Search arXivSearch

arXiv · 2411.17407

Isomer triplets in odd-odd transitional rare earth nuclei: unique features, orbital systematics and characterization

Abstract

The existence of low-lying long-lived isomers, predominantly in odd-odd nuclei of the light rare-earth mass region, is investigated through an extensive survey of available nuclear data. The characteristics of these isomeric states and their systematics has revealed intriguing and unusual properties, including the identification of isomer triplets, a phenomenon specific to odd-odd deformed nuclei close to the transition region. This exclusive feature was observed in the following odd-odd nuclei, namely, 152Pm, 152Eu, 154Tb, 156Tb, 156Ho, 158Ho, 160Ho, 162Lu and 166Lu. We present a detailed overview of these isomer triplets by exploring the systematics of single-quasiparticle proton and neutron orbitals near the Fermi surface relevant in this mass region, to elucidate the factors responsible for their formation. The low-lying level structures of 156Tb and 154Tb, were constructed using the well-tested Two Quasiparticle Rotor Model to resolve the ambiguities in the spin, parity, energy and orbital configuration of these isomeric states. These results were extended to study the systematics of low-lying isomer triplets in the other five light rare-earth nuclei of interest. Our review and analysis of 1qp proton and neutron orbital systematics in the neighboring odd-mass isotopes and isotones highlights the crucial role of high-spin intruder neutron orbital in the formation of these isomer triplets.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

N. Susshma, S. Deepa, K. Vijay Sai, R. Gowrishankar. 2024-11-26. Isomer triplets in odd-odd transitional rare earth nuclei: unique features, orbital systematics and characterization. https://arxiv.org/abs/2411.17407

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Application of the Skyrme Hartree-Fock-Bogoliubov Theory to WIMP-Nucleus Interactions in 40Ar

WIMP scattering from 40Ar is investigated using a self-consistent Skyrme Hartree-Fock-Bogoliubov (HFB) approach. Nuclear form factors relevant to dark matter direct detection are calculated from the resulting one-body density matrix elements and compared with shell-model predictions. Good agreement is found for the spin-independent response, while significant differences are observed for the spin-orbit response due to variations in single-particle occupancies. The effects of particle-number projection are shown to be small for 40Ar. These results demonstrate the sensitivity of certain dark matter response channels to the underlying nuclear structure model and establish a framework for extending mean-field calculations to nuclei beyond the reach of large-scale shell-model studies.

nucl-th

Breakdown of the Plane-Wave Trojan Horse Analysis of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ Fusion Reaction: Critical Role of Coulomb Distortions

Recently, a new Trojan Horse Method (THM) measurement of carbon-carbon fusion was reported by Li \textit{et al.} [Phys. Lett. B (2026) 140675]. The purpose of the present work is to demonstrate the breakdown of the plane-wave approximation used in the analysis of these data and the critical role of Coulomb distortions in the initial and final states. The reaction mechanism underlying the THM analysis of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ fusion reaction using the $^{16}\mathrm{O}+{}^{12}\mathrm{C}\to α_s+α+{}^{20}\mathrm{Ne}$ reaction is investigated. Particular attention is paid to the spectator momentum distribution and to the dependence of the THM reaction amplitude on the relative carbon-carbon energy $E$. It is demonstrated that agreement with the measured spectator momentum distribution does not by itself validate the plane-wave approximation. Although the experimental momentum distribution can be reproduced, inclusion of Coulomb distortions in both the initial and final channels leads to an energy dependence of the THM amplitude that is completely different from the plane-wave result. Consequently, the energy dependence of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ fusion cross section extracted from the THM data can be strongly distorted by the plane-wave treatment. It is concluded that the astrophysical factor extracted in the plane-wave analysis cannot be regarded as reliable and may lead to misleading conclusions concerning the low-energy $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ fusion reaction.

nucl-th