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Mass measurements of ⁶⁰⁻⁶³Ga reduce x-ray burst model uncertainties and extend the evaluated T=1 isobaric multiplet mass equation

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arxiv 2111.12788 v2 pith:HUYLWVGL submitted 2021-11-24 nucl-ex astro-ph.HE

Mass measurements of ⁶⁰⁻⁶³Ga reduce x-ray burst model uncertainties and extend the evaluated T=1 isobaric multiplet mass equation

classification nucl-ex astro-ph.HE
keywords massmeasurementsburstdripequationevaluatedextendimproved
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We report precision mass measurements of neutron-deficient gallium isotopes approaching the proton drip line. The measurements of $^{60-63}$Ga performed with the TITAN multiple-reflection time-of-flight mass spectrometer provide a more than threefold improvement over the current literature mass uncertainty of $^{61}$Ga and mark the first direct mass measurement of $^{60}$Ga. The improved precision of the $^{61}$Ga mass has important implications for the astrophysical rp process, as it constrains essential reaction Q-values near the $^{60}$Zn waiting point. Based on calculations with a one-zone model, we demonstrate the impact of the improved mass data on prediction uncertainties of X-ray burst models. The first-time measurement of the $^{60}$Ga ground-state mass establishes the proton-bound nature of this nuclide; thus, constraining the location of the proton drip line along this isotopic chain. Including the measured mass of $^{60}$Ga further enables us to extend the evaluated $T=1$ isobaric multiplet mass equation up to $A=60$.

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