Ken’ichi Nomoto

most citedThe Impact of

^{12}

α, γ

)

^{16}

O Reaction on the Presupernova Evolution and Supernova Explodability of Massive Stars

4 citations · 5 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2026

Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae

Wenyu Xin, Ken'ichi Nomoto, Chun-Ming Yip +4

Recently discovered very metal-poor (VMP) star LAMOST J1010+2358 shows a peculiar abundance pattern that is remarkably well fit by a Pop III pair-instability supernova (PISN) of $\…

astro-ph.SR2025

Impacts of the $^{16}$ O( $^{16}$ O, n) $^{31}$ S reaction rate on the evolution and nucleosynthesis in Pop III massive stars

Wenyu Xin, Ken'ichi Nomoto, Xianfei Zhang +1

We first present a systematic investigation into the effect of the $^{16}$ O( $^{16}$ O, n) $^{31}$ S reaction rate on the evolution and nucleosynthesis of Population III (Pop III) star…

astro-ph.SR2025★ 1 cited

The impact of new ( $α$ , n) reaction rates on the weak s-process in metal-poor massive stars

Wenyu Xin, Chun-Ming Yip, Ken'ichi Nomoto +2

Massive stars are significant sites for the weak s-process (ws-process). $^{22}$ Ne and $^{16}$ O are, respectively, the main neutron source and poison for the ws-process. In the met…

astro-ph.SR2025★ 4 cited

The Impact of $^{12}$ C( $α, γ$ ) $^{16}$ O Reaction on the Presupernova Evolution and Supernova Explodability of Massive Stars

Wenyu Xin, Ken'ichi Nomoto, Gang Zhao

Among the uncertainties of stellar evolution theory, we investigate how the $^{12}$ C( $α, γ$ ) $^{16}$ O reaction rate affects the evolution of massive stars for the initial masses of…

Nucleosynthesis of Pop III and Fe-enriched Pop II Pair-Instability Supernovae

Impacts of the 16O(16O, n)31S reaction rate on the evolution and nucleosynthesis in Pop III massive stars

The impact of new (α, n) reaction rates on the weak s-process in metal-poor massive stars

The Impact of 12C(α,γ)16O Reaction on the Presupernova Evolution and Supernova Explodability of Massive Stars

Impacts of the $^{16}$ O( $^{16}$ O, n) $^{31}$ S reaction rate on the evolution and nucleosynthesis in Pop III massive stars

The impact of new ( $α$ , n) reaction rates on the weak s-process in metal-poor massive stars

The Impact of $^{12}$ C( $α, γ$ ) $^{16}$ O Reaction on the Presupernova Evolution and Supernova Explodability of Massive Stars