Pyper N C, Naginey T C, Whelan Colm T
Yusuf Hamied Department of Chemistry, University of Cambridge, Lensfield Road, Cambridge CB2 1EW, United Kingdom.
Department of Materials, University of Oxford, Parks Road, Oxford OX13 PH, United Kingdom.
J Chem Phys. 2021 Dec 7;155(21):214301. doi: 10.1063/5.0066626.
Atoms remaining as recognizably distinct constituents of bulk condensed phases can have properties modified from those of the isolated species. Dense helium bubbles at high pressures are a common form of radiation damage degrading the mechanical and electrical properties of host materials. Detailed knowledge is critical for predicting their long term performance. Modifications of the ground and first singlet excited states of confined compressed helium are investigated using an entirely non-empirical theory based on the results of ab initio self-consistent field calculations with corrections for the effects of electron correlation. For finite sized portions representing bulk condensed fcc and bcc phases of helium atoms, Hartree-Fock wavefunctions, energies, and charge distributions were computed as a function of different atomic densities using two models. The first model for the first excited state localizes the excitation on the central atom; in the second model, this is partially delocalized over the closest atomic neighbors. Total energies for the finite size portions are derived by adding the inter-atomic dispersive attractions and a density functional description of the short-range inter-atomic correlation energy. The experimental energy of the first allowed electronic transition increases with density being larger than in an isolated atom. The intra-atomic correlation energy does not contribute to this energy shift. The calculated energy shifts agree well with experiment for both bulk solid and liquid helium. The 2p orbital is increasingly compressed by density enhancement, thus generating the energy shifts. Consequently, calculations of the inelastic electron scattering cross sections are substantially incorrect if the compression of the final 1s2p state is not included. The character of the excitations is examined, and it is argued that these are of Frenkel rather than the Wannier type.
作为大块凝聚相可识别的不同成分而保留的原子,其性质可能会与孤立物种的性质有所不同。高压下的致密氦气泡是一种常见的辐射损伤形式,会降低主体材料的机械和电学性能。详细的知识对于预测它们的长期性能至关重要。利用基于从头算自洽场计算结果并对电子关联效应进行修正的完全非经验理论,研究了受限压缩氦的基态和第一单重激发态的变化。对于代表氦原子体心凝聚面心立方相和体心立方相的有限尺寸部分,使用两种模型计算了作为不同原子密度函数的哈特里 - 福克波函数、能量和电荷分布。第一种激发态模型将激发定域在中心原子上;在第二种模型中,这种激发部分离域在最近的原子邻居上。有限尺寸部分的总能量通过添加原子间色散吸引力和短程原子间关联能的密度泛函描述来推导。第一个允许电子跃迁的实验能量随密度增加,且大于孤立原子中的能量。原子内关联能对这种能量 shift 没有贡献。对于体心固体和液态氦,计算得到的能量 shift 与实验结果吻合良好。2p 轨道因密度增强而越来越压缩,从而产生能量 shift。因此,如果不包括最终 1s2p 态的压缩,非弹性电子散射截面的计算将严重错误。研究了激发的特征,并认为这些激发是弗伦克尔型而非万尼尔型。