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Quantum many body calculations: An improved weighted density approximation to electronic density functional theory and Monte Carlo studies of superfluid vortices.

机译:量子多体计算:电子密度泛函理论和超流旋涡的蒙特卡罗研究的改进加权密度近似。

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摘要

This thesis uses computational methods to investigate two very different many body problems. The first half develops a weighted spin-density approximation (WSDA) to the electronic exchange-correlation functional. The second half describes Monte Carlo simulations of the vortex excitation in superfluid helium.; After reviewing in Chapter 1 the current status of electronic density functional theory, Chapter 2 develops a fully non-local approximation to the exchange-correlation functional for electrons. The energy functional treats correlation locally and exchange in the WSDA. Atomic ground state energies within this approximation are much improved over those within the popular local spin-density approximation (LSDA). This formulation of the weighted spin-density functional is particularly efficient when applied to problems in quantum chemistry and therefore allows for the first tests of this type of functional on molecules. Results for bond lengths, dissociation energies, and vibrational frequencies for some first row dimers are somewhat disappointing. Chapter 3 argues that this deficit results from an unphysical inter-shell interaction, which underestimates the screening between valence electrons and therefore weakens the bonding. When this interaction is removed in a qualitative fashion, the molecular results show good agreement with experiment. While the resulting form is not elegant, it accurately describes molecular properties.; The second part of the thesis describes variational calculations of the properties of a quantum vortex line in both two and three dimensional helium. These Monte Carlo calculations are based on two variations of a "shadow" wave-function. The first generates a singular vortex by simply multiplying the ground state wave-function by a phase. The second form distributes the vorticity over a finite core by exploiting the properties of the "shadow" wave-function. We calculated the radial dependence of the density, velocity field and excitation energy and find that the latter hardly changes as the density is increased from equilibrium to near freezing. This result appears to provide an explanation of why the classical core parameter, obtained from fitting experimental data for the energy and velocity of large vortex rings, expands as the density increases. The last chapter then applies these results to study the binding of a {dollar}sp3{dollar}He impurity to a vortex.
机译:本文使用计算方法来研究两个非常不同的许多身体问题。上半部分开发了电子交换相关函数的加权自旋密度近似(WSDA)。下半部分描述了超流氦中涡旋激发的蒙特卡罗模拟。在第1章回顾了电子密度泛函理论的现状之后,第2章提出了对电子交换相关泛函的完全非局部近似。能源功能部门在WSDA中本地处理关联和交换。与流行的局部自旋密度近似(LSDA)内的能量相比,该近似内的原子基态能量得到了很大的改善。当应用于量子化学中的问题时,这种加权的自旋密度官能团的配方特别有效,因此可以在分子上进行这类官能团的首次测试。一些第一行二聚体的键长,解离能和振动频率的结果有些令人失望。第三章认为,这种缺陷是由于壳之间的非物理相互作用而引起的,这种相互作用低估了价电子之间的屏蔽作用,从而削弱了键合。当以定性的方式消除这种相互作用时,分子结果与实验吻合良好。尽管所得的形式不美观,但它可以准确地描述分子性质。论文的第二部分描述了二维和三维氦中量子涡旋线的性质的变分计算。这些蒙特卡洛计算基于“阴影”波函数的两个变化。第一种方法是通过简单地将基态波函数乘以一个相位来生成奇异涡旋。第二种形式通过利用“影子”波函数的特性将涡旋分布在有限的核心上。我们计算了密度,速度场和激发能的径向依赖性,发现随着密度从平衡增加到接近冻结,后者几乎不变。该结果似乎可以解释为什么从密度大的涡旋环的能量和速度的拟合实验数据中获得的经典核心参数会随着密度的增加而扩展。然后,最后一章将这些结果应用于研究{dol} sp3 {dol}} He杂质与涡旋的结合。

著录项

  • 作者

    Sadd, Michael Alan.;

  • 作者单位

    Cornell University.;

  • 授予单位 Cornell University.;
  • 学科 Physics Condensed Matter.
  • 学位 Ph.D.
  • 年度 1998
  • 页码 128 p.
  • 总页数 128
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 O49;
  • 关键词

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