| Issue |
EPJ Web Conf.
Volume 239, 2020
ND 2019: International Conference on Nuclear Data for Science and Technology
|
|
|---|---|---|
| Article Number | 02003 | |
| Number of page(s) | 4 | |
| Section | Nuclear Masses, Structure and Decay Data Measurements | |
| DOI | https://doi.org/10.1051/epjconf/202023902003 | |
| Published online | 30 September 2020 | |
https://doi.org/10.1051/epjconf/202023902003
Structure of beta-decay strength function Sβ(E) and quenching of axial-vector weak interaction constant in halo nuclei
Joint Institute for Nuclear Research, 141980 Dubna, Russia
* e-mail: izosimov@jinr.ru
Published online: 30 September 2020
Resonance structure of the beta decay strength function Sβ (E) for GT β--decay of halo nuclei 6He and 11Li is analyzed. Compare experimental total strength for β-transitions in gv2/4π units with the Ikeda sum rule (in (gAeff)2/4π units) one can determine the squared ratio of axial-vector and vector weak interaction constants value (g eff/gV)2. We obtained (g eff/gv)1 = 1.272 ± 0.010 for 6He and (gA eff/gv)2 = 1.5±0.2 for 11Li β--decays. Quenching of the weak axial-vector constant gAeff in halo nuclei is discussed. Analysis of the evolution of EGTR - EIAS toward neutron-rich nuclei was done. It is shown that the value Z/N ≈ 0.6 corresponds to the SU(4) Wigner's spin-isospin symmetry region.
© The Authors, published by EDP Sciences, 2020
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