Early Nucleosynthesis and the firt Stars in the Universe

Focusing on the formation of the first stars, this book explores the significance of mass in nucleosynthesis and its implications for stellar evolution. It highlights the role of numerical simulations in revealing the ejecta characteristics of massive and supermassive stars. By comparing these simulations with high-resolution observations of the early Universe's intergalactic medium, the work draws conclusions about the properties and abundances of the earliest stars, providing insights into cosmic history.