Stellar Burning and First Star Nucleosynthesis
Our key research goal is to coordinate within the nuclear astrophysics community an extensive effort, aiming to discuss the production, evolution, and observation of elements, as known in 2016. This will be a multi-disciplinary discussion towards the question: What do we know 60 years after B2FH? In addition, we aim to trigger and boost research within this WG and in collaboration and communication with other JINA-CEE WGs addressing a number of questions and puzzles that require an interdisciplinary effort for their solution. The results of such research initiatives will be published in peer-reviewed journals.