Prediction of giant spin motive force due to Rashba spin-orbit coupling

Magnetization dynamics in a ferromagnet can induce a spin-dependent electric field through a spin motive force. Spin current generated by the spin-dependent electric field can in turn modify the magnetization dynamics through spin-transfer torque. While this feedback effect is usually weak and thus...

Full description

Saved in:
Bibliographic Details
Published inPhysical review letters Vol. 108; no. 21; p. 217202
Main Authors Kim, Kyoung-Whan, Moon, Jung-Hwan, Lee, Kyung-Jin, Lee, Hyun-Woo
Format Journal Article
LanguageEnglish
Published United States 23.05.2012
Online AccessGet more information

Cover

Loading…
Abstract Magnetization dynamics in a ferromagnet can induce a spin-dependent electric field through a spin motive force. Spin current generated by the spin-dependent electric field can in turn modify the magnetization dynamics through spin-transfer torque. While this feedback effect is usually weak and thus ignored, we predict that in Rashba spin-orbit coupling systems with a large Rashba parameter α(R), the coupling generates the spin-dependent electric field [±(α(R)m(e)/eħ)(z[over ^]×∂m/∂t)], which can be large enough to modify the magnetization dynamics significantly. This effect should be relevant for device applications based on ultrathin magnetic layers with strong Rashba spin-orbit coupling.
AbstractList Magnetization dynamics in a ferromagnet can induce a spin-dependent electric field through a spin motive force. Spin current generated by the spin-dependent electric field can in turn modify the magnetization dynamics through spin-transfer torque. While this feedback effect is usually weak and thus ignored, we predict that in Rashba spin-orbit coupling systems with a large Rashba parameter α(R), the coupling generates the spin-dependent electric field [±(α(R)m(e)/eħ)(z[over ^]×∂m/∂t)], which can be large enough to modify the magnetization dynamics significantly. This effect should be relevant for device applications based on ultrathin magnetic layers with strong Rashba spin-orbit coupling.
Author Kim, Kyoung-Whan
Lee, Hyun-Woo
Moon, Jung-Hwan
Lee, Kyung-Jin
Author_xml – sequence: 1
  givenname: Kyoung-Whan
  surname: Kim
  fullname: Kim, Kyoung-Whan
  organization: PCTP and Department of Physics, Pohang University of Science and Technology, Pohang, Korea
– sequence: 2
  givenname: Jung-Hwan
  surname: Moon
  fullname: Moon, Jung-Hwan
– sequence: 3
  givenname: Kyung-Jin
  surname: Lee
  fullname: Lee, Kyung-Jin
– sequence: 4
  givenname: Hyun-Woo
  surname: Lee
  fullname: Lee, Hyun-Woo
BackLink https://www.ncbi.nlm.nih.gov/pubmed/23003294$$D View this record in MEDLINE/PubMed
BookMark eNo1j91KwzAYhoMo7kdvYeQGWr_8NGkPZegUBoro8UiTL1ukbUqaDXb3ij9HLw8PPPAuyOUQByRkxaBkDMTdeDhPCU8d5lwyqEvONAd-QeYMdFNoxuSMLKbpEwAYV_U1mXEBIHgj52TzmtAFm0McaPR0H8yQ6TSGgfYxhxNSH5NF6o5Ic6RvZjq05scXMbUhUxuPYxeG_Q258qab8PZvl-Tj8eF9_VRsXzbP6_ttYYXWuaidRYUWpQfjhLeVqZ1irtWyAt8oqRBEhRoaz5n1jdbKad18kzVSt97wJVn9dsdj26PbjSn0Jp13_4_4F3xwUag
CitedBy_id crossref_primary_10_1103_PhysRevB_103_L100402
crossref_primary_10_1103_PhysRevApplied_10_054038
crossref_primary_10_1103_PhysRevB_93_214429
crossref_primary_10_1063_1_4798288
crossref_primary_10_1103_PhysRevB_101_085405
crossref_primary_10_1103_PhysRevB_88_014430
crossref_primary_10_1103_PhysRevB_104_024414
crossref_primary_10_1103_PhysRevB_109_024413
crossref_primary_10_1103_PhysRevB_88_035130
crossref_primary_10_1063_1_4870919
crossref_primary_10_1103_PhysRevB_107_L100408
crossref_primary_10_15407_ufm_17_03_229
crossref_primary_10_1038_s41598_018_31299_4
crossref_primary_10_1016_j_jmmm_2020_167700
crossref_primary_10_1103_PhysRevB_89_220409
crossref_primary_10_1103_RevModPhys_91_035004
crossref_primary_10_1063_5_0002802
crossref_primary_10_1103_PhysRevB_94_184402
crossref_primary_10_1063_5_0034694
crossref_primary_10_1103_PhysRevB_87_041301
crossref_primary_10_31857_S0015323023600995
crossref_primary_10_7566_JPSJ_83_074710
crossref_primary_10_1038_s41467_022_31493_z
crossref_primary_10_1103_PhysRevB_93_180408
crossref_primary_10_1142_S2010324713300041
crossref_primary_10_1088_1361_648X_ac7994
crossref_primary_10_1103_PhysRevLett_125_187202
crossref_primary_10_1002_andp_201900287
crossref_primary_10_1088_1361_648X_aadbdd
crossref_primary_10_1103_PhysRevB_89_165307
crossref_primary_10_1063_1_4838735
crossref_primary_10_1103_PhysRevB_89_054405
crossref_primary_10_1103_PhysRevLett_117_097202
crossref_primary_10_1109_TMAG_2015_2401534
crossref_primary_10_1063_5_0062541
crossref_primary_10_1103_PhysRevB_87_054403
crossref_primary_10_1103_PhysRevB_94_020405
crossref_primary_10_1016_j_physrep_2013_05_006
crossref_primary_10_1093_ptep_ptz131
crossref_primary_10_7567_APEX_6_033001
crossref_primary_10_7566_JPSJ_83_054717
crossref_primary_10_1103_PhysRevLett_128_147201
crossref_primary_10_1103_PhysRevB_96_104438
crossref_primary_10_1002_adma_201605911
crossref_primary_10_1103_PhysRevB_92_014418
crossref_primary_10_1103_PhysRevB_99_224415
crossref_primary_10_7566_JPSJ_85_033701
crossref_primary_10_1088_1367_2630_17_12_123005
crossref_primary_10_1038_srep06901
crossref_primary_10_1103_PhysRevB_104_L020407
crossref_primary_10_1103_PhysRevB_107_174421
crossref_primary_10_1103_PhysRevB_92_064415
crossref_primary_10_1103_PhysRevB_94_064415
crossref_primary_10_1103_PhysRevLett_128_077201
crossref_primary_10_1209_0295_5075_109_67008
crossref_primary_10_1088_1367_2630_16_1_015016
crossref_primary_10_1103_PhysRevB_99_134409
crossref_primary_10_1103_PhysRevLett_111_246602
crossref_primary_10_35848_1882_0786_acd617
crossref_primary_10_1103_PhysRevB_98_174434
crossref_primary_10_1103_PhysRevB_99_045421
crossref_primary_10_1103_PhysRevB_88_184404
crossref_primary_10_7566_JPSJ_82_102002
crossref_primary_10_1103_Physics_14_92
crossref_primary_10_1103_PhysRevB_101_054517
crossref_primary_10_1103_PhysRevB_99_054407
crossref_primary_10_1051_epjap_2017160350
crossref_primary_10_1103_PhysRevB_107_195202
crossref_primary_10_1103_PhysRevB_97_100402
crossref_primary_10_1103_PhysRevB_98_104408
crossref_primary_10_1038_srep25391
crossref_primary_10_1103_PhysRevB_96_144406
crossref_primary_10_7566_JPSJ_90_081011
crossref_primary_10_1103_PhysRevApplied_12_044007
crossref_primary_10_1063_1_5011130
crossref_primary_10_1103_PhysRevB_94_125143
crossref_primary_10_1103_PhysRevB_91_174437
crossref_primary_10_1016_j_physe_2018_05_011
crossref_primary_10_1103_PhysRevB_94_054415
crossref_primary_10_1063_1_4908147
crossref_primary_10_1103_PhysRevApplied_12_054032
crossref_primary_10_1103_PhysRevLett_123_207001
crossref_primary_10_1103_PhysRevB_100_094424
crossref_primary_10_1103_PhysRevB_98_174422
crossref_primary_10_1103_PhysRevB_91_214401
crossref_primary_10_1103_PhysRevLett_111_216601
crossref_primary_10_1103_PhysRevB_94_235148
crossref_primary_10_1134_S1063783418070053
ContentType Journal Article
DBID NPM
DOI 10.1103/physrevlett.108.217202
DatabaseName PubMed
DatabaseTitle PubMed
DatabaseTitleList PubMed
Database_xml – sequence: 1
  dbid: NPM
  name: PubMed
  url: https://proxy.k.utb.cz/login?url=http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?db=PubMed
  sourceTypes: Index Database
DeliveryMethod no_fulltext_linktorsrc
Discipline Physics
EISSN 1079-7114
ExternalDocumentID 23003294
Genre Journal Article
GroupedDBID ---
-DZ
-~X
123
2-P
29O
3MX
5VS
85S
8NH
ACBEA
ACGFO
ACNCT
AENEX
AEQTI
AFFNX
AFGMR
AGDNE
AJQPL
ALMA_UNASSIGNED_HOLDINGS
APKKM
AUAIK
CS3
D0L
DU5
EBS
EJD
F5P
MVM
N9A
NPBMV
NPM
P0-
P2P
ROL
S7W
SJN
TN5
UBE
UCJ
VQA
WH7
XOL
XSW
YNT
ZPR
~02
ID FETCH-LOGICAL-c377t-8dce6ece4f0ad3fc5a8d61db7450f9646e035e709f21cf9776d7799f2ca47bfa2
IngestDate Tue Oct 15 23:43:25 EDT 2024
IsPeerReviewed true
IsScholarly true
Issue 21
Language English
LinkModel OpenURL
MergedId FETCHMERGED-LOGICAL-c377t-8dce6ece4f0ad3fc5a8d61db7450f9646e035e709f21cf9776d7799f2ca47bfa2
PMID 23003294
ParticipantIDs pubmed_primary_23003294
PublicationCentury 2000
PublicationDate 2012-05-23
PublicationDateYYYYMMDD 2012-05-23
PublicationDate_xml – month: 05
  year: 2012
  text: 2012-05-23
  day: 23
PublicationDecade 2010
PublicationPlace United States
PublicationPlace_xml – name: United States
PublicationTitle Physical review letters
PublicationTitleAlternate Phys Rev Lett
PublicationYear 2012
SSID ssj0001268
Score 2.4668841
Snippet Magnetization dynamics in a ferromagnet can induce a spin-dependent electric field through a spin motive force. Spin current generated by the spin-dependent...
SourceID pubmed
SourceType Index Database
StartPage 217202
Title Prediction of giant spin motive force due to Rashba spin-orbit coupling
URI https://www.ncbi.nlm.nih.gov/pubmed/23003294
Volume 108
hasFullText
inHoldings 1
isFullTextHit
isPrint
link http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwnV1da9swFBVpx6AvY9_fQw97C8oky5bsx1K2hZaWMlratyLJUhvootA4bN2v75VkxyHNxrYXY-tiI_scXa7ke64Q-miEKDNVZ4RWWpCcKU604oZorUL0y61RQe98eCTGp_n-eXE-GPxcyVpaNHpkfm3UlfwPqtAGuAaV7D8gu3woNMA54AtHQBiOf4Xx8U34zdLFfJeAdDOczybTYciwS-W8YdjWi7g9xjc1v9Iq2om_0ZNmaPwi6HEvVwPU4w63VtNyHeU-_R-ftPnywW1wEuTsqufWofetzAMM4x_3Un0OboNhf7LePoZ2cub96vJDyOMoSFIIj2xymVRWRLIkBV36VFqukCdpoJcuUmZRZL3Be9NQRSIs6cA7hvcLGZCj-zcACrPvEVOYQFGepW2S_2xdq6rdmbbQliyDfzwKqzw73dqcKFs1OXTp0-YOhTLS7UPWpiQxNDl5jB61cwq8mwjyBA3s9Cl6mJCcP0Nfe5pg73CkCQ40wIkmONIEA01w43GiCe5pgjuaPEenXz6f7I1Ju38GMVzKhpS1scIamzuqau5MocpasFrLvKCuErmwlBdW0splzDiYCIhaygqujMqldip7gbanfmpfIVwwXTmem0JYl9eUKQXjmzHJM1VSJ9hr9DJ9gYtZKpJy0X2bN7-1vEU7PaHeoQcORqV9DyFeoz9EPO4An2NSxw
link.rule.ids 783
linkProvider National Library of Medicine
openUrl ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Prediction+of+giant+spin+motive+force+due+to+Rashba+spin-orbit+coupling&rft.jtitle=Physical+review+letters&rft.au=Kim%2C+Kyoung-Whan&rft.au=Moon%2C+Jung-Hwan&rft.au=Lee%2C+Kyung-Jin&rft.au=Lee%2C+Hyun-Woo&rft.date=2012-05-23&rft.eissn=1079-7114&rft.volume=108&rft.issue=21&rft.spage=217202&rft_id=info:doi/10.1103%2Fphysrevlett.108.217202&rft_id=info%3Apmid%2F23003294&rft_id=info%3Apmid%2F23003294&rft.externalDocID=23003294