The Road to Black Hole Formation and Gamma-Ray Bursts - Bringing together Core-Collapse Supernova Theory and Numerical Relativity

黑洞形成和伽马射线爆发之路——核心塌陷超新星理论和数值相对论的结合

• 批准号: 0855535
• 负责人: Christian Ott
• 金额: $ 22.2万
• 依托单位: California Institute of Technology
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2009
• 资助国家: 美国
• 起止时间: 2009-09-15 至 2012-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0855535&HistoricalAwards=false
• 关键词: Road; Black; Hole; Formation; Gamma

Dr. Christian Ott (California Institute of Technology) will combine the modeling techniques of numerical relativity and of core-collapse supernova theory to study black hole formation in the late stages of the collapse of massive star cores. He and his collaborators intend to establish the dependence of black hole formation on progenitor star mass, rotational configuration, nuclear equation of state, and neutrino luminosity/heating. The aims include constraining the progenitor characteristics that may lead to collapsar-type gamma-ray bursts and improving estimates of the stellar-mass black hole formation rate in the universe.The results of the project will improve knowledge of the connection between core collapse supernovae and black hole production, and should result in improved estimates of the stellar-mass black hole formation rate. Furthermore, gravitational wave signals extracted from the simulations and improved rate estimates for compact binary systems will be made available. This project will contribute to the training of a graduate student in numerical general relativity, supernova theory, and computational physics. The results, codes, and microphysics inputs of the project will be made publically available to facilitate future research and training of students. Visualizations and animations resulting from the simulations will be used in ongoing outreach projects of the group.

Christian Ott博士（加州理工学院）将结合数值相对论和核心塌缩超新星理论的建模技术来研究大质量恒星核心塌缩后期黑洞的形成。 他和他的合作者打算确定黑洞形成对祖星质量、旋转构型、核状态方程和中微子光度/加热的依赖性。目标包括限制可能导致塌陷型伽马射线暴的前身特征，并改进对宇宙中恒星质量黑洞形成速率的估计。该项目的结果将提高对核心塌陷超新星与黑洞之间联系的认识。黑洞的产生，应该会改进对恒星质量黑洞形成速率的估计。此外，还将提供从模拟中提取的引力波信号以及改进的紧凑双星系统的速率估计。 该项目将有助于对研究生进行数值广义相对论、超新星理论和计算物理学方面的培训。该项目的结果、代码和微观物理输入将公开，以促进学生未来的研究和培训。 模拟产生的可视化和动画将用于该小组正在进行的外展项目。