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PHYSICAL REVIEW B VOLUME 46, NUMBER 21 Superconductivity at 86 K in LuBa2Cu3Q7 R. Pinto, S. P. Pai, A. S. Tamhane, P. R. Apte, L. C. Gupta, Tata Institute of Fundamental Department 1 DECEMBER 1992-I s thin films and R. Vijayaraghavan Research, Homi Bhabha Road, Bombay 400005, India K. I. Gnanasekar and H. V. Keer of Chemistry, Indian Institute of Technology, Bombay 400076, India (Received 20 May 1992) Superconductivity has been observed in thin films of LuBa2Cu307 z, which otherwise does not form the 1:2:3 superconducting phase in bulk, presumably due to the small ionic radius of Lu. From this work, it is clear that the substrate inAuences the nucleation of the 1:2:3 superconducting phase in thin films. Results indicate that LuBa2Cu307 z thin films with as good a quality as that achievable with YBa2Cu307 q thin films can be realized; zero resistance transition temperature ( T, ) of 86 K and critical-current density ( J, ) of 5 X 10' A cm at 77 K have been obtained. Early in the history of high-temperature superconductors, it was found that the superconducting properties of orthorhombically distorted and oxygen-deficient perovskites 8 BazCu307 & were nearly independent of the rare-earth element R. Exceptions to this behavior are Ce, Tb, Pr, and possibly Lu. R =Ce and Tb do not form the superconducting 1:2:3 phase. In the case of R =Pr, the phase does form but is semiconducting and orders magnetically. ' Experimental evidence of superconductivity in LuBa2Cu307 & is rather controversial. Early reports have indicated that LuBaCuO forms the superconducting 1:2:3 phase with transition temperature T, above Later reports, however, have shown absence of 77 K. in this system down to very low temsuperconductivity peratures. ' It has also been shown by Somasundaram et al. that due to the small ionic radius of Lu (0.985 A), LuBaCuO does not form a pure 1:2:3 phase and is multiphasic. It is in this context that we undertook the growth and study of the LuBaCuO system in the thin-film form, which, to the best of our knowledge, has not been reported to date. Thin films, because of their proximity to the substrate, are expected to behave considerably different when compared to the bulk materials. In the case of LuBaCuO, which cannot be formed in the pure 1:2:3 phase because of the small ionic radius of Lu, the substrate may be expected to significantly stabilize the LuBaCuO 1:2:3 phase in the thin-film form. Our results have shown that the pure LuBaCuO 1:2:3 phase can indeed be formed in situ by pulsed-laser ablation on many substrates commonly used to grow YBa2Cu307 & films. In this paper, we and study of superconducting discuss the growth LuBa2Cu307 & thin films. Bulk LuBaCuO pellets and targets for pulsed-laser ablation were prepared by mixing stoichiometric amounts of 99.99% purity Luz03, Ba2CO3, and CuO and by using solid-state reaction similar to that a high-temperature used to prepare R 1:2:3 pellets. Since partial melting occurs for Lu 1:2:3 if the temperature exceeds 910 C, all the reactions were carried out at 910'C followed by annealing stages. Thin films of Lu 1:2:3 material were ' ' 46 prepared by pulsed-laser ablation as has been described elsewhere. Polished MgO, SrTi03, and LaA103 substrates, all with (100) orientation, were used for the growth of the films. The KrF excimer laser deposition parameters were optimized to realize in situ grown Lu 1:2:3 thin films of the best possible quality. The optimized conditions are: 3 mm X1 mm laser spot, 3 J cm Auence, 4. 5 cm target-substrate distance, and 200 mTorr oxygen pressure. The substrate temperature used varied from 680 to 720'C. The growth of Lu 1:2:3 films under optimized conditions has been found to be 50 —70 A/min at the beginning of the growth of the films. This is considerably slower than the deposition rate with the Y 1:2:3 target which gives a film growth rate of —100 A/min under similar growth conditions. The thickness of Lu 1:2:3 films studied was in the range of 300 —2000 A. The composition of the films analyzed using energy-dispersive xray (EDX) analysis in the thin-film mode indicated 1:2:3 stoichiometry in the films similar to the bulk targets. The films were initially characterized using x-ray diffraction (XRD) to determine the crystallinity and phase purity. Shown in Fig. 1(b) is the XRD spectrum of a 700 A-thick Lu 1:2:3 film grown on (100) MgO subc-axis-oriented orthorhombic strate. A predominantly phase is clearly seen with the presence of (001 ) lines. This is compared to the XRD spectrum of the bulk Lu 1:2:3 target in Fig. 1(a) which shows the absence of the Lu 1:2:3 orthorhombic phase. Figure 1(c) shows the XRD spectrum of a thicker (1500 A) Lu 1:2:3 film, indicating once again a predominantly c-axis orientation. In realizing films of LuBa2Cu307 & crystallizing in the 1:2:3 phase, the substrate seems to be playing a crucial role. It acts like a template and thus aids the formation of the 1:2:3 phase. The quality of the films improves as their thickness increases (see following). This shows that a few initial layers of the material must be under a strain which gets progressively relaxed as the film thickness in- creases. The resistivity of films was measured using the standard four-probe technique and evaporated silver film contacts. A closed cycle He cryocooler with a temperature 14 242 1992 The American Physical Society BRIEF REPORTS 46 JJ„J1,. ~&i., (b) CA O CD O O cO O O O O CV O t , i 2 h 53 57 21 8 (deg) FIG. 1. X-ray diffraction spectra of LuBaCuO system: (a) bulk pellet; (b) 700 A-thick film on (100) MgO; and (c) 1500A-thick film on (100) MgO. Films show a predominantly caxis orientation with (001 ) lines. 14 243 crease. The highest value of T, of 86 K has been found for films with thicknesses in the range 800 —2000 A. These films also show a narrow transition width hT of about 1.5 K indicating the high quality of the films. As the thickness increases further, critical current density J, has been found to drop considerably. This is true in general with Y 1:2:3 films as well, since it is known that as the film thickness increases above 2000 A, the a-axis fraction in the film also increases. This reduces J, . The results obtained on the structural and superconducting transition of the films grown on (100) SrTi03 and (100) LaA103 substrates have been found to be comparable to those obtained with the films grown on (100) MgO substrates. The films were highly oriented in both cases with T, -86 K and AT-1. 5 K with optimized conditions. Shown in Fig. 3 is the variation of J, with temperature obtained with 1000-A-thick films grown on (100) MgO. J, was measured using patterned 100-pm-wide microbridges and by using the 1 pV/mm voltage criterion. The best value Of J, obtained with Lu1:2:3 films is 5X10 Acm at 77 K. Both LsA103 and SrTi03 substrates have shown similar results. It can be seen in Fig. 3 that the J, vs T plot of Lu 1:2:3films is linear and is similar to that of Y 1:2:3 films. ' This indicates that the thermally activated self-field-induced flux-creep mechanism operating in Lu 1:2:3 thin films is similar to that existing in the Y1 2:3 films. ' The fact that we can prepare superconducting thin of LuBazCu307 & implies an important relationship between superconductivity and structure: among the compounds RBa2Cu307 & in which the R ion is in the trivalent state, LuBa2Cu307 & is the only one which in bulk does not crystallize in the 1:2:3 phase and does not superconduct. The present work shows that once the structure is restored, superconductivity is also restored. This should have an important on the bearing phenomenon of superconductivity in the 1:2:3materials. To summarize, we have reported the successful growth of thin films of an LuBaCuO system which normally does not form the superconducting 1:2:3 phase in bulk due to films controller was used to electrically characterize the in the temperature range 10—300 K. All the Lu 1:2:3 films showed metallicity with a resistivity -3X10 cm at 300 K. Shown in Fig. 2 are resistancetemperature plots of Lu 1:2:3 films with various thicknesses in situ grown on ( 100) MgO substrates. The transition temperature for zero-resistance T, is about 72 K for the thinnest films (-300 A) studied. As the film thickness increases, the value of T, has been found to in- Lu1:2:3 films 100 100 X10 80— LuBa&Cu307 gThin Film 80o 60- 60- CD E CD 4Q 20— 20- Q 0 0 20 I )00 200 t I 30 t I 40 l I 50 300 Temperature Temperatue (K ) FIG. 2. Resistance-temperature plots of LuBa2Cu307 in situ grown on ( 100) MgO with various thicknesses. z films FIG. 3. Variation of J, 0 I 1 1 60 I 70 80 90 (K) with temperature s film grown on 1000-A-thick LuBa2Cu307 patterned into 100-pm-wide microbridge. obtained with a MgO and (100) 14 244 BRIEF REPORTS the small ionic radius of Lu. The in situ growth of highquality LuBa2Cu30~ & thin films by pulsed laser deposition on MgO, SrTi03, and LaA103 substrates indicates that the substrate strongly influences the nucleation and stabilization of the superconducting Lu 1:2:3phase. 'P. H. Hor, R. L. Meng, Y. Q. Wang, L. Gao, Z. J. Huang, J. Bechtold, K. Forster, and C. W. Chu, Phys. Rev. Lett. 58, 1891 (1987). Z. Fisk, J. D. Thompson, E. Zirngiebl, J. L. Smith, and S. W. Cheong, Solid State Commun. 62, 743 (1987). 3P. Somasundaram, A. Mohan Ram, A. M. Umarji, and C. N. R. Rao, Mater. Res. Bull. 25, 331 (1990). ~L. Soderholm, J. Zhang, D. G. Hinks, M. A. Beno, J. D. Jorgensen, C. U. Segre, and I. K. Schuller, Nature 328, 604 (1987). 5Y. Dalichaouch, M. S. Torikachvili, E. A. Early, B. W. Lee, C. L. Seaman, K. N. Yang, H. Zhou, and M. B. Maple, Solid State Commun. 65, 1001 (1988). 46 The authors would like to thank Dhananjay Kumar, C. P. D'Souza, B. S. Amin, and O. B. Fernandes for experimental assistance. One of the authors would like to thank the Council of Scientific and Industrial Research for financial support. J. M. Tarascon, W. R. McKinnon, L. H. Greene, G. W. Hull, and E. M. Vogel, Phys. Rev. B 36, 226 (1987). 7A. Oota, Y. Sasaki, M. Ohkubo, and T. Hioki, Jpn. J. Appl. Phys. 27, L1425 (1988). R. Pinto, S. P. Pai, C. P. D'Souza, L. C. Gupta, R. Vijayaraghavan, Dhananjay Kumar, and M. Sharon, Physica C 196, 264 (1992). F. Vassenden, G. Linker, and J. Geerk, Physica C 175, 566 (1991), ' Ravi Kumar, S. P. Pai, S. K. Malik, R. Pinto, P. R. Apte, R. and Dhananjay Kumar, Phys. Rev. B 46, Vijayaraghavan, 5766 (1992).