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S. Tarucha, D.G. Austing, T. Honda, R.J. van der Hage, and L.P. Kouwenhoven, Phys. Rev. Lett. 77, 3613 (1996).
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Phys. Rev. Lett.
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Kouwenhoven, L.P.5
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4
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0003372328
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edited by L. L. Sohn, L. P. Kouwenhoven, and G. Schön (Kluwer, Dordrecht)
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L. P. Kouwenhoven, C. M. Marcus, P. L. McEuen, S. Tarucha, R. M. Westervelt, and N. S. Wingreen, Vol. 345 of NATO Advanced Study Institute, Series E, edited by L. L. Sohn, L. P. Kouwenhoven, and G. Schön (Kluwer, Dordrecht, 1997), p. 105.
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Kouwenhoven, L.P.1
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Tarucha, S.4
Westervelt, R.M.5
Wingreen, N.S.6
-
8
-
-
0001365398
-
-
See, e.g., exact calculations by M. Eto, Jpn. J. Appl. Phys., Part 1 36, 3924 (1997); Hartree-Fock calculations by A. Natori, Y. Sugimoto, and M. Fujito, ibid. 36, 3960 (1997); H. Tamura, Physica (Amsterdam) 249B-251B, 210 (1998); M. Rontani, F. Rossi, F. Manghi, and E. Molinari, Phys. Rev. B 59, 10 165 (1999); the spin density-functional theory at B = 0 by In-Ho Lee, V. Rao, R.M. Martin, and J.P. Leburton, ibid. 57, 9035 (1998) and Ref. 43; and also at nonzero B by O. Steffen, U. Rössler, and M. Suhrke, Europhys. Lett. 42, 529 (1998).
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(1997)
Jpn. J. Appl. Phys., Part 1
, vol.36
, pp. 3924
-
-
Eto, M.1
-
9
-
-
0001755108
-
-
See, e.g., exact calculations by M. Eto, Jpn. J. Appl. Phys., Part 1 36, 3924 (1997); Hartree-Fock calculations by A. Natori, Y. Sugimoto, and M. Fujito, ibid. 36, 3960 (1997); H. Tamura, Physica (Amsterdam) 249B-251B, 210 (1998); M. Rontani, F. Rossi, F. Manghi, and E. Molinari, Phys. Rev. B 59, 10 165 (1999); the spin density-functional theory at B = 0 by In-Ho Lee, V. Rao, R.M. Martin, and J.P. Leburton, ibid. 57, 9035 (1998) and Ref. 43; and also at nonzero B by O. Steffen, U. Rössler, and M. Suhrke, Europhys. Lett. 42, 529 (1998).
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(1997)
Jpn. J. Appl. Phys., Part 1
, vol.36
, pp. 3960
-
-
Natori, A.1
Sugimoto, Y.2
Fujito, M.3
-
10
-
-
0032093373
-
-
See, e.g., exact calculations by M. Eto, Jpn. J. Appl. Phys., Part 1 36, 3924 (1997); Hartree-Fock calculations by A. Natori, Y. Sugimoto, and M. Fujito, ibid. 36, 3960 (1997); H. Tamura, Physica (Amsterdam) 249B-251B, 210 (1998); M. Rontani, F. Rossi, F. Manghi, and E. Molinari, Phys. Rev. B 59, 10 165 (1999); the spin density-functional theory at B = 0 by In-Ho Lee, V. Rao, R.M. Martin, and J.P. Leburton, ibid. 57, 9035 (1998) and Ref. 43; and also at nonzero B by O. Steffen, U. Rössler, and M. Suhrke, Europhys. Lett. 42, 529 (1998).
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(1998)
Physica (Amsterdam)
, vol.249-251 B
, pp. 210
-
-
Tamura, H.1
-
11
-
-
0000848450
-
-
See, e.g., exact calculations by M. Eto, Jpn. J. Appl. Phys., Part 1 36, 3924 (1997); Hartree-Fock calculations by A. Natori, Y. Sugimoto, and M. Fujito, ibid. 36, 3960 (1997); H. Tamura, Physica (Amsterdam) 249B-251B, 210 (1998); M. Rontani, F. Rossi, F. Manghi, and E. Molinari, Phys. Rev. B 59, 10 165 (1999); the spin density-functional theory at B = 0 by In-Ho Lee, V. Rao, R.M. Martin, and J.P. Leburton, ibid. 57, 9035 (1998) and Ref. 43; and also at nonzero B by O. Steffen, U. Rössler, and M. Suhrke, Europhys. Lett. 42, 529 (1998).
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(1999)
Phys. Rev. B
, vol.59
, pp. 10165
-
-
Rontani, M.1
Rossi, F.2
Manghi, F.3
Molinari, E.4
-
12
-
-
0000573397
-
-
See, e.g., exact calculations by M. Eto, Jpn. J. Appl. Phys., Part 1 36, 3924 (1997); Hartree-Fock calculations by A. Natori, Y. Sugimoto, and M. Fujito, ibid. 36, 3960 (1997); H. Tamura, Physica (Amsterdam) 249B-251B, 210 (1998); M. Rontani, F. Rossi, F. Manghi, and E. Molinari, Phys. Rev. B 59, 10 165 (1999); the spin density-functional theory at B = 0 by In-Ho Lee, V. Rao, R.M. Martin, and J.P. Leburton, ibid. 57, 9035 (1998) and Ref. 43; and also at nonzero B by O. Steffen, U. Rössler, and M. Suhrke, Europhys. Lett. 42, 529 (1998).
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(1998)
Phys. Rev. B
, vol.57
, pp. 9035
-
-
Lee, I.-H.1
Rao, V.2
Martin, R.M.3
Leburton, J.P.4
-
13
-
-
0041169206
-
-
See, e.g., exact calculations by M. Eto, Jpn. J. Appl. Phys., Part 1 36, 3924 (1997); Hartree-Fock calculations by A. Natori, Y. Sugimoto, and M. Fujito, ibid. 36, 3960 (1997); H. Tamura, Physica (Amsterdam) 249B-251B, 210 (1998); M. Rontani, F. Rossi, F. Manghi, and E. Molinari, Phys. Rev. B 59, 10 165 (1999); the spin density-functional theory at B = 0 by In-Ho Lee, V. Rao, R.M. Martin, and J.P. Leburton, ibid. 57, 9035 (1998) and Ref. 43; and also at nonzero B by O. Steffen, U. Rössler, and M. Suhrke, Europhys. Lett. 42, 529 (1998).
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(1998)
Europhys. Lett.
, vol.42
, pp. 529
-
-
Steffen, O.1
Rössler, U.2
Suhrke, M.3
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16
-
-
0000294919
-
-
For studies pertaining to the geometrical arrangements of classical point charges in a harmonic confinement, see Yu.E. Lozovik, Usp. Fiz. Nauk 153, 356 (1987) [Sov. Phys. Usp. 30, 912 (1987)]; V.M. Bedanov and F.M. Peeters, Phys. Rev. B 49, 2667 (1994).
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(1987)
Usp. Fiz. Nauk
, vol.153
, pp. 356
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Lozovik, Yu.E.1
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17
-
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0041514804
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For studies pertaining to the geometrical arrangements of classical point charges in a harmonic confinement, see Yu.E. Lozovik, Usp. Fiz. Nauk 153, 356 (1987) [Sov. Phys. Usp. 30, 912 (1987)]; V.M. Bedanov and F.M. Peeters, Phys. Rev. B 49, 2667 (1994).
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(1987)
Sov. Phys. Usp.
, vol.30
, pp. 912
-
-
-
18
-
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23544464319
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For studies pertaining to the geometrical arrangements of classical point charges in a harmonic confinement, see Yu.E. Lozovik, Usp. Fiz. Nauk 153, 356 (1987) [Sov. Phys. Usp. 30, 912 (1987)]; V.M. Bedanov and F.M. Peeters, Phys. Rev. B 49, 2667 (1994).
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(1994)
Phys. Rev. B
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, pp. 2667
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Bedanov, V.M.1
Peeters, F.M.2
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19
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0344717984
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W via path-integral Monte Carlo simulations [R. Egger, W. Häusler, C.H. Mak, and H. Grabert, Phys. Rev. Lett. 82, 3320 (1999)]. Since the doubly humped radial electron densities are compatible with the (1,N -1) polygonal structures of classical point charges in the range 6 ≤ N ≤ 8 (after carrying out an azimuthal averaging), this crossover was interpreted as indicating the formation of WM's.
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(1999)
Phys. Rev. Lett.
, vol.82
, pp. 3320
-
-
-
25
-
-
0000336180
-
-
Unlike the HF approach for which a fully developed theory for the restoration of symmetries has long been established (see Sec. IB), the breaking of symmetries within the spin-dependent density functional theory poses a serious dilemma [J.P. Perdew, A. Savin, and K. Burke, Phys. Rev. A 51, 4531 (1995)]. This dilemma has not been resolved todate; several remedies (like projection, ensembles, etc.) are being proposed, but none of them appears to be completely devoid of inconsistencies [A. Savin, in Recent Developments and Applications of Modern Density Functional Theory, edited by J. M. Seminario (Elsevier, Amsterdam, 1996), p. 327]. In addition, due to the unphysical self-interaction energy (which vigorously and erroneously assists the kinetic energy in orbital delocalization), the density functional theory is more resistant against space symmetry breaking [R. Bauernschmitt and R. Ahlrichs, J. Chem. Phys. 104, 9047 (1996)] than the sS-UHF, and thus it fails to describe a whole class of broken symmetries involving electron localization, e.g., the formation at B = 0 of Wigner molecules in QD's (see footnote 7 in Ref. 9), the hole trapping at A1 impurities in silica [J. Laegsgaard and K. Stokbro, Phys. Rev. Lett. 86, 2834 (2001); G. Pacchioni, F. Frigoli, D. Ricci, and J.A. Weil, Phys. Rev. B 63, 054102 (2001)], or the interaction driven localization-delocalization transition in d- and f-electron systems [see, e.g., Strong Coulomb Correlations in Electronic Structure Calculations: Beyond the Local Density Approximation, edited by V. I. Anisimov (Gordon & Breach, Amsterdam, 2000); S.Y. Savrasov, G. Kotliar, and E. Abrahams, Nature (London) 410, 793 (2001)]. In line with the above, no density functional calculations describing space symmetry breaking and formation of Wigner molecules at B = 0 in circular QD's have been reported to date.
-
(1995)
Phys. Rev. A
, vol.51
, pp. 4531
-
-
Perdew, J.P.1
Savin, A.2
Burke, K.3
-
26
-
-
0000336180
-
-
edited by J. M. Seminario (Elsevier, Amsterdam)
-
Unlike the HF approach for which a fully developed theory for the restoration of symmetries has long been established (see Sec. IB), the breaking of symmetries within the spin-dependent density functional theory poses a serious dilemma [J.P. Perdew, A. Savin, and K. Burke, Phys. Rev. A 51, 4531 (1995)]. This dilemma has not been resolved todate; several remedies (like projection, ensembles, etc.) are being proposed, but none of them appears to be completely devoid of inconsistencies [A. Savin, in Recent Developments and Applications of Modern Density Functional Theory, edited by J. M. Seminario (Elsevier, Amsterdam, 1996), p. 327]. In addition, due to the unphysical self-interaction energy (which vigorously and erroneously assists the kinetic energy in orbital delocalization), the density functional theory is more resistant against space symmetry breaking [R. Bauernschmitt and R. Ahlrichs, J. Chem. Phys. 104, 9047 (1996)] than the sS-UHF, and thus it fails to describe a whole class of broken symmetries involving electron localization, e.g., the formation at B = 0 of Wigner molecules in QD's (see footnote 7 in Ref. 9), the hole trapping at A1 impurities in silica [J. Laegsgaard and K. Stokbro, Phys. Rev. Lett. 86, 2834 (2001); G. Pacchioni, F. Frigoli, D. Ricci, and J.A. Weil, Phys. Rev. B 63, 054102 (2001)], or the interaction driven localization-delocalization transition in d- and f-electron systems [see, e.g., Strong Coulomb Correlations in Electronic Structure Calculations: Beyond the Local Density Approximation, edited by V. I. Anisimov (Gordon & Breach, Amsterdam, 2000); S.Y. Savrasov, G. Kotliar, and E. Abrahams, Nature (London) 410, 793 (2001)]. In line with the above, no density functional calculations describing space symmetry breaking and formation of Wigner molecules at B = 0 in circular QD's have been reported to date.
-
(1996)
Recent Developments and Applications of Modern Density Functional Theory
, pp. 327
-
-
Savin, A.1
-
27
-
-
0001122358
-
-
Unlike the HF approach for which a fully developed theory for the restoration of symmetries has long been established (see Sec. IB), the breaking of symmetries within the spin-dependent density functional theory poses a serious dilemma [J.P. Perdew, A. Savin, and K. Burke, Phys. Rev. A 51, 4531 (1995)]. This dilemma has not been resolved todate; several remedies (like projection, ensembles, etc.) are being proposed, but none of them appears to be completely devoid of inconsistencies [A. Savin, in Recent Developments and Applications of Modern Density Functional Theory, edited by J. M. Seminario (Elsevier, Amsterdam, 1996), p. 327]. In addition, due to the unphysical self-interaction energy (which vigorously and erroneously assists the kinetic energy in orbital delocalization), the density functional theory is more resistant against space symmetry breaking [R. Bauernschmitt and R. Ahlrichs, J. Chem. Phys. 104, 9047 (1996)] than the sS-UHF, and thus it fails to describe a whole class of broken symmetries involving electron localization, e.g., the formation at B = 0 of Wigner molecules in QD's (see footnote 7 in Ref. 9), the hole trapping at A1 impurities in silica [J. Laegsgaard and K. Stokbro, Phys. Rev. Lett. 86, 2834 (2001); G. Pacchioni, F. Frigoli, D. Ricci, and J.A. Weil, Phys. Rev. B 63, 054102 (2001)], or the interaction driven localization-delocalization transition in d- and f-electron systems [see, e.g., Strong Coulomb Correlations in Electronic Structure Calculations: Beyond the Local Density Approximation, edited by V. I. Anisimov (Gordon & Breach, Amsterdam, 2000); S.Y. Savrasov, G. Kotliar, and E. Abrahams, Nature (London) 410, 793 (2001)]. In line with the above, no density functional calculations describing space symmetry breaking and formation of Wigner molecules at B = 0 in circular QD's have been reported to date.
-
(1996)
J. Chem. Phys.
, vol.104
, pp. 9047
-
-
Bauernschmitt, R.1
Ahlrichs, R.2
-
28
-
-
0035952915
-
-
Unlike the HF approach for which a fully developed theory for the restoration of symmetries has long been established (see Sec. IB), the breaking of symmetries within the spin-dependent density functional theory poses a serious dilemma [J.P. Perdew, A. Savin, and K. Burke, Phys. Rev. A 51, 4531 (1995)]. This dilemma has not been resolved todate; several remedies (like projection, ensembles, etc.) are being proposed, but none of them appears to be completely devoid of inconsistencies [A. Savin, in Recent Developments and Applications of Modern Density Functional Theory, edited by J. M. Seminario (Elsevier, Amsterdam, 1996), p. 327]. In addition, due to the unphysical self-interaction energy (which vigorously and erroneously assists the kinetic energy in orbital delocalization), the density functional theory is more resistant against space symmetry breaking [R. Bauernschmitt and R. Ahlrichs, J. Chem. Phys. 104, 9047 (1996)] than the sS-UHF, and thus it fails to describe a whole class of broken symmetries involving electron localization, e.g., the formation at B = 0 of Wigner molecules in QD's (see footnote 7 in Ref. 9), the hole trapping at A1 impurities in silica [J. Laegsgaard and K. Stokbro, Phys. Rev. Lett. 86, 2834 (2001); G. Pacchioni, F. Frigoli, D. Ricci, and J.A. Weil, Phys. Rev. B 63, 054102 (2001)], or the interaction driven localization-delocalization transition in d- and f-electron systems [see, e.g., Strong Coulomb Correlations in Electronic Structure Calculations: Beyond the Local Density Approximation, edited by V. I. Anisimov (Gordon & Breach, Amsterdam, 2000); S.Y. Savrasov, G. Kotliar, and E. Abrahams, Nature (London) 410, 793 (2001)]. In line with the above, no density functional calculations describing space symmetry breaking and formation of Wigner molecules at B = 0 in circular QD's have been reported to date.
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(2001)
Phys. Rev. Lett.
, vol.86
, pp. 2834
-
-
Laegsgaard, J.1
Stokbro, K.2
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29
-
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0035134711
-
-
Unlike the HF approach for which a fully developed theory for the restoration of symmetries has long been established (see Sec. IB), the breaking of symmetries within the spin-dependent density functional theory poses a serious dilemma [J.P. Perdew, A. Savin, and K. Burke, Phys. Rev. A 51, 4531 (1995)]. This dilemma has not been resolved todate; several remedies (like projection, ensembles, etc.) are being proposed, but none of them appears to be completely devoid of inconsistencies [A. Savin, in Recent Developments and Applications of Modern Density Functional Theory, edited by J. M. Seminario (Elsevier, Amsterdam, 1996), p. 327]. In addition, due to the unphysical self-interaction energy (which vigorously and erroneously assists the kinetic energy in orbital delocalization), the density functional theory is more resistant against space symmetry breaking [R. Bauernschmitt and R. Ahlrichs, J. Chem. Phys. 104, 9047 (1996)] than the sS-UHF, and thus it fails to describe a whole class of broken symmetries involving electron localization, e.g., the formation at B = 0 of Wigner molecules in QD's (see footnote 7 in Ref. 9), the hole trapping at A1 impurities in silica [J. Laegsgaard and K. Stokbro, Phys. Rev. Lett. 86, 2834 (2001); G. Pacchioni, F. Frigoli, D. Ricci, and J.A. Weil, Phys. Rev. B 63, 054102 (2001)], or the interaction driven localization-delocalization transition in d- and f-electron systems [see, e.g., Strong Coulomb Correlations in Electronic Structure Calculations: Beyond the Local Density Approximation, edited by V. I. Anisimov (Gordon & Breach, Amsterdam, 2000); S.Y. Savrasov, G. Kotliar, and E. Abrahams, Nature (London) 410, 793 (2001)]. In line with the above, no density functional calculations describing space symmetry breaking and formation of Wigner molecules at B = 0 in circular QD's have been reported to date.
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(2001)
Phys. Rev. B
, vol.63
, pp. 054102
-
-
Pacchioni, G.1
Frigoli, F.2
Ricci, D.3
Weil, J.A.4
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30
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-
0000336180
-
-
edited by V. I. Anisimov (Gordon & Breach, Amsterdam
-
Unlike the HF approach for which a fully developed theory for the restoration of symmetries has long been established (see Sec. IB), the breaking of symmetries within the spin-dependent density functional theory poses a serious dilemma [J.P. Perdew, A. Savin, and K. Burke, Phys. Rev. A 51, 4531 (1995)]. This dilemma has not been resolved todate; several remedies (like projection, ensembles, etc.) are being proposed, but none of them appears to be completely devoid of inconsistencies [A. Savin, in Recent Developments and Applications of Modern Density Functional Theory, edited by J. M. Seminario (Elsevier, Amsterdam, 1996), p. 327]. In addition, due to the unphysical self-interaction energy (which vigorously and erroneously assists the kinetic energy in orbital delocalization), the density functional theory is more resistant against space symmetry breaking [R. Bauernschmitt and R. Ahlrichs, J. Chem. Phys. 104, 9047 (1996)] than the sS-UHF, and thus it fails to describe a whole class of broken symmetries involving electron localization, e.g., the formation at B = 0 of Wigner molecules in QD's (see footnote 7 in Ref. 9), the hole trapping at A1 impurities in silica [J. Laegsgaard and K. Stokbro, Phys. Rev. Lett. 86, 2834 (2001); G. Pacchioni, F. Frigoli, D. Ricci, and J.A. Weil, Phys. Rev. B 63, 054102 (2001)], or the interaction driven localization-delocalization transition in d- and f-electron systems [see, e.g., Strong Coulomb Correlations in Electronic Structure Calculations: Beyond the Local Density Approximation, edited by V. I. Anisimov (Gordon & Breach, Amsterdam, 2000); S.Y. Savrasov, G. Kotliar, and E. Abrahams, Nature (London) 410, 793 (2001)]. In line with the above, no density functional calculations describing space symmetry breaking and formation of Wigner molecules at B = 0 in circular QD's have been reported to date.
-
(2000)
Strong Coulomb Correlations in Electronic Structure Calculations: Beyond the Local Density Approximation
-
-
-
31
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0035848894
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Unlike the HF approach for which a fully developed theory for the restoration of symmetries has long been established (see Sec. IB), the breaking of symmetries within the spin-dependent density functional theory poses a serious dilemma [J.P. Perdew, A. Savin, and K. Burke, Phys. Rev. A 51, 4531 (1995)]. This dilemma has not been resolved todate; several remedies (like projection, ensembles, etc.) are being proposed, but none of them appears to be completely devoid of inconsistencies [A. Savin, in Recent Developments and Applications of Modern Density Functional Theory, edited by J. M. Seminario (Elsevier, Amsterdam, 1996), p. 327]. In addition, due to the unphysical self-interaction energy (which vigorously and erroneously assists the kinetic energy in orbital delocalization), the density functional theory is more resistant against space symmetry breaking [R. Bauernschmitt and R. Ahlrichs, J. Chem. Phys. 104, 9047 (1996)] than the sS-UHF, and thus it fails to describe a whole class of broken symmetries involving electron localization, e.g., the formation at B = 0 of Wigner molecules in QD's (see footnote 7 in Ref. 9), the hole trapping at A1 impurities in silica [J. Laegsgaard and K. Stokbro, Phys. Rev. Lett. 86, 2834 (2001); G. Pacchioni, F. Frigoli, D. Ricci, and J.A. Weil, Phys. Rev. B 63, 054102 (2001)], or the interaction driven localization-delocalization transition in d- and f-electron systems [see, e.g., Strong Coulomb Correlations in Electronic Structure Calculations: Beyond the Local Density Approximation, edited by V. I. Anisimov (Gordon & Breach, Amsterdam, 2000); S.Y. Savrasov, G. Kotliar, and E. Abrahams, Nature (London) 410, 793 (2001)]. In line with the above, no density functional calculations describing space symmetry breaking and formation of Wigner molecules at B = 0 in circular QD's have been reported to date.
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Nature (London)
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Savrasov, S.Y.1
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33646599147
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note
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See in particular Chaps. 5.5 and 11 in Ref. 25. However, our terminology (i.e., UHF vs RHF) follows the practice in quantum chemistry (see Ref. 26).
-
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43
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0348058299
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and Chap. 11 in Ref. 25
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For the restoration of broken rotational symmetries in atomic nuclei, see R.E. Peierls and J. Yoccoz, Proc. Phys. Soc. London, Sect. A 70, 381 (1957), and Chap. 11 in Ref. 25.
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Peierls, R.E.1
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For the restoration of broken spin symmetries in natural 3D molecules, see P.O. Löwdin, Phys. Rev. B 97, 1509 (1955); Rev. Mod. Phys. 36, 966 (1964).
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45
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For the restoration of broken spin symmetries in natural 3D molecules, see P.O. Löwdin, Phys. Rev. B 97, 1509 (1955); Rev. Mod. Phys. 36, 966 (1964).
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46
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and (as a function of B)
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For the restoration of broken spin symmetries in the case of double QD's, leading to a generalized Heitler-London approach for the coupling and dissociation of artificial molecules, see (for B = 0) C. Yannouleas and U. Landman, Eur. Phys. J. D 16, 373 (2001) and (as a function of B); C. Yannouleas and U. Landman, Int. J. Quantum Chem. 90, 699 (2002).
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For the restoration of broken spin symmetries in the case of double QD's, leading to a generalized Heitler-London approach for the coupling and dissociation of artificial molecules, see (for B = 0) C. Yannouleas and U. Landman, Eur. Phys. J. D 16, 373 (2001) and (as a function of B); C. Yannouleas and U. Landman, Int. J. Quantum Chem. 90, 699 (2002).
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(Springer, Berlin), and references therein
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L. Jacak, P. Hawrylak, and A. Wojs, Quantum Dots (Springer, Berlin, 1998), and references therein.
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(1998)
Quantum Dots
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Jacak, L.1
Hawrylak, P.2
Wojs, A.3
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57
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3342906428
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J.A. Pople and R.K. Nesbet, J. Chem. Phys. 22, 571 (1954); see also, G. Berthier, C. R. Séances Acad. Sci. 238, 91 (1954).
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(1954)
J. Chem. Phys.
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, pp. 571
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Pople, J.A.1
Nesbet, R.K.2
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58
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0040688243
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J.A. Pople and R.K. Nesbet, J. Chem. Phys. 22, 571 (1954); see also, G. Berthier, C. R. Séances Acad. Sci. 238, 91 (1954).
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(1954)
C. R. Séances Acad. Sci.
, vol.238
, pp. 91
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Berthier, G.1
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59
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33646630018
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note
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β = 0 usually produces broken-symmetry solutions (in the regime where symmetry breaking occurs).
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61
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33646621096
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note
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In some circumstances, SDW's may be obtained from spin density functional calculations (see Ref. 43). In general, however, the breakings of spin and/or spatial symmetries are not properly described within spin density functional theory (see Ref. 18).
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62
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26144433437
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The possibility of ground-state configurations with uniform electron density, but nonuniform spin density, was first discussed for 3D bulk metals using the HF method in A.W. Overhauser, Phys. Rev. Lett. 4, 462 (1960); Phys. Rev. 128, 1437 (1962).
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(1960)
Phys. Rev. Lett.
, vol.4
, pp. 462
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Overhauser, A.W.1
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63
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36149028106
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The possibility of ground-state configurations with uniform electron density, but nonuniform spin density, was first discussed for 3D bulk metals using the HF method in A.W. Overhauser, Phys. Rev. Lett. 4, 462 (1960); Phys. Rev. 128, 1437 (1962).
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(1962)
Phys. Rev.
, vol.128
, pp. 1437
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64
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33646610586
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note
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Depending on the spin polarization, a WM may (or may not) be accompanied by a SDW. Unlike the pure SDW case, however, the SDW of a WM exhibits necessarily the same number of humps as the number of electrons (see, e.g., the case of N = 3 electrons in Sec. III B).
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65
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33646632628
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note
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However, for RW≲1, the formation of a special class of SDW's (often called electron puddles) plays an important role in the coupling and dissociation of quantum dot molecules (see Ref. 32 and Ref. 9).
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66
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33646617205
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note
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In solid-state physics the Hückel approximation is usually referred to as the fight-binding approximation, with β denoted most often as t [t specifies the tunneling (hopping). between sites].
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68
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33646599327
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note
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The group theoretical symbol E for the two-dimensional irreducible representations should not be confused with the same symbol denoting the eigenvalues of the Hückel equation or the UHF orbital energies. For the group theoretical symbols, we follow the Schönflies convention. In addition to E, for one-dimensional irreducible representations, we use the capital letters A and B (see Refs. 33 and 49).
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69
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0037104423
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P.A. Sundqvist, S.Yu. Volkov, Yu.E. Lozovik, and M. Willander, Phys. Rev. B 66, 075335 (2002).
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(2002)
Phys. Rev. B
, vol.66
, pp. 075335
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Sundqvist, P.A.1
Volkov, S.Yu.2
Lozovik, Yu.E.3
Willander, M.4
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76
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33646610772
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note
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The RBS wave functions in Eq. (46) work for the group of states that exhibit magic angular momenta and have the lowest possible energy. In our use of the term, the group of these states forms the "yrast" rotational band: namely, the band of states whose excitation energy represents pure rotational motion (no other excitations, like center-of-mass motion or vibrational modes, are present).
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77
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0003517283
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Addison-Wesley, Reading, MA
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We note that the discrete rotational (and more generally rovibrational) collective spectra associated with symmetry breaking in a QD may be viewed as finite analogs to the Goldstone modes accompanying symmetry-breaking transitions in extended media [see P. W. Anderson, Basic Notions of Condensed Matter Physics (Addison-Wesley, Reading, MA, 1984)].
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(1984)
Basic Notions of Condensed Matter Physics
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Anderson, P.W.1
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79
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33646612754
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note
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Nv point-group symmetries.
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