Abstract
Classical novae are important contributors to the abundances of key isotopes, such as the radioactive , whose observation by satellite missions could provide constraints on nucleosynthesis models in novae. The reaction plays a critical role in the synthesis of both oxygen and fluorine isotopes, but its reaction rate is not well determined because of the lack of experimental data at energies relevant to novae explosions. In this study, the reaction cross section has been measured directly for the first time in a wide energy range appropriate to hydrogen burning in classical novae. In addition, the resonance strength, , has been measured with the highest precision to date. The uncertainty on the reaction rate has been reduced by a factor of 4, thus leading to firmer constraints on accurate models of novae nucleosynthesis.
- Received 14 September 2012
DOI:https://doi.org/10.1103/PhysRevLett.109.202501
© 2012 American Physical Society