The Astrophysics of Hydrogen and Helium Reionization

氢和氦再电离的天体物理学

• 批准号: 0907969
• 负责人: Matias Zaldarriaga
• 金额: $ 79.61万
• 依托单位: Institute For Advanced Study
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2009
• 资助国家: 美国
• 起止时间: 2009-09-15 至 2014-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0907969&HistoricalAwards=false
• 关键词: Astrophysics; Hydrogen; Helium; Reionization

This research program will examine the reionization of the Universe in both hydrogen and helium, combining analytical and numerical approaches to elucidate the physics underlying reionization and how it is influenced by the nature and abundance of the ionizing sources and the properties of the intergalactic medium (IGM). The analysis will be further employed to consider the impact of reionization on observable signatures of this process, including fluctuations in 21 cm radiation from hydrogen at high redshifts, surveys of Ly-alpha emitting galaxies, spectra of gamma-ray bursts, and the statistical properties of the Lyman-alpha forest. The results of this investigation will be used to guide optimal observing strategies for ongoing and future experiments to investigate emission from high-redshift galaxies, quasars, and diffuse gas in the IGM.The broader impacts of this work include training of underrepresented students, and public outreach through visualizations and simulations accessible through the web.

该研究计划将研究宇宙在氢和氦中的再电离，结合分析和数值方法来阐明再电离的物理原理，以及电离源的性质和丰度以及星系际介质（IGM）的性质如何影响它。 ）。 该分析将进一步用于考虑再电离对该过程可观测特征的影响，包括高红移氢的 21 厘米辐射波动、Ly-alpha 发射星系的调查、伽马射线爆发的光谱以及统计特性莱曼阿尔法森林。这项调查的结果将用于指导正在进行和未来实验的最佳观测策略，以研究 IGM 中高红移星系、类星体和扩散气体的发射。这项工作的更广泛影响包括对代表性不足的学生和公众的培训通过网络可访问的可视化和模拟进行推广。