Investigating the computational and statistical aspects of star and planet formation

研究恒星和行星形成的计算和统计方面

• 批准号: 2263733
• 金额: --
• 依托单位: University of Sheffield
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2019
• 资助国家: 英国
• 起止时间: 2019 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2263733
• 关键词: Investigating; computational; statistical; aspects; star

Young stars are often found in high-density environments, this means that encounters between young stars can be common and this will change their binary properties and affect planet-forming discs. A PhD would involve investigating various computational and statistical aspects of young stars and their environments. These include dynamical and hydrodynamical simulations of stellar dynamics, statistical measures of complex distributions, examining and interpreting both observational, simulated and 'fake' data.

年轻恒星通常在高密度环境中被发现，这意味着年轻恒星之间的相遇可能是常见的，这将改变它们的双星属性，并影响行星形成盘。博士学位将涉及研究年轻恒星及其环境的各种计算和统计方面的问题。这些包括恒星动力学的动力学和流体力学模拟，复杂分布的统计测量，检查和解释观测数据、模拟数据和“假”数据。