1965
DOI: 10.1103/physrev.139.a1515
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Superconducting Penetration Depth of Niobium

Abstract: The variation with temperature of the penetration depth of weak magnetic fields into niobium has been measured. The variation was more rapid than expected from the BCS theory of superconductivity, in contrast to the situation in previously measured superconductors where it was less rapid. Just as in the previous cases, the results here can be understood in terms of a variation of the energy gap different from that predicted by the BCS theory. A comparison with the energy gap deduced by Dobbs and Perz from thei… Show more

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Cited by 137 publications
(70 citation statements)
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“…The same value is obtained from extrapolating the linear H c2 (T) dependence observed below 6 K and using the bulk expression for H c2 , H c2 (T) = φ 0 /[2πξ(T) 2 ]. This value is significantly smaller than the BCS coherence length of Nb, ξ 0 = 38 nm [11], indicating that our films are in the dirty limit with a electron mean free path of l = 1.38 ξ(0) 2 /ξ 0 ≈ 5 nm. The Ginzburg-Landau parameter, κ = λ/ξ, can be estimated using the dirty-limit expressions for the penetration depth and the coherence length to κ = 0.72 λ L /l ≈ 7; λ L = 39 nm is the London penetration depth of Nb [11].…”
mentioning
confidence: 75%
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“…The same value is obtained from extrapolating the linear H c2 (T) dependence observed below 6 K and using the bulk expression for H c2 , H c2 (T) = φ 0 /[2πξ(T) 2 ]. This value is significantly smaller than the BCS coherence length of Nb, ξ 0 = 38 nm [11], indicating that our films are in the dirty limit with a electron mean free path of l = 1.38 ξ(0) 2 /ξ 0 ≈ 5 nm. The Ginzburg-Landau parameter, κ = λ/ξ, can be estimated using the dirty-limit expressions for the penetration depth and the coherence length to κ = 0.72 λ L /l ≈ 7; λ L = 39 nm is the London penetration depth of Nb [11].…”
mentioning
confidence: 75%
“…This value is significantly smaller than the BCS coherence length of Nb, ξ 0 = 38 nm [11], indicating that our films are in the dirty limit with a electron mean free path of l = 1.38 ξ(0) 2 /ξ 0 ≈ 5 nm. The Ginzburg-Landau parameter, κ = λ/ξ, can be estimated using the dirty-limit expressions for the penetration depth and the coherence length to κ = 0.72 λ L /l ≈ 7; λ L = 39 nm is the London penetration depth of Nb [11]. Ratios of ξ(0)/a ≈ 0.1 and λ(0)/a ≈ 0.7 are achieved which are substantially larger than in previous reports [1,2] have been studied in superconducting wire networks [7][8][9], Josephson junction arrays [12] and perforated Al films [13].…”
mentioning
confidence: 75%
“…The penetration depth is sensitive to film quality and thickness, and deviates significantly for films thinner than 50 nm [34]. For the 80 nm thick Nb film used, the dependence is less critical, and we use the bulk London penetration depth, 39 nm [35]. The investigated junctions are smaller than or comparable to the Josephson penetration depth, λ Φ πμ…”
Section: Periodicity In φmentioning
confidence: 99%
“…For commonly used SC Nb with λ L ≈ 50 nm [24] and nanoscale thicknesses d SC = 50 ÷ 250 nm, we obtain g * ≈ 200 ÷ 400, which exceeds the electron spin g-factor by at least two orders of magnitude. In contrast to the Zeeman spin splitting [18], the orbital effect considered here does not require high magnetic fields to generate spin splitting, as will be shown below.…”
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confidence: 73%