Observational nuclear astrophysics: neutron-capture element abundances in old, metal-poor stars

TL;DR

This paper reviews neutron-capture element abundances in old, metal-poor stars, discussing their nucleosynthesis origins, production sites, and implications for understanding galactic chemical evolution.

Contribution

It synthesizes current knowledge on neutron-capture processes in metal-poor stars and highlights key uncertainties and future observational prospects.

Findings

Neutron-capture elements reveal multiple nucleosynthesis processes.

Abundance patterns help trace early galactic chemical enrichment.

Future large-scale observations will clarify production sites.

Abstract

The chemical abundances of metal-poor stars provide a great deal of information regarding the individual nucleosynthetic processes that created the observed elements and the overall process of chemical enrichment of the galaxy since the formation of the first stars. Here we review the abundance patterns of the neutron-capture elements (Z > 38) in those metal-poor stars and our current understanding of the conditions and sites of their production at early times. We also review the relative contributions of these different processes to the build-up of these elements within the galaxy over time, and outline outstanding questions and uncertainties that complicate the interpretation of the abundance patterns observed in metal-poor stars. It is anticipated that future observations of large samples of metal-poor stars will help discriminate between different proposed neutron-capture element production sites and better trace the chemical evolution of the galaxy.