Using the recoil mass seperator DRAGON to constrain astrophysical reaction rates

27 Jun 2017, 14:50
20m
Hotel ICC, Daejeon, Korea

Hotel ICC, Daejeon, Korea

4-29 Doryong-dong, Yuseong-gu, Daejeon, Korea; Tel +82 42)866-5000~5003
Oral Presentation Session 3 (Chair: Y. K. Kwon)

Speaker

Charles Akers

Description

The detector of recoils and $\gamma$-rays of nuclear reactions (DRAGON) is used to directly observe radiative capture reactions of astrophysical interest and is located at TRIUMF, Canada. Such measurements are crucial for constraining the uncertainty of nuclear reaction rates, leading to a better understanding of various stellar scenarios. In this talk, DRAGON's measurements of the $^{18}$F($p$,$\gamma$)$^{19}$Ne and $^{76}$Se($\alpha$,$\gamma$)$^{80}$Kr reactions, relevant to satellite observation of novae and the production of heavy proton rich nuclei respectively, are highlighted.

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