Curvature effects in the band structure of carbon nanotubes including spin-orbit coupling
The Kane-Mele model was previously used to describe effective spin-orbit couplings (SOCs) in graphene. Here we extend this model and also incorporate curvature effects to analyze the combined influence of SOC and curvature on the band structure of carbon nanotubes (CNTs). The extended model then rep...
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Veröffentlicht in: | Journal of physics. Condensed matter 2015-11, Vol.27 (44), p.445501-445501 |
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container_title | Journal of physics. Condensed matter |
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creator | Liu, Hong Heinze, Dirk Thanh Duc, Huynh Schumacher, Stefan Meier, Torsten |
description | The Kane-Mele model was previously used to describe effective spin-orbit couplings (SOCs) in graphene. Here we extend this model and also incorporate curvature effects to analyze the combined influence of SOC and curvature on the band structure of carbon nanotubes (CNTs). The extended model then reproduces the chirality-dependent asymmetric electron-hole splitting for semiconducting CNTs and in the band structure for metallic CNTs shows an opening of the band gap and a change of the Fermi wave vector with spin. For chiral semiconducting CNTs with large chiral angle we show that the spin-splitting configuration of bands near the Fermi energy depends on the value of . |
doi_str_mv | 10.1088/0953-8984/27/44/445501 |
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Here we extend this model and also incorporate curvature effects to analyze the combined influence of SOC and curvature on the band structure of carbon nanotubes (CNTs). The extended model then reproduces the chirality-dependent asymmetric electron-hole splitting for semiconducting CNTs and in the band structure for metallic CNTs shows an opening of the band gap and a change of the Fermi wave vector with spin. For chiral semiconducting CNTs with large chiral angle we show that the spin-splitting configuration of bands near the Fermi energy depends on the value of .</description><identifier>ISSN: 0953-8984</identifier><identifier>EISSN: 1361-648X</identifier><identifier>DOI: 10.1088/0953-8984/27/44/445501</identifier><identifier>PMID: 26451898</identifier><identifier>CODEN: JCOMEL</identifier><language>eng</language><publisher>England: IOP Publishing</publisher><subject>band structure ; carbon nanotube ; spin-orbit coupling</subject><ispartof>Journal of physics. 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Condensed matter</title><addtitle>JPhysCM</addtitle><addtitle>J. Phys.: Condens. Matter</addtitle><description>The Kane-Mele model was previously used to describe effective spin-orbit couplings (SOCs) in graphene. Here we extend this model and also incorporate curvature effects to analyze the combined influence of SOC and curvature on the band structure of carbon nanotubes (CNTs). The extended model then reproduces the chirality-dependent asymmetric electron-hole splitting for semiconducting CNTs and in the band structure for metallic CNTs shows an opening of the band gap and a change of the Fermi wave vector with spin. For chiral semiconducting CNTs with large chiral angle we show that the spin-splitting configuration of bands near the Fermi energy depends on the value of .</description><subject>band structure</subject><subject>carbon nanotube</subject><subject>spin-orbit coupling</subject><issn>0953-8984</issn><issn>1361-648X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqFkE1LJDEQhoO46Dj6FyQ3vbSTz05ylEHdBcHLLuyeQpJOtKUnaZOO4L_fHkcFQRACBannraIeAE4xusBIyhVSnDZSSbYiYsXY_DhHeA8sMG1x0zL5dx8sPqBDcFTKI0KIScoOwCFpGcdzYwH-rWt-NlPNHvoQvJsK7COcHjy0JnawTLm6124K0JlsU4TRxDRV67ekG2rXx3tYxj42Kdt-gi7VcZj_jsGPYIbiT97qEvy5vvq9_tnc3t38Wl_eNo5xMjU4SENV6IRXSLDATXDME4qUEFQxhBERnAtCgpestd46arF0QnUCe9uqli7B-W7umNNT9WXSm744Pwwm-lSLxnNYEaU4m9F2h7qcSsk-6DH3G5NfNEZ6q1VvjemtMU2EZkzvtM7B07cd1W589xF79zgDZAf0adSPqeY4n_z91LMvQm7zidJjF-h_LYSPfg</recordid><startdate>20151111</startdate><enddate>20151111</enddate><creator>Liu, Hong</creator><creator>Heinze, Dirk</creator><creator>Thanh Duc, Huynh</creator><creator>Schumacher, Stefan</creator><creator>Meier, Torsten</creator><general>IOP Publishing</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope></search><sort><creationdate>20151111</creationdate><title>Curvature effects in the band structure of carbon nanotubes including spin-orbit coupling</title><author>Liu, Hong ; Heinze, Dirk ; Thanh Duc, Huynh ; Schumacher, Stefan ; Meier, Torsten</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c452t-1f8a39fd7e9074f5afc4e2309773940102755722fe846bebc3b18c79d71eb6963</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>band structure</topic><topic>carbon nanotube</topic><topic>spin-orbit coupling</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Liu, Hong</creatorcontrib><creatorcontrib>Heinze, Dirk</creatorcontrib><creatorcontrib>Thanh Duc, Huynh</creatorcontrib><creatorcontrib>Schumacher, Stefan</creatorcontrib><creatorcontrib>Meier, Torsten</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><jtitle>Journal of physics. 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Here we extend this model and also incorporate curvature effects to analyze the combined influence of SOC and curvature on the band structure of carbon nanotubes (CNTs). The extended model then reproduces the chirality-dependent asymmetric electron-hole splitting for semiconducting CNTs and in the band structure for metallic CNTs shows an opening of the band gap and a change of the Fermi wave vector with spin. For chiral semiconducting CNTs with large chiral angle we show that the spin-splitting configuration of bands near the Fermi energy depends on the value of .</abstract><cop>England</cop><pub>IOP Publishing</pub><pmid>26451898</pmid><doi>10.1088/0953-8984/27/44/445501</doi><tpages>8</tpages></addata></record> |
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subjects | band structure carbon nanotube spin-orbit coupling |
title | Curvature effects in the band structure of carbon nanotubes including spin-orbit coupling |
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