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

Longland, R; Iliadis, C; Karakas, Amanda

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

Date

2012

Authors

Longland, R

Iliadis, C

Karakas, Amanda

Publisher

American Physical Society

Abstract

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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http://hdl.handle.net/1885/68040

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ANU Research Publications

Source

Physical Review C: Nuclear Physics

Type

Journal article

DOI

10.1103/PhysRevC.85.065809

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2037-12-31

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

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