The $R$-Process Alliance: Actinide Abundances, Variation, and Evolution in Metal-Poor Stars

Abstract

The actinides, including thorium (Th), are the heaviest observable elements synthesized in the universe, holding clues to the extremes of the astrophysical and nuclear conditions of $r$-process sites. We present Th abundances based on high-resolution spectroscopy for 47 metal-poor stars, the largest homogeneously analyzed sample to date. The chemical evolution of Th exhibits a decrease in dispersion in [Th/H] and [Th/Fe] from $\sim$0.6 dex at the lowest metallicities to $\sim$0.2 dex at higher metallicities. We also find that Th and the lanthanides Eu and Dy are co-produced remarkably well, with average [Th/Eu]$\sim 0.0$ across $-3.0\lesssim$ [Fe/H] $\lesssim -1.5$, as well as across stars with $0.0\lesssim$ [Eu/Fe] $\lesssim 2.5$. Even so, the absolute range of $\log \hat{I}\mu$(Th/Eu) is 1.02 dex, with an observed standard deviation of $\pm 0.20$ dex and an intrinsic standard deviation of $\pm 0.11$ dex at the lowest metallicities. We infer that $68\%$ of $r$-process events have $\log \hat{I}\mu$(Th/Eu) yields that only vary within a factor of $\pm 1.3$ or $\pm 30\%$, while $5\%$ of $r$-process events have $\log \hat{I}\mu$(Th/Eu) yields that vary by factors $>3.3$ approaching $\sim$10. This serves as a strong constraint for the nuclear and astrophysical models of $r$-process sites, and suggests that achieving an $r$-process site that is both prompt and produces a robust $\log \hat{I}\mu$(Th/Eu) ratio is a challenge for current models.

Submitted to ApJ