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具有巨型Rashba自旋劈裂和量子自旋霍尔效应的材料在自旋电子器件应用中具有重要意义. 基于第一性原理, 提出一种可以将巨型Rashba自旋劈裂和量子自旋霍尔效应实现完美共存的二维(two dimension, 2D)六角晶格材料H-Pb-Cl. 由于系统空间反转对称性的破坏和本征电场的存在, H-Pb-Cl的电子能带中出现了巨型Rashba自旋劈裂现象(αR = 3.78 eV·Å). 此外, H-Pb-Cl的Rashba自旋劈裂是可以随双轴应力(–16%—16%)调控的. 通过分析H-Pb-Cl的电子性质, 发现在H-Pb-Cl费米面附近有一个巨大的带隙(1.31 eV), 并且体系由于Pb原子的s-p轨道翻转使得拓扑不变量Z2 = 1, 这就表明H-Pb-Cl是一个具有巨大拓扑带隙的2D拓扑绝缘体. 我们的研究为探索和实现Rashba自旋劈裂和量子自旋霍尔效应的共存提供了一种优良的潜在候选材料.
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关键词:
- 二维拓扑绝缘体 /
- Rashba自旋劈裂 /
- 空间反演对称性 /
- 自旋轨道耦合
Rashba spin splitting and quantum spin Hall effect have attracted enormous interest due to their great significance in the application of spintronics. According to the first-principles calculation, we propose a two-dimensional hexagonal lattice material H-Pb-Cl, which realizes the coexistence of giant Rashba spin splitting and quantum spin Hall effect. Owing to the break of space inversion symmetry and the existence of intrinsic electric field, H-Pb-Cl has a huge Rashba spin splitting phenomenon (αR = 3.78 eV·Å), and the Rashba spin splitting of H-Pb-Cl(–16%—16%) can be adjusted by changing the biaxial stress. By analyzing the electronic properties of H-Pb-Cl, we find that H-Pb-Cl has a huge band gap near the Fermi surface (1.31 eV), and the topological invariant Z2 = 1 of the system is caused by the inversion of s-p orbit, which indicates that H-Pb-Cl is a two-dimensional topological insulator with a huge topological band gap, and the gap is large enough to observe the topological edge states at room temperature. In addition, we further consider the effect of BN and graphane substrates on the topological band gap of H-Pb-Cl by using the H-Pb-Cl (111)-(1×1) /BN (111)-(2×2) and H-Pb-Cl(1×1)/ graphane (2×2) system, and find that the lattice mismatch between H-Pb-Cl (5.395 Å) and BN (2.615 Å) and between H-Pb-Cl (5.395 Å) and graphane (2.575 Å) are about 3% and 4.5%, respectively. According to our calculation results, H-Pb-Cl still retains the properties of topological insulator under the effect of spin orbit coupling, and is not affected by BN nor graphane. Our results show that the nontrivial topological band gap of H-Pb-Cl can be well preserved under both biaxial stress effect and substrate effect. In addition, H-Pb-Cl can well retain the nontrivial topological band gap under the stress of –16%–16%, and thus there are many kinds of substrate materials used to synthesize this material, which is very helpful in successfully realizing preparation experimentally. Our research provides a promising candidate material for exploring and realizing the coexistence of Rashba spin splitting and quantum spin Hall effect. And the coexistence of giant Rashba spin splitting and quantum spin Hall effect greatly broadens the scope of potential applications of H-Pb-Cl in the field of spintronic devices.-
Keywords:
- two dimensional topological insulator /
- Rashba spin splitting /
- spatial inversion symmetry /
- spin orbit coupling
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图 2 采用PBE和HSE06的2D H-Pb-Cl的能带结构 (a), (c) 不考虑SOC; (b), (d)考虑SOC. 蓝点、红点和绿点分别表示Pb原子的s, px, y和pz轨道的投影权重. 图(b)中的插图表示的是费米面附近的能带劈裂现象
Fig. 2. The band structure of 2D H-Pb-Cl using PBE and HSE06: (a), (c) Without SOC; (b), (d) with SOC. Blue, red and green dots represent the contribution of s, px, y, pz orbitals of Pb atoms, respectively. The illustration in Figure (b) shows the band splitting near the Fermi surface.
图 4 (a) 无双轴应力作用下H-Pb-Cl的功函数, ∆Φ表示的是静电势差; (b) H-Pb-Cl的静电势差在双轴应力从–16% 到16%作用下的变化图
Fig. 4. (a) Work functions of H-Pb-Cl under 0 biaxial stress, where ∆Φ represents the electrostatic potential difference under different biaxial stresses; (b) the variations of electrostatic potential difference ∆Φ of H-Pb-Cl with the biaxial stress of –16% to 16%.
图 5 (a) 在双轴应力(–16%到16%)作用下H-Pb-Cl体系内的Rashba自旋劈裂系数αR的变化图; (b) H-Pb-Cl (1×1)/BN (2×2)的能带结构, 其中红色部分代表的是基底BN在能带中的贡献情况; (c) H-Pb-Cl (1×1)/石墨烷 (2×2), 其中紫色点线代表的是石墨烷在能带中的贡献情况
Fig. 5. (a) The variations of Rashba spin splitting αR of H-Pb-Cl with the biaxial stress of –16% to 16%; (b) band structure of H-Pb-Cl (1×1)/BN (2×2), with the red stars-lines contributed by BN substrate; (c) band structure of H-Pb-Cl (1×1)/graphane (2×2), with the purple dotted line contributed by graphane substrate.
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[1] Moore J E 2010 Nature 464 194Google Scholar
[2] Soumyanarayanan A, Reyren N, Fert A, Panagopoulos C 2016 Nature 539 509Google Scholar
[3] Feng Y, Jiang Q, Feng B J, Yang M, Xu T, Liu W J, Yang X F, Arita M, Schwier E F, Shimada K, Jeschke H O, Thomale R, Shi Y G, Wu X X, Xiao S Z, Qiao S, He S L 2019 Nat. Commun. 10 4765Google Scholar
[4] Lu J P, Yau J B, Shukla S P, Shayegan M 1998 Phys. Rev. Lett. 81 1282Google Scholar
[5] Kuhlen S, Schmalbuch K, Hagedorn M, Schlammes P, Patt M, Lepsa M, Guntherodt G, Beschoten B 2012 Phys. Rev. Lett. 109 146603Google Scholar
[6] Strecker K E, Partridge G B, Truscott A G, Hulet R G 2002 Nature 417 150Google Scholar
[7] Wang Z Y, Cheng X C, Wang B Z, Zhang J Y, Lu Y H, Yi C R, Niu S, Deng Y, Liu X J, Chen S, Pan J W 2021 Science 372 271Google Scholar
[8] Lu Y H, Wang B Z, Liu X J 2020 Sci. Bull. 65 2080Google Scholar
[9] Zezyulin D A, Konotop V V 2022 Phys. Rev. A 105 063323Google Scholar
[10] Xu Z C, Zhou Z, Cheng E H, Lang L J, Zhu S L 2022 Sci. Chin. Phys. Mech. Astron. 65 283011Google Scholar
[11] Zhao Q 2022 Mod. Phys. Lett. B 36 2250070
[12] Liu H, Zhang T, Wang K, Gao F, Xu G, Zhang X, Li S X, Cao G, Wang T, Zhang J, Hu X, Li H O, Guo G P 2022 Phys. Rev. Appl. 17 044052Google Scholar
[13] Smith L W, Chen H B, Chang C W, Wu C W, Lo S T, Chao S H, Farrer I, Beere H E, Griffiths J P, Jones G A C, Ritchie D A, Chen Y N, Chen T M 2022 Phys. Rev. Lett. 128 027701Google Scholar
[14] Dai X Y, Liu B Y 2022 Phys. Rev. A 105 043313Google Scholar
[15] Hai K, Wang Y F, Chen Q, Hai W H 2021 Sci. Rep. 11 18839Google Scholar
[16] Manchon A, Koo H C, Nitta J, Frolov S M, Duine R A 2015 Nat. Mater. 14 871Google Scholar
[17] 红兰, 戈君, 双山, 刘达权 2022 物理学报 71 016301Google Scholar
Hong L, Ge J, Shuang S, Liu D Q 2022 Acta. Phys. Sin. 71 016301Google Scholar
[18] Li Y, Ma X K, Zhai X K, Gao M N, Dai H T, Schumacher S, Gao T G 2022 Nat. Commun. 13 3785Google Scholar
[19] Ghosh D, Roy K, Maitra S, Kumar P 2022 J. Phys. Chem. Lett. 13 5
[20] Schlipf M, Giustino F 2021 Phys. Rev. Lett. 127 237601Google Scholar
[21] Zhu L, Zhang T, Chen G, Chen H 2018 Phys. Chem. Chem. Phys. 20 30133Google Scholar
[22] Awschalom D, Samarth N 2009 Physics 2 50Google Scholar
[23] Henk J, Hoesch M, Osterwalder J, Ernst A, Bruno P 2004 J. Phys. Condens. Matter 16 43
[24] Gong S J, Cai J, Yao Q F, Tong W Y, Wan X, Duan C G, Chu J H 2016 J. Appl. Phys. 119 125310Google Scholar
[25] Krupin O, Bihlmayer G, Starke K, Gorovikov S, Prieto J E, Dobrich K, Blügel S, Kaindl G R 2005 Phys. Rev. B 71 201403Google Scholar
[26] Koroteev Y M, Bihlmayer G, Gayone J E, Chulkov E V, Blugel S, Echenique P M, Hofmann 2004 Phys. Rev. Lett. 93 046403Google Scholar
[27] Vajna S, Simon E, Szilva A, Palotas K, Ujfalussy B, Szunyogh L 2012 Phys. Rev. B 85 075404
[28] Meier F, Dil H, Lobo-Checa J, Patthey L, Osterwalder J 2008 Phys. Rev. B 77 089902Google Scholar
[29] Ast C R, Henk J, Ernst A, Moreschini L, Falub M C, Pacile D, Bruno P, Kern K, Grioni M 2007 Phys. Rev. Lett. 98 186807Google Scholar
[30] Popović D, Reinert F, Hüfner S, Grigoryan V G, Springborg M, Cercellier H, Fagot-Revurat Y, Kierren B, Malterre D 2005 Phys. Rev. B 72 045419Google Scholar
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[32] 龚士静, 段纯刚 2015 物理学报 64 187103Google Scholar
Gong S J, Duan C G, 2015 Acta. Phys. Sin. 64 187103Google Scholar
[33] Peng Q, Lei Y, Deng X, Deng J, Wu G, Li J, He C, Zhong J 2022 Physica E 135 114944Google Scholar
[34] Sakano M, Bahramy M S, Katayama A, Shimojima T, Murakawa H, Kaneko Y, Malaeb W, Shin S, Ono K, Kumigashira H, Arita R, Nagaosa N, Hwang H Y, Tokura Y, Ishizaka K 2013 Phys. Rev. Lett. 110 107204Google Scholar
[35] Bahramy M S, Arita R, Nagaosa N 2011 Phys. Rev. B 84 041202
[36] Narayan A 2015 Phys. Rev. B 92 220101Google Scholar
[37] Xiang F X, Wang X L, Veldhorst M, Dou S X, Fuhrer M S 2015 Phys. Rev. B 92 035123Google Scholar
[38] Krempaský J, Volfova H, Muff S, Pilet N, Landolt G, Radovic M, Shi M, Kriegner D, Holy V, Braun J, Ebert H, Bisti F, Rogalev V A, Strocov V N, Springholz G, Minar J, Dil J H 2016 Phys. Rev. B 94 205111Google Scholar
[39] Di Sante D, Barone P, Bertacco R, Picozzi S 2013 Adv. Mater. 25 509Google Scholar
[40] Ishizaka K, Bahramy M S, Murakawa H, Sakano M, Shimojima T, Sonobe T, Koizumi K, Shin S, Miyahara H, Kimura A, Miyamoto K, Okuda T, Namatame H, Taniguchi M, Arita R, Nagaosa N, Kobayashi K, Murakami Y, Kumai R, Kaneko Y, Onose Y, Tokura Y 2011 Nat. Mater. 10 521Google Scholar
[41] Krempaský J, Muff S, Min´ar J, Pilet N, Fanciulli M, Weber A P, Guedes E B, Caputo M, Müller E, Volobuev V V, Gmitra M, Vaz C A F, Scagnoli V, Springholz G, Dil J H 2018 Phys. Rev. X 8 021067
[42] Bernevig B A, Hughes T L, Zhang S C 2006 Science 314 1757Google Scholar
[43] Knez I, Du R R, Sullivan G 2012 Phys. Rev. Lett. 109 186603Google Scholar
[44] Liu W J, Xiong X L, Liu M L, Xing X W, Chen H L, Ye H, Han J F, Wei Z Y 2022 Appl. Phys. Lett. 120 053108Google Scholar
[45] Yang M, Liu Y D, Zhou W, Liu C, Mu D, Liu Y N, Wang J O, Hao W C, Li J, Zhong J X, Du Y, Zhuang J C 2022 ACS Nano 16 2
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[49] Zhao H, Zhang C W, Ji W X, Zhang R W, Li S S, Yan S S, Zhang B M, Li P, Wang P J 2016 Sci. Rep. 6 20152Google Scholar
[50] Zhou L, Kou L, Sun Y, Felser C, Hu F, Shan G, Smith S C, Yan B, Frauenheim T 2015 Nano Lett. 15 7867Google Scholar
[51] Weng H, Dai X, Fang Z 2014 Phys. Rev. X 4 011002
[52] Li X, Ying D, Ma Y, Wei W, Lin Y, Huang B 2015 Nano Res. 8 2954Google Scholar
[53] Luo W, Xiang H 2015 Nano Lett. 15 3230Google Scholar
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[55] Guo Z P, Yan D Y, Sheng H H, Nie S M, Shi Y G, Wang Z J 2021 Phys. Rev. B 103 115145Google Scholar
[56] Wang X, Wan W H, Ge Y F, Zhang K C, Liu Y 2022 Physica E 143 115325Google Scholar
[57] Perez M N R, Villaos R A B, Feng L Y, Maghirang A B, Cheng C P, Huang Z Q, Hsu C H, Bansil A, Chuang F C 2022 Appl. Phys. Rev. 9 011410Google Scholar
[58] Li J, He C Y, Xiao H P, Tang C, Wei X L, Kim J, Kioussis N, Stocks M, Zhong J X 2015 Sci. Rep. 5 14115Google Scholar
[59] Yuhara J, He B, Matsunami N, Nakatake M, Le Lay G 2019 Adv. Mater. 31 e1901017Google Scholar
[60] Kresse G, Furthmüller J 1996 Phys. Rev. B 54 11169Google Scholar
[61] Perdew J P, Burke K, Ernzerhof M 1998 Phys. Rev. Lett. 77 3865
[62] Mostofi A A, Yates J R, Lee Y S, Souza I, Vanderbilt D, Marzari N 2008 Comput. Phys. Commun. 178 685Google Scholar
[63] Wu Q S, Zhang S N, Song H F, Troyer M, Soluyanov A A 2018 Comput. Phys. Commun. 224 405Google Scholar
[64] Togo A, Oba F, Tanaka I 2008 Phys. Rev. B 78 134106Google Scholar
[65] Kane C L, Mele E J 2005 Phys. Rev. Lett. 95 226801Google Scholar
[66] Kane C L, Mele E J 2005 Phys. Rev. Lett. 95 146802Google Scholar
[67] Zhang H J, Liu C X, Qi X L, Dai X, Fang Z, Zhang S C 2009 Nat. Phys. 5 438Google Scholar
[68] König M, Wiedmann S, Brüne C, Roth A, Buhmann H, W. Molenkamp L, Qi X L, Zhang S C 2007 Science 318 766Google Scholar
[69] Liu Q, Guo Y, Freeman A 2013 Nano Lett. 13 5264Google Scholar
[70] Gong Q, Zhang G L 2022 Int. J. Mol. Sci. 23 7629Google Scholar
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