메뉴 건너뛰기




Volumn 80, Issue 15, 2009, Pages

Many-body electronic structure and Kondo properties of cobalt-porphyrin molecules

Author keywords

[No Author keywords available]

Indexed keywords


EID: 72449132992     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.80.155443     Document Type: Article
Times cited : (41)

References (47)
  • 14
    • 33745799041 scopus 로고    scopus 로고
    • 10.1021/nl0602847
    • P. Huang and E. A. Carter, Nano Lett. 6, 1146 (2006). 10.1021/nl0602847
    • (2006) Nano Lett. , vol.6 , pp. 1146
    • Huang, P.1    Carter, E.A.2
  • 16
    • 33747702246 scopus 로고    scopus 로고
    • 10.1103/PhysRevLett.97.076806
    • G. Chiappe and E. Louis, Phys. Rev. Lett. 97, 076806 (2006). 10.1103/PhysRevLett.97.076806
    • (2006) Phys. Rev. Lett. , vol.97 , pp. 076806
    • Chiappe, G.1    Louis, E.2
  • 18
    • 61349182274 scopus 로고    scopus 로고
    • 10.1021/nl0804203
    • P. Huang and E. A. Carter, Nano Lett. 8, 1265 (2008). 10.1021/nl0804203
    • (2008) Nano Lett. , vol.8 , pp. 1265
    • Huang, P.1    Carter, E.A.2
  • 23
    • 0035100639 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.63.085404
    • M. Plihal and J. W. Gadzuk, Phys. Rev. B 63, 085404 (2001). 10.1103/PhysRevB.63.085404
    • (2001) Phys. Rev. B , vol.63 , pp. 085404
    • Plihal, M.1    Gadzuk, J.W.2
  • 26
  • 34
    • 72449209450 scopus 로고    scopus 로고
    • http://www.ices.utexas.edu/parsec/
  • 41
    • 34347372420 scopus 로고    scopus 로고
    • 10.1103/PhysRevB.75.235102
    • M. Shishkin and G. Kresse, Phys. Rev. B 75, 235102 (2007). 10.1103/PhysRevB.75.235102
    • (2007) Phys. Rev. B , vol.75 , pp. 235102
    • Shishkin, M.1    Kresse, G.2
  • 42
    • 0001021183 scopus 로고
    • 10.1103/PhysRevB.47.15413
    • E. L. Shirley and R. M. Martin, Phys. Rev. B 47, 15413 (1993). 10.1103/PhysRevB.47.15413
    • (1993) Phys. Rev. B , vol.47 , pp. 15413
    • Shirley, E.L.1    Martin, R.M.2
  • 43
    • 72449120596 scopus 로고    scopus 로고
    • As a general rule, we can use the majority-minority splitting from GW to estimate U for partially occupied d orbitals in other TBrPP- M (M=transition metal-atom) compounds. The strength of U depends crucially on the total magnetization of the molecule (TBrPP-Mn, for instance, has values of U several eVs larger than TBrPP-Co) and on the strength of the TBrPP molecular field.
    • As a general rule, we can use the majority-minority splitting from GW to estimate U for partially occupied d orbitals in other TBrPP- M (M=transition metal-atom) compounds. The strength of U depends crucially on the total magnetization of the molecule (TBrPP-Mn, for instance, has values of U several eVs larger than TBrPP-Co) and on the strength of the TBrPP molecular field.
  • 44
    • 72449178721 scopus 로고    scopus 로고
    • The HOMO-1, HOMO-2, and HOMO-3 orbitals, although closer in energy to EF than 3 d z2, are localized further away from the center of the molecule level, with a high amplitude on the phenyl-bromine radicals. Thus, their contribution to the STM signal with the tip placed on top of the Co atom is negligible.
    • The HOMO-1, HOMO-2, and HOMO-3 orbitals, although closer in energy to EF than 3 d z2, are localized further away from the center of the molecule level, with a high amplitude on the phenyl-bromine radicals. Thus, their contribution to the STM signal with the tip placed on top of the Co atom is negligible.
  • 47
    • 72449197263 scopus 로고    scopus 로고
    • In this approximation, we are neglecting many-body contributions due to the Coulomb interactions between the electrons in orbital i entering the model (e.g., cobalt d3 z2 -1 electrons) and the electrons in the surface. Such contributions are likely to be much smaller than the interaction effects of electrons within orbital i, which are well captured by the GW calculation in vacuum.
    • In this approximation, we are neglecting many-body contributions due to the Coulomb interactions between the electrons in orbital i entering the model (e.g., cobalt d3 z2 -1 electrons) and the electrons in the surface. Such contributions are likely to be much smaller than the interaction effects of electrons within orbital i, which are well captured by the GW calculation in vacuum.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.