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      Re-examining the \({}^{26}\mathrm{Mg}(\alpha ,{\alpha }^{\prime }){}^{26}\mathrm{Mg}\) reaction: Probing astrophysically important states in \({}^{26}\mathrm{Mg}\)

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          \({}_{}{}^{22}{}_{}{}^{}Ne(\alpha ,\mathit{n}){}_{}{}^{25}{}_{}{}^{}Mg\): The Key Neutron Source in Massive Stars

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            S-process nucleosynthesis in massive stars and the weak component. II - Carbon burning and galactic enrichment

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              S-process nucleosynthesis in massive stars and the weak component. I - Evolution and neutron captures in a 25 solar mass star

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                Author and article information

                Journal
                PRVCAN
                Physical Review C
                Phys. Rev. C
                American Physical Society (APS)
                2469-9985
                2469-9993
                November 2017
                November 8 2017
                : 96
                : 5
                Article
                10.1103/PhysRevC.96.055802
                b4c57c85-f8e5-4d36-80e7-b139aa42e236
                © 2017

                https://link.aps.org/licenses/aps-default-license

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