作者: Ken'ichi Nomoto , Daiichiro Sugimoto , Sadayuki Neo
DOI: 10.1007/BF00648354
关键词: Carbon detonation 、 Deflagration 、 Supernova 、 Astrophysics 、 Stellar evolution 、 Deflagration to detonation transition 、 Mechanics 、 Convective heat transfer 、 Detonation 、 Iron peak 、 Physics
摘要: As an alternative to the carbon detonation, we present a carbondeflagration supernova model by full hydrodynamic computation. A deflagration wave, which propagates through core due convective heat transport, does not grow into detonation. Though it results in complete disruption of star, difficulty overproduction iron peak elements can be avoided if is relatively slow.