Orbital M1 versus E2 strength in deformed nuclei: A new energy weighted sum rule
E. Moya de Guerra, L. Zamick
Abstract
Within the unified model of Bohr and Mottelson we derive the following linear energy weighted sum rule for low energy orbital 1+ excitations in even-even deformed nuclei S LE lew (M1 orb) (6/5) ε(B(E2; 0+1 → 21+ K=0)/Z e2<r2>2) μ2N with B(E2) the E2 strength for the transition from the ground state to the first excited state in the ground state rotational band, <r2> the charge r.m.s. radius squared and ε the binding energy per nucleon in the nuclear ground state. It is shown that this energy weighted sum rule is in good agreement with available experimental data. The sum rule is derived using a simple ansatz for the intrinsic ground state wave function that predicts also high energy 1+ strength at 2 ω carrying 50\% of the total m1 moment of the orbital M1 operator.
Create a lesson
Related papers
Scale Invariance and Compact Star Matter
Hyun Kyu Lee, Won-Gi Paeng
Optimizing artificial neural networks for dipole strength predictions in light nuclei
Tim Egert, Weiguang Jiang, Sonia Bacca
Coupled-channel scattering from artificial confinement
Tafat Weiss Attia, Itay Horin, Betzalel Bazak
From twelve to three active qubits: Ancilla-recycled rodeo filtering for trapped neutron-proton scattering
Myeong-Hwan Mun, Jubin Park, Myung-Ki Cheoun et al.
Single-particle potentials in asymmetric nuclear matter within the LOCV framework
Zahra Ziarati, Hamidreza Moshfegh
Frontier Questions and Emerging Directions in Nuclear Science and Technology
Yu-Gang Ma