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Reaction rates for the s-process neutron source 22 Ne + α

Longland, R; Iliadis, C; Karakas, Amanda


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

CollectionsANU Research Publications
Date published: 2012
Type: Journal article
Source: Physical Review C: Nuclear Physics
DOI: 10.1103/PhysRevC.85.065809


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