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Eds. A.R. Burns, E.B. Stechel and D.R. Jennison Springer, Berlin
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J.A. Prybyla, T.F. Heinz, J.A. Misewich, M.M.T. Loy and J.H. Glownia, Phys. Rev. Lett. 64 (1990) 1537; F. Budde, T.F. Heinz, A. Kalamarides, M.M.T. Loy and J.A. Misewich, Surf. Sci. 283 (1993) 143.
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19
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30244573154
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note
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c = 1.3 eV for NO/Cu(111), and a similar value is expected for NO/Ag(111).
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20
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3342922611
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Experimental values for D are 0.52 and 0.28 eV for CO/ Cu(111) and CO/Ag(111), respectively (see B. Hammer, Y. Morikawa and J.K. Nørskov, Phys. Rev. Lett. 76 (1996) 2141). Since D for NO/Ag(111) (though for bridge species) is estimated to be 0.26 eV (R.J. Behm and C.R. Brundle, J. Vac. Sci. Technol. A 2 (1984) 1040), which is similar to that for CO/Ag(111), D for NO/Cu(111) is expected to be about 0.5 eV.
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(1996)
Phys. Rev. Lett.
, vol.76
, pp. 2141
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Hammer, B.1
Morikawa, Y.2
Nørskov, J.K.3
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21
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0343294487
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Experimental values for D are 0.52 and 0.28 eV for CO/ Cu(111) and CO/Ag(111), respectively (see B. Hammer, Y. Morikawa and J.K. Nørskov, Phys. Rev. Lett. 76 (1996) 2141). Since D for NO/Ag(111) (though for bridge species) is estimated to be 0.26 eV (R.J. Behm and C.R. Brundle, J. Vac. Sci. Technol. A 2 (1984) 1040), which is similar to that for CO/Ag(111), D for NO/Cu(111) is expected to be about 0.5 eV.
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(1984)
J. Vac. Sci. Technol. A
, vol.2
, pp. 1040
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Behm, R.J.1
Brundle, C.R.2
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