Loading…
Persistent charge and spin currents in the long-wavelength regime for graphene rings
We address the problem of persistent charge and spin currents on a Corbino disk built from a graphene sheet. We consistently derive the Hamiltonian including kinetic, intrinsic (ISO), and Rashba spin-orbit interactions in cylindrical coordinates. The Hamiltonian is carefully considered to reflect he...
Saved in:
Published in: | Physical review. B, Condensed matter and materials physics Condensed matter and materials physics, 2014-03, Vol.89 (12), Article 125413 |
---|---|
Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-c424t-5a1ae7b0463ae918742c02c75670d0135c60668caa03ae3e5167b7864f0a60623 |
---|---|
cites | cdi_FETCH-LOGICAL-c424t-5a1ae7b0463ae918742c02c75670d0135c60668caa03ae3e5167b7864f0a60623 |
container_end_page | |
container_issue | 12 |
container_start_page | |
container_title | Physical review. B, Condensed matter and materials physics |
container_volume | 89 |
creator | Bolívar, N. Medina, E. Berche, B. |
description | We address the problem of persistent charge and spin currents on a Corbino disk built from a graphene sheet. We consistently derive the Hamiltonian including kinetic, intrinsic (ISO), and Rashba spin-orbit interactions in cylindrical coordinates. The Hamiltonian is carefully considered to reflect hermiticity and covariance. We compute the energy spectrum and the corresponding eigenfunctions separately for the intrinsic and Rashba spin-orbit interactions. In order to determine the charge persistent currents, we use the spectrum equilibrium linear response definition. We also determine the spin and pseudospin polarizations associated with such equilibrium currents. For the intrinsic case, one can also compute the correct currents by applying the bare velocity operator to the ISO wave functions or alternatively the ISO group velocity operator to the free wave functions. Charge currents for both SO couplings are maximal in the vicinity of half-integer flux quanta. Such maximal currents are protected from thermal effects because the contributing levels plunge (~1 K) into the Fenni sea at half-integer flux values. Such a mechanism, makes them observable at readily accessible temperatures. Spin currents only arise for the Rashba coupling, due to the spin symmetry ofthe ISO spectrum. For the Rashba coupling, spin currents are canceled at half-integer fluxes but they remain finite in the vicinity, and the same scenario as above protects spin currents. |
doi_str_mv | 10.1103/PhysRevB.89.125413 |
format | article |
fullrecord | <record><control><sourceid>proquest_hal_p</sourceid><recordid>TN_cdi_hal_primary_oai_HAL_hal_01275577v1</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1701003295</sourcerecordid><originalsourceid>FETCH-LOGICAL-c424t-5a1ae7b0463ae918742c02c75670d0135c60668caa03ae3e5167b7864f0a60623</originalsourceid><addsrcrecordid>eNo9kEtPwzAQhCMEEuXxBzj5CIeUXTuOk2OpgCJVokJF4ma57uaBUifYaVH_PakKnHY082mknSi6QRgjgrhfVPvwRruHcZaPkcsExUk0Qikh5kJ-nA4a8iwG5HgeXYTwCYBJnvBRtFyQD3XoyfXMVsaXxIxbs9DVjtmt94Mf2KD7iljTujL-NjtqyJV9xTyV9YZY0XpWetNV5Ij52pXhKjorTBPo-vdeRu9Pj8vpLJ6_Pr9MJ_PYJjzpY2nQkFpBkgpDOWYq4Ra4VTJVsAYU0qaQppk1BgZAkMRUrVSWJgWYIeHiMro79lam0Z2vN8bvdWtqPZvM9cEbHlZSKrXDgb09sp1vv7YUer2pg6WmMY7abdCoAAEEz-WA8iNqfRuCp-K_G0Ef5tZ_c-ss18e5xQ_2enPC</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1701003295</pqid></control><display><type>article</type><title>Persistent charge and spin currents in the long-wavelength regime for graphene rings</title><source>American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)</source><creator>Bolívar, N. ; Medina, E. ; Berche, B.</creator><creatorcontrib>Bolívar, N. ; Medina, E. ; Berche, B.</creatorcontrib><description>We address the problem of persistent charge and spin currents on a Corbino disk built from a graphene sheet. We consistently derive the Hamiltonian including kinetic, intrinsic (ISO), and Rashba spin-orbit interactions in cylindrical coordinates. The Hamiltonian is carefully considered to reflect hermiticity and covariance. We compute the energy spectrum and the corresponding eigenfunctions separately for the intrinsic and Rashba spin-orbit interactions. In order to determine the charge persistent currents, we use the spectrum equilibrium linear response definition. We also determine the spin and pseudospin polarizations associated with such equilibrium currents. For the intrinsic case, one can also compute the correct currents by applying the bare velocity operator to the ISO wave functions or alternatively the ISO group velocity operator to the free wave functions. Charge currents for both SO couplings are maximal in the vicinity of half-integer flux quanta. Such maximal currents are protected from thermal effects because the contributing levels plunge (~1 K) into the Fenni sea at half-integer flux values. Such a mechanism, makes them observable at readily accessible temperatures. Spin currents only arise for the Rashba coupling, due to the spin symmetry ofthe ISO spectrum. For the Rashba coupling, spin currents are canceled at half-integer fluxes but they remain finite in the vicinity, and the same scenario as above protects spin currents.</description><identifier>ISSN: 1098-0121</identifier><identifier>EISSN: 1550-235X</identifier><identifier>DOI: 10.1103/PhysRevB.89.125413</identifier><language>eng</language><publisher>American Physical Society</publisher><subject>Charge ; Condensed Matter ; Electric current ; Flux ; Graphene ; Joining ; Mesoscopic Systems and Quantum Hall Effect ; Operators ; Physics ; Spin-orbit interactions ; Spintronics ; Wave functions</subject><ispartof>Physical review. B, Condensed matter and materials physics, 2014-03, Vol.89 (12), Article 125413</ispartof><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c424t-5a1ae7b0463ae918742c02c75670d0135c60668caa03ae3e5167b7864f0a60623</citedby><cites>FETCH-LOGICAL-c424t-5a1ae7b0463ae918742c02c75670d0135c60668caa03ae3e5167b7864f0a60623</cites><orcidid>0000-0002-1566-0170 ; 0000-0002-4254-807X</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,27901,27902</link.rule.ids><backlink>$$Uhttps://hal.science/hal-01275577$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Bolívar, N.</creatorcontrib><creatorcontrib>Medina, E.</creatorcontrib><creatorcontrib>Berche, B.</creatorcontrib><title>Persistent charge and spin currents in the long-wavelength regime for graphene rings</title><title>Physical review. B, Condensed matter and materials physics</title><description>We address the problem of persistent charge and spin currents on a Corbino disk built from a graphene sheet. We consistently derive the Hamiltonian including kinetic, intrinsic (ISO), and Rashba spin-orbit interactions in cylindrical coordinates. The Hamiltonian is carefully considered to reflect hermiticity and covariance. We compute the energy spectrum and the corresponding eigenfunctions separately for the intrinsic and Rashba spin-orbit interactions. In order to determine the charge persistent currents, we use the spectrum equilibrium linear response definition. We also determine the spin and pseudospin polarizations associated with such equilibrium currents. For the intrinsic case, one can also compute the correct currents by applying the bare velocity operator to the ISO wave functions or alternatively the ISO group velocity operator to the free wave functions. Charge currents for both SO couplings are maximal in the vicinity of half-integer flux quanta. Such maximal currents are protected from thermal effects because the contributing levels plunge (~1 K) into the Fenni sea at half-integer flux values. Such a mechanism, makes them observable at readily accessible temperatures. Spin currents only arise for the Rashba coupling, due to the spin symmetry ofthe ISO spectrum. For the Rashba coupling, spin currents are canceled at half-integer fluxes but they remain finite in the vicinity, and the same scenario as above protects spin currents.</description><subject>Charge</subject><subject>Condensed Matter</subject><subject>Electric current</subject><subject>Flux</subject><subject>Graphene</subject><subject>Joining</subject><subject>Mesoscopic Systems and Quantum Hall Effect</subject><subject>Operators</subject><subject>Physics</subject><subject>Spin-orbit interactions</subject><subject>Spintronics</subject><subject>Wave functions</subject><issn>1098-0121</issn><issn>1550-235X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><recordid>eNo9kEtPwzAQhCMEEuXxBzj5CIeUXTuOk2OpgCJVokJF4ma57uaBUifYaVH_PakKnHY082mknSi6QRgjgrhfVPvwRruHcZaPkcsExUk0Qikh5kJ-nA4a8iwG5HgeXYTwCYBJnvBRtFyQD3XoyfXMVsaXxIxbs9DVjtmt94Mf2KD7iljTujL-NjtqyJV9xTyV9YZY0XpWetNV5Ij52pXhKjorTBPo-vdeRu9Pj8vpLJ6_Pr9MJ_PYJjzpY2nQkFpBkgpDOWYq4Ra4VTJVsAYU0qaQppk1BgZAkMRUrVSWJgWYIeHiMro79lam0Z2vN8bvdWtqPZvM9cEbHlZSKrXDgb09sp1vv7YUer2pg6WmMY7abdCoAAEEz-WA8iNqfRuCp-K_G0Ef5tZ_c-ss18e5xQ_2enPC</recordid><startdate>20140310</startdate><enddate>20140310</enddate><creator>Bolívar, N.</creator><creator>Medina, E.</creator><creator>Berche, B.</creator><general>American Physical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-1566-0170</orcidid><orcidid>https://orcid.org/0000-0002-4254-807X</orcidid></search><sort><creationdate>20140310</creationdate><title>Persistent charge and spin currents in the long-wavelength regime for graphene rings</title><author>Bolívar, N. ; Medina, E. ; Berche, B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c424t-5a1ae7b0463ae918742c02c75670d0135c60668caa03ae3e5167b7864f0a60623</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Charge</topic><topic>Condensed Matter</topic><topic>Electric current</topic><topic>Flux</topic><topic>Graphene</topic><topic>Joining</topic><topic>Mesoscopic Systems and Quantum Hall Effect</topic><topic>Operators</topic><topic>Physics</topic><topic>Spin-orbit interactions</topic><topic>Spintronics</topic><topic>Wave functions</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bolívar, N.</creatorcontrib><creatorcontrib>Medina, E.</creatorcontrib><creatorcontrib>Berche, B.</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Physical review. B, Condensed matter and materials physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bolívar, N.</au><au>Medina, E.</au><au>Berche, B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Persistent charge and spin currents in the long-wavelength regime for graphene rings</atitle><jtitle>Physical review. B, Condensed matter and materials physics</jtitle><date>2014-03-10</date><risdate>2014</risdate><volume>89</volume><issue>12</issue><artnum>125413</artnum><issn>1098-0121</issn><eissn>1550-235X</eissn><abstract>We address the problem of persistent charge and spin currents on a Corbino disk built from a graphene sheet. We consistently derive the Hamiltonian including kinetic, intrinsic (ISO), and Rashba spin-orbit interactions in cylindrical coordinates. The Hamiltonian is carefully considered to reflect hermiticity and covariance. We compute the energy spectrum and the corresponding eigenfunctions separately for the intrinsic and Rashba spin-orbit interactions. In order to determine the charge persistent currents, we use the spectrum equilibrium linear response definition. We also determine the spin and pseudospin polarizations associated with such equilibrium currents. For the intrinsic case, one can also compute the correct currents by applying the bare velocity operator to the ISO wave functions or alternatively the ISO group velocity operator to the free wave functions. Charge currents for both SO couplings are maximal in the vicinity of half-integer flux quanta. Such maximal currents are protected from thermal effects because the contributing levels plunge (~1 K) into the Fenni sea at half-integer flux values. Such a mechanism, makes them observable at readily accessible temperatures. Spin currents only arise for the Rashba coupling, due to the spin symmetry ofthe ISO spectrum. For the Rashba coupling, spin currents are canceled at half-integer fluxes but they remain finite in the vicinity, and the same scenario as above protects spin currents.</abstract><pub>American Physical Society</pub><doi>10.1103/PhysRevB.89.125413</doi><orcidid>https://orcid.org/0000-0002-1566-0170</orcidid><orcidid>https://orcid.org/0000-0002-4254-807X</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1098-0121 |
ispartof | Physical review. B, Condensed matter and materials physics, 2014-03, Vol.89 (12), Article 125413 |
issn | 1098-0121 1550-235X |
language | eng |
recordid | cdi_hal_primary_oai_HAL_hal_01275577v1 |
source | American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list) |
subjects | Charge Condensed Matter Electric current Flux Graphene Joining Mesoscopic Systems and Quantum Hall Effect Operators Physics Spin-orbit interactions Spintronics Wave functions |
title | Persistent charge and spin currents in the long-wavelength regime for graphene rings |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-08T11%3A09%3A31IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_hal_p&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Persistent%20charge%20and%20spin%20currents%20in%20the%20long-wavelength%20regime%20for%20graphene%20rings&rft.jtitle=Physical%20review.%20B,%20Condensed%20matter%20and%20materials%20physics&rft.au=Bol%C3%ADvar,%20N.&rft.date=2014-03-10&rft.volume=89&rft.issue=12&rft.artnum=125413&rft.issn=1098-0121&rft.eissn=1550-235X&rft_id=info:doi/10.1103/PhysRevB.89.125413&rft_dat=%3Cproquest_hal_p%3E1701003295%3C/proquest_hal_p%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c424t-5a1ae7b0463ae918742c02c75670d0135c60668caa03ae3e5167b7864f0a60623%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1701003295&rft_id=info:pmid/&rfr_iscdi=true |