Beta-decay properties of neutron-rich rare-earth isotopes

TL;DR

This study models the beta-decay properties of neutron-rich rare-earth isotopes using a microscopic approach, providing insights into their role in astrophysical processes and comparing theoretical predictions with experimental data.

Contribution

It introduces a self-consistent microscopic model for beta-decay properties of neutron-rich rare-earth isotopes, incorporating deformed Hartree-Fock calculations with Skyrme interactions.

Findings

Calculated beta-decay half-lives agree with experimental data.

Predicted beta-delayed neutron-emission probabilities match observed trends.

Energy distributions of Gamow-Teller strength offer new insights into nuclear structure.

Abstract

In this paper, beta-decay properties of even-even neutron-rich isotopes in the rare-earth mass region are studied within a microscopic theoretical approach based on a proton-neutron quasiparticle random-phase approximation. The underlying mean field is constructed selfconsistently from a deformed Hartree-Fock calculation with Skyrme interactions and pairing correlations to which particle-hole and particle-particle residual interactions are added. Nuclei in this mass region participate in the astrophysical rapid neutron capture process and are directly involved in the generation of the rare-earth peak in the isotopic abundance pattern centered at A=160. The energy distributions of the Gamow-Teller strength as well as the beta-decay half-lives and the beta-delayed neutron-emission probabilities are discussed and compared with the available experimental information and with calculations based on different approaches.