Reaction rates for the s-process neutron source 22 Ne + α
The 22Ne(α,n)25Mg reaction is an important source of neutrons for the s-process. In massive stars responsible for the weak component of the s-process, 22Ne(α,n)25Mg is the dominant source of neutrons, both during core helium burning and in carbon-shell
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|Source:||Physical Review C: Nuclear Physics|
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