Abstract
The F-18(p, alpha)O-15 reaction rate is crucial for understanding the final abundance of F-18 predicted by nova models. The gamma-ray emission in the first few hours after a nova outburst is expected to be dominated by 511 keV annihilation photons from the decay of F-18, and so understanding its production can provide important constraints on the conditions during the outburst when compared with observations. Results are presented from the lowest-energy direct measurement to date, performed at the Isotope Separator and Accelerator radioactive beam facility at the TRIUMF laboratory, Canada. Cross section measurements at center-of-mass energies of 250, 330, 453, and 673 keV are obtained and the results compared to previous data and R-matrix calculations. The implications for the overall reaction rate in the context of nova explosions have been discussed.
Original language | English |
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Article number | 042801 |
Pages (from-to) | 1-4 |
Number of pages | 4 |
Journal | Physical Review C |
Volume | 83 |
Issue number | 4 |
DOIs | |
Publication status | Published - 12 Apr 2011 |
Keywords
- ENERGIES