Formation of the Bi2Sr2CaCu2O8 + δ superconductor with Mg1 − xCuxO inclusions: the phases compatibility and the effect of the preparation route on the material microstructure and properties

Pavel E. Kazin*a, Yuri D. Tretyakova, Vasili V. Lennikova and Martin Jansenb
aChemistry Department, Moscow State University, 119899, Moscow, Russia
bMax-Plank-Institut für Festkörperforschung, D-70569, Stuttgart, Germany

Received 7th April 2000, Accepted 2nd June 2000

First published on UnassignedUnassigned6th October 2000


Abstract

A compatibility between Bi2Sr2CaCu2O8 + δ (Bi-2212) and MgO was investigated, and the Bi-2212–Mg1 − xCuxO composite materials were obtained and characterised. It was established that Bi-2212 interacts with the MgO powder at 850[thin space (1/6-em)]°C producing (Sr,Ca)4 − yBi2Oz and the Mg1 − xCuxO solid solution, while single crystal MgO is stable against Bi-2212 solid and melt up to 1100[thin space (1/6-em)]°C. The Bi-2212 phase is found to coexist with Mg1 − xCuxO, where x ≥ 0.08, at 850[thin space (1/6-em)]°C in air. Magnesium oxide content is estimated to be under 1 mol% in the solid Bi-2212 phase, as well as in the phases formed via the Bi-2212 peritectic decomposition, and in the Bi–Sr–Ca–Cu–O melt. The Bi-2212–Mg1 − xCuxO superconducting composites were prepared by melt-processing using different precursors. The effect of the precursor on the material microstructure and superconducting properties was investigated. The Mg1 − xCuxO submicron particles were found to be rather uniformly distributed in the Bi-2212 matrix, their size depending on the preparation conditions. Application of the nanosize MgO powder as a precursor indicated substantial coarsening of the magnesium oxide particles during the composite processing, the average particle size exceeding 0.2 µm. The composites exhibited higher critical current density as well as better field stability at enhanced temperatures in comparison with the Bi-2212 samples.


1. Introduction

An opportunity for the improvement of high-Tc superconductor parameters such as critical current density (Jc) and mechanical strength is connected with the formation of composite materials consisting of a superconductor matrix and homogeneously distributed inclusions of non-superconducting phases.1–4 The second phase inclusions can act as effective pinning centres for magnetic flux providing an increase in the critical current and its stability in the magnetic field. The problem of low pinning energy especially concerns the Bi2Sr2CaCu2O8 + δ (Bi-2212) superconductor which in other ways is very suitable for the production of long items such as wires, tapes and rods.5–7

Magnesium oxide is often used as an additive to Bi-2212 owing to its stability and ability to retain the materials superconductivity.8–16 Introduction of micrometer size whiskers of MgO provided a better texture and mechanical strength for the Bi-2212 melt-processed material, and thus a several fold increase in Jc.8–10 10 vol.% of the MgO powder was added to keep the sample form and prevent second phase separation during the peritectic melting in a magnetic field.11 It led to bulk textured samples with Jc as high as 1650 MA m−2 at a temperature of 4 K.12 Addition of nanosize MgO powder was found to increase the material magnetization hysteresis width at low temperatures.13 A similar increase in the magnetization was observed below 20 K in the Bi-2212 single crystal with imbedded MgO particles which was attributed to a high density of dislocations within the sample.14 Interesting results were obtained by Yang and Lieber,15 a film of Bi-2212 was deposited on the MgO substrate covered by a “forest” of MgO whiskers with a diameter of 20–30 nm. Such a microstructure is very effective for pinning the flux lines, and the Jc increased by an order of magnitude at 77 K reaching 100 MA m−2 in a field of 0.1 T.

At the same time, both the MgO chemical compatibility with Bi-2212 and its behaviour in the material processing have not been closely investigated. Doping of Bi-2212 with MgO was briefly discussed in our previous works.3,16 In the present paper we report a study on the compatibility between Bi-2212 and MgO and on the formation of the superconductor composites starting from different precursors.

2. Experimental

The precursor powders with cation stoichiometry corresponding to Bi2.1Sr2CaCu2O8 + δ and Bi2.1Sr2CaCu2O8 + δ + 0.8MgO were prepared using nitrate and sol–gel methods.

In the former method a nitrate solution of all metal cations was evaporated and decomposed at 200–400[thin space (1/6-em)]°C. The residue was annealed at 800[thin space (1/6-em)]°C for 6 h, reground and annealed at 850[thin space (1/6-em)]°C for 6 h (precursor 1).

In the sol–gel method 1 g of precursor 1 was added to 6 ml of a solution containing 3 g of citric acid on heating with subsequent dropwise addition of a solution of 25% NH3 to obtain a clear solution. The solution was gently evaporated, the homogeneous solid was decomposed at 250–600[thin space (1/6-em)]°C and annealed at 800[thin space (1/6-em)]°C for 24 h.

The glassified samples were prepared by melting precursor 1 at 1100[thin space (1/6-em)]°C for 15 min and quenching it between copper plates.

The Bi-2212 ceramics were prepared using precursor 1 which was pelletised and annealed at 860[thin space (1/6-em)]°C for 24 h.

The nanocrystalline MgO powders were obtained: (i) by thermal decomposition of Mg(OH)2 at 340[thin space (1/6-em)]°C for 6 h; (ii) by thermal decomposition of MgC2O4 at 550[thin space (1/6-em)]°C for 12 h.

The Bi-2212–Mg1 − xCuxO composites with nominal composition Bi-2212 + 0.8MgO were prepared via melt processing using the following precursors: the glassified material (sample A), the oxide products obtained by the sol–gel method (sample B), the oxide products obtained by the nitrate method (sample C), the mixture of commercial Bi-2212 (Hoechst) and nanosize MgO prepared from MgC2O4 (sample D) or Mg(OH)2 (sample E). The pellets produced from the precursors ground in an agate mortar were heated in air on a MgO single crystal substrate for several hours up to 890–910[thin space (1/6-em)]°C, and kept at this temperature for 1 h (optionally heated to 920–950[thin space (1/6-em)]°C and kept at this temperature for 0.2 h with fast cooling to 880–890[thin space (1/6-em)]°C at 300[thin space (1/6-em)]°C h−1) and slowly solidified by cooling to 850[thin space (1/6-em)]°C at 1[thin space (1/6-em)]°C h−1. The maximum heating temperature was varied to optimise the superconductor Tc and Jc values. For comparison, the Bi-2212 materials without the MgO additive were prepared under the same conditions utilising the procedures used for samples A–D.

For the phase compatibility study, two kinds of experiments were carried out. In the first one, the fine commercial MgO powder (99%) was annealed at 1400[thin space (1/6-em)]°C for 1 h to achieve 0.5–1 micron size MgO grains. Then it was mixed with Bi-2212 to obtain the Bi-2212 + 10MgO composition, pressed into pellets and annealed at 850[thin space (1/6-em)]°C for 24 h. In the second experiment, the small pieces of Bi-2212 ceramic were placed on the MgO single crystals with ca. 1 mm thickness. The separate specimens were annealed in air at either: 850[thin space (1/6-em)]°C for 120 h, 900[thin space (1/6-em)]°C for 24 h, 1000[thin space (1/6-em)]°C for 1 h or 1100[thin space (1/6-em)]°C for 1 h, and quenched in liquid nitrogen. The polished cross-sections of the specimens were examined by scanning electron microscopy.

Powder X-ray diffraction was performed on a DRON-3M diffractometer with CuKα radiation.

Microstructure and chemical composition of the phases were studied using scanning electron microscopes (a Philips ESEM and a Zeiss DSM device) equipped with options for energy dispersive X-ray analysis (EDX). The samples were cut and polished prior to the investigation.

AC magnetic susceptibility was measured on a specially designed susceptometer17 in the temperature range of 15–100 K in AC fields of 0.1 and 10 mT and a frequency of 27 Hz. Magnetisation was measured on a Quantum Design MPMS device at temperatures of 5, 30 and 60 K in fields up to 5 T. For the magnetic measurements, the samples were cut to get rectangular bars of ca. 1 mm thickness, which were placed along the field.

3. Results and discussion

3.1. Compatibility between Bi-2212 and MgO

In our earlier work, we mentioned that in the melt-processed Bi-2212 with inclusions of MgO, the latter, keeping its crystal structure, incorporates some Cu-cations.16 That must change the cation ratio in the Bi–Sr–Ca–Cu–O part of the system, and the secondary phases may appear. At the same time there is evidence that even for a large MgO content the composites exhibit very good superconducting properties.10,12 These facts initiated us firstly to clear up the aspects of the compatibility between Bi-2212 and MgO.
3.1.1. Interaction of Bi-2212 with MgO in the mixture at 850[thin space (1/6-em)]°C. Annealing the pellet of Bi-2212 + 10MgO caused a partial decomposition of the Bi-2212 phase. In an XRD pattern a few new peaks appeared (Fig. 1). They correspond to the monoclinic phase (Sr,Ca)4Bi2O718 which was also considered as having somewhat different stoichiometry Sr11 − xCa5 + xBi9Oz.19,20 The EDX analysis suggests its approximate composition to be (Sr,Ca)4 − yBi2Oz with y ≈ 0.4 that is close to the one reported in the latter work. The major part of the magnesium oxide resides in submicron particle agglomerations from a few to a hundred microns in size. The analysis of different regions in the agglomerations revealed that they contain 0–1 at.% of Bi, Sr, Ca and about 8 at.% of Cu in reference to Mg. The Cu content did not appreciably depend on the size of the agglomerate or on the distance from the interface between the agglomerate and the Bi–Sr–Ca–Cu–O matrix. That confirms that the reaction between MgO and Bi-2212 is virtually complete. The observed compound Mg1 − xCuxO (x = 0.08) retains the MgO crystal structure. Its composition belongs to a solid solution range of CuO in MgO, which was reported to extend at 850[thin space (1/6-em)]°C to x = 0.2, according to Assal et al.,21 or to x ≈ 0.12, according to Paranthaman et al.22 In the Bi-2212 and (Sr,Ca)4−yBi2Oz phases the magnesium oxide content was under the EDX sensitivity level of about 1 mol%.
X-Ray diffraction
pattern of the Bi-2212 + 10MgO sample after the annealing:
Bi-2212 (triangles), (Sr,Ca)4 − yBi2Oz
(plus symbols), Mg1 − xCuxO
(crosses).
Fig. 1 X-Ray diffraction pattern of the Bi-2212 + 10MgO sample after the annealing: Bi-2212 (triangles), (Sr,Ca)4 − yBi2Oz (plus symbols), Mg1 − xCuxO (crosses).

From the cation ratio consideration one can expect formation of additional phases, but that was not observed. This can be explained by taking into consideration the existence of a solid solution range for Bi2 + ySr2CaCu2Oz with 0 < y < 0.3.23 The initial sample had a bulk composition close to Bi2Sr2CaCu2O8 + x. After the annealing, the Bi content was slightly increased, i.e. Bi-2212 was able to accept the Bi surplus that appeared as a result of the formation of the Sr,Ca-rich bismuthate. The change in the phase composition during the reaction is shown in Fig. 2. With decreasing Cu content, the configuration point A moves to the two-phase region: Bi-2212 solid solution–(Sr,Ca)4 − yBi2Oz (point B). At lower Cu contents, one can expect a transition to the three-phase region including the Bi2(Sr,Ca)2CuOz (Bi-2201) phase and possibly to a four-phase region.


Part of the BiO1.5–CuO–Sr2/3Ca1/3O
phase diagram. (1) Bi2 + ySr2CaCu2O8 + δ
solid solution, (2) Bi2(Sr,Ca)2CuO6,
(3) (Sr,Ca)6Bi7O16.5, (4) (Sr,Ca)3.6Bi2Oz.
Point A (cross)
— initial composition of the Bi–Sr–Ca–Cu–O
part of the Bi-2212 + 10MgO sample, point B — the
composition after the sample annealing.
Fig. 2 Part of the BiO1.5–CuO–Sr2/3Ca1/3O phase diagram. (1) Bi2 + ySr2CaCu2O8 + δ solid solution, (2) Bi2(Sr,Ca)2CuO6, (3) (Sr,Ca)6Bi7O16.5, (4) (Sr,Ca)3.6Bi2Oz. Point A (cross) — initial composition of the Bi–Sr–Ca–Cu–O part of the Bi-2212 + 10MgO sample, point B — the composition after the sample annealing.
3.1.2. Interaction of the Bi-2212 melt with a single crystal of MgO. After 120 h annealing at 850[thin space (1/6-em)]°C there was no noticeable change at the interface between the Bi-2212 ceramics and the MgO single crystal. For the samples annealed at and above 900[thin space (1/6-em)]°C, the Bi–Sr–Ca–Cu–O part represented a drop of melt wetting the MgO substrate. At 900[thin space (1/6-em)]°C, the quenched melt contained (Sr,Ca)CuO2, (Sr,Ca)4 − yBi2Oz and Bi-2201 crystals distributed in the glassy matrix; at 1000[thin space (1/6-em)]°C, only grains of CaO were found in the matrix; and at 1100[thin space (1/6-em)]°C, the Bi–Sr–Ca–Cu–O part represented homogeneous glass. In all the cases no additional cations were found in the MgO part starting from 2 µm from the interface with Bi-2212. That limits the possible contents of Bi, Sr,Ca and Cu oxides in MgO to ca. 0.5 mol%. At smaller distances from the interface the cations are detected due to X-ray emission from the adjacent Bi–Sr–Ca–Cu–O part. In the Bi–Sr–Ca–Cu–O parts magnesium oxide was not observed above 1 mol%.

Therefore, the experiments described above allow us to conclude that magnesium oxide in the form of micrometer powder extracts CuO from Bi-2212, thus causing its decomposition toward strontium–calcium bismuthate. In the equilibrium between Bi-2212 and Mg1 − xCuxO the copper content x in the latter phase cannot be less than 0.08. However, cation diffusion from Bi–Sr–Ca–Cu–O into the MgO single crystal is not observed. Hence, the composition of magnesium oxide based inclusions in the superconductor may depend on the route of the MgO introduction.

3.2. The Bi-2212–Mg1 − xCuxO composites

3.2.1. Microstructure and phase composition. The typical SEM micrographs of the Bi-2212–Mg1−xCuxO composites are shown in Fig. 3, the XRD pattern in Fig. 4. All the composites contain two main phases: Bi-2212 and magnesium oxide. The Bi-2212 phase forms large plate-like grains, several hundred microns in size. Small quantities of secondary phases (Sr,Ca)CuO2, (Sr,Ca)2CuO3, (Sr,Ca)4 − yBi2Oz, and Bi-2201 are observed, which are usually present in the melt-processed Bi-2212.
SEM (BSE)
micrographs of the Bi-2212–Mg1 − xCuxO
composites: a) sample D, b) sample E. Light-grey area —
Bi-2212, black submicron particles — Mg1 − xCuxO.
Fig. 3 SEM (BSE) micrographs of the Bi-2212–Mg1 − xCuxO composites: a) sample D, b) sample E. Light-grey area — Bi-2212, black submicron particles — Mg1 − xCuxO.

X-Ray diffraction
pattern of the Bi-2212–Mg1 − xCuxO
composite (sample E): Bi-2212 (triangles), Mg1 − xCuxO
(crosses).
Fig. 4 X-Ray diffraction pattern of the Bi-2212–Mg1 − xCuxO composite (sample E): Bi-2212 (triangles), Mg1 − xCuxO (crosses).

The magnesium cations are not detected in the Bi-2212 phase as well as in the secondary phases. The magnesium oxide submicron particles are found to be rather uniformly distributed inside the Bi-2212 matrix without any agglomeration on the Bi-2212 grain boundaries. Such a behaviour of MgO differs from that of the particles of many other stable phases such as SrZrO3, (Sr,Ca)SnO3, (Sr,Ca)In2O4 and BiSr1.5Ca0.5Al2Oz which have been found to agglomerate partially between Bi-2212 lamella.3,24–27

Sometimes magnesium oxide particles of the same size are observed in the grains of the secondary phases. These phases were formed on the Bi-2212 peritectic melting and partly remained in the sample after the solidification process. It appears that the magnesium oxide particles had existed in the melt and were captured by formed grains of the secondary phases and afterwards by the growing Bi-2212 crystallites.

The composition of the inclusions in all the cases except sample A corresponds to Mg1 − xCuxO with x = 0.08–0.1, i.e. the magnesium oxide has acquired a composition close to an equilibrium one with Bi-2212, rather than staying inert. That implies a 4% deficiency of Cu-ions in the Bi–Sr–Ca–Cu–O part, but it seems to be rather small to affect the sample phase composition and properties, since after the peritectic formation of Bi-2212 some amount of unreacted phases resides both in the undoped Bi-2212 material and in the composite.

In the sample A the x-value is increased to 0.12. Most probably, MgO has acquired additional CuO during the precursor melting at 1100[thin space (1/6-em)]°C. The solubility of CuO in MgO increases with temperature up to 1050[thin space (1/6-em)]°C,22 and one should expect an increase in the cation diffusivity at higher temperature. All this promotes the CuO transfer from the Bi–Sr–Ca–Cu–O melt into the MgO particles.

The size of the included Mg1 − xCuxO lies within a rather narrow range of 0.1–2 µm and varies with the composite preparation method (Table 1). The biggest particles of 1 µm in size were formed from the glassified precursor (method A). Melt-processing of the “single source” precursors (methods B and C) led to somewhat smaller particles. The application of a mixture of Bi-2212 and the nanosize MgO powders provided the smallest grain size of 0.2–0.4 µm.

Table 1 Superconducting parameters of the melt processed materials and the included Mg1 − xCuxO particle size in the Bi-2212–Mg1 − xCuxO composites
MaterialMg1 − xCuxO size/µmTc/KJc at 60 K/MA m−2
Bi-2212–Mg1 − xCuxO:
Sample A1.068913
Sample B0.809317
Sample C0.589134
Sample D0.439246
Sample E0.268948
    
Bi-2212:
Method A 9310
Method B 943
Method C 9126
Method D 9020


The size of the initial MgO nanoparticles was of the order of 10 nm, according to transmission electron microscopy. Analysis of the widening of the XRD lines (Fig. 5) gave a particle size of ≈7 nm for the sample prepared from hydroxide, and ≈14 nm for the sample prepared from oxalate. Hence, considerable coarsening of the MgO particles took place during the material processing. This is probably connected with their recrystallisation in the melt. Thus, the highest temperature applied in method A (1100[thin space (1/6-em)]°C) caused an almost two-fold increase in the particle size in comparison with method C in which the same precursor was used, but without high-temperature melting. Apparently MgO is soluble in the Bi–Sr–Ca–Cu–O melt to some extent, although its solubility appears to be low even at 1100[thin space (1/6-em)]°C.


X-Ray diffraction
patterns of the MgO nanopowders: a) prepared from MgC2O4,
b) prepared from Mg(OH)2, and c) the reference
MgO powder with 0.5–1 µm grain size.
Fig. 5 X-Ray diffraction patterns of the MgO nanopowders: a) prepared from MgC2O4, b) prepared from Mg(OH)2, and c) the reference MgO powder with 0.5–1 µm grain size.
3.2.2. Superconducting properties. In Fig. 6 the AC susceptibility curves are shown for two of the samples. They are typical for all the samples prepared. The composites exhibit Tc = 89–93 K, which is virtually the same as for the undoped Bi-2212 materials (Table 1). At the same time the composites show the sharper transition on the χ′(T) curves, and the χ″(T) peak at a higher temperature. Only one χ″(T) peak and nearly full screening at low temperature allows us to suggest that the supercurrent flows around the whole sample.
Temperature dependence
of AC susceptibility at an AC field of 10 mT: broken line — the
Bi-2212 sample prepared by method C, solid line — the Bi-2212–Mg1 − xCuxO composite (sample D).
Fig. 6 Temperature dependence of AC susceptibility at an AC field of 10 mT: broken line — the Bi-2212 sample prepared by method C, solid line — the Bi-2212–Mg1 − xCuxO composite (sample D).

The critical current density was estimated using the imaginary part of the AC susceptibility at the field of 10 mT and applying Bean’s model for the flux penetration in the superconductor using expressions described in ref. 28. The composites normally show higher critical current density than the corresponding Bi-2212 samples (Table 1). In Fig. 7 the Jc values are plotted vs. the average Mg1 − xCuxO particle size in the composites. The critical current density increases with decreasing particle size. This is quite expected, because at a constant inclusion phase content the number of the inclusions and correspondingly of the flux pinning sites increases, and Jc will be proportional to 1/a, where a is the inclusion size.2 A certain scatter of the Jc data can be connected with other factors, such as defect structure and Tc.


Critical current density Jc
at T = 60 K vs. average Mg1 − xCuxO
particle size d in the Bi-2212–Mg1 − xCuxO
composites.
Fig. 7 Critical current density Jc at T = 60 K vs. average Mg1 − xCuxO particle size d in the Bi-2212–Mg1 − xCuxO composites.

Jc at different magnetic fields was estimated from magnetisation data using the expression Jc = 2ΔM/d (corresponding to the Bean’s model for a slab geometry29) in SI units, where ΔM is the hysteresis magnetisation width at a certain field, and d is the sample thickness. The field dependence of Jc is presented in Fig. 8 for sample D and the Bi-2212 sample (prepared via method C), showed the best characteristics. At T = 5 K, the Jc values are slightly higher for the Bi-2212–Mg1 − xCuxO sample. At T = 60 K the composite reveals a Jc value twice as high at 10 mT and an order of magnitude higher at 80 mT in comparison with the Bi-2212 sample. Relative enhancement in Jc and its field stability at increased temperatures is commonly attributed to the increase in the number of pinning centres with high energy, which remain active at high temperature.4,24 Such pinning centres are quite easy to identify with the Mg1 − xCuxO submicron inclusions.


Field dependence of
the critical current density: the Bi-2212 sample prepared by method C
(triangles), the Bi-2212–Mg1 − xCuxO
composite (sample D, circles).
Fig. 8 Field dependence of the critical current density: the Bi-2212 sample prepared by method C (triangles), the Bi-2212–Mg1 − xCuxO composite (sample D, circles).

4. Conclusions

The Bi-2212 phase interacts with the MgO powder yielding Mg1−xCuxO and (Sr,Ca)4 − yBi2Oz. The Bi-2212 phase coexists with Mg1−xCuxO at x ≥ 0.08. In contrast to that, single crystal MgO is chemically stable against the Bi-2212 solid and melt up to 1100[thin space (1/6-em)]°C. The solubility of magnesium oxide in solid Bi-2212, (Sr,Ca)CuO2, (Sr,Ca)2CuO3, (Sr,Ca)4 − yBi2Oz, Bi-2201, as well as in the Bi–Sr–Ca–Cu–O melt up to 1100[thin space (1/6-em)]°C is limited to low values, under 1 mol%. The composites Bi-2212–Mg1 − xCuxO obtained using different precursor preparation methods consist mainly of the Bi-2212 matrix with uniformly distributed submicron inclusions of Mg1 − xCuxO, their size depending on the precursors used. When applying even nanocrystalline MgO, the Mg1 − xCuxO grains in the composites attain sizes above 0.2 µm due to recrystallisation in the Bi–Sr–Ca–Cu–O melt. The Bi-2212–Mg1 − xCuxO composites exhibit both higher critical current density and better field stability of Jc at enhanced temperatures in comparison with Bi-2212, that discriminates the Mg1 − xCuxO inclusions as effective pinning centres.

Acknowledgements

The work is supported by Russian Fund for Basic Research (projects 97-03-33249a, 00-03-32597a) and Russian Ministry of Science (project “Composite”).

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Footnote

Basis of a presentation given at Materials Discussion No. 3, 26–29 September, 2000, University of Cambridge, UK.

This journal is © The Royal Society of Chemistry 2001
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