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arXiv 2102.06174physics.chem-ph
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含时无轨道密度泛函理论:背景和泡利核近似

Time-dependent Orbital-free Density Functional Theory: Background and Pauli kernel approximations

Kaili Jiang, Michele Pavanello

摘要:

含时无轨道密度泛函理论是计算大尺度量子系统动力学性质的一种有效方法,与标准含时密度泛函理论相比,它具有计算量小的优点。我们将真实的相互作用费米子系统映射到一个虚构的非相互作用玻色子系统上,从而形式化了这种方法。动力学泡利势和相关的内核出现的时间依赖的轨道自由DFT的关键成分。利用均匀电子气作为模型系统,我们导出了一个近似的频率依赖的泡利核。飞行员计算表明,空间非局部性是这个内核的一个关键特征。非局部项已经在关于无单位频率和倒易空间变量的二阶展开中出现(分别为$\fracω{q\, k_F}$和$\frac{q}{2\, k_F}$)。考虑到所提出的内核令人鼓舞的性能,我们预计它将导致更准确的无轨道DFT模拟纳米级系统的平衡。此外,所提出的制定非绝热泡利内核的路径提出了几种进一步改进的途径,可以在未来的工作中加以利用,以改善结果。

英文摘要:

Time-dependent orbital-free DFT is an efficient method for calculating the dynamic properties of large scale quantum systems due to the low computational cost compared to standard time-dependent DFT. We formalize this method by mapping the real system of interacting fermions onto a fictitious system of non-interacting bosons. The dynamic Pauli potential and associated kernel emerge as key ingredients of time-tependent orbital-free DFT. Using the uniform electron gas as a model system, we derive an approximate frequency-dependent Pauli kernel. Pilot calculations suggest that space nonlocality is a key feature for this kernel. Nonlocal terms arise already in the second order expansion with respect to unitless frequency and reciprocal space variable ($\fracω{q\, k_F}$ and $\frac{q}{2\, k_F}$, respectively). Given the encouraging performance of the proposed kernel, we expect it will lead to more accurate orbital-free DFT simulations of nanoscale systems out of equilibrium. Additionally, the proposed path to formulate nonadiabatic Pauli kernels presents several avenues for further improvements which can be exploited in future works to improve the results.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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