Atomic and Molecular Structure

P. Peebles
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Abstract

This chapter assesses some applications drawn from atomic and molecular structure. It deals with the structures of the lighter atoms and the simplest molecule, molecular hydrogen. The main approximation method used here is the energy variational principle, which is a powerful technique for computing the low-lying energies of a system such as an atom or molecule. The chapter then introduces the Pauli exclusion principle, which governs the symmetry of the state vector for a system of identical particles such as electrons. Two general features of the exclusion principle are worth noting. First, although the spins make only a very weak contribution to the Hamiltonians for helium, the lowest energy state with spin one is above the spin zero ground state, which is a considerable difference. Second, an electron arriving as a cosmic ray particle from a distant galaxy has to have a wave function antisymmetric with respect to the local electrons, even though the new electron has been away from us for a long time.
原子与分子结构
本章评估了原子和分子结构的一些应用。它研究的是较轻的原子和最简单的分子氢分子的结构。这里使用的主要近似方法是能量变分原理,这是一种强大的技术,用于计算原子或分子等系统的低洼能量。本章随后介绍了泡利不相容原理,该原理支配着由相同粒子(如电子)组成的系统的状态向量的对称性。不相容原则的两个一般特征值得注意。首先,尽管自旋对氦的哈密顿量的贡献很小,但自旋为1的最低能态高于自旋为0的基态,这是一个相当大的区别。其次,作为宇宙射线粒子从遥远星系到达的电子必须具有相对于本地电子的反对称波函数,即使新电子已经离开我们很长时间了。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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