Reaction Rates Of Ge-64(P,Gamma)As-65 And As-65(P,Gamma)Se-66 And The Extent Of Nucleosynthesis In Type I X-Ray Bursts

The extent of nucleosynthesis in models of type I X-ray bursts (XRBs) and the associated impact on the energy released in these explosive events are sensitive to nuclear masses and reaction rates around the Ge-64 waiting point. Using the well known mass of Ge-64, the recently measured As-65 mass, and large-scale shell model calculations, we have determined new thermonuclear rates of the Ge-64(p,gamma)As-65 and As-65(p,gamma)Se-66 reactions with reliable uncertainties. The new reaction rates differ significantly from previously published rates. Using the new data, we analyze the impact of the new rates and the remaining nuclear physics uncertainties on the Ge-64 waiting point in a number of representative one-zone XRB models. We find that in contrast to previous work, when all relevant uncertainties are considered, a strong Ge-64 rp-process waiting point cannot be ruled out. The nuclear physics uncertainties strongly affect XRB model predictions of the synthesis of Zn-64, the synthesis of nuclei beyond A = 64, the energy generation, and the burst light curve. We also identify key nuclear uncertainties that need to be addressed to determine the role of the Ge-64 waiting point in XRBs. These include the remaining uncertainty in the As-65 mass, the uncertainty of the Se-66 mass, and the remaining uncertainty in the As-65(p,gamma)Se-66 reaction rate, which mainly originates from uncertain resonance energies.