Mass measurements of neutron-rich gallium isotopes refine production of nuclei of the first r -process abundance peak in neutron-star merger calculations

M. P. Reiter, S. Ayet San Andrés, S. Nikas, J. Lippuner, C. Andreoiu, C. Babcock, B. R. Barquest, J. Bollig, T. Brunner, T. Dickel, J. Dilling, I. Dillmann, E. Dunling, G. Gwinner, L. Graham, C. Hornung, R. Klawitter, B. Kootte, A. A. Kwiatkowski, Y. LanD. Lascar, K. G. Leach, E. Leistenschneider, G. Martínez-Pinedo, J. E. McKay, S. F. Paul, W. R. Plaß, L. Roberts, H. Schatz, C. Scheidenberger, A. Sieverding, R. Steinbrügge, R. Thompson, M. E. Wieser, C. Will, D. Welch

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15 Scopus citations

Abstract

We report mass measurements of neutron-rich Ga isotopes Ga80-85 with TRIUMF's Ion Trap for Atomic and Nuclear science. The measurements determine the masses of Ga80-83 in good agreement with previous measurements. The masses of Ga84 and Ga85 were measured for the first time. Uncertainties between 25 and 48 keV were reached. The new mass values reduce the nuclear uncertainties associated with the production of A≈84 isotopes by the r-process for astrophysical conditions that might be consistent with a binary neutron star (BNS) merger producing a blue kilonova. Our nucleosynthesis simulations confirm that BNS merger may contribute to the first abundance peak under moderate neutron-rich conditions with electron fractions Ye=0.35-0.38.

Original languageEnglish
Article number025803
JournalPhysical Review C
Volume101
Issue number2
DOIs
StatePublished - Feb 2020
Externally publishedYes

Funding

The authors thank the TRILIS group at TRIUMF for Ga beam development and beautiful operation of the IG-LIS ion source and J. Bergmann for the Massdata-Acquisition software package used for the MR-TOF-MS, and discussions with F.-K. Thielemann are also acknowledged. This work was partially supported by Canadian agencies NSERC and CFI, U.S.A. NSF (Grants No. PHY-1419765 and No. PHY-1614130) and DOE (Grant No. DE-SC0017649), Brazil's CNPq (Grant No. 249121/2013-1), United Kingdom's STFC (Grants No. ST/L005816/1 and No. ST/L005743/1), the Canada-UK Foundation, German institutions DFG (Grants No. FR 601/3-1 and No. SFB 1245 and through PRISMA Cluster of Excellence), BMBF (Grants No. 05P15RGFN1 and No. 05P12RGFN8), the Helmholtz Association through NAVI (Grant No. VH-VI-417), HMWK through the LOEWE Center HICforFAIR, by the JLU and GSI under the JLU-GSI strategic Helmholtz partnership agreement, the ChETEC COST Action (CA16117) supported by COST (European Cooperation in Science and Technology), and the Los Alamos National Laboratory and has been assigned report number LA-UR-18-28439. Los Alamos National Laboratory is operated by Los Alamos National Security, LLC, for the National Nuclear Security Administration of US Department of Energy (Contract No. DEAC52-06NA25396). TRIUMF receives federal funding via NRC-CNRC.

FundersFunder number
Canadian agencies NSERC
HMWK
National Science Foundation1419765, PHY-1419765, PHY-1614130
National Science Foundation
U.S. Department of EnergyDE-SC0017649
U.S. Department of Energy
Los Alamos National LaboratoryLA-UR-18-28439
Los Alamos National Laboratory
Justus Liebig Universität Gießen
Science and Technology Facilities CouncilST/L005743/1, ST/L005816/1
Science and Technology Facilities Council
European Cooperation in Science and Technology
Deutsche ForschungsgemeinschaftFR 601/3-1, SFB 1245
Deutsche Forschungsgemeinschaft
Canada Foundation for Innovation
Bundesministerium für Bildung und Forschung05P15RGFN1, 05P12RGFN8
Bundesministerium für Bildung und Forschung
Conselho Nacional de Desenvolvimento Científico e Tecnológico249121/2013-1
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Helmholtz AssociationVH-VI-417
Helmholtz Association
GSI Helmholtzzentrum für Schwerionenforschung GmbHCA16117
GSI Helmholtzzentrum für Schwerionenforschung GmbH
Foundation for Canadian Studies in the United Kingdom

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