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arXiv 1201.6523cond-mat.str-elhep-th
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一维自旋1/2海森堡-伊辛磁体对微波的吸收

On the absorption of microwaves by the one-dimensional spin-1/2 Heisenberg-Ising magnet

M. Brockmann, F. Göhmann, M. Karbach, A. Klümper, A. Weiße

摘要:

我们分析了微波吸收的海森伯-伊辛链结合精确计算,模型的可积性的基础上,与数值计算。在线性响应理论中,吸收强度由动态磁化率的虚部决定。归一化强度的矩可以用来定义由相互作用引起的共振频率的偏移和独立于谱线形状的线宽。这些力矩可以精确地计算为温度和外部磁场强度的函数,只要磁场沿着链的对称轴定向。这使我们能够讨论的线宽和共振位移为一个给定的磁场在整个范围内的可能的各向异性参数。对于这些数据的解释,我们需要一个定性的知识,我们从完全数值计算有限链的线形。目前的理论还不能给出精确的线形分析结果。从我们的数值计算工作中,我们可以提取,但是,在高温下,这是非常准确的各向异性参数的范围很广,是准确的自由费米子点和各向同性点的线形的经验无参数模型。在零温度和零磁场极限下,可以对线形进行另一种预测,其中充分各向异性的模型显示出强吸收。对于各向异性参数在大量的阶段,我们得到确切的两个自旋贡献的谱线。从强度和规则,它可以被估计,如果各向异性参数是适度高于其值在各向同性点,该贡献占80%以上的光谱权重。

英文摘要:

We analyze the absorption of microwaves by the Heisenberg-Ising chain combining exact calculations, based on the integrability of the model, with numerical calculations. Within linear response theory the absorbed intensity is determined by the imaginary part of the dynamical susceptibility. The moments of the normalized intensity can be used to define the shift of the resonance frequency induced by the interactions and the line width independently of the shape of the spectral line. These moments can be calculated exactly as functions of temperature and strength of an external magnetic field, as long as the field is directed along the symmetry axis of the chain. This allows us to discuss the line width and the resonance shift for a given magnetic field in the full range of possible anisotropy parameters. For the interpretation of these data we need a qualitative knowledge of the line shape which we obtain from fully numerical calculations for finite chains. Exact analytical results on the line shape are out of reach of current theories. From our numerical work we could extract, however, an empirical parameter-free model of the line shape at high temperatures which is extremely accurate over a wide range of anisotropy parameters and is exact at the free fermion point and at the isotropic point. Another prediction of the line shape can be made in the zero-temperature and zero magnetic field limit, where the sufficiently anisotropic model shows strong absorption. For anisotropy parameters in the massive phase we derive the exact two-spinon contribution to the spectral line. From the intensity sum rule it can be estimated that this contribution accounts for more than 80% of the spectral weight if the anisotropy parameter is moderately above its value at the isotropic point.

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