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1
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0000795243
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For an impressive bibliography, see
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For an impressive bibliography, see W F. Egelhoff, J. Appl. Phys.79, 2491 (1996).
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(1996)
J. Appl. Phys.
, vol.79
, pp. 2491
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Egelhoff, W.F.1
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15
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26144450583
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as parametrized by, and
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as parametrized by J. Perdew and A. Zunger, Phys. Rev. B23, 5048 (1981).
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(1981)
Phys. Rev. B
, vol.23
, pp. 5048
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Perdew, J.1
Zunger, A.2
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16
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0003754095
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P. Ziesche, H. Eschrig, Akademie-Verlag, Berlin, in, edited by, and
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J P. Perdew, in Electronic Structure of Solids ’91, edited by P. Ziesche and H. Eschrig (Akademie-Verlag, Berlin, 1991);
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(1991)
Electronic Structure of Solids ’91
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Perdew, J.P.1
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22
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85038968787
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unpublished)
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and (unpublished).
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23
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0003692531
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B. J. Berne, G. Ciccotti, D. F. Coker, World Scientific, Singapore, and, in, edited by, and
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H. Jónsson, G. Mills, and K W. Jacobsen, in Classical and Quantum Dynamics in Condensed Phase Simulations, edited by B. J. Berne, G. Ciccotti, and D. F. Coker (World Scientific, Singapore, 1998).
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(1998)
Classical and Quantum Dynamics in Condensed Phase Simulations
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Jónsson, H.1
Mills, G.2
Jacobsen, K.W.3
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85038909608
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Since the NEB calculation provides not just the energy at each replica geometry, but also the energy gradient along the chain of states, a two-node calculation provides four pieces of information, quite enough to construct a smooth spline fit: R. Stumpf (unpublished)
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Since the NEB calculation provides not just the energy at each replica geometry, but also the energy gradient along the chain of states, a two-node calculation provides four pieces of information, quite enough to construct a smooth spline fit: R. Stumpf (unpublished).
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30
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85038954391
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G. Kresse, Guide, http://cms.mpi.univie.ac.at/vasp/guide/node143.html
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G. Kresse, VASP Guide, http://cms.mpi.univie.ac.at/vasp/guide/node143.html.
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0001653755
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LDA and GGA estimates of the work function of Pt(001), obtained in the present work, are 6.1 and 5.7 eV. According to early field emission measurements [, and
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LDA and GGA estimates of the work function of Pt(001), obtained in the present work, are 6.1 and 5.7 eV. According to early field emission measurements [B E. Nieuwenhuys and W H M. Sachtler, Surf. Sci.34, 317 (1973)].
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(1973)
Surf. Sci.
, vol.34
, pp. 317
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Nieuwenhuys, B.E.1
Sachtler, W.H.M.2
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32
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0003240052
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the Pt(001) and Pt(111) work functions are 5.84 and 5.93 eV. These results are reasonably consistent with a more recent photoemission-threshold value of (formula presented) for Pt(111) and
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the Pt(001) and Pt(111) work functions are 5.84 and 5.93 eV. These results are reasonably consistent with a more recent photoemission-threshold value of (formula presented) for Pt(111) [G N. Derry and Z. Ji-Zhong, Phys. Rev. B39, 1940 (1989)].
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(1989)
Phys. Rev. B
, vol.39
, pp. 1940
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Derry, G.N.1
Ji-Zhong, Z.2
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85038943248
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This was inadvertent. On abandoning efforts to converge the electron densities of seven-layer Pt(001) slabs in favor of the more stable five-layer case, I neglected to reduce the width of the periodically repeated cell. I did reduce it, though, to ∼3 Å for calculations with a 1.5-V/Å external field
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This was inadvertent. On abandoning efforts to converge the electron densities of seven-layer Pt(001) slabs in favor of the more stable five-layer case, I neglected to reduce the width of the periodically repeated cell. I did reduce it, though, to ∼3 Å for calculations with a 1.5-V/Å external field.
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34
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85038970595
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Here as everywhere in this article, a positive field is defined as a field that pushes electrons into the metal
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Here as everywhere in this article, a positive field is defined as a field that pushes electrons into the metal.
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35
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85038943814
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The ratio of hopping to concerted substitution prefactors should perhaps be taken more seriously, both in the theoretical and experimental analyses. The results in Table I make it clear that as the external field increases from -0.4 to 0.8 V/Å, the energy of the symmetric dimer configuration rises until it is virtually equal to the energy of the concerted substitution barrier. At 0.8 V/Å, the energy hypersurface for concerted substitution is unusually flat in the vicinity of the transition geometry, and one might expect a larger than usual concerted-substitution prefactor. (Note that to compare the energies of symmetric dimer and the transition state for each field strength, subtract the hollow-site binding energy in column 1 of Table I from the symmetric exchange energy in column 3 and compare the result to the substitution barrier energy in column 5.)
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The ratio of hopping to concerted substitution prefactors should perhaps be taken more seriously, both in the theoretical and experimental analyses. The results in Table I make it clear that as the external field increases from -0.4 to 0.8 V/Å, the energy of the symmetric dimer configuration rises until it is virtually equal to the energy of the concerted substitution barrier. At 0.8 V/Å, the energy hypersurface for concerted substitution is unusually flat in the vicinity of the transition geometry, and one might expect a larger than usual concerted-substitution prefactor. (Note that to compare the energies of symmetric dimer and the transition state for each field strength, subtract the hollow-site binding energy in column 1 of Table I from the symmetric exchange energy in column 3 and compare the result to the substitution barrier energy in column 5.)
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