Massive Stellar Evolution, Supernovae, and Nucleosynthesis

大规模恒星演化、超新星和核合成

• 批准号: 9417161
• 负责人: Stanford Woosley
• 金额: $ 22.5万
• 依托单位: University of California-Santa Cruz
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 1995
• 资助国家: 美国
• 起止时间: 1995-09-15 至 1999-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9417161&HistoricalAwards=false
• 关键词: Massive; Stellar; Evolution; Supernovae; Nucleosynthesis

Woosley, Stanford 9417161 Woosley and his group will continue theoretical studies of stellar evolution, supernovae and nucleosynthesis. They plan to improve the physics in their computer models for stars more massive than eight solar-masses, to continue their efforts to find the prototypical theoretical counterparts for supernovae of various types (SN 1993J,for example), to build more realistic multidimensional computer models of the supernova explosion itself for massive stars and white dwarfs, and to explore the entire range of isotopic nucleosynthesis created in these events. ***

伍斯利，斯坦福大学9417161伍斯利和他的小组将继续恒星演化，超新星和核合成的理论研究。 他们计划改进质量超过8个太阳质量的恒星的计算机模型中的物理学，继续努力寻找各种类型超新星的原型理论对应物（例如SN 1993 J），为大质量恒星和白色矮星建立更真实的超新星爆炸本身的多维计算机模型，并探索这些事件中产生的同位素核合成的整个范围。 ***