21–25 May 2018
US/Eastern timezone

Improving Uncertainties in the $^{17}\mathrm{O}(\alpha,n){}^{20}\mathrm{Ne}$ cross section

23 May 2018, 16:30
1h 30m

Speaker

Kevin Macon (University of Notre Dame)

Description

The $^{17}\mathrm{O}(\alpha,n)$ reaction recycles neutrons for the most efficient neutron absorber ($^{16}\mathrm{O}(n,\gamma)^{17}\mathrm{O}$) during both the core He-burning and shell C-burning phases of the weak s-process. In order to improve uncertainties in the reaction rate, we are performing $(a,n)$ and ($a,n'\gamma$) cross section measurements at the 5U accelerator of the Notre Dame Nuclear Science Laboratory. We will report on a recent measurement that was performed with LaBr$_3$:Ce gamma-ray detectors from the HAGRiD array in combination with a deuterated liquid scintillator neutron detector. The employed digital electronics allow for pulse shape discrimination in both detector types, and spectral unfolding is used to obtain neutron energy information from the observed light output spectrum in the liquid scintillation detector.

Primary authors

Axel Boeltzig (University of Notre Dame) Kevin Macon (University of Notre Dame)

Co-authors

Febbraro Michael (Oak Ridge National Lab) Kate Jones (University of Tennessee Knoxville) Prof. Michael Wiescher (University of Notre Dame) Dr Richard J. deBoer (University of Notre Dame) Dr Shea Mosby (P27 Los Alamos National Lab) Dr Xesús Pereira-Lopez (University of Tennessee Knoxville)

Presentation materials

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