English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We study the evolution of rapid neutron-capture process (r-process) isotopesin the Galaxy. We analyze relative contributions from core collapse supernovae(CCSNe), neutron star mergers (NSMs) and collapsars under a range ofastrophysical conditions and nuclear input data. Although the r-process in eachof these sites can lead to similar (or differing) isotopic abundances, oursimulations reveal that the early contribution of r-process material to theGalaxy was dominated by CCSNe and collapsar r-process nucleosynthesis, whilethe NSM contribution is unavoidably delayed even under the assumption of theshortest possible minimum merger time.

Contribution of collapsars, supernovae, and neutron star mergers to the evolution of r-process elements in the Galaxy