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1
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0004287161
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Dekker, N.Y.
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For reviews of the weak and the strong coupling theories of superconductivity, see for example Superconductivity, ed. by R. D. Parks (Dekker, N.Y., 1969)
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Superconductivity
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Parks, R.D.1
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6
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35949014943
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Phys. Rev. B 39, 11663 (1989);
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Phys. Rev. B
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8
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33749403155
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Phys. Rev. B 42, 7967 (1990).
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Phys. Rev. B
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10
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33847533065
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C. M. Varma, P. B. Littlewood, S. Schmitt-Rink, E. Abrahams, and A. E. Ruckenstein, Phys. Rev. Lett. 63, 1996 (1989).
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Varma, C.M.1
Littlewood, P.B.2
Schmitt-Rink, S.3
Abrahams, E.4
Ruckenstein, A.E.5
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11
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0001240661
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For a review of the present situation, see J. P. Carbotte, Rev. Mod. Phys. 62, 1027 (1990).
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Rev. Mod. Phys.
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Carbotte, J.P.1
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25844465500
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Progr. in Low Temp. Phys. X
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ed. D. F. Brewer, and P. B. Allen, and B. Mitrovic, ed. F. Seitz, D. Turnbull, and H. Ehrenreich Academic, N.Y.
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See for example D. Rainer, Progr. in Low Temp. Phys. X, ed. D. F. Brewer, and P. B. Allen, and B. Mitrovic, Sol. State Phys. 37 , ed. F. Seitz, D. Turnbull, and H. Ehrenreich (Academic, N.Y., 1982).
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Rainer, D.1
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13
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25844501249
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note
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This is also our estimated numerical precision in this work (although many of our calculations have a much better precision). When on some occasions we quote errors of order 1% or below, we mean relative errors between calculations made in the same conditions.
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21
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0010427362
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3/2 which is analytical. The coefficients in the expansions themselves are obtained by comparison with the numerical results. In this respect the large λ limit of 11.8 which we give here is 7% below the precise result of 12.6 obtained in the very large λ limit by F. Marsiglio and J. P. Carbotte, Phys. Rev. B 43, 5355 (1991)
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(1991)
Phys. Rev. B
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, pp. 5355
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Marsiglio, F.1
Carbotte, J.P.2
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22
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0001033724
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(see also J. P. Carbotte, F. Marsiglio, and B. Mitrovic, Phys. Rev. B 33, 6135 (1986)). This slight discrepancy is due to the slow variation of Δ with λ in this range and does not imply numerical disagreement with their work. Actually our coefficients give a very precise agreement with our numerical results, up to λ = 25, as indicated in Sec. VI, but also agree with their results within 1% for λ = 100.
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(1986)
Phys. Rev. B
, vol.33
, pp. 6135
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Carbotte, J.P.1
Marsiglio, F.2
Mitrovic, B.3
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24
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33749833904
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the Proceedings of LT19
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B. Batlogg in the Proceedings of LT19, Physica B 169, 7 (1991)
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Physica B
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, pp. 7
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Batlogg, B.1
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29
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85087580707
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note
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c is calculated exactly from the linear Eliashberg equations.
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30
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84913474280
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This formula has actually been proposed, but not explored in R. Combescot, Europhys. Lett. 10, 177 (1989).
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(1989)
Europhys. Lett.
, vol.10
, pp. 177
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Combescot, R.1
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