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Perturbation theory for strongly frustrated finite spin systems.

机译:强受挫有限自旋系统的摄动理论。

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摘要

The topic of this study is the magnetic properties of closed clusters. The first issue addressed is the connection between magnetic properties and connectivity in essentially exact solutions of S = ½ quantum spin clusters. The second is the effect of magnetic anisotropy in a cluster on spin coherence.; The first issue is investigated for a set of model systems whose magnetic properties have strong dependence on connectivity at the classical approximation [1, 2]. The magnetization or its first derivative has a discontinuity as a function of applied field, depending on the number of sites in the system. The question I address is whether this dependence on connectivity survives in exact solutions for S = ½ clusters.; An effective Hamiltonian for degenerate states derived from classical ground states is calculated as a power series in the strength of quantum fluctuations, λ. These series converge asymptotically and are summed using Padé approximants. I have found that this dependence of magnetization on the number of sites is reflected in the analytic structure of the ground state energies and wavefunctions as functions of λ. This study exploits the use of large scale computing facilities to carry out high-precision perturbation expansions to high orders, ∼200–300.; The second issue investigated is the influence of magnetic anisotropy on magnetic clusters which are complexes of Fe, Mn and V atoms and behave as groups of up to 15 magnetic moments isolated from one another in crystals [3, 4]. These clusters have interesting magnetic properties and, most recently, it has been shown how one of them could be exploited as a qubit, a bit for a quantum computer [5].; I investigate a model for V15, a complex of 15 S = ½ Vanadium atoms. The model includes a Heisenberg term and a symmetry allowed Dzyaloshinskii-Moriya (DM) interaction. I calculate the properties of this model as a function of temperature and external field using perturbation theory. By comparing with data I evaluate the parameters of the DM interaction. I show that this magnetic anisotropy term is an intrinsic source of decoherence for moments induced by external fields even at zero temperature.
机译:这项研究的主题是封闭星团的磁性。解决的第一个问题是在 S = 1/2量子自旋簇的精确解中,磁性能与连通性之间的联系。第二个是簇中的磁各向异性对自旋相干性的影响。对于第一个问题,研究了一组模型系统,这些模型系统的磁性能在经典近似下强烈依赖于连通性[1,2]。磁化强度或其一阶导数具有不连续性,取决于应用场的数量,具体取决于系统中站点的数量。我要解决的问题是,对于 S =½个簇的精确解决方案,这种对连接性的依赖性是否仍然存在。计算从经典基态导出的简并态的有效哈密顿量,将其作为量子涨落强度λ中的幂级数。这些级数渐近收敛,并使用Padé近似值求和。我发现,磁化强度对位点数量的依赖性反映在基态能量和波函数作为λ函数的解析结构中。这项研究利用大型计算机设施将高精度扰动扩展到200〜300的高阶。研究的第二个问题是磁各向异性对磁性簇的影响,这些簇是Fe,Mn和V原子的复合物,在晶体中以相互隔离的最多15个磁矩的形式出现[3,4]。这些簇具有有趣的磁学性质,最近已经证明了其中的一个簇可以如何被用作量子比特,特别是量子计算机[5]。我研究了V 15 的模型,V 15 是15个 S =½钒原子的复合物。该模型包括一个Heisenberg项和一个对称的Dzyaloshinskii-Moriya(DM)相互作用。我使用扰动理论计算了该模型的特性,该特性是温度和外部场的函数。通过与数据比较,我评估了DM交互的参数。我表明,即使在零温度下,对于外部磁场引起的力矩,该磁各向异性项也是退相干的内在来源。

著录项

  • 作者

    Konstantinidis, Nikolaos P.;

  • 作者单位

    State University of New York at Buffalo.;

  • 授予单位 State University of New York at Buffalo.;
  • 学科 Physics Condensed Matter.
  • 学位 Ph.D.
  • 年度 2002
  • 页码 134 p.
  • 总页数 134
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 O49;
  • 关键词

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