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Reaction Rate Uncertainties: NeNa and MgAl in AGB Stars

Robert Izzard·Maria Lugaro·Christian Iliadis·Amanda Karakas
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Abstract

We study the effect of uncertainties in the proton-capture reaction rates of the NeNa and MgAl chains on nucleosynthesis due to the operation of hot bottom burning (HBB) in intermediate-mass asymptotic giant branch (AGB) stars. HBB nucleosynthesis is associated with the production of sodium, radioactive Al26 and the heavy magnesium isotopes, and it is possibly responsible for the O, Na, Mg and Al abundance anomalies observed in globular cluster stars. We model HBB with an analytic code based on full stellar evolution models so we can quickly cover a large parameter space. The reaction rates are varied first individually, then all together. This creates a knock-on effect, where an increase of one reaction rate affects production of an isotope further down the reaction chain. We find the yields of Ne22, Na23 and Al26 to be the most susceptible to current nuclear reaction rate uncertainties.

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Robert Izzard, Maria Lugaro, Christian Iliadis, Amanda Karakas. 2006-07-24. Reaction Rate Uncertainties: NeNa and MgAl in AGB Stars. https://arxiv.org/abs/astro-ph/0607536

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