治靶型在间接驱动冲击波实验中的应用. 物理学报, 2011, 60(11): 115203. doi: 10.7498/aps.60.115203
    [13] 冯宁博, 谷岩, 刘雨生, 聂恒昌, 陈学锋, 王根水, 贺红亮, 董显林. 冲击波加载下孔隙率对Pb0.99(Zr0.95Ti0.05)0.98Nb0.02O3 铁电陶瓷去极化性能的影响. 物理学报, 2010, 59(12): 8897-8902. doi: 10.7498/aps.59.8897
    [14] 俞宇颖, 谭 华, 胡建波, 戴诚达, 陈大年, 王焕然. 冲击波作用下铝的等效剪切模量. 物理学报, 2008, 57(4): 2352-2357. doi: 10.7498/aps.57.2352
    [15] 陈登平, 贺红亮, 黎明发, 经福谦. 冲击压缩下非均质脆性固体的弛豫破坏研究. 物理学报, 2007, 56(1): 423-428. doi: 10.7498/aps.56.423
    [16] 何章明, 王登龙. 凝聚体中亮孤子和暗孤子的交替演化. 物理学报, 2007, 56(6): 3088-3091. doi: 10.7498/aps.56.3088
    [17] 崔新林, 祝文军, 邓小良, 李英骏, 贺红亮. 冲击波压缩下含纳米孔洞单晶铁的结构相变研究. 物理学报, 2006, 55(10): 5545-5550. doi: 10.7498/aps.55.5545
    [18] 徐 岩, 薛德胜, 左 维, 李发伸. 非均匀交换各向异性铁磁介质的非线性表面自旋波. 物理学报, 2003, 52(11): 2896-2900. doi: 10.7498/aps.52.2896
    [19] 洪学仁, 段文山, 孙建安, 石玉仁, 吕克璞. 非均匀尘埃等离子体中孤子的传播. 物理学报, 2003, 52(11): 2671-2677. doi: 10.7498/aps.52.2671
    [20] 王晓生, 佘卫龙. 部分空间非相干光光伏空间孤子. 物理学报, 2002, 51(3): 573-577. doi: 10.7498/aps.51.573
计量
  • 文章访问数:  555
  • PDF下载量:  36
  • 被引次数: 0
出版历程
  • 收稿日期:  2024-02-02
  • 修回日期:  2024-02-27
  • 上网日期:  2024-04-11
  • 刊出日期:  2024-06-05

/

返回文章
返回