论文标题
通过选定的配置相互作用和扰动理论对量子纳米结构中相互作用载体的准确描述
Accurate and efficient description of interacting carriers in quantum nanostructures by selected configuration interaction and perturbation theory
论文作者
论文摘要
我们提出了一种基于原子的紧密结合计算以及迭代选择构型和扰动理论的结合的方法来计算百万个原子量子纳米结构中相互作用载体的多体状态。该方法可以对具有接近完整的配置相互作用精度的大型激子复合物和多电子系统进行研究,即使对完整的多体希尔伯特空间的一个小子空间进行了采样,从而节省了计算资源中的幅度。该方法的重要优点是,收敛性受单个参数,阈值,地面和激发态可以在相等的基础上进行处理。我们通过对多达13个激子组成的复合物的数值研究来证明该方法的极端效率,这需要将状态填充到第四个电子壳中。我们发现该方法通常是阈值函数快速收敛的,这是由于扰动校正而从显着增强中获利的。讨论了选择单粒子基态的作用。发现该算法仅针对高电动系统(库仑排斥力占主导地位)而以哈特里栅极为基础收敛得更快。最后,基于二阶扰动能量校正仅取决于多体哈密顿量的偏离元素的观察结果,我们提出了一种准确计算多体状态的方法,该状态仅需要相对较少的库仑矩阵元素。
We present a method to calculate many-body states of interacting carriers in million atom quantum nanostructures based on atomistic tight-binding calculations and a combination of iterative selection of configurations and perturbation theory. This method enables investigations of large excitonic complexes and multi-electron systems with near full configuration interaction accuracy, even though only a small subspace of the full many-body Hilbert space is sampled, thus saving orders of magnitudes in computational resources. Important advantages of this method are that the convergence is controlled by a single parameter, the threshold, and that ground and excited states can be treated on an equal footing. We demonstrate the extreme efficiency of the method by numerical studies of complexes composed of up to 13 excitons, which requires filling of states up to the fourth electronic shell. We find that the method generally converges fast as a function of the threshold, profiting from a significant enhancement due to the perturbative corrections. The role of the choice of single-particle basis states is discussed. It is found that the algorithm converges faster in the Hartree-Fock basis only for highly charged systems, where Coulomb repulsion dominates. Finally, based on the observation that second order perturbative energy corrections only depend on off-diagonal elements of the many-body Hamiltonian, we present a way to accurately calculate many-body states that requires only a relatively small number of Coulomb matrix elements.