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arXiv 0709.2250cond-mat.mtrl-scicond-mat.str-el
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自旋三聚体化合物Ca3 Cu3xNix(PO4)4(x= 0,1,2)的晶体和磁性结构

Crystal and magnetic structures of the spin-trimer compounds Ca3 Cu3xNix (PO4)4 (x=0,1,2)

V. Yu. Pomjakushin, A. Furrer, D. V. Sheptyakov, E. V. Pomjakushina, K. Conder

摘要:

用中子粉末衍射方法研究了一系列新的量子自旋三聚体体系Ca 3Cu 3xNix(PO 4)4(x= 0,1,2)在1.5-290 K温度下的晶体和磁性结构.每个三聚体含一个Ni(x=1)的组合物具有单斜结构(空间群P21/a,no.14),晶胞参数a = 17.71 A,b = 4.89 A,c = 8.85 A和= 123.84 deg(T=290 K)。(x=2)组成在C2/c空间群(no.15)中结晶,具有沿c轴的双重晶胞。每个三聚体由两个晶体学位置形成:一个在三聚体的中间,第二个在三聚体的末端。我们发现,在(x=1)的三聚体中,Cu ~(2+)占据中间位置,而在(x=2)的三聚体中,Cu ~(2+)和Ni ~(2+)占据末端位置。在TN = 20 K以下,(x=2)化合物显示出反铁磁有序,传播矢量星{[1/2,1/2,0],[-1/2,1/2,0]}用不可约表示τ 22很好地描述了磁性结构,其中使用了具有Ni 2+和Cu 2+的磁矩为1.89(1)μ B和0.62(2)μ B的恒星{k}的两臂离子,分别。我们注意到,我们的粉末衍射数据不能用只包含传播矢量星的一个臂的模型来拟合。Cu/Ni自旋在不同的三聚体中形成平行和反平行构型,这意味着三聚体间相互作用对整体磁性结构的实质性影响。

英文摘要:

Crystal and magnetic structures of a series of novel quantum spin trimer system Ca3Cu3xNix(PO4)4 (x=0,1,2) were studied by neutron powder diffraction at the temperatures 1.5-290 K. The composition with one Ni per trimer (x=1) has a monoclinic structure (space group P 21 /a, no. 14) with the unit cell parameters a = 17.71 A, b = 4.89 A, c = 8.85 A and = 123.84 deg at T=290 K. The (x=2) composition crystallizes in the C 2/c space group (no. 15) with the doubled unit cell along c-axis. Each trimer is formed by two crystallographic positions: one in the middle and the second one at the ends of the trimer. We have found that the middle position is occupied by the Cu2+, whereas the end positions are equally populated with the Cu2+ and Ni2+ for (x=1) while in the (x=2) the trimers were found to be of only one type Ni-Cu-Ni. Below TN = 20 K the (x=2) compound shows an antiferromagnetic ordering with propagation vector star {[1/2,1/2, 0], [-1/2,1/2, 0]} The magnetic structure is very well described with the irreducible representation tau22 using both arms of the star {k} with the magnetic moments 1.89(1) muB and 0.62(2) muB for Ni2+ and Cu2+ ions, respectively. We note that our powder diffraction data cannot be fitted by a model containing only one arm of the propagation vector star. The Cu/Ni-spins form both parallel and antiparallel configurations in the different trimers, implying substantial effect of the inter-trimer interaction on the overall magnetic structure.

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