Measurement of the Am 240 ( n , f ) cross section using the surrogate-ratio method
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The 17 F(d,n) 18 Ne reaction is part of the astrophysical “hot CNO” cycles that are important in astrophysical environments like novae. Here, its thermal reaction rate is small owing to the relatively high energy of the resonances and therefore is dominated by direct, non-resonant capture in stellar environments at temperatures below 0.4 GK.
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