JOURNAL OF APPLIED PHYSICS VOLUME 96, NUMBER 6 15 SEPTEMBER 2004 Observation of dendritic flux instabilities in YNi2B2C thin films S. C. Wimbusha) and B. Holzapfel IFW Dresden, P.O. Box 270016, 01171 Dresden, Germany Ch. Jooss Institut für Materialphysik, University of Göttingen, Tammanstrasse 1, 37077 Göttingen, Germany (Received 10 March 2004; accepted 14 June 2004) Magneto-optical imaging and magnetization measurements performed on thin films of the borocarbide superconductor YNi2B2C reveal the occurrence of magnetic flux instabilities upon reducing the applied magnetic field towards the remanent state. In contrast to other low-Tc materials such as Nb and MgB2, where similar instabilities occur in both increasing and decreasing magnetic fields, dendritic flux patterns are observed in YNi2B2C for decreasing fields only. Also in the magnetization measurements, a distinct asymmetry is evident between increasing and decreasing fields. The effect does not depend on the sweep rate of the field, but is strongly dependent on the maximum field applied before reduction. The observation of spontaneous flux instabilities in this additional family of low-temperature superconductors suggests that the responsible mechanism is universal to this class of materials. © 2004 American Institute of Physics. [DOI: 10.1063/1.1778816] cases. The addition of the borocarbide family of superconductors to those in which such patterns have been observed generalizes the phenomenon and opens up new possibilities for its investigation. A question of particular interest is whether a similar behavior can be observed in bulk samples, since the connection between its occurrence in thin films and bulk material is currently not clear. Thin film samples of YNi2B2C were prepared by pulsed laser deposition, as described in Ref. 10. The deposition conditions were chosen to produce samples with a high degree of c-axis orientation and optimized Tc values lying between 14.5 and 14.6 K (at 90% of the normal state resistivity, measured inductively and thus representative of the entire sample volume, as appropriate for the other measurement techniques used) with a transition width (90%–10%) less than 0.3 K. The in-plane orientation was here of secondary consideration and samples having only a weak in-plane texture (predominant fibre texture) were selected. After preparation, the samples were cleaved to an approximate size of 5 ⫻ 5 mm2 for further investigation. Two distinct measurement techniques were applied for investigation of the samples: bulk magnetization measurements via a dc extraction technique, and high-resolution magneto-optical imaging (MOI). These techniques reveal different features of interest in the investigation of flux jumps. A primary advantage of the magnetization measurements is that they allow easy access to lower temperatures and higher fields than the magneto-optical technique can attain, whereas MOI provides a spatially resolved visualization of the flux patterns leading to the overall magnetization signal. The MOI technique is based on the principle of Faraday rotation. By placing a doped iron garnet layer as a magnetooptically active sensing element on top of the superconductor, the normal component of the magnetic flux density distribution can be measured with a spatial resolution of up The observation of dendritic flux penetration in thin films of the superconductor MgB2 (Refs. 1 and 2) triggered renewed interest in the origin and mechanisms of this effect,3,4 which exhibits a surprising variety of features in different materials. Flux jumps were first observed magnetooptically in superconducting Nb disks,5 and later, with the invention of high-resolution magneto-optical imaging, were shown to be dendritic in nature.6 Dendritic flux patterns have been observed to occur spontaneously in thin films of MgB2 for both increasing and decreasing external fields,1 and similar patterns can also be triggered by pulsed transport currents,7 whereas in thin films of YBa2Cu3O7−␦, spontaneous dendritic flux patterns are usually not observed but may be induced by means of local laser pulse heating.8 A common feature in all cases is the requirement for low temperatures— dendritic flux patterns occur only up to a fraction of the superconducting transition temperature Tc (reported to be around 0.65 for Nb and 0.25 for MgB2), being replaced by a usual critical state flux penetration at higher temperatures. Conventionally, flux jumps are explained in terms of a thermomagnetic instability arising from the heat generated by vortex motion.9 A rise in the local temperature lowers the local critical current density Jc, encouraging further vortex motion and thus resulting in a macroscopic vortex avalanche. More recent theoretical work3 is also able to explain the dendritic shape of the flux patterns. Experiments on MgB2 thin films under varying thermal conditions have shown that this mechanism is in fact at work in this material.4 We report the observation of spontaneous dendritic flux patterns on approaching the remanent state in YNi2B2C thin films, similar to those seen in MgB2. We also highlight the important differences in the flux patterns observed in the two a) Present address: National Institute for Materials Science, International Center for Young Scientists, 1-1 Namiki, Tsukuba, Ibaraki 305-0044, Japan; electronic mail: s.c.wimbush@ifw-dresden.de 0021-8979/2004/96(6)/3589/3/$22.00 3589 © 2004 American Institute of Physics Downloaded 09 Nov 2004 to 129.240.85.155. Redistribution subject to AIP license or copyright, see http://jap.aip.org/jap/copyright.jsp 3590 J. Appl. Phys., Vol. 96, No. 6, 15 September 2004 Wimbush, Holzapfel, and Jooss FIG. 2. Magneto-optical images of the flux distribution within the sample at 4 K under decreasing applied fields after application of 0Hex = 66.0 mT. No flux instability is observed down to the remanent state. FIG. 1. Magneto-optical images of the flux distribution within the sample at 4 K under decreasing applied fields after application of 0Hex = 92.4 mT, revealing the occurrence of a dendritic flux instability around 0Hex ⬇ 20 mT and its persistence down to the remanent state. The irregularity visible in the upper right corner of all the images is a structural defect resulting from the cleaving of the sample. to 1 m.11 A varying external magnetic field was applied perpendicular to the plane of the film (parallel to the c axis of the borocarbide unit cell) with a sweep rate between 150 and 300 mT s−1, and the resulting flux penetration into the superconductor (held at 4 K) observed. Magnetization measurements were performed at different temperatures after zero-field cooling of the sample. As for the MOI measurements, the field was oriented parallel to the c axis of the borocarbide unit cell. An applied field sweep rate of 1 mT s−1 was used, and magnetization data were collected at the maximum possible rate, without averaging. The data are presented as measured, without correcting for the background (substrate, sample holder), although this too was measured (just above Tc) and found to be negligible. The series of magneto-optical images in Fig. 1 shows the development of the magnetic instability in decreasing magnetic field. After zero-field cooling and application of a maximum external field 0Hex = 92.4 mT, this external field was gradually reduced. Down to 0Hex = 26.4 mT, a typical critical state rooflike pattern of trapped flux is visible. The different sizes of the four current domains (separated by bright lines in the image, the so-called discontinuity lines) suggest that the critical current in the sample is slightly inhomogeneous, most likely due to a thickness variation across the film. Upon further reduction of Hex the instability abruptly appears at 0Hex ⬇ 20 mT. As Hex is then reduced to zero, the dendritic flux pattern remains unchanged, with critical state behavior occurring around it. The flux pattern can be overridden by remagnetization of the sample, and no instability was ever observed while increasing Hex. The appearance of the instability in decreasing Hex, however, depends on the value of the maximum applied external field. This can be seen in Fig. 2, where the sample is shown in decreasing Hex after application of a lower maximum 0Hex = 66.0 mT. In this case, the rooflike pattern is visible right down to the remanent state 共0Hex = 0 mT兲. This implies that a minimum flux density (flux line proximity) within the sample is necessary for the instability to develop. A further interesting feature of the instability is that it always develops towards the same region of the sample, the region of maximum trapped flux. On repeating the experiment with the same maximum 0Hex = 92.4 mT, but using different sweep rates of the external field, the position, size, and general features of the dendritic flux pattern remain unchanged. However, its finer structure is different in each experiment. Figure 3 shows the magnetization loops of the sample measured at different temperatures. An irregular scattering of the data points at low fields, typically interpreted as fluxjump behavior, is seen for temperatures as high as 10 K 共0.7Tc兲. With decreasing temperature, the scattering becomes more pronounced, and extends to higher applied fields (up to 200 mT at 2 K). This is similar to the temperature dependence of the flux instability in other materials, which is seen to occur only below a specific temperature T ⬍ Tc. To confirm the thermomagnetic origin of the instability, an experiment was performed on the sample, whereby it was successively coated in an increasing quantity of gold and remeasured at each stage. The effect on the magnetization loop at 2 K is shown in Fig. 4. An initial gold coating is seen to strongly suppress the flux-jump behavior, while further coating leads the behavior closer to the “ideal” (non-fluxjump) state. This is consistent with the interpretation given above, with the gold layer facilitating the transport of heat away from the critical site, allowing sufficient dissipation to prevent the occurrence of the instability. FIG. 3. Magnetization loops measured at temperatures from 14 to 2 K in 2 K intervals. The inset shows in detail the region of irregular behavior at low fields, highlighting the asymmetry of the curves, the varying extent of the flux-jump regime, and the absence of irregularity at higher temperatures. Downloaded 09 Nov 2004 to 129.240.85.155. Redistribution subject to AIP license or copyright, see http://jap.aip.org/jap/copyright.jsp J. Appl. Phys., Vol. 96, No. 6, 15 September 2004 FIG. 4. Effect on the magnetization loop of successive coating with an increasing quantity of gold, measured at 2 K. The inset highlights the effect within the flux-jump regime. A distinct asymmetry is also evident in all of the magnetization results, with far more scattering occurring in the quadrants of decreasing applied field than increasing. In the increasing field quadrants, the curves are close to “ideal.” This asymmetry, evidenced by both measurement techniques, can again be related to the requirement for a minimum flux density within the sample before an instability will occur. For maximum applied fields higher than those at which the instability can occur (which is the case for all the measurements presented here, and appears from the result of Fig. 2 to be a requirement for instabilities to occur at all), there will always be a higher flux density within the sample during decreasing field than increasing. Thus, flux instabilities are generally observed in this material only when decreasing the applied field. Our observation of dendritic flux instabilities in YNi2B2C superconducting films raises the general question as to which materials are capable of exhibiting this behavior, and under which conditions it arises. Comparing Nb, MgB2, and YNi2B2C with the high-Tc superconductors, in which such spontaneous instabilities are usually not observed, we note that the strength of thermal fluctuations (quantified in terms of the Ginzburg number12) differs by orders of magnitude in the different materials (10−9 for Nb, 10−4 for YNi2B2C and MgB2, and 100 for YBa2Cu3O7−␦). This suggests that strong thermal relaxation in the high-Tc’s helps to prevent such instabilities, since locally generated “hot spots” can easily be thermalized in the vortex system (the exception to this being experiments where the formation of a “hot spot” is artificially forced8). Furthermore, in general, stronger flux Wimbush, Holzapfel, and Jooss 3591 creep is present at higher temperatures and larger magnetic fields, where no instability is observed. This ties in with the theoretical treatment of Aranson, Gurevich, and Vinokur3 who define a parameter relating the thermal and magnetic flux diffusivities. Strong flux creep implies a very small and reduced Jc, resulting in the absence of flux instabilities. For small , the instability will be localized, while for large, it will grow to consume the entire sample. This may explain the different scale of the dendritic patterns observed with respect to MgB2, with YNi2B2C having a comparatively large . Aranson also considers a parameter ␣, defining a threshold Jc for the instability to occur in terms of the thermal conditions and the resistivity of the sample. The occurrence of flux instabilities predominantly in decreasing field suggests that this value ␣ is close to the critical value; this explains why flux instabilities have first been observed in borocarbides in these samples, having Bean model zero-field Jc values of the order of 106 A cm−2, some two orders of magnitude higher than previously reported samples. In summary, the families of low-Tc superconductors combining moderate Tc values with large coherence lengths provide experimental access to a fuller understanding of the well-established phenomenon of thermomagnetic flux instability. ACKNOWLEDGMENTS Work at the IFW Dresden was supported by the Deutsche Forschungsgemeinschaft as part of SFB463, “Rare earth transition metal compounds: structure, magnetism, and transport.” The work in Göttingen was also supported by the Deutsche Forschungsgemeinschaft. 1 T. H. Johansen et al., Supercond. Sci. Technol. 14, 726 (2001). T. H. Johansen et al., Europhys. Lett. 59, 599 (2002). I. Aranson, A. Gurevich, and V. Vinokur, Phys. Rev. Lett. 87, 067003 (2001). 4 M. Baziljevich, A. V. Bobyl, D. V. Shantsev, E. Altshuler, T. H. Johansen, and S. I. Lee, Physica C 369, 93 (2002). 5 B. B. Goodman and M. Wertheimer, Phys. Lett. 18, 236 (1965). 6 C. A. Durán, P. L. Gammel, R. E. Miller, and D. J. Bishop, Phys. Rev. B 52, 75 (1995). 7 A. V. Bobyl, D. V. Shantsev, T. H. Johansen, W. N. Kang, H. J. Kim, E. M. Choi, and S. I. Lee, Appl. Phys. Lett. 80, 4588 (2002). 8 P. Leiderer, J. Boneberg, P. Brüll, V. Bujok, and S. Herminghaus, Phys. Rev. Lett. 71, 2646 (1993). 9 P. S. Swartz and C. P. Bean, J. Appl. Phys. 39, 4991 (1968). 10 S. C. Wimbush, K. Häse, L. Schultz, and B. Holzapfel, J. Phys.: Condens. Matter 13, L355 (2001). 11 Ch. Jooss, J. Albrecht, H. Kuhn, S. Leonhardt, and H. Kronmüller, Rep. Prog. Phys. 65, 651 (2002). 12 G. Blatter, M. V. Feigel’man, V. B. Geshkenbein, A. I. Larkin, and V. M. Vinokur, Rev. Mod. Phys. 66, 1125 (1994). 2 3 Downloaded 09 Nov 2004 to 129.240.85.155. Redistribution subject to AIP license or copyright, see http://jap.aip.org/jap/copyright.jsp