Abstract
We report precision mass measurements of neutron-deficient gallium isotopes approaching the proton drip line. The measurements of Ga60-63 performed with the TITAN multiple-reflection time-of-flight mass spectrometer provide a more than threefold improvement over the current literature mass uncertainty of Ga61 and mark the first direct mass measurement of Ga60. The improved precision of the Ga61 mass has important implications for the astrophysical rp process, as it constrains essential reaction Q values near the Zn60 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 Ga60 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 Ga60 further enables us to extend the evaluated T=1 isobaric multiplet mass equation up to A=60.
Original language | English |
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Article number | 065803 |
Journal | Physical Review C |
Volume | 104 |
Issue number | 6 |
DOIs | |
State | Published - Dec 2021 |
Externally published | Yes |
Funding
We would like to thank the TRIUMF Beam Delivery and Resonant Ionization Laser Ion Source groups for their excellent support in the realization of this experiment. This work was supported by the Natural Sciences and Engineering Research Council of Canada (NSERC), the Canada Foundation for Innovation (CFI), the Canada-UK Foundation, the Brazilian Conselho Nacional de Desenvolvimento Cient'fico e Technológico (CNPq) under Grant No. 249121/2013-1, the Helmholtz Association of German Research Centers through the Nuclear Astrophysics Virtual Institute (VH-VI-417), German Research Foundation (DFG) Grant No. SCHE 1969/2-1, the German Federal Ministry for Education and Research (BMBF) Grants No. 05P19RGFN1 and No. 05P21RGFN1, the Hessian Ministry for Science and Art through the LOEWE Center HICforFAIR, the JLU and GSI under the JLU-GSI strategic Helmholtz partnership agreement, the UKRI Science and Technology Facilities Council (STFC) Grant No. ST/P004008/1, the U.S. National Science Foundation under Grants No. PHY-1419765, No. PHY 14-30152 (Joint Institute for Nuclear Astrophysics JINA-CEE), No. PHY-1913554, and No. IN2P3/CNRS (France) via the ENFIA Master Project, the U.S. Department of Energy (DOE) Office of Science under Grant No. DE-SC0017649, and the Deutsche Forschungsgemeinschaft (DFG) under Grant No. FR 601/3-1. TRIUMF receives federal funding via the National Research Council of Canada (NRC).