Abstract
For the first time, a comparison to the predicted behavior for parallel critical field is carried out for the model of Kogan and the model of Hara and Nagai. In this study, thin niobium films in the moderately dirty regime were considered. Experimental values of the \(-C_{2}\) term are seen to be lower than those from the model of Hara and Nagai. A possible reason for this could be not including the non-spherical Fermi surface of niobium into the model. There is clearly disagreement with the model of Kogan as the films get cleaner and thinner, and two films which should be below his critical thickness still show positive values of \(-C_{2}\), in disagreement with his theory.
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Acknowledgements
The author would like to gratefully acknowledge the assistance of A. Hunziker and A. Davis in the film production and measurement, the support of Covenant College for this work, and Prof. C. B. Eom for the X-ray analysis. This work was performed in part at the Georgia Tech Institute for Electronics and Nanotechnology, a member of the National Nanotechnology Coordinated Infrastructure, which is supported by the National Science Foundation (Grant ECCS-1542174).
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Appendix
Appendix
Niobium samples used in this study | ||||||||||
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Sample | Substrate | d (nm) | RRR | \(\rho _{\mathrm {10K}}\ (\mathrm {n}\Omega \mathrm {m}) \) | \(T_\mathrm{c0}\) (K) | \(D=d/\xi \) | \(\lambda _{\mathrm {tr}} \) | \(-C_{2} (\mathrm {Exp.}) \) | \(-C_{2} (\mathrm {HN}) \) | \(-C_{2} (\mathrm {Kogan}) \) |
A | (100) Si | 48 | 4.04 | 49 | 8.946 | 1.3 | 4.4 | 0.064 | 0.071 | 0.066 |
B | (100) Si | 23 | 2.68 | 89 | 7.777 | 0.54 | 10 | 0.0052(3) | 0.0065 | 0.0054 |
C | (100) Si | 48 | 2.68 | 89 | 8.262 | 1.2 | 9.5 | 0.027(1) | 0.036 | 0.035 |
D | (100) Si | 25 | 2.51 | \(1.0{\times }10^{2} \) | 8.426 | 0.63 | 10 | 0.0072(2) | 0.0087 | 0.0079 |
E | A plane Sap | 25 | 4.82 | 39 | 8.284 | 0.63 | 4.2 | 0.014 | 0.017 | 0.0072 |
F | C plane Sap | 52 | 3.77 | 54 | 8.649 | 1.4 | 5.5 | 0.056 | 0.074 | 0.066 |
G | (100) Si | 25 | 3.13 | 70 | 8.504 | 0.65 | 7.3 | 0.011 | 0.012 | 0.010 |
H | A plane Sap | 22 | 7.24 | 24 | 8.644 | 0.57 | 2.4 | 0.014 | 0.017 | \(-\)0.017 |
J | C plane Sap | 25 | 4.07 | 49 | 8.477 | 0.64 | 5.0 | 0.012 | 0.015 | 0.0094 |
K | C plane Sap | 16 | 2.53 | 98 | 7.615 | 0.37 | 11 | 0.0021 | 0.0027 | 0.0019 |
L | A plane Sap | 16 | 4.12 | 48 | 8.021 | 0.39 | 5.3 | 0.0043 | 0.0049 | \(-\)0.0072 |
M | C plane Sap | 26 | 2.63 | 92 | 8.264 | 0.64 | 9.8 | 0.0077 | 0.0092 | 0.0084 |
N | (100) Si | 24 | 3.01 | 75 | 8.600 | 0.63 | 7.6 | 0.0093(1) | 0.011 | 0.0090 |
P | C plane Sap | 20 | 2.68 | 89 | 8.050 | 0.49 | 9.7 | 0.0045 | 0.0053 | 0.0043 |
R | C plane Sap | 20 | 2.59 | 94 | 8.060 | 0.50 | 10 | 0.0051(3) | 0.0055 | 0.0044 |
S | C plane Sap | 39 | 3.27 | 66 | 8.520 | 1.0 | 6.8 | 0.024 | 0.032 | 0.029 |
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Broussard, P.R. Parallel Critical Field in Thin Niobium Films: Comparison to Theory. J Low Temp Phys 189, 108–119 (2017). https://doi.org/10.1007/s10909-017-1792-0
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DOI: https://doi.org/10.1007/s10909-017-1792-0