Gap formation in helical edge states with magnetic impurities

dc.contributor.authorWozny, Simon
dc.contributor.authorVyborny, Karel
dc.contributor.authorBelzig, Wolfgang
dc.contributor.authorErlingsson, Sigurdur I.
dc.date.accessioned2018-10-18T12:22:44Z
dc.date.available2018-10-18T12:22:44Z
dc.date.issued2018-07-04T22:09:59Zeng
dc.description.abstractHelical edge states appear at the surface of two dimensional topological insulators and are characterized by spin up traveling in one direction and the spin down traveling in the opposite direction. Such states are protected by time reversal symmetry and no backscattering due to scalar impurities can occur. However, magnetic impurities break time reversal symmetry and lead to backscattering. Often their presence is unintentional, but in some cases they are introduced into the sample to open up gaps in the spectrum. We investigate the influence of random impurities on helical edge states, specifically how the gap behaves in the realistic case of impurities having both a magnetic and a scalar component. It turns out that for a fixed magnetic contribution the gap closes when either the scalar component, or Fermi velocity is increased. We compare diagrammatic techniques in the self-consistent Born approximation to numerical calculations which yields good agreement. For experimentally relevant parameters we find that even moderate scalar components can be quite detrimental for the gap formation.eng
dc.description.versionpublishedeng
dc.identifier.arxiv1807.01799eng
dc.identifier.doi10.1103/PhysRevB.98.165423eng
dc.identifier.ppn51213765X
dc.identifier.urihttps://kops.uni-konstanz.de/handle/123456789/42794.2
dc.language.isoengeng
dc.rightsterms-of-use
dc.rights.urihttps://rightsstatements.org/page/InC/1.0/
dc.subject.ddc530eng
dc.subject.pacs73.63.Hs,71.70.Ej,73.40.-c
dc.titleGap formation in helical edge states with magnetic impuritieseng
dc.typeJOURNAL_ARTICLEeng
dspace.entity.typePublication
kops.citation.bibtex
@article{Wozny2018-07-04T22:09:59Zforma-42794.2,
  year={2018},
  doi={10.1103/PhysRevB.98.165423},
  title={Gap formation in helical edge states with magnetic impurities},
  number={16},
  volume={98},
  issn={2469-9950},
  journal={Physical Review B},
  author={Wozny, Simon and Vyborny, Karel and Belzig, Wolfgang and Erlingsson, Sigurdur I.},
  note={Article Number: 165423}
}
kops.citation.iso690WOZNY, Simon, Karel VYBORNY, Wolfgang BELZIG, Sigurdur I. ERLINGSSON, 2018. Gap formation in helical edge states with magnetic impurities. In: Physical Review B. 2018, 98(16), 165423. ISSN 2469-9950. eISSN 2469-9969. Available under: doi: 10.1103/PhysRevB.98.165423deu
kops.citation.iso690WOZNY, Simon, Karel VYBORNY, Wolfgang BELZIG, Sigurdur I. ERLINGSSON, 2018. Gap formation in helical edge states with magnetic impurities. In: Physical Review B. 2018, 98(16), 165423. ISSN 2469-9950. eISSN 2469-9969. Available under: doi: 10.1103/PhysRevB.98.165423eng
kops.citation.rdf
<rdf:RDF
    xmlns:dcterms="http://purl.org/dc/terms/"
    xmlns:dc="http://purl.org/dc/elements/1.1/"
    xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#"
    xmlns:bibo="http://purl.org/ontology/bibo/"
    xmlns:dspace="http://digital-repositories.org/ontologies/dspace/0.1.0#"
    xmlns:foaf="http://xmlns.com/foaf/0.1/"
    xmlns:void="http://rdfs.org/ns/void#"
    xmlns:xsd="http://www.w3.org/2001/XMLSchema#" > 
  <rdf:Description rdf:about="https://kops.uni-konstanz.de/server/rdf/resource/123456789/42794.2">
    <dc:date rdf:datatype="http://www.w3.org/2001/XMLSchema#dateTime">2018-10-18T12:22:44Z</dc:date>
    <dcterms:rights rdf:resource="https://rightsstatements.org/page/InC/1.0/"/>
    <dcterms:isPartOf rdf:resource="https://kops.uni-konstanz.de/server/rdf/resource/123456789/41"/>
    <dc:creator>Belzig, Wolfgang</dc:creator>
    <dcterms:hasPart rdf:resource="https://kops.uni-konstanz.de/bitstream/123456789/42794.2/3/Wozny_2-5bc3fv9oxckb6.pdf"/>
    <dc:creator>Vyborny, Karel</dc:creator>
    <dc:creator>Erlingsson, Sigurdur I.</dc:creator>
    <dcterms:title>Gap formation in helical edge states with magnetic impurities</dcterms:title>
    <foaf:homepage rdf:resource="http://localhost:8080/"/>
    <dc:rights>terms-of-use</dc:rights>
    <dspace:isPartOfCollection rdf:resource="https://kops.uni-konstanz.de/server/rdf/resource/123456789/41"/>
    <void:sparqlEndpoint rdf:resource="http://localhost/fuseki/dspace/sparql"/>
    <dcterms:available rdf:datatype="http://www.w3.org/2001/XMLSchema#dateTime">2018-10-18T12:22:44Z</dcterms:available>
    <dspace:hasBitstream rdf:resource="https://kops.uni-konstanz.de/bitstream/123456789/42794.2/3/Wozny_2-5bc3fv9oxckb6.pdf"/>
    <dcterms:issued>2018-07-04T22:09:59Z</dcterms:issued>
    <dc:contributor>Vyborny, Karel</dc:contributor>
    <dc:language>eng</dc:language>
    <dc:contributor>Erlingsson, Sigurdur I.</dc:contributor>
    <dc:contributor>Wozny, Simon</dc:contributor>
    <dcterms:abstract xml:lang="eng">Helical edge states appear at the surface of two dimensional topological insulators and are characterized by spin up traveling in one direction and the spin down traveling in the opposite direction. Such states are protected by time reversal symmetry and no backscattering due to scalar impurities can occur. However, magnetic impurities break time reversal symmetry and lead to backscattering. Often their presence is unintentional, but in some cases they are introduced into the sample to open up gaps in the spectrum. We investigate the influence of random impurities on helical edge states, specifically how the gap behaves in the realistic case of impurities having both a magnetic and a scalar component. It turns out that for a fixed magnetic contribution the gap closes when either the scalar component, or Fermi velocity is increased. We compare diagrammatic techniques in the self-consistent Born approximation to numerical calculations which yields good agreement. For experimentally relevant parameters we find that even moderate scalar components can be quite detrimental for the gap formation.</dcterms:abstract>
    <dc:creator>Wozny, Simon</dc:creator>
    <dc:contributor>Belzig, Wolfgang</dc:contributor>
    <bibo:uri rdf:resource="https://kops.uni-konstanz.de/handle/123456789/42794.2"/>
  </rdf:Description>
</rdf:RDF>
kops.description.openAccessopenaccessgreen
kops.flag.isPeerReviewedtrueeng
kops.flag.knbibliographytrue
kops.identifier.nbnurn:nbn:de:bsz:352-2-5bc3fv9oxckb6
kops.sourcefieldPhysical Review B. 2018, <b>98</b>(16), 165423. ISSN 2469-9950. eISSN 2469-9969. Available under: doi: 10.1103/PhysRevB.98.165423deu
kops.sourcefield.plainPhysical Review B. 2018, 98(16), 165423. ISSN 2469-9950. eISSN 2469-9969. Available under: doi: 10.1103/PhysRevB.98.165423deu
kops.sourcefield.plainPhysical Review B. 2018, 98(16), 165423. ISSN 2469-9950. eISSN 2469-9969. Available under: doi: 10.1103/PhysRevB.98.165423eng
relation.isAuthorOfPublication221e1a3b-d55c-4334-acee-247fea9e126b
relation.isAuthorOfPublication5008f36c-f1e5-403a-b331-40c1df19add6
relation.isAuthorOfPublication.latestForDiscovery221e1a3b-d55c-4334-acee-247fea9e126b
source.bibliographicInfo.articleNumber165423eng
source.bibliographicInfo.issue16eng
source.bibliographicInfo.volume98eng
source.identifier.eissn2469-9969eng
source.identifier.issn2469-9950eng
source.periodicalTitlePhysical Review Beng

Dateien

Originalbündel

Gerade angezeigt 1 - 1 von 1
Vorschaubild nicht verfügbar
Name:
Wozny_2-5bc3fv9oxckb6.pdf
Größe:
142.46 KB
Format:
Adobe Portable Document Format
Beschreibung:
Wozny_2-5bc3fv9oxckb6.pdf
Wozny_2-5bc3fv9oxckb6.pdfGröße: 142.46 KBDownloads: 333

Lizenzbündel

Gerade angezeigt 1 - 1 von 1
Vorschaubild nicht verfügbar
Name:
license.txt
Größe:
3.88 KB
Format:
Item-specific license agreed upon to submission
Beschreibung:
license.txt
license.txtGröße: 3.88 KBDownloads: 0

Versionsgeschichte

Gerade angezeigt 1 - 2 von 2
VersionDatumZusammenfassung
2*
2018-10-17 10:47:47
2018-07-06 14:49:15
* Ausgewählte Version