Research on Explosion Energy of Type II-Supernova in 11~40MΘ Progenitor Stars Model
作者: 夏雄平 ：桂林理工大学理学院，桂林;
Abstract: In the paper, we apply four various definitions of explosion energy, based on modified the state equation in LLPR model and the II supernova explosion code “WLYW-89”, to research explosion energy of type II-supernova in new progenitor stars model of the main-sequence mass (: the sun mass). Apply the results of the discrete explosion energy in various mass cell and explosive energy with time, and compare with theoretical and observation results, we find that, in four various definitions of explosion energy, the second definition of explosion energy is the most suitable to supernova explosion in new progenitor stars model, especially, for , theoretical results are good agreement with experimental observation data. It is because that, on one the hand, is defined by the view of energy, on the other hand, its shock velocity in agreement with the experimental observation and it can reduce the gap of theoretical and observation results.
文章引用: 夏雄平 (2013) 11~40MΘ前新星模型下的II型超新星爆发能研究。 天文与天体物理， 1， 14-19. doi: 10.12677/AAS.2013.12003
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