메뉴 건너뛰기




Volumn 94, Issue 14, 2009, Pages

Impact of oxide defects on band offset at GeO2 /Ge interface

Author keywords

[No Author keywords available]

Indexed keywords

ATOMIC SOURCES; BAND ALIGNMENTS; BAND OFFSETS; CONDUCTION BAND OFFSETS; HIGH QUALITIES; HIGH RESOLUTIONS; OXIDATION STAGES; PROJECTED DENSITY OF STATE; VALENCE BAND OFFSETS; X-RAY PHOTOEMISSION SPECTROSCOPIES;

EID: 64349120851     PISSN: 00036951     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.3115824     Document Type: Article
Times cited : (70)

References (28)
  • 1
    • 31044455312 scopus 로고    scopus 로고
    • RPPHAG 0034-4885 10.1088/0034-4885/69/2/R02.
    • J. Robertson, Rep. Prog. Phys. RPPHAG 0034-4885 10.1088/0034-4885/69/2/ R02 69, 327 (2006).
    • (2006) Rep. Prog. Phys. , vol.69 , pp. 327
    • Robertson, J.1
  • 4
    • 0029273669 scopus 로고
    • SUSCAS 0039-6028 10.1016/0039-6028(94)00746-2.
    • K. Prabhakaran and T. Ogino, Surf. Sci. SUSCAS 0039-6028 10.1016/0039-6028(94)00746-2 325, 263 (1995).
    • (1995) Surf. Sci. , vol.325 , pp. 263
    • Prabhakaran, K.1    Ogino, T.2
  • 5
  • 9
    • 46749092958 scopus 로고    scopus 로고
    • JCPSA6 0021-9606 10.1063/1.2955446.
    • A. Molle, S. Spiga, and M. Fanciulli, J. Chem. Phys. JCPSA6 0021-9606 10.1063/1.2955446 129, 011104 (2008).
    • (2008) J. Chem. Phys. , vol.129 , pp. 011104
    • Molle, A.1    Spiga, S.2    Fanciulli, M.3
  • 16
    • 64349112732 scopus 로고    scopus 로고
    • According to Tanuma-Powell-Penn method (), the mean free path for Ge 3d photoelectron induced by Al radiation is around 3.3 nm.
    • According to Tanuma-Powell-Penn method (http://www.nist.gov/srd/nist71. htm), the mean free path for Ge 3d photoelectron induced by Al radiation is around 3.3 nm.
  • 19
    • 0033208007 scopus 로고    scopus 로고
    • SUSCAS 0039-6028 10.1016/S0039-6028(99)00866-3.
    • J. S. Hovis, R. J. Hamers, and C. M. Greenlief, Surf. Sci. SUSCAS 0039-6028 10.1016/S0039-6028(99)00866-3 440, L815 (1999).
    • (1999) Surf. Sci. , vol.440 , pp. 815
    • Hovis, J.S.1    Hamers, R.J.2    Greenlief, C.M.3
  • 20
    • 0037427849 scopus 로고    scopus 로고
    • SUSCAS 0039-6028 10.1016/S0039-6028(02)02354-3.
    • N. Tabet, M. Faiz, N. M. Hamdan, and Z. Hussain, Surf. Sci. SUSCAS 0039-6028 10.1016/S0039-6028(02)02354-3 523, 68 (2003).
    • (2003) Surf. Sci. , vol.523 , pp. 68
    • Tabet, N.1    Faiz, M.2    Hamdan, N.M.3    Hussain, Z.4
  • 22
    • 12844286241 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.47.558, ();, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.48.13115 48, 13115 (1993).
    • G. Kresse and H. Hafner, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.47.558 47, 558 (1993); G. Kresse and H. Hafner, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.48.13115 48, 13115 (1993).
    • (1993) Phys. Rev. B , vol.47 , pp. 558
    • Kresse, G.1    Hafner, H.2    Kresse, G.3    Hafner, H.4
  • 23
    • 0030190741 scopus 로고    scopus 로고
    • CMMSEM 0927-0256 10.1016/0927-0256(96)00008-0.
    • G. Kresse and J. Furthmuller, Comput. Mater. Sci. CMMSEM 0927-0256 10.1016/0927-0256(96)00008-0 6, 15 (1996).
    • (1996) Comput. Mater. Sci. , vol.6 , pp. 15
    • Kresse, G.1    Furthmuller, J.2
  • 24
    • 25744460922 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.50.17953.
    • P. E. Blöchl, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.50. 17953 50, 17953 (1994).
    • (1994) Phys. Rev. B , vol.50 , pp. 17953
    • Blöchl, P.E.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.