Late Phases of the Evolution of Massive Stars

大质量恒星演化的后期

• 批准号: 1954831
• 金额: --
• 依托单位: Keele University
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2017
• 资助国家: 英国
• 起止时间: 2017 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-1954831
• 关键词: Late; Phases; Evolution; Massive; Stars

Massive Stars play a key role in the Universe through the light they shine, the chemical elements they produce and their explosive deaths (supernovae, gamma-ray bursts). They leave behind neutron stars or black holes, the merger of which has recently been observed by LIGO and VIRGO. This opened a new window on the universe via gravitational waves. In order to predict the fate of massive stars, improvements in their modelling is needed, in particular the treatment of convection and nuclear burning during the late phases. This will be the focus of this PhD.

大质量恒星通过它们发出的光线、它们产生的化学元素以及它们的爆炸性死亡(超新星、伽马射线爆发)在宇宙中发挥着关键作用。它们留下了中子星或黑洞，LIGO和处女座最近观察到了它们的合并。这打开了一扇通过引力波观察宇宙的新窗口。为了预测大质量恒星的命运，需要改进它们的模拟，特别是在后期阶段对流和核燃烧的处理。这将是本博士论文的重点。

项目成果

Developing Capacity in Dissemination and Implementation Research in the Eastern Mediterranean Region: Evaluation of a Training Workshop.

发展东地中海地区传播和实施研究的能力：培训研讨会的评估。

• DOI: 10.1007/978-3-030-13876-9_67
• 发表时间: 2022
• 期刊: Global implementation research and applications
• 作者: Salloum RG

3D Simulations and MLT: II. Onsager's Ideal Turbulence

3D 模拟和 MLT：II。

• DOI: 10.48550/arxiv.1810.04659
• 发表时间: 2018
• 期刊: arXiv e-prints
• 作者: Arnett W. David

Nuclei in the Cosmos XV

宇宙中的原子核 XV

• DOI: 10.1007/978-3-030-13876-9_71
• 发表时间: 2019
• 作者: Kaiser E

The Formation of a 70 Msun Black Hole at High Metallicity

高金属丰度 70 Msun 黑洞的形成

• 发表时间: 2019
• 期刊: arXiv e-prints
• 作者: Belczynski K.