CRYSTAL-STRUCTURE AND MAGNETIC-ORDERING OF THE RARE-EARTH AND CU MOMENTS IN RBA2CU2NBO8 (R = ND,PR)

被引:27
|
作者
ROSOV, N
LYNN, JW
RADOUSKY, HB
BENNAHMIAS, M
GOODWIN, TJ
KLAVINS, P
SHELTON, RN
机构
[1] UNIV MARYLAND,CTR SUPERCOND RES,DEPT PHYS,COLL PK,MD 20742
[2] LAWRENCE LIVERMORE NATL LAB,LIVERMORE,CA 94550
[3] UNIV CALIF DAVIS,DEPT PHYS,DAVIS,CA 95616
来源
PHYSICAL REVIEW B | 1993年 / 47卷 / 22期
关键词
D O I
10.1103/PhysRevB.47.15256
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
Using neutron diffraction, we have studied the crystal structure and magnetic ordering of the rare-earth and Cu moments in the layered perovskite systems NdBa2Cu2NbO8 (Nd 2:2:1:8) and PrBa2Cu2NbO8 (Pr 2:2:1:8). These are systems similar to RBa2Cu3O6+, [R 1:2:3:(6+x)] for which the chain Cu-O layers have been fully replaced by layers of Nb-O octahedra. Powder profile refinements below 20 K show that both Nd 2:2:1:8 and Pr 2:2:1:8 are in space group I4/mcm, because the near-neighbor Nb-O octahedra are rotated about the c axis in opposite senses. The Cu moments are ordered below 375(10) K for Nd 2:2:1:8 and 340(15) K for Pr 2:2:1:8, with saturation moments in both cases of 0.5(1)mu(B). The near-neighbor Cu spins are aligned antiparallel, just as for the Cu ''plane'' ordering in R 1:2:3:(6+x). The rare-earth moments order at 1.69(5) and 12.6(1) K for Nd 2:2:1:8 and Pr 2:2:1:8, respectively, with saturated values of [mu(z)] =0.74(5)mu(B) and 1.2(1)mu(B). The near-neighbor R spins, both in the ab plane and along the c axis, are also aligned antiparallel. As in the case of Pr 1:2:3:(6+x), the Pr sublattice of Pr 2:2:1:8 has an ordering temperature that is much higher than other rare-earth moments in these layered perovskites, suggesting that the Pr in Pr 2:2:1:8 experiences the same f-electron hybridization as has been observed in Pr 1:2:3:(6+x). The rare-earth ordering of both Nd 2:2:1:8 and Pr 2:2:1:8 is not completely three-dimensional in nature: rather, the ordering within the a-b plane is two-dimensional with only short-range order along the c axis. The presence of oxygen defects appears to affect the c-axis correlation length.
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收藏
页码:15256 / 15264
页数:9
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