...编辑供稿: 蔡峥 ( University of Arizona ) 背景介绍: 我们说星系际介质的随红移的演化,主要指的是电离状态(ionization state),而这个星系际介质的电离状态是由紫外背景(UV background)决定的(波长<91.2nm光子可以电离氢原子)。
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solid state ionization detector 固态电离探测器
valence-state ionization potential 价态电离势
ionization of donor state 施主能态电离
The ionization energy must then be nothing more than, that is the energy to go from the ground state here to n equals infinity, so that would be the energy at state infinity minus the energy of the ground state.
这个电离能一定不会大于,从基态到n为无限大时的能量,而是等于,无限远处的能量减去基态能量。
So, if, for example, we were looking at a hydrogen atom in the case where we have the n equals 1 state, so the electron is in that ground state, the ionization energy, it makes sense, is going to be the difference between the ground state and the energy it takes to be a free electron.
电离氢原子所需要的能量,如果我们看n等于1的情况,电子在基态,那电离能,很合理的就是基态,和自由电子态的能量差。
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