The O(,)Ne Breakout Reaction and Impact on X-Ray Bursts
arXiv:0706.2349 · doi:10.1103/PhysRevLett.98.242503
Abstract
The breakout reaction O()Ne, which regulates the flow between the hot CNO cycle and the rp-process, is critical for the explanation of the burst amplitude and periodicity of X-ray bursters. We report on the first successful measurement of the critical -decay branching ratios of relevant states in Ne populated via F(He,t)Ne. Based on the experimental results and our previous lifetime measurements of these states, we derive the first experimental rate of O()Ne. The impact of our experimental results on the burst pattern and periodicity for a range of accretion rates is analyzed.
arXiv comment4 pages with 5 figures
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- Hydrodynamic Models of Type I X-Ray Bursts: Metallicity Effects
- Nuclear Physics of the Outer Layers of Accreting Neutron Stars
- New measurement of C+C fusion reaction at astrophysical energies
- The Impact of Uncertainties in Reaction Q-values on Nucleosynthesis in Type I X-Ray Bursts
- Consistent Modeling of GS 1826-24 X-ray Bursts for Multiple Accretion Rates Demonstrates the Possibility to Constrain rp-process Reaction Rates
- Reaction Rate and Composition Dependence of the Stability of Thermonuclear Burning on Accreting Neutron Stars
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- Lifetimes of states in 19Ne above the 15 O + alpha breakup threshold
- On the dependence of X-ray burst rate on accretion and spin rate
- Spectroscopy of Ne for the thermonuclear O()Ne and F()O reaction rates
- Doppler Broadening in Mg()Ne Decay
- New -ray Transitions Observed in Ne with Implications for the O(,)Ne Reaction Rate