A simple model of time-dependent ionization in Type IIP supernova envelopes

被引:1
|
作者
Potashov, M. [1 ,2 ]
Yudin, A. [1 ,3 ]
机构
[1] NRC Kurchatov Inst, ITEP, Ul Bolshaya Cheremushkinskaya 25, Moscow 117218, Russia
[2] Novosibirsk State Univ, Pirogova 1, Novosibirsk 630090, Russia
[3] NRC Kurchatov Inst, Akad Kurchatova Pl 1, Moscow 123182, Russia
基金
俄罗斯科学基金会; 俄罗斯基础研究基金会;
关键词
atomic processes; methods: analytical; stars: atmospheres; supernovae: general; RECOMBINATION-LINE-INTENSITIES; HYDROGENIC IONS; SOBOLEV APPROXIMATION; EIGENSOLVER; DISTANCES; FEAST;
D O I
10.1093/mnras/stz3152
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose a model kinetic system of the hydrogen atom (two levels plus continuum) under the conditions typical for atmospheres of Type IIP supernovae in the plateau stage. Despite the simplicity of this system, it describes realistically the basic properties of the complete system. Analysis shows that the ionization `freeze-out' effect is always manifest at large times. We give a simple criterion for checking the statistical equilibrium of a system under the given conditions at any time. It is shown that if the system is in non-equilibrium at early times, the time-dependent effect of ionization necessarily exists. We also generalize this criterion to the case of arbitrary multilevel systems. We discuss various factors that affect the strength of the time-dependent effect in the kinetics during the photospheric phase of a supernova explosion.
引用
收藏
页码:2674 / 2687
页数:14
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