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High current superconductivity in FeSe0.5Te0.5-coated conductors at 30 tesla

Nature Communications volume 4, Article number: 1347 (2013) | Download Citation

Abstract

Although high-temperature superconductor cuprates have been discovered for more than 25 years, superconductors for high-field application are still based on low-temperature superconductors, such as Nb3Sn. The high anisotropies, brittle textures and high manufacturing costs limit the applicability of the cuprates. Here we demonstrate that the iron superconductors, without most of the drawbacks of the cuprates, have a superior high-field performance over low-temperature superconductors at 4.2 K. With a CeO2 buffer, critical current densities >106  A cm−2 were observed in iron-chalcogenide FeSe0.5Te0.5 films grown on single-crystalline and coated conductor substrates. These films are capable of carrying critical current densities exceeding 105 A cm−2 under 30 tesla magnetic fields, which are much higher than those of low-temperature superconductors. High critical current densities, low magnetic field anisotropies and relatively strong grain coupling make iron-chalcogenide-coated conductors particularly attractive for high-field applications at liquid helium temperatures.

Introduction

Iron-based superconductors are semi-metallic materials with transition temperatures, Tc, up to 55 K. The combination of extremely high upper critical fields, Hc2(0) (estimated to be on the order of 100 T), moderate Hc2ab/Hc2c anisotropies (on the order of 1–8) and high irreversibility fields, Hirr, makes this class of superconductors particularly appealing for high-field applications1,2,3,4,5,6,7,8, where the critical current density, Jc, is a major limiting factor. Although the high-Tc cuprates currently hold the records of Jc value among all superconductors, there are quite a few obstacles for their practical application. The extremely high anisotropies up to thousands have made it very difficult to obtain superconducting tapes or wires with their best Jc. The rapid decrease of Jc upon the grain boundary misorientation also made their fabrication much more difficult and complicated. Their brittle textures as well as the high production and raw material costs also hold back their application. Currently, superconductors for high-field application are still based on Nb3Sn, a low Tc superconductor that allows fields in excess of 20 T to be achieved at 4.2 K. We argue that iron superconductors may be a more competitive candidate to replace these low Tc superconductors for high-field application at liquid helium temperatures.

To achieve this goal, a key task is to find a technique to increase the Jc of iron-superconductor films (or wires) made on practical metal substrates (or inside metal sheath). One of these techniques is to make a proper buffer layer between the superconductor and the substrate. A suitable buffer layer can often prevent undesirable reactions between the superconductor and the substrate, or enhance the superconducting properties of the films and wires. For iron-pnictide films, Tarantini et al.9 recently reported that single-crystalline (La, Sr)(Al, Ta)O3 substrates with 100 unit cells of epitaxial SrTiO3 (STO) resulted in higher Tc and Jc for Co-doped BaFe2As2 films. Higher Tc and sharper out-of-plane and in-plane textures of the Fe/BaFe2As2 bilayers were also realized with 20-nm thick epitaxial Fe buffer layers10. A self-field Jc >1 MA cm−2 at 4.2 K has been reported in both Co-doped BaFe2As2 and SmFeAs(O, F) systems1,2, as well as in Co-doped BaFe2As2 thin films on coated conductor substrates4. However, the results of high-field performance up close to their Hirr at 4.2 K are still missing.

Here we show that epitaxially grown iron-chalcogenide thin films with a CeO2 buffer layer have a superior high-field performance up to 30 T with Jc >1 MA cm−2 in self-field. Chalcogenides are an interesting sub-class of iron-based superconductors. Even though the Tc of chalcogenides are typically <20 K, it was found that the Tc of FeSe can reach 37 K under a pressure of ~7 GPa (ref. 11). Recently, it was reported that a single-unit cell film of FeSe on a STO substrate may be superconducting >77 K (ref. 12). They also have the simplest structures among the iron-based superconductors and exhibit lower anisotropies ~2, compared with the pnictides, with comparable Hc2(0) approaching 50 T (refs 13, 14, 15). We have previously reported on the successful growth of FeSe0.5Te0.5 (FST) thin films on textured metal templates with biaxially aligned MgO layers, made via ion-beam-assisted deposition (IBAD)3. These films carry Jc >104  A cm−2 under magnetic fields as high as 25 T at about 4 K. However, MgO has a cubic lattice constant of ~4.11 Å, which is fairly larger than the in-plane lattice constant of FST, which is around 3.81 Å. CeO2, a commonly used buffer layer for high-temperature superconductor (HTS) cuprates, has a much closer lattice constant (cubic, ) with FST. In this article, we show that CeO2 buffer can significantly improve the Tc and Jc of FST films both on single-crystalline substrates and coated conductors, such as the rolling-assisted biaxially textured substrate (RABiTS), which have a biaxially textured CeO2 layer at the top16. These films have a self-field Jc as high as 1 MA cm−2 and maintain a nearly isotropic Jc on the order of 1 × 105 A cm−2 up to 30 T at 4.2 K.

Results

Structure of FST films on CeO2-buffered substrates

Figure 1a shows a θ-2θ X-ray diffraction (XRD) scan of a typical FST film grown on a (100) Yttria-stabilized zirconia (YSZ) substrate with a buffer layer of CeO2. Figure 1b shows the same scan for a film grown on a RABiTS substrate. For both films, only the (00l) peaks from the FST film, CeO2 buffer and substrates are present, indicating that the out-of-plane alignments are good. The CeO2, YSZ and Y2O3 layers, with the NiW base layer, in the RABiTS substrate are clearly seen in the XRD scan. Figure 1c–e shows the φ scan of the (101) peak from the thin film and the (202) peak from the CeO2 and YSZ buffer layers in the RABiTS substrate. All of them have four peaks with 90° intervals consistent with four-fold symmetry. Peaks from the thin film and the CeO2/YSZ buffer layers are separated by 45°, indicating that the lattice of the film is rotated by 45° in the ab plane compared with the lattice of CeO2/YSZ buffer layers and is now aligned cube-on-cube with the NiW substrate. The c-axis lattice constant is about 5.90–5.94 Å for both types of films, which is shorter than that of the bulk sample (6.02 Å). This is consistent with our previous results from films grown on other substrates3,17.

Figure 1: Structure analysis of FST films by XRD.
Figure 1

θ-2θ scan of FST films grown on (a) a YSZ single-crystalline substrate with CeO2 buffer layer and (b) a RABiTS substrate. φ scan of (c) (101) peak from the FST film, (d) (202) peak from the CeO2 buffer layer and (e) (202) peak from YSZ buffer layer in a FST film grown on a RABiTS subtrate. Both the film and buffer layers are well aligned in-plane and out-of-plane. The lattice of the FST film is rotated by 45° in the ab plane compared with the lattice of CeO2/YSZ buffer layers.

T c comparison of various FST films and the bulk material

Figure 2 shows the resistive superconducting transitions of various FST thin films and the bulk material. It is clearly seen that FST films (except for that grown on IBAD substrates) have Tc 2–5 K higher than that of bulk. The highest Tc is achieved with a CeO2 buffer layer, which has an onset Tc >20 K and zero resistance Tc >18 K. The transition width (10–90% normal resistance level) is under 1 K. The most striking finding is that the film grown on RABiTS has a higher Tc than the film grown on single-crystalline substrate without a CeO2 buffer layer, although the latter actually has a smaller in-plane texture. The full-width half maximum of the (101) peak from the φ scan (Δφ101) is about 6°, which is smaller than the CeO2 texture in the RABiTS substrate (Δφ202~7°). This behaviour was also observed in Ba(Fe1−xCox)2As2 films by Katase et al.4 However, Δφ101 for films on single-crystalline substrates without a CeO2 buffer are just ~2°. Even films on IBAD substrates have better textures (Δφ101~5°) (ref. 3). These results suggest that the CeO2 buffer has a much more profound effect on the superconducting properties of FST thin films than the sharpness of the texture in the films themselves. Films on IBAD substrates have the lowest Tc (~11 K) as shown in Fig. 2. This is probably due to its largest lattice mismatch to the FST3.

Figure 2: Resistive superconducting transition of various FST films and the bulk material.
Figure 2

Tc of FST films (except for that grown on the IBAD substrate) are 2–5 K higher than that of bulk. Films with CeO2 buffer layers have the highest Tc with an onset Tc >20 K and zero resistance Tc >18 K.

J c of FST films

Figure 3 shows the magnetic field dependence of the Jc of the FST films grown on both CeO2-buffered single-crystalline YSZ and RABiTS substrates at various temperatures. The Jc of films grown on both substrates are shown to be >1 MA cm−2 in self-field at 4.2 K, and remain on the order of 1 × 105 A cm−2 up to 31 T—the maximum field we could apply. Notably, the decrease of Jc does not accelerate much at high fields at liquid helium temperatures, which is important for high-field magnet applications. Surprisingly, the Jc of the RABiTS film under higher magnetic fields or at higher temperatures is somehow higher than those of films on single-crystalline substrates, although the film grown on the RABiTS substrate has a macroscopic 6° in-plane misalignment of epitaxial grains, which is much higher than that of the film grown on single-crystalline substrates. It has been well known that a key factor limiting the applications of HTS wires is the high-angle grain boundaries that cause the rapid decrease of Jc. Our X-ray texture analysis indicates an average 7° grain boundary misalignment in the RABiTS substrates we used. It is interesting to note that very high Jc of >3 MA cm−2 (77 K, self-field) with well-linked behaviour is routinely obtained for YBa2Cu3O7 (YBCO) films on these substrates. This seems to be the case in the FST films. Our observation is markedly different from an earlier report on grain boundaries of Ba(Fe1−xCox)2As2 films, which shows that grain boundaries could significantly reduce the Jc even at low angles18. A recent report on films of iron-based superconductors by Katase et al.19 has shown that the critical angle for the rapid Jc decrease is about 9°. This is consistent with our studies, although their films are pnictides, whereas our films are chalcogenides.

Figure 3: Critical current densities (Jc) of FST films.
Figure 3

Jc of FST films on (a) a YSZ substrate with a CeO2 buffer layer and (b) a RABiTS substrate at various temperatures with magnetic field parallel (solid symbols) and perpendicular (open symbols) to the ab plane (tape surface). The self-field Jc of both films are above 1 MA cm−2 at 4.2 K. Under 30 T of magnetic fields, both films still carry Jc around 1 × 105 A cm−2.

Discussion

In Fig. 4a, we show the field dependence of the volume pinning force Fp for a FST film grown on a RABiTS substrate with the literature data of the second-generation YBCO wire20,21, thermomechanically processed Nb47Ti alloy22,23 and small-grain Nb3Sn wire24,25. Clearly, the FST film exhibits superior high-field performance (above ~7 T) over those of other low-temperature superconductors. YBCO and other HTSs currently have higher Jc than the ones typical of iron chalcogenides, but their applications are impeded by high production costs, higher anisotropies, and the rapid decrease of Jc upon grain boundary misorientation. We noted that the cost of the coated conductors mainly depends on the cost of the processing methodologies, not the raw materials. This cost is mostly related to the growth of the thick multiple textured oxide buffer layers, partially to prevent metal template from oxidation, as well as the sophisticated procedures necessary for growing YBCO films near 800 °C and the oxygen annealing afterwards. For the new iron-based coated conductors, the processing temperature is much lower (~400°C) (ref. 17). At this moderate temperature, we expect very limited oxidation of the metal templates, hence thinner and less-complicated buffer structures are likely to produce the same result. Furthermore, oxygen annealing is no longer required. As such, we expect the manufacturing cost of iron-based coated conductors will be reduced, which may make them more attractive on the cost-performance basis.

Figure 4: Pinning force analysis for a FST film grown on RABiTS.
Figure 4

(a) Fp at 4.2 K of a FST film grown on a RABiTS substrate, compared with the literature data of YBCO 2 G wire20,21, TCP Nb47Ti22,23 and Nb3Sn24,25. Solid lines are Kramer’s scaling approximations. (b) Kramer’s scaling of pinning force density fp versus reduced field h for a FST film grown on a RABiTS substrate at various temperatures with field perpendicular (solid symbols) and parallel (open symbols) to c-axis.

In Fig. 4b, we show the Kramer’s scaling law approximation (solid line), fp~hp(1−h)q, for a FST film grown on a RABiTS substrate at various temperatures with the field applied both parallel and perpendicular to the tape surface, where fp=Fp/Fpmax is the normalized pinning force density and h=H/Hc2 is the reduced field. The data for all temperatures and both directions fall approximately on a single line. This appears to suggest that the pinning mechanism is independent of the temperature and field direction. q is found to be equal to 2, which is expected considering that the (1−h)2 term describes the reduction of the superconducting order parameter at high fields26. p is found to be ~0.85 (h0.85), close to 1. This low-field term indicates that a point-defect core pinning mechanism is at play26, which is consistent with our previous results of FST films grown on IBAD substrates3. In the core pinning regime, Fp is a product of the individual Fp times the pinning centre density. This means that the Jc of FST may still be enhanced by adding more defects to act as pinning centres.

It is not clear what types of defects are responsible for the high Jc values we observed so far, in particular, what is the role of the CeO2 buffer layer. We attempted to answer these questions by examining the structure properties of our FST films. Our preliminary high-resolution transmission electron microscope study revealed that there might be some intergrowth at the interface between the FST films and the CeO2 buffer layers. We noted that certain types of intergrowth defects can be effective flux pinning centres in cuprates27. Perhaps, they also contribute to the enhanced pinning observed in the FST films on the CeO2 buffer layers, and result in significantly improved Jc. To understand the flux pinning mechanism, a detailed study of the structure–properties relationship is needed. This is our ongoing effort, and findings will be reported elsewhere.

In conclusion, robust c-axis oriented superconducting FST tapes on CeO2-buffered single-crystalline and RABiTS coated conductor substrates have been made by pulsed-laser deposition. These tapes have a self-field Jc on the order of 1 MA cm−2 and carry a nearly isotropic Jc~105 A cm−2 under 30 T at 4.2 K. The CeO2 buffer layer dramatically improves the superconducting performance of the FST films. It was also found that the low-angle (up to 7°) substrate grain boundary does not depress the Jc of the coated conductor films. These properties show that FST has a very promising future for high-field applications at liquid helium temperatures.

Methods

We used pulsed-laser deposition to grow the FST films and CeO2 buffer layers17. Films were deposited on both single-crystalline substrates, such as LaAlO3, STO and YSZ, and RABiTS. RABiTS substrates were originally developed and are presently being used extensively in the production of high-Tc cuprate films. They are comprised of a Ni–W alloy with a series of buffer materials, such as Y2O3, YSZ and CeO2, on top. The topmost is a biaxially textured CeO2 layer with an in-plane texture of about 7°16. Structural characterizations of the various films were performed by XRD at beamline X18A at the National Synchrotron Light Source at Brookhaven National Laboratory. The beam energy is 10 keV. The resistivities and the Jc were measured utilizing a standard four-probe method. Experiments at magnetic fields as high as 31 T were conducted at the National High Magnetic Field Laboratory in Tallahassee, Florida.

Additional information

How to cite this article: Si, W. et al. High current superconductivity in FeSe0.5Te0.5-coated conductors at 30 tesla. Nat. Commun. 4:1347 doi: 10.1038/ncomms2337 (2013).

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Acknowledgements

This work was supported by the US Department of Energy, Office of Basic Energy Science, Materials Sciences and Engineering Division, under contract no. DE-AC0298CH10886. RABiTS is a registered trademark of Oak Ridge National Laboratory (ORNL). The RABiTS templates were fabricated at ORNL under funding from the US Department of Energy, Office of Electricity. A portion of this work was performed at the National Synchrotron Light Source (NSLS) and the National High Magnetic Field Laboratory (NHMFL). NSLS is funded by the US Department of Energy. NHMFL is supported by National Science Foundation Cooperative Agreement No. DMR-0654118, the State of Florida and the US Department of Energy.

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Affiliations

  1. Condensed Matter Physics & Materials Science Department, Brookhaven National Laboratory, Upton, New York 11973, USA

    • Weidong Si
    • , Su Jung Han
    • , Xiaoya Shi
    •  & Qiang Li
  2. National Synchrotron Light Source, Brookhaven National Laboratory, Upton, New York 11973, USA

    • Steven N. Ehrlich
  3. National High Magnetic Field National Laboratory, Florida State University, 1800 E. Paul Dirac Drive, Tallahassee, Florida 32310, USA

    • J Jaroszynski
  4. Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA

    • Amit Goyal

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Contributions

W.S. and Q.L. designed the study and wrote the manuscript. W.S. made the thin films. W.S., S.J.H. and Q.L. did the low-field measurement. W.S., X.S. and J.J. did the high-field measurement. W.S. and S.N.E. did the XRD experiment. A.G. provided the RABiTS. Q.L. supervised the project. All the authors contributed to discussion on the results for the manuscript.

Competing interests

The authors declare no competing financial interests.

Corresponding authors

Correspondence to Weidong Si or Qiang Li.

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