Kavli Affiliate: Anna Frebel | Summary:The astrophysical origin of the rapid neutron-capture process (r-process), which produces about half of the elements heavier than iron, remains uncertain. The oldest, most metal-poor stars preserve the chemical signatures of early nucleosynthesis events and can reveal the nature of the r-process sites. We present a homogeneous chemical abundance analysis […]
Continue.. The R-Process Alliance: Exploring the cosmic scatter among ten r-process sites with stellar abundances