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Magnetic properties of undoped YBa_2Cu_3O_(6+x) system

机译:未掺杂YBa_2Cu_3O_(6 + x)系统的磁性

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In the present paper, we study the magnetic properties of bilayer cuprate antiferromagnets. In order to evaluate the expressions for spin-wave dispersion, sublattice magnetization, Neel temperature and the magnetic contribution to the specific heat, the double time Green's function technique has been employed in the random phase approximation (RPA). The spin wave dispersion curve for a bilayer antiferromagnetic system is found to consist of one acoustic and one optic branch. The "optical magnon gap" has been attributed solely to the intra-bilayer exchange coupling (J_⊥) as its magnitude does not change significantly with the inter-bilayer exchange coupling (J_z). However J_z is essential to obtain the acoustic mode contribution to the magnetization. The numerical calculations show that the Neel temperature (T_N) of the bilayer antiferromagnetic system increases with the J_z and a small change in J_z gives rise to a large change in the Neel temperature of the system. The magnetic specific heat of the system follows a T~2 behaviour but in the presence of J_z it varies faster than T~2.
机译:在本文中,我们研究了双层铜酸盐反铁磁体的磁性。为了评估自旋波色散,亚晶格磁化强度,尼尔温度和磁对比热的表达式,在随机相位近似(RPA)中采用了双重时间格林函数技术。发现双层反铁磁系统的自旋波频散曲线由一个声学分支和一个光学分支组成。 “光学磁振子间隙”仅归因于双层内交换耦合(J_⊥),因为其大小不会随双层间交换耦合(J_z)显着改变。但是,J_z对于获得声模对磁化的贡献至关重要。数值计算表明,双层反铁磁系统的Neel温度(T_N)随J_z的增加而增加,而J_z的小变化会引起系统的Neel温度的大变化。系统的磁比热遵循T〜2行为,但是在存在J_z时,它的变化快于T〜2。

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