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

超级里德伯原子间的稳态关联集体激发与量子纠缠

白健男 韩嵩 陈建弟 韩海燕 严冬

引用本文:
Citation:

超级里德伯原子间的稳态关联集体激发与量子纠缠

白健男, 韩嵩, 陈建弟, 韩海燕, 严冬

Correlated collective excitation and quantum entanglement between two Rydberg superatoms in steady state

Bai Jian-Nan, Han Song, Chen Jian-Di, Han Hai-Yan, Yan Dong
PDF
HTML
导出引用
  • 处于同一偶极阻塞区域的里德伯原子系综可以看作一个超级原子, 如果它们被捕获在两个不同的光偶极阱中, 那么每一个光偶极阱中的子原子系综可以看作为一个亚超级原子. 由于这两个亚超级原子共享不超过一个激发的里德伯原子, 所以它们会强烈地关联起来. 本文研究这两个里德伯亚超级原子的稳态关联集体激发特性和量子纠缠行为. 结果表明原子数目带来的影响非常明显: 里德伯亚超级原子越大(包含原子数目越多), 集体激发概率越大; 最大纠缠只发生在等大的两个里德伯亚超级原子之间. 通过增加原子数目, 可以实现介观领域的量子纠缠, 对量子-经典对应的研究以及量子信息处理有着重要的作用.
    Owing to the unique physical characteristics of Rydberg atoms, which play an important role in quantum information and quantum computation, the theoretical and applied research of Rydberg atoms have become the hot spots of scientific research in recent years. With the large polarizability of Rydberg atoms, even a small electric field could cause a considerable electric dipole moment, resulting in a strong dipole-dipole interaction between Rydberg atoms. The multiple excitations of the Rydberg states are strongly inhibited because of the strong dipole interaction between atoms within a mesoscopic interaction (blockade) region. We call this phenomenon the dipole blockade effect. The dipole blockade effect makes it possible to build single-photon quantum devices, implement quantum gates, generate quantum entanglement, and simulate many-body quantum problems, etc.A Rydberg atomic ensemble in the same blockade region can be regarded as a superatom. In the same way, if these atoms trapped in two optical dipole traps, each sub-ensemble can be considered as a sub-superatom which is closely related to the superatom. According to the fact that two Rydberg sub-superatoms can be strongly correlated due to sharing no more than one excited Rydberg atom, we study correlated collective excitation and quantum entanglement between two Rydberg sub-superatoms in a steady state. With the superatom model, the problem of exponentially increasing system size with the number of atoms can be circumvented to a certain extent in studying many-body physics. By solving the two-body Lindblad’s master equation accurately, we obtain the analytical expressions for the collective excitation probabilities of the two sub-superatoms, and the concurrence measuring the bipartite entanglement between them. Our results show that they are all sensitive to the number of atoms in each Rydberg superatom: the bigger (including more atoms) the Rydberg superatom, the higher the collective Rydberg excitation probability is. And that the maximally entangled state can only be obtained with two equal-sized Rydberg superatoms. When this condition is fulfilled, the mesoscopic entanglement can be generated by adding the number of atoms in each Rydberg superatom. This may provide an attractive platform for studying the quantum-classical correspondence and have potential promising applications in quantum information processing.
      通信作者: 严冬, ydbest@126.com
    • 基金项目: 国家自然科学基金(批准号: 11874004, 11204019)、吉林省教育厅科学基金(批准号: JJKH20200557KJ)、吉林省科技厅自然科学基金(批准号: 20210101411JC)和长春大学基金资助的课题.
      Corresponding author: Yan Dong, ydbest@126.com
    • Funds: Project supported by the National Natural Science Foundation of China (Grant Nos. 11874004, 11204019), the Science Foundation of Education Department of Jilin Province, China (Grant No. JJKH20200557KJ), the Nature Science Foundation of Science and Technology Department of Jilin Province, China (Grant No. 20210101411JC), and the Science Foundation of Changchun University, China.
    [1]

    Martin G 2015 Phys. Rev. A 92 013629Google Scholar

    [2]

    Zhou M T, Liu J T, Sun P F, An Z Y, Li J, Bao X H, Pan J W 2020 Phys. Rev. A 102 013706Google Scholar

    [3]

    Pitalúa-García D 2013 Phys. Rev. Lett. 110 210402Google Scholar

    [4]

    Rao D D B, Klaus M 2014 Phys. Rev. A 89 030301Google Scholar

    [5]

    Gorniaczyk H, Tresp C, Schmidt J, Fedder H, Hofferberth S 2014 Phys. Rev. Lett. 113 053601Google Scholar

    [6]

    David P, Georgios M N 2014 Phys. Rev. A 89 013419Google Scholar

    [7]

    Li D X, Shao X Q 2018 Phys. Rev. A 98 062338Google Scholar

    [8]

    Mario B, Fernando G, Brandão S L 2018 Phys. Rev. Lett. 121 040504Google Scholar

    [9]

    Feng D, Hu X Y 2020 Phys. Rev. A 102 042404Google Scholar

    [10]

    Dong Y, Zhang S Y, Wang Y, Duan L M, Deng D L 2022 Phys. Rev. R 4 023095Google Scholar

    [11]

    Zhang C H, Peter G, Wolynes, Martin G 2022 Phys. Rev. A 105 033322Google Scholar

    [12]

    Parmee C D, Cooper N R 2018 Phys. Rev. A 97 053616Google Scholar

    [13]

    Bhaktavatsala R D D, Klaus M 2014 Phys. Rev. A 90 062319Google Scholar

    [14]

    Thomas M, Ivana V, Michael J H, Walter H 2016 Phys. Rev. A 94 013809Google Scholar

    [15]

    Soriente M, Donner T, Chitra R, Zilberberg O 2018 Phys. Rev. Lett. 120 183603Google Scholar

    [16]

    Stanojevic J, Côté R 2009 Phys. Rev. A 80 033418Google Scholar

    [17]

    Johannes Z, Peter S, Sebastian H 2015 Phys. Rev. X 5 031015Google Scholar

    [18]

    Fabian L 2017 New J. Phys. 19 113014Google Scholar

    [19]

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

    [20]

    Asaf P, Christoph B, Jan K, Christoph T, Ivan M 2017 Phys. Rev. X 7 041010Google Scholar

    [21]

    Luo Y H, Zhong H S, Manuel E, Wang X L, Peng L, Mario K, Xiao J, Li L, Liu N L, Lu C Y, Anton Z, Pan J W 2019 Phys. Rev. Lett. 123 070505Google Scholar

    [22]

    Nicolas G, Grégoire R, Wolfgang T, Hugo Z 2002 Rev. Mod. Phys. 74 145Google Scholar

    [23]

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

    [24]

    Damian M, Barry C S 2008 Phys. Rev. A 78 042309Google Scholar

    [25]

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

    [26]

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

    [27]

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

    [28]

    Robert R, Daniel E, Browne Hans J, Briegel 2003 Phys. Rev. A 68 022312Google Scholar

    [29]

    James A P, Zhang Y T, Gennady P B, Sabre K 2013 Phys. Rev. E 87 062704Google Scholar

    [30]

    Li T, Yin Z Q 2016 Sci. Bull. 61 163Google Scholar

    [31]

    Horodecki R, Horodecki P, Horodecki M, Horodecki K 2009 Rev. Mo. Phys. 81 865Google Scholar

    [32]

    Deng D L, Li X, Das Sarma S 2017 Phys. Rev. X 7 021021Google Scholar

    [33]

    Ji Y Q, Liu Y L, Zhou S J, Xiu X M, Dong L, Dong H K, Gao Y J, Yi X X 2019 Phys. Rev. A 99 023808Google Scholar

    [34]

    Wang T J, Lu Y, Long G L 2012 Phys. Rev. A 86 042337Google Scholar

    [35]

    Kiesel N, Schmid C, Tóth G, Solano E, Weinfurter H 2007 Phys. Rev. Lett. 98 063604Google Scholar

    [36]

    Nicolas L 2016 Phys. Rep. 6 008Google Scholar

    [37]

    Maksym K, Cao J S 2005 Phys. Rev. Lett. 95 180405Google Scholar

    [38]

    Salcedo L L 2012 Phys. Rev. A 85 022127Google Scholar

    [39]

    Yan D, Bai W J, Bai J N, Chen L, Han H Y, Wu J H 2022 Photonics 9 242Google Scholar

  • 图 1  (a)二能级里德伯原子的能级结构. 基态$ \left| g \right\rangle $和里德伯态$ \left| r \right\rangle $通过单模激光场($ \varOmega $为拉比频率; $ \varDelta $为单光子失谐)耦合, 两个同时激发到里德伯态的原子之间存在范德瓦耳斯势(vdW)相互作用. (b)处于同一偶极阻塞区域但是捕获在两个光偶极阱中的原子系综最多共享一个里德伯原子(红色小球). (c)里德伯超级原子的能级结构. 整个原子系综可以看作一个里德伯超级原子(左图), 而两个光偶极阱中的子原子系综(原子数目分别为$ {n_1} $$ {n_2} $)可以看作是较小的两个亚里德伯超级原子(右图). 右图中有效拉比频率分别为${\varOmega _1} = $$ \sqrt {{n_1}} ( {1 - \langle {{{\hat \varSigma }_{{R_2}{R_2}}}} \rangle } )\varOmega$${\varOmega _2} = \sqrt {{n_2}} ( {1 - \langle {{{\hat \varSigma }_{{R_1}{R_1}}}} \rangle } )\varOmega$, 这里$ \left\langle \cdot \right\rangle $代表任意量子态的平均值

    Fig. 1.  (a) Level structure of a two-level Rydberg atom, the ground state $ \left| g \right\rangle $ and the Rydberg state $ \left| r \right\rangle $ are coupled by the single-mode field with Rabi frequency $ \varOmega $ and single-photon detuning $ \varDelta $. Two Rydberg atoms interact via a van der Waals (vdW) potential. (b) All atoms are loaded in two optical dipole traps but in the same the blockade region represented by big green circle. The red pellet denotes an atom excited to the Rydberg state. (c) Level structures of a superatom containing $ n $ atoms and a sub superatom containing $ {n_1} $ ($ {n_2} $) atoms, respectively. They represent the whole atomic ensemble, and the sub-ensemble of $ {n_1} $ ($ {n_2} $) atoms trapped in one optical dipole trap.

    图 2  $ \varOmega /\gamma = 2.0 $, $ \varDelta = 0 $时, 稳态超级原子和亚超级原子激发概率 $ P $, $ {P_1} $, $ {P_2} $以及并发纠缠C作为(a)亚超级原子中数目$ {n_1} $($ n = {n_1} + {n_2} = 42 $保持不变)和(b)总原子数$ n $(其$ {n_2} - {n_1} = 1 $保持不变)的函数

    Fig. 2.  Steady-state excitation probabilities of superatoms, sub-superatom $ P $, $ {P_1} $, $ {P_2} $ and the concurrence C as a function of the number $ {n_1} $ for fixed $ n = {n_1} + {n_2} = 42 $ (a) and the total number $ n $ of atoms for fixed $ {n_2} - {n_1} = 1 $ (b) with $ \varOmega /\gamma = 2.0 $, $ \varDelta = 0 $.

    图 3  $ \varDelta = 0 $时, 稳态亚超级原子激发概率$ {P_1} $, $ {P_2} $以及并发纠缠C作为$ \varOmega /\gamma $的函数(绿色实心圆点和粉色正方形点代表$ C = 0.15 $) (a)$ {n_1} = 1 $, $ {n_2} = 41 $; (b)$ {n_1} = 21 $, $ {n_2} = 21 $; (c)$ {n_1} = 41 $, $ {n_2} = 1 $

    Fig. 3.  Steady-state excitation probabilities of sub-superatoms $ {P_1} $, $ {P_2} $ and the concurrence C as a function of $ \varOmega /\gamma $ with $ \varDelta = 0 $: (a)$ {n_1} = 1 $, $ {n_2} = 41 $; (b)$ {n_1} = 21 $, ${n_2} = $$ 21$; (c)$ {n_1} = 41 $, $ {n_2} = 1 $.

    图 4  $ \varOmega /\gamma = 0.2 $(第一行)和$ \varOmega /\gamma = 2 $(第二行)下, 稳态亚超级原子激发概率$ {P_1} $, $ {P_2} $以及并发纠缠$ C $作为$ \varDelta /\gamma $的函数 (a1), (a2)$ {n_1} = 1 $, $ {n_2} = 41 $; (b1), (b2)$ {n_1} = 21 $, $ {n_2} = 21 $; (c1), (c2) $ {n_1} = 41 $, $ {n_2} = 1 $

    Fig. 4.  Steady-state excitation probabilities of sub-superatoms $ {P_1} $, $ {P_2} $ and the concurrence $ C $ as a function of $ \varDelta /\gamma $ with $ \varOmega /\gamma = 0.2 $ (the first row) and $ \varOmega /\gamma = 2 $(the second row): (a1), (a2)$ {n_1} = 1 $, $ {n_2} = 41 $; (b1), (b2)$ {n_1} = 21 $, $ {n_2} = 21 $; (c1), (c2)$ {n_1} = 41 $, $ {n_2} = 1 $.

    图 5  (a1)—(c1) $ \varDelta = 0 $时, 稳态亚超级原子激发概率$ {P_1} $, $ {P_2} $以及并发纠缠$ C $作为$ \varOmega /\gamma $$ {n_1} $函数; (a2)—(c2)$ \varOmega /\gamma = 2 $时, 稳态亚超级原子激发概率$ {P_1} $, $ {P_2} $以及并发纠缠$ C $作为$ \varDelta /\gamma $$ {n_1} $函数; (c1), (c2) 红色截面代表$ C \equiv 0.15 $的平面, 其他参数$ n = 42 $

    Fig. 5.  (a1)–(c1) Steady-state excitation probabilities of sub-superatoms $ {P_1} $, $ {P_2} $ and the concurrence $ C $ as a function of $ \varOmega /\gamma $ and $ {n_1} $with $ \varDelta = 0 $; (a2)–(c2) the steady-state excitation probabilities of sub-superatoms $ {P_1} $, $ {P_2} $ and the concurrence $ C $ as a function of $ \varDelta /\gamma $ and $ {n_1} $ with $ \varOmega /\gamma = 2 $; (c1), (c2) the red cross sections in panel (c1) and (c2) denote $ C \equiv 0.15 $, other parameter is $ n = 42 $.

  • [1]

    Martin G 2015 Phys. Rev. A 92 013629Google Scholar

    [2]

    Zhou M T, Liu J T, Sun P F, An Z Y, Li J, Bao X H, Pan J W 2020 Phys. Rev. A 102 013706Google Scholar

    [3]

    Pitalúa-García D 2013 Phys. Rev. Lett. 110 210402Google Scholar

    [4]

    Rao D D B, Klaus M 2014 Phys. Rev. A 89 030301Google Scholar

    [5]

    Gorniaczyk H, Tresp C, Schmidt J, Fedder H, Hofferberth S 2014 Phys. Rev. Lett. 113 053601Google Scholar

    [6]

    David P, Georgios M N 2014 Phys. Rev. A 89 013419Google Scholar

    [7]

    Li D X, Shao X Q 2018 Phys. Rev. A 98 062338Google Scholar

    [8]

    Mario B, Fernando G, Brandão S L 2018 Phys. Rev. Lett. 121 040504Google Scholar

    [9]

    Feng D, Hu X Y 2020 Phys. Rev. A 102 042404Google Scholar

    [10]

    Dong Y, Zhang S Y, Wang Y, Duan L M, Deng D L 2022 Phys. Rev. R 4 023095Google Scholar

    [11]

    Zhang C H, Peter G, Wolynes, Martin G 2022 Phys. Rev. A 105 033322Google Scholar

    [12]

    Parmee C D, Cooper N R 2018 Phys. Rev. A 97 053616Google Scholar

    [13]

    Bhaktavatsala R D D, Klaus M 2014 Phys. Rev. A 90 062319Google Scholar

    [14]

    Thomas M, Ivana V, Michael J H, Walter H 2016 Phys. Rev. A 94 013809Google Scholar

    [15]

    Soriente M, Donner T, Chitra R, Zilberberg O 2018 Phys. Rev. Lett. 120 183603Google Scholar

    [16]

    Stanojevic J, Côté R 2009 Phys. Rev. A 80 033418Google Scholar

    [17]

    Johannes Z, Peter S, Sebastian H 2015 Phys. Rev. X 5 031015Google Scholar

    [18]

    Fabian L 2017 New J. Phys. 19 113014Google Scholar

    [19]

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

    [20]

    Asaf P, Christoph B, Jan K, Christoph T, Ivan M 2017 Phys. Rev. X 7 041010Google Scholar

    [21]

    Luo Y H, Zhong H S, Manuel E, Wang X L, Peng L, Mario K, Xiao J, Li L, Liu N L, Lu C Y, Anton Z, Pan J W 2019 Phys. Rev. Lett. 123 070505Google Scholar

    [22]

    Nicolas G, Grégoire R, Wolfgang T, Hugo Z 2002 Rev. Mod. Phys. 74 145Google Scholar

    [23]

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

    [24]

    Damian M, Barry C S 2008 Phys. Rev. A 78 042309Google Scholar

    [25]

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

    [26]

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

    [27]

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

    [28]

    Robert R, Daniel E, Browne Hans J, Briegel 2003 Phys. Rev. A 68 022312Google Scholar

    [29]

    James A P, Zhang Y T, Gennady P B, Sabre K 2013 Phys. Rev. E 87 062704Google Scholar

    [30]

    Li T, Yin Z Q 2016 Sci. Bull. 61 163Google Scholar

    [31]

    Horodecki R, Horodecki P, Horodecki M, Horodecki K 2009 Rev. Mo. Phys. 81 865Google Scholar

    [32]

    Deng D L, Li X, Das Sarma S 2017 Phys. Rev. X 7 021021Google Scholar

    [33]

    Ji Y Q, Liu Y L, Zhou S J, Xiu X M, Dong L, Dong H K, Gao Y J, Yi X X 2019 Phys. Rev. A 99 023808Google Scholar

    [34]

    Wang T J, Lu Y, Long G L 2012 Phys. Rev. A 86 042337Google Scholar

    [35]

    Kiesel N, Schmid C, Tóth G, Solano E, Weinfurter H 2007 Phys. Rev. Lett. 98 063604Google Scholar

    [36]

    Nicolas L 2016 Phys. Rep. 6 008Google Scholar

    [37]

    Maksym K, Cao J S 2005 Phys. Rev. Lett. 95 180405Google Scholar

    [38]

    Salcedo L L 2012 Phys. Rev. A 85 022127Google Scholar

    [39]

    Yan D, Bai W J, Bai J N, Chen L, Han H Y, Wu J H 2022 Photonics 9 242Google Scholar

  • [1] 张学超, 乔佳慧, 刘瑶, 苏楠, 刘智慧, 蔡婷, 何军, 赵延霆, 王军民. 基于里德伯原子天线的低频电场波形测量. 物理学报, 2024, 73(7): 070201. doi: 10.7498/aps.73.20231778
    [2] 刘瑶, 何军, 苏楠, 蔡婷, 刘智慧, 刁文婷, 王军民. 用于铯原子里德伯态激发的509 nm波长脉冲激光系统. 物理学报, 2023, 72(6): 060303. doi: 10.7498/aps.72.20222286
    [3] 王勤霞, 王志辉, 刘岩鑫, 管世军, 何军, 张鹏飞, 李刚, 张天才. 腔增强热里德伯原子光谱. 物理学报, 2023, 72(8): 087801. doi: 10.7498/aps.72.20230039
    [4] 王鑫, 任飞帆, 韩嵩, 韩海燕, 严冬. 里德伯原子辅助光力系统的完美光力诱导透明及慢光效应. 物理学报, 2023, 72(9): 094203. doi: 10.7498/aps.72.20222264
    [5] 高洁, 杭超. 里德伯原子中非厄米电磁诱导光栅引起的弱光孤子偏折及其操控. 物理学报, 2022, 71(13): 133202. doi: 10.7498/aps.71.20220456
    [6] 吴逢川, 林沂, 武博, 付云起. 里德伯原子的射频脉冲响应特性. 物理学报, 2022, 71(20): 207402. doi: 10.7498/aps.71.20220972
    [7] 白文杰, 严冬, 韩海燕, 华硕, 谷开慧. 三体里德堡超级原子的关联动力学研究. 物理学报, 2022, 71(1): 014202. doi: 10.7498/aps.71.20211284
    [8] 赵嘉栋, 张好, 杨文广, 赵婧华, 景明勇, 张临杰. 基于里德伯原子电磁诱导透明效应的光脉冲减速. 物理学报, 2021, 70(10): 103201. doi: 10.7498/aps.70.20210102
    [9] 高小苹, 梁景睿, 刘堂昆, 李宏, 刘继兵. 巨梯型四能级里德伯原子系统透射光谱性质的调控. 物理学报, 2021, 70(11): 113201. doi: 10.7498/aps.70.20202077
    [10] 计彦强, 王洁, 刘颖莉, 张大伟, 肖瑞杰, 董莉, 修晓明. 基于里德伯超级原子快速制备三粒子单重态. 物理学报, 2021, 70(12): 120301. doi: 10.7498/aps.70.20201841
    [11] 金钊, 李芮, 公卫江, 祁阳, 张寿, 苏石磊. 基于共振里德伯偶极-偶极相互作用的双反阻塞机制及量子逻辑门的实现. 物理学报, 2021, 70(13): 134202. doi: 10.7498/aps.70.20210059
    [12] 严冬, 王彬彬, 白文杰, 刘兵, 杜秀国, 任春年. 里德伯电磁感应透明中的相位. 物理学报, 2019, 68(8): 084203. doi: 10.7498/aps.68.20181938
    [13] 张秦榕, 王彬彬, 张孟龙, 严冬. 稀薄里德伯原子气体中的两体纠缠. 物理学报, 2018, 67(3): 034202. doi: 10.7498/aps.67.20172052
    [14] 丛美艳, 杨晶, 黄燕霞. 在不同初态下Dzyaloshinskii-Moriya相互作用及内禀退相干对海森伯系统的量子纠缠的影响. 物理学报, 2016, 65(17): 170301. doi: 10.7498/aps.65.170301
    [15] 卢道明. 腔外原子操作控制腔内原子的纠缠特性. 物理学报, 2010, 59(12): 8359-8364. doi: 10.7498/aps.59.8359
    [16] 陈宇, 邹健, 李军刚, 邵彬. 耗散环境下三原子之间稳定纠缠的量子反馈控制. 物理学报, 2010, 59(12): 8365-8370. doi: 10.7498/aps.59.8365
    [17] 赵建明, 张临杰, 李昌勇, 贾锁堂. 里德伯原子向超冷等离子体的自发转化. 物理学报, 2008, 57(5): 2895-2898. doi: 10.7498/aps.57.2895
    [18] 单传家, 夏云杰. Tavis-Cummings模型中两纠缠原子纠缠的演化特性. 物理学报, 2006, 55(4): 1585-1590. doi: 10.7498/aps.55.1585
    [19] 胡要花, 方卯发, 廖湘萍, 郑小娟. 二项式光场与级联三能级原子的量子纠缠. 物理学报, 2006, 55(9): 4631-4637. doi: 10.7498/aps.55.4631
    [20] 王成志, 方卯发. 双模压缩真空态与原子相互作用中的量子纠缠和退相干. 物理学报, 2002, 51(9): 1989-1995. doi: 10.7498/aps.51.1989
计量
  • 文章访问数:  1658
  • PDF下载量:  64
  • 被引次数: 0
出版历程
  • 收稿日期:  2022-10-22
  • 修回日期:  2023-04-18
  • 上网日期:  2023-04-26
  • 刊出日期:  2023-06-20

/

返回文章
返回