메뉴 건너뛰기




Volumn 80, Issue 15, 2009, Pages

Two-impurity Kondo model with spin-orbit interactions

Author keywords

[No Author keywords available]

Indexed keywords


EID: 72449131955     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.80.155302     Document Type: Article
Times cited : (32)

References (61)
  • 11
  • 12
  • 13
    • 34249913377 scopus 로고
    • 10.1103/PhysRev.106.893
    • K. Yosida, Phys. Rev. 106, 893 (1957). 10.1103/PhysRev.106.893
    • (1957) Phys. Rev. , vol.106 , pp. 893
    • Yosida, K.1
  • 14
    • 18144418587 scopus 로고    scopus 로고
    • 10.1103/PhysRevLett.94.086602
    • P. Simon, R. Lopez, and Y. Oreg, Phys. Rev. Lett. 94, 086602 (2005). 10.1103/PhysRevLett.94.086602
    • (2005) Phys. Rev. Lett. , vol.94 , pp. 086602
    • Simon, P.1    Lopez, R.2    Oreg, Y.3
  • 15
  • 19
    • 49149086665 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.78.035449
    • D. F. Mross and H. Johannesson, Phys. Rev. B 78, 035449 (2008). 10.1103/PhysRevB.78.035449
    • (2008) Phys. Rev. B , vol.78 , pp. 035449
    • Mross, D.F.1    Johannesson, H.2
  • 20
  • 23
    • 0003989585 scopus 로고    scopus 로고
    • edited by R. Kaiser, C. Westbrook, and F. David (Springer Verlag, Berlin
    • A. Ekert, P. M. Hayden, and H. Inamori, in Coherent Atomic Matter Waves, edited by, R. Kaiser, C. Westbrook, and, F. David, (Springer Verlag, Berlin, 2001).
    • (2001) Coherent Atomic Matter Waves
    • Ekert, A.1    Hayden, P.M.2    Inamori, H.3
  • 24
  • 27
    • 33749158677 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.72.033308
    • Y. Rikitake and H. Imamura, Phys. Rev. B 72, 033308 (2005). 10.1103/PhysRevB.72.033308
    • (2005) Phys. Rev. B , vol.72 , pp. 033308
    • Rikitake, Y.1    Imamura, H.2
  • 28
    • 33144471889 scopus 로고    scopus 로고
    • 10.1103/PhysRevA.73.012109
    • S. Y. Cho and R. H. McKenzie, Phys. Rev. A 73, 012109 (2006). 10.1103/PhysRevA.73.012109
    • (2006) Phys. Rev. A , vol.73 , pp. 012109
    • Cho, S.Y.1    McKenzie, R.H.2
  • 29
    • 4243684526 scopus 로고    scopus 로고
    • 10.1103/PhysRevLett.80.2245
    • W. K. Wootters, Phys. Rev. Lett. 80, 2245 (1998). 10.1103/PhysRevLett.80. 2245
    • (1998) Phys. Rev. Lett. , vol.80 , pp. 2245
    • Wootters, W.K.1
  • 34
    • 0036997184 scopus 로고    scopus 로고
    • 10.1103/PhysRevA.66.062314;
    • L.-A. Wu and D. A. Lidar, Phys. Rev. A 66, 062314 (2002) 10.1103/PhysRevA.66.062314
    • (2002) Phys. Rev. A , vol.66 , pp. 062314
    • Wu, L.-A.1    Lidar, D.A.2
  • 36
    • 27744439879 scopus 로고    scopus 로고
    • 10.1103/PhysRevLett.94.226803;
    • S. Debald and C. Emary, Phys. Rev. Lett. 94, 226803 (2005) 10.1103/PhysRevLett.94.226803
    • (2005) Phys. Rev. Lett. , vol.94 , pp. 226803
    • Debald, S.1    Emary, C.2
  • 38
  • 40
    • 35348989734 scopus 로고    scopus 로고
    • 10.1007/s10955-007-9414-x
    • J. Malecki, J. Stat. Phys. 129, 741 (2007). 10.1007/s10955-007-9414-x
    • (2007) J. Stat. Phys. , vol.129 , pp. 741
    • Malecki, J.1
  • 41
    • 4243343522 scopus 로고
    • 10.1103/PhysRev.100.580
    • G. Dresselhaus, Phys. Rev. 100, 580 (1955). 10.1103/PhysRev.100.580
    • (1955) Phys. Rev. , vol.100 , pp. 580
    • Dresselhaus, G.1
  • 43
    • 0012396897 scopus 로고
    • 10.1088/0022-3719/17/33/015
    • Y. A. Bychkov and E. I. Rashba, J. Phys. C 17, 6039 (1984). 10.1088/0022-3719/17/33/015
    • (1984) J. Phys. C , vol.17 , pp. 6039
    • Bychkov, Y.A.1    Rashba, E.I.2
  • 45
    • 0343826150 scopus 로고    scopus 로고
    • 10.1103/PhysRevLett.84.6074
    • D. Grundler, Phys. Rev. Lett. 84, 6074 (2000). 10.1103/PhysRevLett.84. 6074
    • (2000) Phys. Rev. Lett. , vol.84 , pp. 6074
    • Grundler, D.1
  • 49
    • 4243826847 scopus 로고
    • 10.1103/PhysRevLett.4.228
    • T. Moriya, Phys. Rev. Lett. 4, 228 (1960). 10.1103/PhysRevLett.4.228
    • (1960) Phys. Rev. Lett. , vol.4 , pp. 228
    • Moriya, T.1
  • 53
    • 72449187550 scopus 로고    scopus 로고
    • The physics does not, of course, depend on the order in which the system is set up. A similar argument holds for starting with the RKKY interaction and then adding the Kondo-screening channels.
    • The physics does not, of course, depend on the order in which the system is set up. A similar argument holds for starting with the RKKY interaction and then adding the Kondo-screening channels.
  • 54
    • 0000719127 scopus 로고
    • 10.1103/PhysRevB.40.324
    • B. A. Jones and C. M. Varma, Phys. Rev. B 40, 324 (1989). 10.1103/PhysRevB.40.324
    • (1989) Phys. Rev. B , vol.40 , pp. 324
    • Jones, B.A.1    Varma, C.M.2
  • 55
    • 33745666442 scopus 로고
    • 10.1103/PhysRevB.51.8287
    • J. Gan, Phys. Rev. B 51, 8287 (1995). 10.1103/PhysRevB.51.8287
    • (1995) Phys. Rev. B , vol.51 , pp. 8287
    • Gan, J.1
  • 56
    • 72449162134 scopus 로고    scopus 로고
    • The marginal operator O that becomes allowed in the presence of a Dzyaloshinski-Moriya interaction can be written as O= (h1†) A (h2) A y, where hi are isospin- SU (2) 1 Wess-Zumino-Witten (WZW) fields with spin 1/2 and is a spin- SU (2) 2 WZW field with spin 1 (Ref.).
    • The marginal operator O that becomes allowed in the presence of a Dzyaloshinski-Moriya interaction can be written as O= (h1†) A (h2) A y, where hi are isospin- SU (2) 1 Wess-Zumino-Witten (WZW) fields with spin 1/2 and is a spin- SU (2) 2 WZW field with spin 1 (Ref.).
  • 57
    • 72449120902 scopus 로고    scopus 로고
    • Conversely, a system that is not critical at first may become critical upon introducing spin-orbit interactions.
    • Conversely, a system that is not critical at first may become critical upon introducing spin-orbit interactions.
  • 58
    • 72449189188 scopus 로고    scopus 로고
    • It should be kept in mind that in the presence of charge transfer, the fixed point is stable only in the case of particle-hole symmetry (Ref.).
    • It should be kept in mind that in the presence of charge transfer, the fixed point is stable only in the case of particle-hole symmetry (Ref.).
  • 61
    • 2942610744 scopus 로고    scopus 로고
    • For a review, see 10.1103/RevModPhys.76.323
    • For a review, see I. ZCtić Jaroslav Fabian, and S. Das Sarma, Rev. Mod. Phys. 76, 323 (2004). 10.1103/RevModPhys.76.323
    • (2004) Rev. Mod. Phys. , vol.76 , pp. 323
    • Zctić, I.1    Fabian, J.2    Das Sarma, S.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.