Search arXiv⌕ Search

arXiv · 2610.23211

Isovector Monopole Resonance

Abstract

We present a theoretical study of the three isospin channels of the isovector giant monopole resonance (IVGMR) within self-consistent Skyrme Hartree-Fock plus Random-Phase Approximation. A modified charge-exchange monopole operator is introduced to remove the dominant isobaric-analog-state contribution, thereby isolating the genuine radial isovector response. We derive the associated non-energy- and energy-weighted sum rules and establish approximate relations between the charge-exchange and non-charge-exchange strengths. The relative locations of the three IVGMR centroids are interpreted in terms of Coulomb displacement energies, the neutron-proton mass difference, and the finite-nucleus symmetry potential. Calculations for \(^{48}\)Ca, \(^{90}\)Zr, and \(^{208}\)Pb show that the non-charge-exchange centroid is accurately approximated by the average of the two charge-exchange centroids in medium-heavy and heavy nuclei. Using a broad set of Skyrme energy-density functionals, we find that the centroid energies of the three channels display a weak model dependence for a fixed nucleus, whereas the non-charge-exchange monopole polarizability exhibits a clear sensitivity to the density dependence of the symmetry energy. These results clarify the isospin structure of the IVGMR and support its use as a complementary probe of isovector nuclear properties.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Xavier Roca Maza, Gianluca Colò. 2026-10-16. Isovector Monopole Resonance. https://arxiv.org/abs/2610.23211

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

KEEP EXPLORING

Related papers

Dynamical Triaxial Correlations in the Charge Radii of Neutron-Rich Ruthenium Isotopes

Nuclear charge radii are fundamental observables that track changes in nuclear structure. Recent measurements of neutron-rich Ru isotopes, interpreted using mean-field density-functional calculations, have highlighted the sensitivity of charge radii to static triaxial deformation. Whether dynamical shape fluctuations involving triaxial configurations---known to affect both nuclear ground- and excited-state properties---can reshape the charge-radii evolution remains unresolved. In this Letter, we investigate the charge radii of even-even neutron-rich $^{106-114}$Ru within a nuclear density-functional framework that combines three-dimensional angular-momentum projection with the generator-coordinate method. Including dynamical triaxial shape fluctuations yields charge radii in good agreement with experiment, without introducing additional adjustable parameters. By successively incorporating static triaxial deformation, dynamical axial shape fluctuations, and dynamical triaxial shape fluctuations, we trace how the predicted charge radii change at each step. These results demonstrate that triaxial shape dynamics can leave a substantial imprint on charge radii. They also inform the interpretation of experimental charge-radius measurements used to trace the evolution of nuclear structure, since charge radii alone cannot uniquely determine the underlying nuclear shape.

nucl-th↗

Parameter dependence of the mapping of the mean-field Ising model onto QCD in the first-order phase transition regime

We map the mean-field Ising equation of state onto the QCD phase diagram and investigate how scaling parameters alter the metastable and unstable regions, as well as the symmetrized pressure and density along an isotherm on the QCD $T-μ_B$ phase plane. We find that, for both the conventional mapping scheme and the scheme valid in the small-quark-mass limit, increasing the scaling parameters $w$ and $ρ$ narrows the metastable and unstable regions. In the small-quark-mass-limit scheme, larger $w$ and $ρ$ reduce both the Ising-symmetrized pressure and density. For the conventional scheme, increasing $w$ reduces these quantities, while increasing $ρ$ raises the Ising-symmetrized pressure and has only a small effect on the density.

nucl-th↗

Deformability of neutron-deficient Sn nuclei studied with semi-realistic interaction

Although Sn nuclei have long been considered typical spherical nuclei, the $E2$ transitions in neutron-deficient Sn nuclei have posed a puzzle. We argue that their deformability may resolve this issue, based on self-consistent calculations with a semi-realistic interaction. The significant role of the pseudo-spin symmetry, which is attributed to the effects of the tensor force, is also discussed.

nucl-th↗