Analytical Model of Time-Dependent Ionization in the Envelopes of Type II Supernovae at the Photospheric Phase

被引:0
|
作者
Potashov, M. Sh. [1 ,2 ]
Blinnikov, S. I. [1 ,3 ,4 ]
机构
[1] NRC Kurchatov Inst ITEP, Ul Bolshaya Cheremushkinskaya 25, Moscow 117218, Russia
[2] Novosibirsk State Univ, Ul Pirogova 2, Novosibirsk 630090, Russia
[3] Russian Acad Sci, Space Res Inst, Profsoyuznaya Ul 84-32, Moscow 117997, Russia
[4] Univ Tokyo, Inst Phys & Math Universe, Kashiwa, Chiba, Japan
关键词
supernovae; atmospheres; spectral line formation; LINE FORMATION; RECOMBINATION; DISTANCES;
D O I
10.1134/S1063773719050062
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate a simplified kinetic system of the hydrogen atom (two levels plus continuum) under conditions of a type IIP supernova at the plateau phase that realistically describes the basic properties of the complete system. We have found the Lyapunov function for the reduced system using which we have analytically obtained the ionization freeze-out effect on long time scales. Since the system completely recombines in the equilibrium approximation on long time scales, which does not occur in reality, this result confirms the necessity of allowance for the time-dependent effect in the kinetics during the photospheric phase in a supernova explosion.
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页码:276 / 281
页数:6
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