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Spin response in HTSC cuprates: generalized RPA approach with projection operators method

机译:HTSC铜酸盐中的自旋响应:带投影算子方法的广义RPA方法

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We derive the dynamical spin susceptibility in the t-J-G model combining the random phase approximation (RPA) and projection operator method, which allows describing the mutual interplay between the local and the itinerant components of susceptibility. Near the antiferromagnetic wave vector the calculated dispersion of the spin excitations reproduces well the so-called hour-glass dispersion, characteristic for several layered cuprates. It is formed as a result of competition between the original spin-gap in magnon-like excitations spectrum and the superconducting gap, which affects the itinerant component of the susceptibility. Furthermore, the calculated collective spin excitations along (0,0)-(0,π) are in agreement with the positions of the absorption peaks in the inelastic X-ray scattering spectra. They refer to the paramagnon-like modes, characteristic to the itinerant spin system, rather than magnon-like excitations that originate from short range order effect in the system of local spins at Cu sites.
机译:我们结合随机相位近似(RPA)和投影算子方法,在t-J-G模型中得出了动态自旋磁化率,从而可以描述磁化率的局部分量和迭代分量之间的相互作用。在反铁磁波向量附近,自旋激发的计算出的色散很好地再现了所谓的沙漏色散,这是多层铜酸盐的特征。它的形成是由于类磁振子激发光谱中的原始自旋间隙与超导间隙之间的竞争而造成的,这影响了磁化率的迭代分量。此外,沿着(0,0)-(0,π)计算的集体自旋激发与非弹性X射线散射光谱中的吸收峰的位置一致。他们指的是巡回旋自旋系统特有的顺磁子状模式,而不是源自Cu位置局部自旋系统中短程有序效应的磁子状激发。

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