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- W2396005303 abstract "New results on the properties of energy levels in ${}^{17}$O improve our understanding of the slow or $s$ process which produces more than half of the nuclei heavier than Fe in the cosmos. One of the main sources of neutrons for the $s$ process is the ${}^{13}$C + $ensuremath{alpha}{ensuremath{rightarrow}}^{16}$O + $n$ reaction where position and width of energy levels in ${}^{17}$O near the reaction threshold can change the reaction rate. In contrast, depending on the width of other levels in ${}^{17}$O, the ${}^{16}$O$+n{ensuremath{rightarrow}}^{17}$O$+ensuremath{gamma}$ reaction can be a neutron ``poison'' reducing the production of heavy elements. This new work reduces uncertainties for both of these reactions." @default.
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- W2396005303 date "2015-11-17" @default.
- W2396005303 modified "2023-10-14" @default.
- W2396005303 title "Broad levels in<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mmultiscripts><mml:mtext>O</mml:mtext><mml:mprescripts /><mml:none /><mml:mn>17</mml:mn></mml:mmultiscripts></mml:math>and their relevance for the astrophysical<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML><mml:mi>s</mml:mi></mml:math>process" @default.
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- W2396005303 doi "https://doi.org/10.1103/physrevc.92.052802" @default.
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