-
2
-
-
0035252138
-
-
S. N. Taraskin, Y. L. Loh, G. Natarajan, and S. R. Elliott, Phys. Rev. Lett. 86, 1255 (2001).
-
(2001)
Phys. Rev. Lett.
, vol.86
, pp. 1255
-
-
Taraskin, S.N.1
Loh, Y.L.2
Natarajan, G.3
Elliott, S.R.4
-
6
-
-
0001538315
-
-
A. P. Sokolov, U. Buchenau, W. Steffen, B. Frick, and A. Wischnewski, Phys. Rev. B 52, R9815 (1995).
-
(1995)
Phys. Rev. B
, vol.52
, pp. 9815
-
-
Sokolov, A.P.1
Buchenau, U.2
Steffen, W.3
Frick, B.4
Wischnewski, A.5
-
14
-
-
0035826590
-
-
V. Martin-Mayor, M. M̀zard, G. Parisi, and P. Verrocchio, J. Chem. Phys. 114, 8068 (2001).
-
(2001)
J. Chem. Phys.
, vol.114
, pp. 8068
-
-
Martin-Mayor, V.1
M̀zard, M.2
Parisi, G.3
Verrocchio, P.4
-
15
-
-
0035920918
-
-
T. S. Grigera, V. Martin-Mayor, G. Parisi, and P. Verrocchio, Phys. Rev. Lett. 87, 085502 (2001).
-
(2001)
Phys. Rev. Lett.
, vol.87
, pp. 085502
-
-
Grigera, T.S.1
Martin-Mayor, V.2
Parisi, G.3
Verrocchio, P.4
-
16
-
-
0242414555
-
-
S. Ciliberti, T. S. Grigera, V. Martin-Mayor, G. Parisi, and P. Verrocchio, J. Chem. Phys. 119, 8577 (2003).
-
(2003)
J. Chem. Phys.
, vol.119
, pp. 8577
-
-
Ciliberti, S.1
Grigera, T.S.2
Martin-Mayor, V.3
Parisi, G.4
Verrocchio, P.5
-
18
-
-
0000456245
-
-
R. E. Larsen, E. F. David, G. Goodyear, and R. M. Stratt, J. Chem. Phys. 107, 524 (1997).
-
(1997)
J. Chem. Phys.
, vol.107
, pp. 524
-
-
Larsen, R.E.1
David, E.F.2
Goodyear, G.3
Stratt, R.M.4
-
28
-
-
0141815508
-
-
A. Medina, J. M. M. Roco, A. Calvo Hernandez, and S. Velasco, J. Chem. Phys. 119, 5176 (2003).
-
(2003)
J. Chem. Phys.
, vol.119
, pp. 5176
-
-
Medina, A.1
Roco, J.M.M.2
Calvo, H.A.3
Velasco, S.4
-
29
-
-
20844441525
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-
note
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In Ref. 18, the binary mode of a MNN pair is only referred for the vibrational motion of the two particles.
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-
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30
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20844434271
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note
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ij, relative to the reference frame of the imulation cubic box.
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32
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20844463514
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note
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To investigate any finite-size effects of the MD simulation on the numerical data of the perturbed binary-mode DOS shown in Fig. 6, we have performed similar calculations for 500 configurations of 1728 particles and 2000 configurations of 432 particles at the same thermodynamic conditions. The results turn out to be that there is no noticeable difference around the cusp in the curves obtained from 1728 and 864 particles. For the system of 432 particles, the system size has some weak effect on the width of the cusp, which is slightly narrower than those of 864 and 1728 particles. This investigation indicates that the system size of 864 particles is large enough to neglect the boundary effects of the MD simulation box on the perturbation calculations for the numerical curves shown in Fig. 6.
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33
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20844458675
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note
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We have tested the numerical accuracy of our calculations for the cusp in the DOS of the perturbed vibrational binary modes by dividing the width of the frequency histograms into half. The results show that the shape of the cusp does not change at all.
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2442652840
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E. Duval, A. Mermet, R. Le Parc, and B. Champagnon, Philos. Mag. 84, 1433 (2004).
-
(2004)
Philos. Mag.
, vol.84
, pp. 1433
-
-
Duval, E.1
Mermet, A.2
Le Parc, R.3
Champagnon, B.4
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