<i>s</i>-process production in rotating massive stars at solar and low metallicities
<i>s</i>-process production in rotating massive stars at solar and low metallicities
Rotation was shown to have a strong impact on the structure and light element nucleosynthesis in massive stars. In particular, models including rotation can reproduce the primary nitrogen observed in halo extremely metal-poor (EMP) stars. Additional exploratory models showed that rotation may enhance $s$-process production at low metallicity. Here we …