Abstract
We investigate the temperature dependence of the upper critical field H c2 as a tool to probe the possible presence of multiband superconductivity at the interface between LaAlO 3 and SrTiO 3 (LAO/STO). The behaviour of H c2 can clearly indicate two-band superconductivity through its nontrivial temperature dependence. For the disorder scattering dominated two-dimensional LAO/STO interface, we find a characteristic non- monotonic curvature of the H c2(T). We also analyse the H c2 for multiband bulk STO and find similar behaviour.
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Acknowledgments
We are grateful to K. Behnia, R. Fernandes, J. Haraldsen, J.X. Zhu and S. Lederer for useful discussions and H. Haraldsen, K. Moler and K. Behnia for comments on the draft. We would also like to thank K. Behnia for showing us some of the data in Ref. [22] prior to publication. Work was supported by Nordita, VR 621-2012-2983 and ERC 321031-DM. Work at Los Alamos was supported by the Office of Basic Energy Sciences and by LDRD.
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Appendix: A. Induced Triplet Superconductivity
Appendix: A. Induced Triplet Superconductivity
1.1 A. 1 Induced Triplet Components Δa,Δb and Δc
We now look at the triplet component of superconductivity that is induced by spin-orbit coupling and show that it is not relevant for our calculations. We treat spin-orbit coupling in a perturbative way and assume that it is smaller than the Fermi energy. The self consistent expression for the gap Δ within a single band in the absence of spin-orbit coupling is given by [49]
with \(\xi _{p}=\frac {p^{2}}{2m}-\mu \) and V is the interaction potential . We now take spin-orbit coupling into account. We thus write Δ as a matrix according to (23) and ξ turns into
If we assume the existence of a singlet gap Δ s , we can obtain to lowest order in α the perturbed expression for \(\tilde {\Delta } \)
We may now decompose V(p) into a singlet (momentum independent) potential V s and a spin-dependent triplet component V t (p). We are not aware of any experimental evidence which shows that V T is large. Although spin-orbit coupling may induce a triplet pairing amplitude, a genuine triplet pairing gap in addition requires a triplet pairing potential. As, in general, triplet superconductivity is a rare phenomenon however, we make the reasonable assumption that V t ≪V s . The induced triplet components are then given by
Since Δa and Δb contain a sum over all k y or k x values, only the term proportional to V t (p) survives. Since V t ≪V s , we conclude that
At this order, we thus conclude that the p-wave components are negligible and we set Δa = Δb = Δc = 0.
1.2 A.2 Induced Triplet Components f a,f b and f c
Here, we estimate the relative strength of the singlet and triplet components of the function \(\tilde f\). We show that for the regime we are interested in the triplet components of \(\tilde f\) are an order of magnitude smaller than that of the singlet components, which we will subsequently neglect.
We start from (24), which gives rise to four equations for the four Pauli matrices σ i , i∈{0,x,y,z}.
We see that (37c) does not couple to the other three equations. From Appendix A.1, we may now conclude that Δa,b,c = 0. The remaining set of coupled three differential equations remains very difficult to solve. In order to estimate the relative importance of the singlet and triplet components of \(\tilde f\), we approximate this system of differential equations by a system of algebraic equations, replacing ∇ x with \(l_{B}^{-1}\) and x with l B . In analogy with what we did in Section 6, we also replace \({\nabla _{z}^{2}}\) with \(-\frac {\pi ^{2}}{4d^{2}} \). This yields
We choose the magnetic length as
This choice ensures that the terms \(\left ({\nabla _{x}^{2}} - \frac {4\pi ^{2} H^{2} x^{2}}{{\phi _{0}^{2}}} \right )\) \( \exp (-\pi H x^{2}/\phi _{0})= \left (l_{B}^{-2} - \frac {4\pi ^{2} H^{2} {l_{B}^{2}}}{{\phi _{0}^{2}}}\right ) \exp (-\pi H x^{2}/\phi _{0})\) where \(\exp (-\pi H x^{2}/\phi _{0})\) is the envelope function from (5).
We solve this system of three equations for f s , f a and f c. In order to estimate the relative magnitude of these three terms, we insert typical values for H,d,D and Δ s . For ν and d, we choose the same values as in Section 6, for Δ s , we choose the value from the largest singlet gap [16], and for H, we choose the typical value for the upper critical field [42, 46]
The resulting approximate values for f s , f a and f c as a function of ω are plotted in Fig. 11. We see that the triplet components f a and f c are at least an order of magnitude smaller than f s . We thus only make a small mistake by neglecting f a and f c, when solving for the dominant component f s in the main text. This corresponds to solving only the single differential (37a), as opposed to the full set of three coupled differential (37a–37d). The result of solving only (37a) is also shown in Fig. 11 as \({f_{s}^{0}}\) and we find that \(f_{s}\approx {f_{s}^{0}}\).
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Edge, J.M., Balatsky, A.V. Upper Critical Field as a Probe for Multiband Superconductivity in Bulk and Interfacial STO. J Supercond Nov Magn 28, 2373–2384 (2015). https://doi.org/10.1007/s10948-015-3052-3
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DOI: https://doi.org/10.1007/s10948-015-3052-3