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Volumn 67, Issue 8, 2003, Pages 814031-814034

Origin of positive core-level shifts in Au clusters on oxides

Author keywords

[No Author keywords available]

Indexed keywords

GOLD DERIVATIVE; MAGNESIUM OXIDE; METAL OXIDE; OXIDE; TITANIUM DIOXIDE;

EID: 0037304686     PISSN: 01631829     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevB.67.081403     Document Type: Article
Times cited : (20)

References (32)
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    • Zongxian Yang, Ruqian Wu, and D.W. Goodman, Phys. Rev. B 61, 14 066 (2000); Zongxian Yang, Ruqian Wu, Qiming Zhang, and D.W. Goodman, ibid. 65, 155407 (2002).
    • (2000) Phys. Rev. B , vol.61 , pp. 14066
    • Yang, Z.1    Wu, R.2    Goodman, D.W.3
  • 18
    • 0037089364 scopus 로고    scopus 로고
    • Zongxian Yang, Ruqian Wu, and D.W. Goodman, Phys. Rev. B 61, 14 066 (2000); Zongxian Yang, Ruqian Wu, Qiming Zhang, and D.W. Goodman, ibid. 65, 155407 (2002).
    • (2002) Phys. Rev. B , vol.65 , pp. 155407
    • Yang, Z.1    Wu, R.2    Zhang, Q.3    Goodman, D.W.4
  • 19
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    • note
    • 2 show that the GGA overestimates the lattice parameters by about 2%-3%. By contrast, results of lattice sizes and bulk moduli obtained through the LDA agree well with experiment. Furthermore, the LDA is also known to describe the Au lattice better than does the GGA. The LDA is hence used here to determine the equilibrium structures.
  • 20
    • 33744589690 scopus 로고
    • J.M. Soler and A.R. Williams, Phys. Rev. B 40, 1560 (1989); R. Yu, D. Singh, and H. Krakauer, ibid. 43, 6411 (1992).
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    • Soler, J.M.1    Williams, A.R.2
  • 21
  • 29
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    • B for Au (001), Rh (001), and Pd (001) are -0.4 [P.H. Citrin et al., Phys. Rev. Lett. 41, 1425 (1978)], -0.65 eV [F. Strisland, Surf. Sci. 415, L1020 (1998)], and - 0.44 eV [R. Nyholm et al., J. Phys. C 4, 277 (1992)], respectively. These values are overall very close to our corresponding theoretical data, -0.64 eV, -0.67 eV, and -0.35 eV.
    • (1978) Phys. Rev. Lett. , vol.41 , pp. 1425
    • Citrin, P.H.1
  • 30
    • 0032500410 scopus 로고    scopus 로고
    • B for Au (001), Rh (001), and Pd (001) are -0.4 [P.H. Citrin et al., Phys. Rev. Lett. 41, 1425 (1978)], -0.65 eV [F. Strisland, Surf. Sci. 415, L1020 (1998)], and - 0.44 eV [R. Nyholm et al., J. Phys. C 4, 277 (1992)], respectively. These values are overall very close to our corresponding theoretical data, -0.64 eV, -0.67 eV, and -0.35 eV.
    • (1998) Surf. Sci. , vol.415 , pp. L1020
    • Strisland, F.1
  • 31
    • 0000108467 scopus 로고
    • B for Au (001), Rh (001), and Pd (001) are -0.4 [P.H. Citrin et al., Phys. Rev. Lett. 41, 1425 (1978)], -0.65 eV [F. Strisland, Surf. Sci. 415, L1020 (1998)], and - 0.44 eV [R. Nyholm et al., J. Phys. C 4, 277 (1992)], respectively. These values are overall very close to our corresponding theoretical data, -0.64 eV, -0.67 eV, and -0.35 eV.
    • (1992) J. Phys. C , vol.4 , pp. 277
    • Nyholm, R.1
  • 32
    • 84988739511 scopus 로고    scopus 로고
    • note
    • 2(110) 5.79 Å, and 6.35 Å, is still insufficient.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.