activity
19982025
most citedSpecific features and symmetries for magnetic and chiral bands in nuclei

59 citations · 746 across the 64 of their papers we have counts for

collaborators

65 papers

nucl-th2025

Semi-classical and boson descriptions of scissors states

A. A. Raduta, C. M. Raduta, R. Poenaru +1

A two interacting rotors Hamiltonian is alternatively treated semi-classically and by a Dyson boson expansion method. The linearized equations of motion lead to dispersion equation…

nucl-th2024

Semiclassical Features of Wobbling and Chiral Properties in Nuclei

Apolodor Aristotel Raduta, Cristian Mircea Raduta, Robert Poenaru

A semiclassical approach is used to describe the wobbling and chiral motion in even-even and odd-even nuclei The trial function involved in the variational equation for the quantal…

nucl-th2022★ 6 cited

Simultaneous description of wobbling and chiral properties in even-odd triaxial nuclei

C. M. Raduta, A. A. Raduta, R. Poenaru +1

A particle-triaxial rigid core Hamiltonian is semi-classically treated. The coupling term corresponds to a particle rigidly coupled to the triaxial core, along a direction that doe…

nucl-th2021

Parity Partner Bands in Lu: A novel approach for describing the negative parity states from a triaxial super-deformed band

R. Poenaru, A. A. Raduta

The wobbling spectrum of Lu is described through a novel approach, starting from a triaxial rotor model within a semi-classical picture, and obtaining a new set of equation…

nucl-th2020

New results about the canonical transformation for boson operators

C. M. Raduta, A. A. Raduta

The Bogoliubov transformation for a monopole boson induces an unitary transformation connecting the Fock spaces of initial and correlated boson-s. Here we provide a very simple met…

nucl-th2020★ 12 cited

A new boson approach for the wobbling motion in even-odd nuclei

A. A. Raduta, C. M. Raduta, R. Poenaru

A triaxial core rotating around the middle axis, i.e. 2-axis, is cranked around the 1-axis, due to the coupling of an odd proton from a high j orbital. Using the Bargmann represent…