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Impact of nuclear β-decay rates on the r-process rare-earth peak abundances

Y.-W. Hao1,2, Y.-F. Niu1,2,*, and Z.-M. Niu3

  • 1MOE Frontiers Science Center for Rare Isotopes, Lanzhou University, Lanzhou 730000, People's Republic of China
  • 2School of Nuclear Science and Technology, Lanzhou University, Lanzhou 730000, People's Republic of China
  • 3School of Physics and Optoelectronic Engineering, Anhui University, Hefei 230601, People's Republic of China

  • *niuyf@lzu.edu.cn

Phys. Rev. C 108, L062802 – Published 19 December, 2023

DOI: https://doi.org/10.1103/PhysRevC.108.L062802

Abstract

The impact of β-decay rates of an individual nucleus on the r-process rare-earth peak abundances has been studied in different astrophysical scenarios. The variation in β-decay rates by a factor of 10 can produce large abundance uncertainties in the rare-earth mass region, while fission deposition can significantly reduce this uncertainty, which is not a suggested case by the current simulations of neutron-star mergers with moderately neutron-rich conditions where fission is less active. The most impactful nuclei include even-neutron-number (N) nuclei on the early r-process equilibrium path or r-process freeze-out path and nuclei with N=100, 102, and 104. It is found that the variations in the β-decay rate of nuclei located to the left and right sides of the r-process freeze-out path have significant different effects on rare-earth peak abundance.

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