English

Beta-decay spectroscopy of $^{27}$S

Nuclear Experiment 2019-06-19 v2

Abstract

Background: Beta-decay spectroscopy provides valuable nuclear physics input for thermonuclear reaction rates of astrophysical interest and stringent test for shell-model theories far from the stability line. Purpose: The available decay properties of proton drip-line nucleus 27^{27}S is insufficient to constrain the properties of the key resonance in 26^{26}Si(p,γ)27(p,\gamma)^{27}P reaction rate and probe the possible isospin asymmetry. The decay scheme of 27^{27}S is complicated and far from being understood, which has motivated but also presented challenges for our experiment. Method: The 27^{27}S ions were implanted into a double-sided silicon strip detector array surrounded by the high-purity germanium detectors, where the β\beta-delayed protons and γ\gamma rays were measured simultaneously. Results: The improved spectroscopic properties including the precise half-life of 27^{27}S, the excitation energies, β\beta-decay branching ratios, log~ftft values, and BB(GT) values for the states of 27^{27}P populated in the β\beta decay of 27^{27}S were measured and compared to the 27^{27}Mg mirror states and the shell-model calculations. The present work has expanded greatly on the previously established decay scheme of 27^{27}S. Conclusions: The precise proton-separation energy of 27^{27}P, the energy and the ratio between γ\gamma and proton partial widths of the 3/2+3/2^+ resonance were obtained, thereby determining the 26^{26}Si(p,γ)27(p,\gamma)^{27}P reaction rate based mainly on experimental constraints. The first evidence for the observation of a large isospin asymmetry for the mirror decays of 27^{27}S and 27^{27}Na is also provided. The experimental spectroscopic information can be reproduced by the shell-model calculation taking the weakly bound effect of the proton 1s1/21s_{1/2} orbit into account.

Keywords

Cite

@article{arxiv.1809.02987,
  title  = {Beta-decay spectroscopy of $^{27}$S},
  author = {L. J. Sun and X. X. Xu and S. Q. Hou and C. J. Lin and J. José and J. Lee and J. J. He and Z. H. Li and J. S. Wang and C. X. Yuan and D. X. Wang and H. Y. Wu and P. F. Liang and Y. Y. Yang and Y. H. Lam and P. Ma and F. F. Duan and Z. H. Gao and Q. Hu and Z. Bai and J. B. Ma and J. G. Wang and F. P. Zhong and C. G. Wu and D. W. Luo and Y. Jiang and Y. Liu and D. S. Hou and R. Li and N. R. Ma and W. H. Ma and G. Z. Shi and G. M. Yu and D. Patel and S. Y. Jin and Y. F. Wang and Y. C. Yu and Q. W. Zhou and P. Wang and L. Y. Hu and X. Wang and H. L. Zang and P. J. Li and Q. Q. Zhao and L. Yang and P. W. Wen and F. Yang and H. M. Jia and G. L. Zhang and M. Pan and X. Y. Wang and H. H. Sun and Z. G. Hu and R. F. Chen and M. L. Liu and W. Q. Yang and Y. M. Zhao and H. Q. Zhang},
  journal= {arXiv preprint arXiv:1809.02987},
  year   = {2019}
}