Abstract
Since the identification of ongoing production in the universe, the reaction sequence ()()() has been studied intensively. At temperatures where the radiative capture on ( s) becomes faster than the decay, the production of can be reduced due to the depletion of . To determine the resonances relevant for the () bypass reaction, we measured the reaction with high-energy precision using the Grand Raiden spectrometer at the Research Center for Nuclear Physics, Osaka. Several new energy levels were found above the threshold and for known states excitation energies were determined with smaller uncertainties. The calculated stellar rates of the bypass reaction agree well with previous results, suggesting that these rates are well established.
2 More- Received 15 June 2010
DOI:https://doi.org/10.1103/PhysRevC.82.025807
©2010 American Physical Society