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Physica C 185-189 (1991) 601-602 North-Holland
SUPERCONDUCTIVITY AT 60K IN L a 2 . x S r x C a C u 2 0 O I0<x '%0,4} SYNTHESIZED USING AN 0 2 .
HIP T E C H N I Q U E
Takeshi SAKURAI, Toru YAMASHITA', H. YAMAUCHi and Shoji TANAKA
Superconductivity Research Laboratory, ISTEC. 10-13 Shinonome 1-chome, Koto-ku, Tokyo ! 35, JAPAN
Superconducting La2.xSrxCaCu206 1326 phase) samples (with x in the range of 0 < x <0.4) exhibiting Tc °nset at 60K
were synthesized using an O2-H1P (hot isostatic press) technique. The HIP-processing temperature, Ta. was found to be
the key parameter for obtaining superconductivity Csuperconductor-izalion") in the 326 samples, as long as the other
parameters unchanged. A cation ordering between two cation sites, i.e. 4e and 2a sites, was concluded in the
superconducting 326 sample with x=O,2 by structural refinement. The cation ordering is thought to be one of the major
reasons for the superconductor-ization of 326 samples.
I: INTRODUCTION
As the 326 compound posses crystallographic as well as
chemical features common with conventional high Tc
superconducting cuprates, it had been thought that
superconductivity should occur by chemical dopingll-5l.
Nonetheless, no one had been successful up until Cava.
et.al[6] recently reported that they had successfully
synthesized Lal.6Sro.4CaCu206 with Tc °riser at 60K,
They employed a long-time annealing under a high 0 2
pressure of 20arm. In this present work, we attempt to
search for the optimum condition to "superconductor-ize"
326 samples using an O2-HIP technique and discuss the
reasons for such superconductor-ization.
2: EXPERIMENTAL PROCEDURE
The samples were prepared by a conventional solid-state
reaction method plus an O2-HIP process[7]. Samples
sintered at a variety of temperatures, Ts, (900 °C < Ts~_ 1070
°C), were HIP-processed at various temperatures, Ta, 1920
C _ Ta_ 1270 C), for various periods of time, t, up to
10Oh. For HIP-processing, a mixture of 80%-Ar gas and
20%-0 2 gas of the toL-'d pressure of 1000atm was utilized
The crystallographic structure of the samples were
analyzed by x-ray diffraction. A neutron diffraction was
performed for the structural refinement. Electrical
resistivity was measured as a function of temperature using a
conventional four-probe techmque. The magnetic
susceptibility was measured in a d.c. magnetic field of 10 Oe
using a SQUID magnetometer.
3: RESULTS AND DISCUSSION
Superconducting 326 phase was contained in all samples
with compositions, x=0.1, 0,2.0.3 and 0.4. It seems that
the formed phases and supercondcting properties depend on
Ta. but only a little on Ts. As Ta increases, the normal state
resistivity gets lower, while Tc °nsct remains near 60K for
all the samples except one that HiP-processed at g29 °C.
Vvq~en Ta exceeds 1070 °C, Tc°nSet's gets deteriorated. Ta
higher than 970 ~ is required in order to superconductor-ize
!he 37~6 pha~e. The optimum value for Ta is found zo be
1070'~" for the superconductor-ization. Note that sampte~
with Ta betv~een 970 ~ ar.,d 1170'(" are ~1 single pha~e.
Figure 1 show's the electrical resistivity -vs- temperature
curves for the samples witr~ x=0,2 which were HIF-
processed at various period~ up ~.o ' ~, , =
' Present address: Electron Microscope' Centre, University of Queensland, St. Lucia. Brisbane, Queensland 4G72.
AUSTRALIA
0921-4534/91/$03.50 © 1991 - Elsevier Science Publishers B.V, All rights rcsc~'ed.
602 7". Sakurai et aL / Superconductivi~ at 60K in La2aSrxCaCu206 (O <x~0.4) synthesized
100 . . . . , . . . . , . . . . , . . . . , . . . . , . . . .
• Oh; I s i lnlerl ld
,o :\
a 6 ~ , , a ~ a611'mb '
0 5 0 1 0 0 150 2 0 0 2 5 0 3 0 0
Temperature (K)
Fig.l. Electrical resistivity -vs- temperature for
the "326" samples, La 1.8Sr0.2CaCu206,
in terms of the HIP-process periods, t
=6h, 27h, 50h and 100h, when (Ts, Ta) =
(950 ~ , 1020 L').
(950 ~, 1020 L'-'). As t increases, the quality of the sample gets better. Another evidence was detected in the magnetic susceptibility measurement. The longer t is, the larger the Meissner volume fraction is.
The crystal structure refinement was made for the
superconducting La 1.8Sr0.2CaCu206.01 +0.01 [81. In the
final refinement, a cation ordering was concluded. That is,
Sr ions occupy the 4e sites exclusively and Ca ions occupy
the 4e sites with a very low value of occupancy. This result agrees with other refinement data[9](Table. I ).
There seems to be two independent effects in the O2-HIP-
process. One is the total pressure effect, which should act a
driving force for the cation ordering. The other is the
oxygen pressure effect, that may control the oxygen content. It is suspected that a high oxygen pressure effectively
introduces oxygen ions into the defect sites around the cation
at 4e site, Therefore, in the 326 sample O2-HIP-processed ,
the Sr ion substituting only for La ion should be effective as a hole donor to the CuO 2 planes.
4: CONCLUSION
The "superconductor-ized" 326 compounds were
successfully obtained by means of an O2-HIP technique.
The superconducting 326 compounds were obtained in the
range of 0<x~<0.4, when Ta>970~C. The optimum
value of Ta was determined to be 1070~, regardless the
Table.l. Refined structure parameters for the
superconducting "326" samples.
3ornpot,,~l 3ond length 3aAa.O I xa
This work Lal .SSdL2CaCu206.O,I
2.4934(~ 2.6530(9), 2.1537(31
,2.345911si
,,,,t/..~ a-O 1 )(4 La/Sr/Cs-02 )(4 L.a/S~/Ca-02 xl Cu-O],y4, 1.911510' ) Cu-02 xt 2.3068(20) ~u-03 I(1 1.6704~1 C a t i o n . r a t i o
Laur~/Cil (2a} La/Sr/Ca (4e) Occupancy 01 02 03 Lattice parameter a c
0.14(010.~4~i
CavJ's 9roupe 191 ,. ka1.6.SrO.4C&Cu205.94
2.348(~ 1.91201 ' 2.293(61
0.1gl I0 I 0.8'15 0.63 / 0.1, / 0.07 0.708 / 0.2 10,096
1.02 1.02 0.97 0.03
0.955
3.0207 3.8208 19.5434 19.5993
2.11 2.14
value of Ts. Single phase compounds were obtained for the Sr content in the range of 0.1 < x _ 0 . 3 5 .
A cation ordering was determined by a joint x-ray/neutron
diffraction technique for the superconducting sample. Cation ordering occurred under a high pressure, i.e. during
HIP-processing, was likely to be one of the reasons for the superconductor-ization of the 326 compounds.
ACKNOWLEDGEMENT
Authors acknowledge to Dr. J. O. Willis of SRL-ISTEC
and Dr. G. H. Kwei of Los Alamos National Laboratory for
their helpful discussions. This work was supported by
New Energy and Industry Technology Development
Organization as a part of program for R&D of Basic Technology for Future Industries
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