First Results from the CARIBU Facility: Mass Measurements on the r-Process Path
arXiv:1307.0429 · doi:10.1103/PhysRevLett.111.061102
Abstract
The Canadian Penning Trap mass spectrometer has made mass measurements of 33 neutron-rich nuclides provided by the new Californium Rare Isotope Breeder Upgrade (CARIBU) facility at Argonne National Laboratory. The studied region includes the 132Sn double shell closure and ranges in Z from In to Cs, with Sn isotopes measured out to A = 135, and the typical measurement precision is at the 100 ppb level or better. The region encompasses a possible major waiting point of the astrophysical r process, and the impact of the masses on the r process is shown through a series of simulations. These first-ever simulations with direct mass information on this waiting point show significant increases in waiting time at Sn and Sb in comparison with commonly used mass models, demonstrating the inadequacy of existing models for accurate r-process calculations.
5 pages, 3 figures, accepted to Physical Review Letters
References in corpus (5)
- The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
- Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII: Stiffness and stability of neutron-star matter
- Precision Mass Measurements beyond Sn: Anomalous behaviour of odd-even staggering of binding energies
- Mass measurements near the -process path using the Canadian Penning Trap mass spectrometer
- Atomic mass measurements of short-lived nuclides around the doubly-magic 208Pb
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