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奇异夸克相变对II型超新星激波能量的影响
谢佐恒1; 王惟中2; 王贻仁1; 张锁春1
2000
Source Publication天体物理学报
ISSN0253-2379
Volume020Issue:003Pages:233
Abstract在模拟超新星演化时,考虑非奇异-奇异夸克相变因素,与没有考虑奇异相变的情况相比,得到了更强的激波,这可能是奇异相变增加了星核区对流不稳定性所致,在本文的计算环境里,一阶奇异夸克相变的结果使具有1.28M铁星核的WW(88)模型爆发,打破了瞬发机制只能使约1.1M铁星核模型爆发的上限,并支持了戴子高等人所作出的奇异夸克相变能超新爆发机会的论断。
Language英语
Document Type期刊论文
Identifierhttp://ir.amss.ac.cn/handle/2S8OKBNM/37265
Collection中国科学院数学与系统科学研究院
Affiliation1.中国科学院数学与系统科学研究院
2.北京大学
Recommended Citation
GB/T 7714
谢佐恒,王惟中,王贻仁,等. 奇异夸克相变对II型超新星激波能量的影响[J]. 天体物理学报,2000,020(003):233.
APA 谢佐恒,王惟中,王贻仁,&张锁春.(2000).奇异夸克相变对II型超新星激波能量的影响.天体物理学报,020(003),233.
MLA 谢佐恒,et al."奇异夸克相变对II型超新星激波能量的影响".天体物理学报 020.003(2000):233.
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