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二维各向异性SSH模型的拓扑性质研究

郭思嘉 李昱增 李天梓 范喜迎 邱春印

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二维各向异性SSH模型的拓扑性质研究

郭思嘉, 李昱增, 李天梓, 范喜迎, 邱春印

Topological properties of non-isotropic two-dimensional SSH model

Guo Si-Jia, Li Yu-Zeng, Li Tian-Zi, Fan Xi-Ying, Qiu Chun-Yin
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  • 二维Su-Schrieffer-Heeger(SSH)模型是在拓扑物理领域受到广泛研究的一种模型, 具有许多独特的物理性质. 它属于高阶拓扑绝缘体, 在第二条和第三条能带间会产生具有连续谱束缚态(bound states in the continuum, BICs)性质的角态. 本文首先介绍了二维SSH模型的拓扑性质, 在此基础上论证了第二条和第三条能带何时会在整个布里渊区上产生能隙. 随后, 计算了模型的电荷极化分布和电荷密度分布, 证明了当x方向上胞内跃迁几率和胞间跃迁几率较大时, x方向的边缘电荷极化激发了y方向的边缘态, 反之亦然. 同时, 边缘电荷极化激发了角上的异常填充, 产生了具有良好局域性与鲁棒性的拓扑角态. 最后, 构建了一种声学谐振腔模型, 并证明了该模型可以较好的模拟各向异性二维SSH模型的拓扑性质.
    The one-dimensional (1D) Su-Schrieffer-Heeger (SSH) chain is a model that has been widely studied in the field of topological physics. The two-dimensional (2D) SSH model is a 2D extension of the 1D SSH chain and has many unique physical properties. It is a higher-order topological insulator (HOTI), in which corner states with bound states in the continuum (BIC) properties will arise between the second energy band and the third energy band. There are two different topological phases in the isotropic 2D SSH model, and a topological phase transition will happen when the intracell coupling strength is equal to the intercell coupling strength.In this paper, we first break the isotropy of the isotropic 2D SSH model, defining the ratio of the x-directional coupling strength to the y-directional coupling strength as α and the ratio of the intercell coupling strength to the intracell coupling strength as β, which represent the strength of the topological property and anisotropy respectively. We use α and β to calibrate all possible models, classify them as three different types of phases, and draw their phase diagrams.Then we argue when the energy gap between the second energy band and the third energy band emerges over the entire Brillouin zone.Meanwhile, we use a method to calculate the spatial distribution of polarization when the model is half-filled, and it is shown that there is 1/2 polarization localized at the edges in the direction with larger intracell coupling, but no edge polarization in the other direction. The edge polarization excites the edge dipole moment, giving rise to a topological edge state in the energy gap. At the same time, when the model has an entire open boundary, the dipole moment directs the charge to accumulate on the corners, which can be observed from the local charge density distribution. This type of fractional charge is a filling anomaly and formed spontaneously by the lattice to maintain electrical neutrality and rotational symmetry simultaneously. This fractional charge induces the aforementioned corner state. And by its nature of filling anomaly, this corner state is better localized and robust. It will not couple with the bulk state as long as the rotational symmetry or chirality of the model is not broken.Finally, we construct an acoustic resonant cavity model: a rectangular shaped resonant cavity is used to simulate individual lattice points and the coupling strength between the lattice points is controlled by varying the diameter of the conduit between the resonant cavities. According to the Comsol calculation results, we can see that the topological properties of the anisotropic two-dimensional SSH model are well simulated by this model.
      通信作者: 邱春印, cyqiu@whu.edu.cn
    • 基金项目: 国家自然科学基金(批准号: 11890701)资助的课题.
      Corresponding author: Qiu Chun-Yin, cyqiu@whu.edu.cn
    • Funds: Project supported by the National Natural Science Foundation of China (Grant No. 11890701).
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    Huber S D 2016 Nat. Phys. 12 621Google Scholar

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    Ozawa T, Price H M, Amo A, Goldman N, Hafezi M, Lu L, Rechtsman M C, Schuster D, Simon J, Zilberberg O, Carusotto I 2019 Rev. Mod. Phys. 91 015006Google Scholar

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    Wang Z, Chong Y, Joannopoulos J D, Soljacic M 2009 Nature 461 772Google Scholar

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    Song Z, Fang Z, Fang C 2017 Phys. Rev. Lett. 119 246402Google Scholar

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    Langbehn J, Peng Y, Trifunovic L, von Oppen F, Brouwer P W 2017 Phys. Rev. Lett. 119 246401Google Scholar

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    Serra G M, Peri V, Susstrunk R, Bilal O R, Larsen T, Villanueva L G, Huber S D 2018 Nature 555 342Google Scholar

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    Peterson C W, Benalcazar W A, Hughes T L, Bahl G 2018 Nature 555 346Google Scholar

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    Imhof S, Berger C, Bayer F, Brehm J, Molenkamp L W, Kiessling T, Schindler F, Lee C H, Greiter M, Neupert T, Thomale R 2018 Nat. Phys. 14 925Google Scholar

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    Noh J, Benalcazar W A, Huang S, Collins M J, Chen K P, Hughes T L, Rechtsman M C 2018 Nat. Photonics 12 408Google Scholar

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    Mittal S, Orre V V, Zhu G, Gorlach M A, Poddubny A, Hafezi M 2019 Nat. Photonics 13 692Google Scholar

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    Chen X D, Deng W M, Shi F L, Zhao F L, Chen M, Dong J W 2019 Phys. Rev. Lett. 122 233902Google Scholar

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    El Hassan A, Kunst F K, Moritz A, Andler G, Bergholtz E J, Bourennane M 2019 Nat. Photonics 13 697Google Scholar

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    Fan H, Xia B, Tong L, Zheng S, Yu D 2019 Phys. Rev. Lett. 122 204301Google Scholar

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    Liu S, Gao W, Zhang Q, Ma S, Zhang L, Liu C, Xiang Y J, Cui T J, Zhang S 2019 Research 2019 8609875Google Scholar

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    Serra G M, Süsstrunk R, Huber S D 2019 Phys. Rev. B 99 020304Google Scholar

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    Xue H, Yang Y, Gao F, Chong Y, Zhang B 2019 Nat. Mater. 18 108Google Scholar

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    Ni X, Weiner M, Alù A, Khanikaev A B 2019 Nat. Mater. 18 113Google Scholar

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    Zhang X, Wang H X, Lin Z K, Tian Y, Xie B, Lu M H, Chen Y F, Jiang J H 2019 Nat. Phys. 15 582Google Scholar

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    Zhang X, Xie B Y, Wang H F, Xu X, Tian Y, Jiang J H, Lu M H, Chen Y F 2019 Nat. Commun. 10 5331Google Scholar

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    Weiner M, Ni X, Li M, Alù A, Khanikaev A B 2020 Sci. Adv. 6 eaay4166Google Scholar

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    Qi Y, Qiu C, Xiao M, He H, Ke M, Liu Z 2020 Phys. Rev. Lett. 124 206601Google Scholar

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    Xie B Y, Su G X, Wang H F, Su H, Shen X P, Zhan P, Lu M H, Wang Z L, Chen Y F 2019 Phys. Rev. Lett. 122 233903Google Scholar

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    Coutant A, Achilleos V, Richoux O, Theocharis G, Pagneux V 2021 J. Appl. Phys. 129 125108Google Scholar

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    Obana D, Liu F, Wakabayashi K 2019 Phys. Rev. B 100 075437Google Scholar

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    Lieu S 2018 Phys. Rev. B 97 045106Google Scholar

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    Yuce C, Ramezani H 2019 Phys. Rev. A 100 032102Google Scholar

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    Dangel F, Wagner M, Cartarius H, Main J, Wunner G 2018 Phys. Rev. A 98 013628Google Scholar

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    Bomantara R W, Zhou L, Pan J, Gong J 2019 Phys. Rev. B 99 045441Google Scholar

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    Xie B Y, Wang H F, Wang H X, Zhu X Y, Jiang J H, Lu M H, Chen Y F 2018 Phys. Rev. B 98 205147Google Scholar

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    Zhen B, Hsu C W, Lu L, Stone A D, Soljacic M 2014 Phys. Rev. Lett. 113 257401Google Scholar

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    Molina M I, Miroshnichenko A E, Kivshar Y S 2012 Phys. Rev. Lett. 108 070401Google Scholar

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    Weimann S, Xu Y, Keil R, Miroshnichenko A E, Tunnermann A, Nolte S, Sukhorukov A A, Szameit A, Kivshar Y S 2013 Phys. Rev. Lett. 111 240403Google Scholar

    [40]

    Benalcazar W A, Cerjan A 2020 Phys. Rev. B 101 161116Google Scholar

    [41]

    Benalcazar W A, Bernevig B A, Hughes T L 2017 Phys. Rev. B 96 245115Google Scholar

    [42]

    Hsu C W, Zhen B, Stone A D, Joannopoulos J D, Soljačić M 2016 Nat. Rev. Mater. 1 16048Google Scholar

    [43]

    Stillinger F H, Herrick D R 1975 Phys. Rev. A 11 446Google Scholar

    [44]

    Friedrich H, Wintgen D 1985 Phys. Rev. A:Gen Phys 32 3231Google Scholar

    [45]

    Marinica D C, Borisov A G, Shabanov S V 2008 Phys. Rev. Lett. 100 183902Google Scholar

    [46]

    Shipman S P, Venakides S 2005 Phys. Rev. E:Stat. Nonlinear Soft Matter Phys. 71 026611Google Scholar

    [47]

    Moiseyev N 2009 Phys. Rev. Lett. 102 167404Google Scholar

    [48]

    Plotnik Y, Peleg O, Dreisow F, Heinrich M, Nolte S, Szameit A, Segev M 2011 Phys. Rev. Lett. 107 183901Google Scholar

    [49]

    Lee J, Zhen B, Chua S L, Qiu W, Joannopoulos J D, Soljacic M, Shapira O 2012 Phys. Rev. Lett. 109 067401Google Scholar

    [50]

    Evans D V, Levitin M, Vassiliev D 2006 J. Fluid Mech. 261 21Google Scholar

    [51]

    Koshelev K, Lepeshov S, Liu M, Bogdanov A, Kivshar Y 2018 Phys. Rev. Lett. 121 193903Google Scholar

    [52]

    Liu F, Wakabayashi K 2017 Phys. Rev. Lett. 118 076803Google Scholar

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    Benalcazar W A, Bernevig B A, Hughes T L 2017 Science 357 61Google Scholar

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    Benalcazar W A, Li T H, Hughes T L 2019 Phys. Rev. B 99 245151Google Scholar

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    Li C A, Wu S S 2020 Phys. Rev. B 101 195309Google Scholar

  • 图 1  (a) 二维SSH模型原胞示意图; (b) 二维SSH模型在倒空间的示意图; (c) 二维SSH模型的相图. 图中黑色, 绿色, 蓝色五角星标记了三种典型的拓扑相, 其代表的参数$\left( {\alpha , \beta } \right)$分别为$\left( {1.5, 3} \right)$, $\left( {2, 3} \right)$, $\left( {2.5, 3} \right)$; (d) 图1(c)中黑色五角星代表的模型的带结构图, 红色圆形标记了高对称点X上第二条和第三条能带的变化过程; (e) 绿色五角星代表的模型的带结构图; (f) 蓝色五角星代表的模型的带结构图

    Fig. 1.  (a) Schematic diagram of the original cell of the 2D SSH model; (b) schematic diagram of the 2D SSH model in inverse space; (c) phase diagram of the 2D SSH model. The black, green and blue pentagrams in the figure mark the three typical topological phases with the parameters $\left( {\alpha , \beta } \right)$ as $\left( {1.5, 3} \right)$, $\left( {2, 3} \right)$ and $\left( {2.5, 3} \right)$ respectively; (d) a diagram of the band structure of the model represented by the black pentagram in Fig. 1(c), and the red circles mark the evolution process of the second and third energy bands at the high symmetry point X; (e) band structure for the model represented by the green pentagram; (f) band structure for the model represented by the blue pentagram.

    图 2  电荷极化与电荷密度分布计算结果 (a) 电荷极化分布计算结果. 使用的参数为$ \alpha = 5, \beta = 4 $, 计算中使用了半无限大的条带模型, 开放边界的一侧计算了有20个原胞, 从左至右分别为电荷极化的x方向分量和y方向分量; (b) 拓扑平庸态下的电荷极化分布. 使用的参数为$\alpha = 5, \beta = 0.25$; (c) 电荷密度分布计算结果, 计算中使用了20 × 20个原胞; (d) 拓扑平庸态下的电荷极化分布

    Fig. 2.  Calculation result of polarization and charge density distribution: (a) Calculated results of the polarization intensity distribution. The parameters used are $\alpha = 5, \beta = 4$, a semi-infinite strip model is used, and there are 20 primary cells on the side of the open boundary. From left to right, for the x- and y-directional components of the polarization; (b) calculated results of the polarization intensity distribution in topological trival phase. The parameters used are $\alpha = 5, \beta = 0.25$; (c) calculated results of the charge density distribution, 20 × 20 unit cells used in the calculation; (d) calculated results of the charge density distribution in topological trival phase.

    图 3  (a) 二维SSH模型的态密度分布. 使用的参数为$ \alpha = 5, \beta = 4 $, 计算中使用了20 × 20个原胞; (b) x方向投影能带图, 蓝色标记部分为边缘态, 计算中使用了50个原胞; (c) y方向投影能带图; (d) 体态的局域态密度分布; (e) 边缘态的局域态密度分布; (f) 角态的局域态密度分布

    Fig. 3.  (a) Density of states distribution for the 2D SSH model. The parameters used are $\alpha = 5, \beta = 4$. 20 × 20 unit cells used in the calculation; (b) projected band diagram in x-direction, with edge states marked in blue, 50 unit cells used in the calculation; (c) projected band diagram in y-direction; (d) local density distribution of bulk states; (e) local density distribution of edge states; (f) local density distribution of corner states.

    图 4  (a) 计算中使用的原胞模型示意图; (b) 模拟计算的带结构图; (c) 模拟计算的态密度分布图, 计算中使用了8 × 8个原胞; (d) 体态声压场分布示意图; (e) 边缘态声压场分布示意图; (f) 角态声压场分布示意图.

    Fig. 4.  (a) Schematic diagram of the unit cell model used in the calculations; (b) diagram of the band structure for the simulations; (c) diagram of the density of states distribution for the simulations with 8 × 8 unit cells used; (d) schematic diagram of the bulk sound pressure field distribution; (e) schematic diagram of the edge state sound pressure field distribution; (f) schematic diagram of corner state sound pressure field distribution.

    表 1  运用威尔森循环法计算二维SSH模型Zak phase的结果

    Table 1.  Results of the two-dimensional SSH model Zak phase using the Willson Loop method.

    占据的能带数目
    1234
    相①(左半部分)(1/2, 1/2)(0, 0)(0, 0)(1/2, 1/2)
    相①(右半部分)(1/2, 1/2)(0, 0)(0, 0)(1/2, 1/2)
    相②(1/2, 1/2)(0, 0)(0, 0)(1/2, 1/2)
    相③(0, 0)(0, 0)(0, 0)(0, 0)
    下载: 导出CSV
  • [1]

    Klitzing K V, Dorda G, Pepper M 1980 Phys. Rev. Lett. 45 494Google Scholar

    [2]

    Thouless D J, Kohmoto M, Nightingale M P, Den Nijs M 1982 Phys. Rev. Lett. 49 405Google Scholar

    [3]

    Ma G, Xiao M, Chan C T 2019 Nat. Rev. Phys. 1 281Google Scholar

    [4]

    Huber S D 2016 Nat. Phys. 12 621Google Scholar

    [5]

    Ozawa T, Price H M, Amo A, Goldman N, Hafezi M, Lu L, Rechtsman M C, Schuster D, Simon J, Zilberberg O, Carusotto I 2019 Rev. Mod. Phys. 91 015006Google Scholar

    [6]

    Zhang X J, Xiao M, Cheng Y, Lu M H, Christensen J 2018 Commun. Phys. 1 97Google Scholar

    [7]

    Lu L, Joannopoulos J D, Soljačić M 2014 Nat. Photonics 8 821Google Scholar

    [8]

    Haldane F D, Raghu S 2008 Phys. Rev. Lett. 100 013904Google Scholar

    [9]

    Wang Z, Chong Y, Joannopoulos J D, Soljacic M 2009 Nature 461 772Google Scholar

    [10]

    Song Z, Fang Z, Fang C 2017 Phys. Rev. Lett. 119 246402Google Scholar

    [11]

    Langbehn J, Peng Y, Trifunovic L, von Oppen F, Brouwer P W 2017 Phys. Rev. Lett. 119 246401Google Scholar

    [12]

    Serra G M, Peri V, Susstrunk R, Bilal O R, Larsen T, Villanueva L G, Huber S D 2018 Nature 555 342Google Scholar

    [13]

    Peterson C W, Benalcazar W A, Hughes T L, Bahl G 2018 Nature 555 346Google Scholar

    [14]

    Imhof S, Berger C, Bayer F, Brehm J, Molenkamp L W, Kiessling T, Schindler F, Lee C H, Greiter M, Neupert T, Thomale R 2018 Nat. Phys. 14 925Google Scholar

    [15]

    Noh J, Benalcazar W A, Huang S, Collins M J, Chen K P, Hughes T L, Rechtsman M C 2018 Nat. Photonics 12 408Google Scholar

    [16]

    Mittal S, Orre V V, Zhu G, Gorlach M A, Poddubny A, Hafezi M 2019 Nat. Photonics 13 692Google Scholar

    [17]

    Chen X D, Deng W M, Shi F L, Zhao F L, Chen M, Dong J W 2019 Phys. Rev. Lett. 122 233902Google Scholar

    [18]

    El Hassan A, Kunst F K, Moritz A, Andler G, Bergholtz E J, Bourennane M 2019 Nat. Photonics 13 697Google Scholar

    [19]

    Fan H, Xia B, Tong L, Zheng S, Yu D 2019 Phys. Rev. Lett. 122 204301Google Scholar

    [20]

    Liu S, Gao W, Zhang Q, Ma S, Zhang L, Liu C, Xiang Y J, Cui T J, Zhang S 2019 Research 2019 8609875Google Scholar

    [21]

    Serra G M, Süsstrunk R, Huber S D 2019 Phys. Rev. B 99 020304Google Scholar

    [22]

    Xue H, Yang Y, Gao F, Chong Y, Zhang B 2019 Nat. Mater. 18 108Google Scholar

    [23]

    Ni X, Weiner M, Alù A, Khanikaev A B 2019 Nat. Mater. 18 113Google Scholar

    [24]

    Zhang X, Wang H X, Lin Z K, Tian Y, Xie B, Lu M H, Chen Y F, Jiang J H 2019 Nat. Phys. 15 582Google Scholar

    [25]

    Zhang Z, Long H, Liu C, Shao C, Cheng Y, Liu X, Christensen J 2019 Adv. Mater. 31 1904682Google Scholar

    [26]

    Zhang X, Xie B Y, Wang H F, Xu X, Tian Y, Jiang J H, Lu M H, Chen Y F 2019 Nat. Commun. 10 5331Google Scholar

    [27]

    Weiner M, Ni X, Li M, Alù A, Khanikaev A B 2020 Sci. Adv. 6 eaay4166Google Scholar

    [28]

    Qi Y, Qiu C, Xiao M, He H, Ke M, Liu Z 2020 Phys. Rev. Lett. 124 206601Google Scholar

    [29]

    Xie B Y, Su G X, Wang H F, Su H, Shen X P, Zhan P, Lu M H, Wang Z L, Chen Y F 2019 Phys. Rev. Lett. 122 233903Google Scholar

    [30]

    Coutant A, Achilleos V, Richoux O, Theocharis G, Pagneux V 2021 J. Appl. Phys. 129 125108Google Scholar

    [31]

    Obana D, Liu F, Wakabayashi K 2019 Phys. Rev. B 100 075437Google Scholar

    [32]

    Lieu S 2018 Phys. Rev. B 97 045106Google Scholar

    [33]

    Yuce C, Ramezani H 2019 Phys. Rev. A 100 032102Google Scholar

    [34]

    Dangel F, Wagner M, Cartarius H, Main J, Wunner G 2018 Phys. Rev. A 98 013628Google Scholar

    [35]

    Bomantara R W, Zhou L, Pan J, Gong J 2019 Phys. Rev. B 99 045441Google Scholar

    [36]

    Xie B Y, Wang H F, Wang H X, Zhu X Y, Jiang J H, Lu M H, Chen Y F 2018 Phys. Rev. B 98 205147Google Scholar

    [37]

    Zhen B, Hsu C W, Lu L, Stone A D, Soljacic M 2014 Phys. Rev. Lett. 113 257401Google Scholar

    [38]

    Molina M I, Miroshnichenko A E, Kivshar Y S 2012 Phys. Rev. Lett. 108 070401Google Scholar

    [39]

    Weimann S, Xu Y, Keil R, Miroshnichenko A E, Tunnermann A, Nolte S, Sukhorukov A A, Szameit A, Kivshar Y S 2013 Phys. Rev. Lett. 111 240403Google Scholar

    [40]

    Benalcazar W A, Cerjan A 2020 Phys. Rev. B 101 161116Google Scholar

    [41]

    Benalcazar W A, Bernevig B A, Hughes T L 2017 Phys. Rev. B 96 245115Google Scholar

    [42]

    Hsu C W, Zhen B, Stone A D, Joannopoulos J D, Soljačić M 2016 Nat. Rev. Mater. 1 16048Google Scholar

    [43]

    Stillinger F H, Herrick D R 1975 Phys. Rev. A 11 446Google Scholar

    [44]

    Friedrich H, Wintgen D 1985 Phys. Rev. A:Gen Phys 32 3231Google Scholar

    [45]

    Marinica D C, Borisov A G, Shabanov S V 2008 Phys. Rev. Lett. 100 183902Google Scholar

    [46]

    Shipman S P, Venakides S 2005 Phys. Rev. E:Stat. Nonlinear Soft Matter Phys. 71 026611Google Scholar

    [47]

    Moiseyev N 2009 Phys. Rev. Lett. 102 167404Google Scholar

    [48]

    Plotnik Y, Peleg O, Dreisow F, Heinrich M, Nolte S, Szameit A, Segev M 2011 Phys. Rev. Lett. 107 183901Google Scholar

    [49]

    Lee J, Zhen B, Chua S L, Qiu W, Joannopoulos J D, Soljacic M, Shapira O 2012 Phys. Rev. Lett. 109 067401Google Scholar

    [50]

    Evans D V, Levitin M, Vassiliev D 2006 J. Fluid Mech. 261 21Google Scholar

    [51]

    Koshelev K, Lepeshov S, Liu M, Bogdanov A, Kivshar Y 2018 Phys. Rev. Lett. 121 193903Google Scholar

    [52]

    Liu F, Wakabayashi K 2017 Phys. Rev. Lett. 118 076803Google Scholar

    [53]

    Benalcazar W A, Bernevig B A, Hughes T L 2017 Science 357 61Google Scholar

    [54]

    Benalcazar W A, Li T H, Hughes T L 2019 Phys. Rev. B 99 245151Google Scholar

    [55]

    Li C A, Wu S S 2020 Phys. Rev. B 101 195309Google Scholar

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出版历程
  • 收稿日期:  2021-10-22
  • 修回日期:  2021-11-20
  • 上网日期:  2022-01-26
  • 刊出日期:  2022-04-05

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