Aviso: para depositar documentos, por favor, inicia sesión e identifícate con tu cuenta de correo institucional de la UCM con el botón MI CUENTA UCM. No emplees la opción AUTENTICACIÓN CON CONTRASEÑA
 

Unexpected magnetism in low dimensional systems: the role of symmetry

dc.contributor.authorMuñoz, María del Carmen
dc.contributor.authorChico, L.
dc.contributor.authorLópez-Sancho, M. P.
dc.contributor.authorBeltrán Fínez, Juan Ignacio
dc.contributor.authorGallego, S.
dc.contributor.authorCerdá, J.
dc.date.accessioned2023-06-20T10:57:21Z
dc.date.available2023-06-20T10:57:21Z
dc.date.issued2006
dc.description© 2006 IOP Publishing Ltd. International School on Theoretical Physics (8. 2005. Myczkowce-Poland). This work has been partially financed by the Spanish Ministerio de Educación y Ciencia and the DGES under contracts MAT2002-04095-C02-01, MAT2002-04540-C05-03 and MAT2003-04278, and by the Comunidad Autónoma de Madrid under CAM2004-0440. S.G. acknowledges financial support from the Ramón y Cajal program of the Spanish Ministerio de Educación y Ciencia, and J.I.B. from the I3P program of the CSIC.
dc.description.abstractThe symmetry underlying the geometric structure of materials determines most of their physical properties. In low dimensional systems the role of symmetry is enhanced and can give rise to new phenomena. Here, we report on unexpected magnetism in carbon nanotubes and O-rich surfaces of ionic oxides, to show how its existence is closely related to the symmetry conditions. First, based on tight-binding models, we demonstrate that chiral carbon nanotubes present spin splitting at the Fermi level in the absence of a magnetic field, whereas achiral tubes preserve spin degeneracy. These remarkably different behaviors of chiral and non-chiral nanotubes are due to the intrinsic symmetry dependence of the spin-orbit interaction. Second, the occurence of spin-polarization at ZrO_(2), Al_(2)O_(3) and MgO surfaces is proved by means of abinitio calculations within the density functional theory. Large spin moments develop at O-ended polar terminations, transforming the non-magnetic insulator into a half-metal. The magnetic moments mainly reside in the surface oxygen atoms, and their origin is related to the existence of 2p holes of well-defined spin polarization at the valence band of the ionic oxide. The direct relation between magnetization and local loss of donor charge shows that at the origin of these phenomena is the reduced surface symmetry.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipSpanish Ministerio de Educación y Ciencia
dc.description.sponsorshipDGES
dc.description.sponsorshipComunidad Autónoma de Madrid
dc.description.sponsorshipRamón y Cajal program of the Spanish Ministerio de Educación y Ciencia
dc.description.sponsorshipI3P program of the CSIC
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/31408
dc.identifier.doi10.1088/1742-6596/30/1/026
dc.identifier.issn1742-6588
dc.identifier.officialurlhttp://dx.doi.org/10.1088/1742-6596/30/1/026
dc.identifier.relatedurlhttp://iopscience.iop.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/51509
dc.journal.titleJournal of physics. Conference series
dc.language.isoeng
dc.page.final223
dc.page.initial215
dc.publisherIOP Publishing Ltd
dc.relation.projectIDMAT2002-04095-C02-01
dc.relation.projectIDMAT2002-04540-C05-03
dc.relation.projectIDMAT2003-04278
dc.relation.projectIDCAM2004-0440
dc.rightsAtribución 3.0 España
dc.rights.accessRightsopen access
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/es/
dc.subject.cdu537
dc.subject.keywordSpin-orbit interaction
dc.subject.keywordCarbon nanotubes
dc.subject.keywordBand-structure
dc.subject.keywordElectronic-structure
dc.subject.keywordSurfaces
dc.subject.keywordMetallicity
dc.subject.keywordZirconia
dc.subject.keywordExhange.
dc.subject.ucmElectricidad
dc.subject.ucmElectrónica (Física)
dc.subject.unesco2202.03 Electricidad
dc.titleUnexpected magnetism in low dimensional systems: the role of symmetry
dc.typejournal article
dc.volume.number30
dcterms.references[1] Wolf, S. A., et al, 2001, Science, 294, 1488. [2] Prinz, G. A., 1998, Science, 282, 1660. [3] Saito, R., Dresselhaus, G., Dresselhaus, M., 1998, Physical Properties of Carbon Nanotubes, London (Imperial College Press). [4] Wildöer, J. W. G., et al., 1998, Nature, 391, 59. [5] Odom, T. W., et al., 1998, Nature, 391, 62. [6] Chico, L., López-Sancho, M. P., Muñoz, M. C., 2004, Phys. Rev. Lett., 93, 176402. [7] Gallego, S., Beltránm J, I,, Cerdá, J., Muñoz, M. C., 2005, J. Phys.: Condens. Matter, 17, L451. [8] Slater, J. C., Koster, J. F., 1954, Phys. Rev., 94, 1498. [9] Tománek, D., Louie, S. G., 1988, Phys. Rev. B, 37, 8327. [10] Blase, X., et al., 1994, Phys. Rev. Lett., 72, 1878. [11] Wang, C. S., Callaway, J., 1974, Phys. Rev. B, 9, 4897. [12] Gallego, S., Muñoz, M. C., 1999, Surf. Sci., 423, 324. [13] Moroz, A. V., Barnes, C. H. W., 1999, Phys. Rev. B, 60, 14272. [14] Chen, G. H., Raikh, M. E., 1999, Phys. Rev. B, 60, 4826. [15] Valín-Rodríguez, M., 2004, Phys. Rev. B, 70, 033306. [16] Rashba, E. I., Efros, A. L., 2003, Phys. Rev. Lett., 91, 126405. [17] Kleiner, A., Eggert, S., 2001, Phys. Rev. B, 63, 73408. [18] Howard, C. J., Hill, R. J., Reichert, B. E., 1988, Acta Crystallogr. Sect. B: Struct. Sci., 44, 116. [19] Perdew, J. P., et al., 1992, Phys. Rev. B, 46, 6671. [20] Kralik, B., Chang, E. K., Louie, S. G., 1998, Phys. Rev. B, 57, 7027. [21] Jansen, H. J. F., 1991, Phys. Rev. B, 43, 7267. [22] Eichler, A., 2001, Phys. Rev. B, 64, 174103. [23] Zhao, X., Vanderblit, D., 2002, Phys. Rev. B, 65, 075105. [24] Ordejón, P., Artacho, E., Soler, J. M., 1996, Phys. Rev. B, 53, R10441. [25] Soler, J. M., et al., 2002, J. Phys.: Condens. Matter, 14, 2745. [26] Beltrán, J. I., et al., 2003, Phys. Rev. B, 68, 075401. [27] Ando, T., 2000, J. Phys. Soc. Jpn., 69, 1757. [28] Tsukagoshi, K., Alphenaar, B. W., Ago, H., 1999, Nature, 401, 572. [29] Cobden, D. H., et al., 1998, Phys. Rev. Lett., 81, 681. [30] Cobden, D. H., Nygård, J., 2002, Phys. Rev. Lett., 89, 046803. [31] Liang, W., Bockrath, M., Park, H., 2002, Phys. Rev. Lett., 88, 126801. [32] Tans, S. J., et al., 1998, Nature, 394, 761. [33] Tasker, P. W., 1979, J. Phys. C: Sol. State Phys., 12, 4977. [34] Venkatesan, M., Fitzgerald, C. B., Coey, J. M. D., 2004, Nature, 430, 630. [35] M. Coey, Abstract U5.00005 of 2005 APS March Meeting
dspace.entity.typePublication
relation.isAuthorOfPublication4e2ad5cb-9ebe-40f4-8dcb-6d6f60066da5
relation.isAuthorOfPublication.latestForDiscovery4e2ad5cb-9ebe-40f4-8dcb-6d6f60066da5

Download

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
BeltranFinez JI 10 LIBRE.pdf
Size:
922.48 KB
Format:
Adobe Portable Document Format

Collections