Abstract
Background: The reaction plays a major role both in the big bang nucleosynthesis producing the majority of the primordial , and in the chain of solar hydrogen burning, where it is the branching point between the -I and -II,-III chains. As a few-nucleon system, this reaction is often used to validate ab initio theoretical calculations and/or test -matrix theory and code implementations. For the latter, experimental data in an extended energy range is of crucial importance to test the fit and extrapolation capabilities of the different codes.
Purpose: The reaction cross section has been measured by several groups up to the first resonance ( MeV) in the reaction. However, only one data set exists above the proton separation threshold measured in a narrow energy range ( MeV). In this work we extend the available experimental capture cross section database to the energy range of known levels, where only particle scattering experiments are available for testing the models.
Method: The activation method was used for the reaction cross section determination. The experiment was performed using a thin-window gas cell with two high-purity Al foils as entrance and exit windows. The activity of the nuclei implanted in the exit/catcher foil was measured by detecting the yield of the emitted rays using shielded high-purity germanium detectors.
Results: New experimental reaction cross section data were obtained for the first time in the MeV energy region, corresponding to MeV excitation energies of . The new data set with about 0.2 MeV step covers the energy range of known levels and particle separation thresholds. No prominent structures are observer around the levels.
Conclusions: The measured reaction cross section is slowly increasing with increasing energy in the range of MeV from to . Above the threshold, a decrease starts in the cross section trend and reaches a value of about around MeV. The overall structure of the cross section suggest a broad resonance peaking around MeV excitation energy, with a width of 8 MeV.
- Received 28 April 2023
- Accepted 13 July 2023
DOI:https://doi.org/10.1103/PhysRevC.108.025802
©2023 American Physical Society