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Control of chiral orbital currents in a colossal magnetoresistance material

  • Yu Zhang
  • , Yifei Ni
  • , Hengdi Zhao
  • , Sami Hakani
  • , Feng Ye
  • , Lance DeLong
  • , Itamar Kimchi
  • , Gang Cao

Producción científica: Articlerevisión exhaustiva

53 Citas (Scopus)

Resumen

Colossal magnetoresistance (CMR) is an extraordinary enhancement of the electrical conductivity in the presence of a magnetic field. It is conventionally associated with a field-induced spin polarization that drastically reduces spin scattering and electric resistance. Ferrimagnetic Mn3Si2Te6 is an intriguing exception to this rule: it exhibits a seven-order-of-magnitude reduction in ab plane resistivity that occurs only when a magnetic polarization is avoided1,2. Here, we report an exotic quantum state that is driven by ab plane chiral orbital currents (COC) flowing along edges of MnTe6 octahedra. The c axis orbital moments of ab plane COC couple to the ferrimagnetic Mn spins to drastically increase the ab plane conductivity (CMR) when an external magnetic field is aligned along the magnetic hard c axis. Consequently, COC-driven CMR is highly susceptible to small direct currents exceeding a critical threshold, and can induce a time-dependent, bistable switching that mimics a first-order ‘melting transition’ that is a hallmark of the COC state. The demonstrated current-control of COC-enabled CMR offers a new paradigm for quantum technologies.

Idioma originalEnglish
Páginas (desde-hasta)467-472
Número de páginas6
PublicaciónNature
Volumen611
N.º7936
DOI
EstadoPublished - nov 17 2022

Nota bibliográfica

Publisher Copyright:
© 2022, The Author(s), under exclusive licence to Springer Nature Limited.

Financiación

G.C. thanks M. Lee, R. Nandkishore, X. Chen, M. Hermele, D. Singh, D. Reznik, D. Dessau and N. Clark for useful discussions. I.K. thanks E. Berg, M. Mourigal, B. Uchoa, C. Varma and Z. Wang for useful discussions. This work is supported by National Science Foundation via grants no. DMR 1903888 and DMR 2204811. The theoretical part of this work is in part performed at Aspen Center for Physics, which is supported by National Science Foundation grant PHY-1607611. The work at the Spallation Neutron Source at the Oak Ridge Natinoal Laboratory is sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences, US Department of Energy.

FinanciadoresNúmero del financiador
U.S. Department of Energy
Scientific User Facilities Division
DOE Basic Energy Sciences
National Science Foundation Arctic Social Science Program2204811, DMR 2204811, PHY-1607611, DMR 1903888

    ASJC Scopus subject areas

    • General

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