Hiroki Kawashimo

most citedImpacts of the

^{12} C (α, γ)^{16} O

reaction rate on

^{56} Ni

nucleosynthesis in pair-instability supernovae

4 citations · 4 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.SR2026

Temperature-resolved sensitivities of $^{56} Ni$ production to helium-burning reactions in pair-instability supernovae

Hiroki Kawashimo, Nobuya Nishimura, Yudai Suwa

We propose a temperature-resolved Monte Carlo (MC) approach to identify the temperature regimes in which low-energy helium-burning reaction rates most strongly affect nucleosynthes…

astro-ph.SR2023★ 4 cited

Impacts of the $^{12} C (α, γ)^{16} O$ reaction rate on $^{56} Ni$ nucleosynthesis in pair-instability supernovae

Hiroki Kawashimo, Ryo Sawada, Yudai Suwa +3

Nuclear reactions are key to our understanding of stellar evolution, particularly the $^{12} C (α, γ)^{16} O$ rate, which is known to significantly influence the…

Temperature-resolved sensitivities of 56Ni production to helium-burning reactions in pair-instability supernovae

Impacts of the 12C(α,γ)16O reaction rate on 56Ni nucleosynthesis in pair-instability supernovae

Temperature-resolved sensitivities of $^{56} Ni$ production to helium-burning reactions in pair-instability supernovae

Impacts of the $^{12} C (α, γ)^{16} O$ reaction rate on $^{56} Ni$ nucleosynthesis in pair-instability supernovae