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Spin Hall and spin Nernst effects in graphene with intrinsic and Rashba spin-orbit interactions |
Zhu Guo-Bao (朱国宝 ) |
Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China |
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Abstract Spin Hall and spin Nernst effects in graphene are studied based on Green's function formalism. We calculate intrinsic contributions to spin Hall and spin Nernst conductivities in Kane-Mele model with various structures. When both intrinsic and Rashba spin-orbit interactions are present, their interplay leads to some characteristics of the dependence of spin Hall and spin Nernst conductivities on the Fermi level. When Rashba spin-orbit interaction is smaller than intrinsic spin-orbit coupling, a weak kink in the conductance appears. The kink disappears and a divergence appears when the Rashba spin-orbit interaction enhances. When the Rashba spin-orbit interaction approaches and is stronger than intrinsic spin-orbit coupling, the divergence becomes more obvious.
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Received: 30 March 2012
Revised: 04 June 2012
Accepted manuscript online:
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PACS:
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73.43.-f
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(Quantum Hall effects)
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73.20.Hb
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(Impurity and defect levels; energy states of adsorbed species)
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73.61.Wp
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(Fullerenes and related materials)
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Fund: Project supported by the National Natural Science Foundation of China (Grant No. 10934010), and the National Key Basic Research Special Foundation of China (Grant Nos. 2011CB921502 and 2012CB821305). |
Corresponding Authors:
Zhu Guo-Bao
E-mail: zhuguobao@gmail.com
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Cite this article:
Zhu Guo-Bao (朱国宝 ) Spin Hall and spin Nernst effects in graphene with intrinsic and Rashba spin-orbit interactions 2012 Chin. Phys. B 21 117309
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[1] |
Hirsch J E 1999 Phys. Rev. Lett. 83 1834
|
[2] |
Murakami S, Nagaosa N and Zhang S C 2003 Science 301 1348
|
[3] |
Sinova J, Culcer D, Niu Q, Sinitsyn N A, Jungwirth T and MacDonald A H 2004 Phys. Rev. Lett. 92 126603
|
[4] |
Kato Y K, Myers R C, Gossard A C and Awschalom D D 2004 Science 306 1910
|
[5] |
Kimura T and Otani Y 2007 Phys. Rev. Lett. 99 196604
|
[6] |
Brüne C, Roth A, Novik E G, König M, Buhmann H, Hankiewicz E M, Hanke W, Sinova J and Molenkamp L W 2010 Nature Phys. 6 448
|
[7] |
Berry M V 1984 Proc. R. Soc. London Ser. B 392 45
|
[8] |
Sundaram G and Niu Q 1999 Phys. Rev. B 59 14915
|
[9] |
Uchida K, Takahashi S, Harii K, Ieda J, Koshibae W, Ando K, Meakawa S and Saitoh E 2008 Nature 455 778
|
[10] |
Jaworski C M, Yang J, Mack S, Awschalom D D, Heremans J P and Myers R C 2010 Nature Mater. 9 898
|
[11] |
Xiao D, Yao Y, Fang Z and Niu Q 2006 Phys. Rev. Lett. 97 026603
|
[12] |
Novoselov K S, Geim A K, Morozov S V, Jiang D, Zhang Y, Dubonos S V, Grigorieva I V and Firsov A A 2004 Science 306 666
|
[13] |
Kane C L and Mele E J 2005 Phys. Rev. Lett. 95 146802
|
[14] |
Kane C L and Mele E J 2005 Phys. Rev. Lett. 95 226801
|
[15] |
Dedkov Y S, Fonin M, Rüdiger U and Laubscha C 2008 Phys. Rev. Lett. 100 107602
|
[16] |
Varykhalov A, Sanchez-Barriga J, Shikin A M, Biswas C, Vescovo E, Rybkin A, Marchenko D and Rader O 2008 Phys. Rev. Lett. 101 157601
|
[17] |
Castro Neto A H and Guinea F 2009 Phys. Rev. Lett. 103 026804
|
[18] |
Imura K, Kuramoto Y and Nomura K 2009 Phys. Rev. B 80 085119
|
[19] |
Yamakage A, Imura K, Cayssol J and Kuramoto Y 2011 Phys. Rev. B 83 125401
|
[20] |
Onoda S, Sugimoto N and Nagaosa N 2006 Phys. Rev. Lett. 97 126602
|
[21] |
Onoda S, Sugimoto N and Nagaosa N 2008 Phys. Rev. B 77 165103
|
[22] |
Kovalev A A, Tserkovnyak Y, Vyborny K and Sinova J 2009 Phys. Rev. B 79 195129
|
[23] |
Kovalev A A, Sinova J and Tserkovnyak Y 2010 Phys. Rev. Lett. 105 036601
|
[24] |
Smrcka L and Streda P 1977 J. Phys. C 10 2153
|
[25] |
Dyrdal A, Dugaev V K and Barnas J 2009 Phys. Rev. B 80 155444
|
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