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基于超绝热技术快速制备里德伯超级原子W态

杨丽萍 王纪平 董莉 修晓明 计彦强

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基于超绝热技术快速制备里德伯超级原子W态

杨丽萍, 王纪平, 董莉, 修晓明, 计彦强
cstr: 32037.14.aps.74.20241694

Rapid preparation of Rydberg superatom W state using superadiabatic techniques

YANG Liping, WANG Jiping, DONG Li, XIU Xiaoming, JI Yanqiang
cstr: 32037.14.aps.74.20241694
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  • W态作为一种具有鲁棒性的多体纠缠态, 在量子信息处理、量子网络构建以及量子计算等领域具有重要应用. 本文借助里德伯超级原子的有效能级进行编码, 运用超绝热迭代技术, 提出一种快速制备里德伯超级原子W态的方案. 该方案无需对实验参数和交互时间进行精确控制, 且其反绝热哈密顿量与有效哈密顿量形式相同. 数值模拟结果表明, 此方案不仅能够快速制备W态, 还具备较高的保真度和良好的实验可操作性. 进一步数值模拟分析显示, 在面对原子自发辐射和光子泄漏引发的退相干问题时, 该方案展现出较强的鲁棒性. 此外, 该方案可扩展至 N 个里德伯超级原子的情况, 这展示了该技术在大规模多体纠缠态制备中的潜力.
    The W state, as a robust multipartite entangled state, plays an important role in quantum information processing, quantum network construction and quantum computing. In this paper, a three-level ladder-type Rydberg atomic system is placed into a Rydberg blocking sphere to form a superatom. Each superatom has many collective states including just one Rydberg excitation constrained by the Rydberg blockade effect. In the weak cavity field limit, at most one atom can be pumped into excited state, then we can describe the superatom by using a three-level ladder-type system. Afterwards we encode quantum information about the effective energy levels of Rydberg superatoms and propose a fast scheme for preparing the Rydberg superatom W state based on the superadiabatic iterative technique and quantum Zeno dynamics.This scheme can be achieved in only one step by controlling the laser pulses. In this scheme, the superatoms are trapped in spatially separated cavities connected by optical fibers, thereby greatly improving the feasibility of experimental manipulation. A remarkable feature is that it does not need to accurately control experimental parameters and interaction time. Meanwhile, the form of counterdiabatic Hamiltonian is the same as that of the effective Hamiltonian. Through numerical simulations, the fidelity of this scheme can reach 99.94%. Even considering decoherence effects, including atomic spontaneous emission and photon leakage, the fidelity can still exceed 97.5%, thereby further demonstrating the strong robustness of the solution. In addition, the Rabi frequency can be characterized as a linear superposition of Gaussian functions, and this representation significantly alleviates the complexity encountered in practical experiments. Futhermore, we also analyze the influence of parameter fluctuations on the fidelity, and the results show that this scheme is robust against parameter fluctuations. Finally, the present scheme is extended to the case of N Rydberg superatoms, which shows the scalability of our scheme.
      通信作者: 计彦强, jiyanqiang@qymail.bhu.edu.cn
    • 基金项目: 国家自然科学基金(批准号: 11947078)、辽宁省自然科学基金(批准号: 2020-BS-234)和辽宁省教育厅基本科研项目(批准号: LJ212410167045, LJKZ1015)资助的课题.
      Corresponding author: JI Yanqiang, jiyanqiang@qymail.bhu.edu.cn
    • Funds: Project supported by the National Natural Science Foundation of China (Grant No. 11947078), the Natural Science Foundation of Liaoning Province, China (Grant No. 2020-BS-234), and the Department of Education of Liaoning Province, China (Grant Nos. LJ212410167045, LJKZ1015).
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  • 图 1  (a)单个里德伯原子能级结构图; (b)里德伯超级原子的等效能级结构图

    Fig. 1.  (a) Energy level structure diagram of a single Rydberg atom; (b) the equivalent energy level structure diagram of Rydberg superatom.

    图 2  里德伯超级原子与腔系统的示意图, SA是里德伯超级原子, $ \varOmega_k $是第k个腔中经典场的拉比频率

    Fig. 2.  Schematic diagram of the structure of the Rydberg superatom-cavity system, SA denots the Rydberg superatom, and $ \varOmega_k $ is the classical field Rabi frequency in the k-th cavity.

    图 3  $ \theta_1(t) $随时间的变化关系. 选取的参数为$ t_0 = 0.14 T $和$ t_{\mathrm{c}} = 0.19 T $

    Fig. 3.  The $ \theta_1(t) $ as a function of the time. The parameters $ t_0 = 0.14 T $ and $ t_{\mathrm{c}} = 0.19 T $.

    图 4  $ \theta_2(t) $随时间的变化关系. 选取的参数为$ t_0 = 0.14 T $和$ t_{\mathrm{c}} = 0.19 T $

    Fig. 4.  The $ \theta_2(t) $ as a function of the time. The parameters $ t_0 = 0.14 T $and $ t_{\mathrm{c}} = 0.19 T $.

    图 5  $ \varOmega_0(T^{-1}) $对保真度$ F(T) $的影响图. 当$ \varOmega_0 = 8 T^{-1} $时, 保真度$ F(T) = 0.9994 $

    Fig. 5.  The influence of $ \varOmega_0(T^{-1}) $ on fidelity $ F(T) $. When $ \varOmega_0 = 8 T^{-1} $, the fidelity $ F(T) = 0.9994 $.

    图 6  (a)对比脉冲$ \varOmega'_1(t) $和拟合的高斯脉冲$ \widetilde{\varOmega}_1(t) $; (b)对比脉冲$ \varOmega'_2(t) $和拟合的高斯脉冲$ \widetilde{\varOmega}_2(t) $

    Fig. 6.  (a) Comparing the pulse $ \varOmega '_1 (t) $ and the fitting of gaussian pulse $ \widetilde {\varOmega} _1 (t) $; (b) comparing the pulse $ \varOmega '_2 (t) $ and the fitting of gaussian pulse $ \widetilde {\varOmega} _2 (t) $.

    图 7  W态的保真度在超绝热迭代$ T = 8/\varOmega_0 $、绝热演化$ T = 8/\varOmega_0 $、绝热演化$ T = 35/\varOmega_0 $三种不同情况下随时间的变化

    Fig. 7.  Under the three different conditions: superadiabatic iteration $ T = 8/\varOmega_0 $, adiabatic evolution $ T = 8/\varOmega_0 $ and adiabatic evolution $ T = 35/\varOmega_0 $, the fidelity of W state as a function of the time.

    图 8  哈密顿量$ H_{{\mathrm{tot}}} $的控制下的W态的保真度与$ \kappa/\lambda $和$ \gamma/\lambda $的关系, $ T = 8/\varOmega_0, \varOmega_0 = 0.1\lambda $

    Fig. 8.  The relationship between the fidelity of the W state and $ \kappa/\lambda $, $ \gamma/\lambda $ by the Hamiltonian $ H_{{\mathrm{tot}}} $, $ T = 8 / \varOmega_0, $$ \varOmega_0 = 0.1\lambda $.

    图 9  (a)保真度随$ \delta \widetilde{\varOmega}_1 $和$ \delta \widetilde{\varOmega}_2 $的变化; (b)保真度随$ \delta \lambda $和$ \delta v $的变化

    Fig. 9.  (a) The fidelity versus $ \delta \widetilde{\varOmega}_1 $ and $ \delta \widetilde{\varOmega}_2 $; (b) the fidelity versus $ \delta \lambda $ and $ \delta v $.

    图 10  N个里德伯超级原子-腔系统结构型的示意图, 每个里德伯超级原子被分别放置在不同的真空腔中, 第2到第N个腔均与第1个腔相连, $ \varOmega_N $是第N个腔中经典场驱动的拉比频率

    Fig. 10.  Schematic diagram illustrating the structure of N-Rydberg superatom-cavity system, each of the Rydberg superatom is placed in a separate vacuum cavity, with cavities 2 through N all connected to cavity 1, $ \varOmega_N $ is the classical field-driven Rabi frequency in the N-th cavity.

  • [1]

    Gisin N, Ribordy G, Tittel W, Zbinden H 2002 Rev. Mod. Phys. 74 145Google Scholar

    [2]

    Markham D, Sanders B C 2008 Phys. Rev. A 78 042309Google Scholar

    [3]

    Bennett C H, Brassard G, Crépeau C, Jozsa R, Peres A, Wootters W K 1993 Phys. Rev. Lett. 70 1895Google Scholar

    [4]

    Luo Y H, Zhong H S, Erhard M, Wang X L, Peng L C, Krenn M, Jiang X, Li L, Liu N L, Lu C Y, Zeilinger A, Pan J W 2019 Phys. Rev. Lett. 123 070505Google Scholar

    [5]

    Xia Y, Song J, Lu P M, Song H S 2010 JOSA B 27 A1Google Scholar

    [6]

    Ekert A K 1991 Phys. Rev. Lett. 67 661Google Scholar

    [7]

    Bennett C H, Brassard G, Mermin N D 1992 Phys. Rev. Lett. 68 557Google Scholar

    [8]

    Long G L, Liu X S 2002 Phys. Rev. A 65 032302Google Scholar

    [9]

    Scarani V, Bechmann-Pasquinucci H, Cerf N J, Dušek M, Lütkenhaus N, Peev M 2009 Rev. Mod. Phys. 81 1301Google Scholar

    [10]

    Briegel H J, Browne D E, Dür W, Raussendorf R, Van den Nest M 2009 Nat. Phys. 5 19Google Scholar

    [11]

    Zhao P Z, Cui X D, Xu G, Sjöqvist E, Tong D 2017 Phys. Rev. A 96 052316Google Scholar

    [12]

    Su S L, Gao Y, Liang E, Zhang S 2017 Phys. Rev. A 95 022319Google Scholar

    [13]

    Wu J L, Su S L, Wang Y, Song J, Xia Y, Jiang Y Y 2020 Opt. Lett. 45 1200Google Scholar

    [14]

    Li X H, Deng F G, Zhou H Y 2006 Phys. Rev. A 74 054302Google Scholar

    [15]

    Zhu A D, Xia Y, Fan Q B, Zhang S 2006 Phys. Rev. A 73 022338Google Scholar

    [16]

    Li T, Long G L 2020 New J. Phys. 22 063017Google Scholar

    [17]

    Greenberger D M, Horne M A, Zeilinger A 1989 In Bell’s Theorem, Quantum Theory and Conceptions of the Universe (Springer) pp69–72

    [18]

    Shao X Q, Liu F, Xue X W, Mu W, Li W B 2023 Phys. Rev. Appl 20 014014Google Scholar

    [19]

    Dür W, Vidal G, Cirac J I 2000 Phys. Rev. A 62 062314Google Scholar

    [20]

    Cabello A 2002 Phys. Rev. A 65 032108Google Scholar

    [21]

    Agrawal P, Pati A 2006 Phys. Rev. A 74 062320Google Scholar

    [22]

    Wang A, Wei Y Z, Li Z Y, Jiang M 2023 IET Quantum Commun. 4 200Google Scholar

    [23]

    Renner R 2008 Int. J. Quantum Inf. 6 1Google Scholar

    [24]

    Lo H K, Ma X, Chen K 2005 Phys. Rev. Lett. 94 230504Google Scholar

    [25]

    Lipinska V, Murta G, Wehner S 2018 Phys. Rev. A 98 052320Google Scholar

    [26]

    Miguel-Ramiro J, Riera-Sàbat F, Dür W 2023 PRX Quantum 4 040323Google Scholar

    [27]

    Su S L, Shao X Q, Wang H F, Zhang S 2014 Phys. Rev. A 90 054302Google Scholar

    [28]

    Han J X, Wu J L, Wang Y, Xia Y, Jiang Y Y, Song J 2021 Phys. Rev. A 103 032402Google Scholar

    [29]

    Shao X Q, Wang Z, Liu H, Yi X 2016 Phys. Rev. A 94 032307Google Scholar

    [30]

    Shao X Q, Su S L, Li L, Nath R, Wu J H, Li W 2024 Appl. Phys. Rev. 11 031320Google Scholar

    [31]

    Shao Q P, Wang J, Ji Y, Liu Y, Dong L, Xiu X M 2023 J. Opt. Soc. Am. B 41 143Google Scholar

    [32]

    Zhang W Y, Wang C Q, Ji Y Q, Shao Q P, Wang J P, Wang J, Yang L P, Dong L, Xiu X M 2024 Adv. Quantum Technol. 7 2300140Google Scholar

    [33]

    Saffman M, Walker T G, Mølmer K 2010 Rev. Mod. Phys. 82 2313Google Scholar

    [34]

    Beguin L, Vernier A, Chicireanu R, Lahaye T, Browaeys A 2013 Phys. Rev. Lett. 110 263201Google Scholar

    [35]

    Xing T, Zhao P, Tong D 2021 Phys. Rev. A 104 012618Google Scholar

    [36]

    Lukin M D, Fleischhauer M, Cote R, Duan L, Jaksch D, Cirac J I, Zoller P 2001 Phys. Rev. Lett. 87 037901Google Scholar

    [37]

    Urban E, Johnson T A, Henage T, Isenhower L, Yavuz D, Walker T, Saffman M 2009 Nat. Phys. 5 110Google Scholar

    [38]

    Gaëtan A, Miroshnychenko Y, Wilk T, Chotia A, Viteau M, Comparat D, Pillet P, Browaeys A, Grangier P 2009 Nat. Phys. 5 115Google Scholar

    [39]

    Wilk T, Gaëtan A, Evellin C, Wolters J, Miroshnychenko Y, Grangier P, Browaeys A 2010 Phys. Rev. Lett. 104 010502Google Scholar

    [40]

    Dudin Y O, Li L, Bariani F, Kuzmich A 2012 Nat. Phys. 8 790Google Scholar

    [41]

    Shao X Q, Wu J, Yi X 2017 Phys. Rev. A 95 062339Google Scholar

    [42]

    Su S L, Li W 2021 Phys. Rev. A 104 033716Google Scholar

    [43]

    Wu J L, Wang Y, Han J X, Su S L, Xia Y, Jiang Y, Song J 2021 Phys. Rev. A 103 012601Google Scholar

    [44]

    Zeiher J, Schauß P, Hild S, Macrì T, Bloch I, Gross C 2015 Phys. Rev. X 5 031015Google Scholar

    [45]

    Yang L, Wang J, Ji Y, Wang J, Zhang Z, Liu Y, Dong L, Xiu X 2024 Eur. Phys. J. Plus 139 1Google Scholar

    [46]

    Xu W, Venkatramani A V, Cantú S H, Šumarac T, Klüsener V, Lukin M D, Vuletić V 2021 Phys. Rev. Lett. 127 050501Google Scholar

    [47]

    Zhao P Z, Wu X, Xing T, Xu G, Tong D 2018 Phys. Rev. A 98 032313Google Scholar

    [48]

    Paris-Mandoki A, Braun C, Kumlin J, Tresp C, Mirgorodskiy I, Christaller F, Büchler H P, Hofferberth S 2017 Phys. Rev. X 7 041010Google Scholar

    [49]

    Liu Y L, Ji Y Q, Han X, Cui W X, Zhang S, Wang H F 2023 Adv. Quantum Technol. 6 2200173Google Scholar

    [50]

    Baksic A, Ribeiro H, Clerk A A 2016 Phys. Rev. Lett. 116 230503Google Scholar

    [51]

    Wu J L, Ji X, Zhang S 2017 Sci. Rep. 7 46255Google Scholar

    [52]

    Chen Y H, Qin W, Wang X, Miranowicz A, Nori F 2021 Phys. Rev. Lett. 126 023602Google Scholar

    [53]

    Giannelli L, Arimondo E 2014 Phys. Rev. A 89 033419Google Scholar

    [54]

    王雪梅, 张安琪, 赵生妹 2022 物理学报 71 150301Google Scholar

    Wang X M, Zhang A Q, Zhao S M 2022 Acta Phys. Sin. 71 150301Google Scholar

    [55]

    Berry M V 2009 J. Phys. A: Math. Theor. 42 365303Google Scholar

    [56]

    Ibáñez S, Chen X, Muga J 2013 Phys. Rev. A 87 043402Google Scholar

    [57]

    Song X K, Ai Q, Qiu J, Deng F G 2016 Phys. Rev. A 93 052324Google Scholar

    [58]

    Huang B H, Chen Y H, Wu Q C, Song J, Xia Y 2016 Laser Phys. Lett. 13 105202Google Scholar

    [59]

    Wu J L, Su S L, Ji X, Zhang S 2017 Ann. Phys. 386 34Google Scholar

    [60]

    Löw R, Weimer H, Nipper J, Balewski J B, Butscher B, Büchler H P, Pfau T 2012 J. Phys. B: At., Mol. Opt. Phys. 45 113001Google Scholar

    [61]

    Su S L, Sun L N, Liu B J, Yan L L, Yung M H, Li W, Feng M 2023 Phys. Rev. Appl. 19 044007Google Scholar

    [62]

    Du F F, Fan Z G, Ren X M, Ma M, Liu W Y 2024 Chin. Phys. B 34 010303Google Scholar

    [63]

    Shao X Q 2020 Phys. Rev. A 102 053118Google Scholar

    [64]

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出版历程
  • 收稿日期:  2024-12-08
  • 修回日期:  2025-02-25
  • 上网日期:  2025-03-20

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