Sensitivity study for the C()O astrophysical reaction rate
R. J. Holt🇺🇸 · B. W. Filippone🇺🇸 · Steven C. Pieper🇺🇸
The C()O reaction has a key role in nuclear astrophysics. A multilevel R-matrix analysis was used to make extrapolations of the astrophysical S factor for this reaction to the stellar energy of 300 keV. The statistical precision of the S-factor extrapolation was determined by performing multiple fits to existing randomized E1 and E2 ground state data, according to experimental errors. The impact of a future proposed experiment at Jefferson Laboratory (JLab) was assessed within this framework. The proposed JLab experiment will make use of a high-intensity low-energy bremsstrahlung beam that impinges on an oxygen-rich single-fluid bubble chamber in order to measure the total cross section for the inverse O()C reaction. The importance of low energy data as well as high precision data was investigated.