Particle decay of astrophysically-important 19Ne levels
The 15O(α,γ)19Ne reaction is an important trigger reaction leading to the rapid proton (rp) capture process in X-ray bursts. The primary uncertainty in determining its astrophysical rate is the uncertain α branching ratios of levels near Ex = 4.1 MeV in 19Ne. These states have been populated in a study of the 20Ne(p, d)19Ne reaction, and α branching ratios are reported in this manuscript.
Publication Source (Journal or Book title)
Journal of Physics: Conference Series
Bardayan, D., Chipps, K., Ahn, S., Blackmon, J., Greife, U., Jones, K., Kontos, A., Kozub, R., Linhardt, L., Manning, B., Matos, M., O'Malley, P., Ota, S., Pain, S., Peters, W., Pittman, S., Sachs, A., Schmitt, K., Smith, M., & Thompson, P. (2019). Particle decay of astrophysically-important 19Ne levels. Journal of Physics: Conference Series, 1308 (1) https://doi.org/10.1088/1742-6596/1308/1/012004