# Isoscalar dipole excitations in $^{16}$O

**Authors:** Yoshiko Kanada-En'yo, Yuki Shikata

arXiv: 1903.01075 · 2019-07-10

## TL;DR

This paper investigates isoscalar monopole and dipole excitations in $^{16}$O using advanced nuclear modeling, revealing significant low-energy transition strengths and novel dipole modes related to cluster structures, aligning well with experimental data.

## Contribution

The study introduces a detailed analysis of low-energy isoscalar dipole modes in $^{16}$O, highlighting the coexistence of compressive and vortical modes with cluster structures, using the shifted basis antisymmetrized molecular dynamics method.

## Key findings

- Significant low-energy IS monopole and dipole transition strengths below giant resonances.
- Identification of vortical dipole mode in the $1^-_1$ state.
- The $1^-_1$ state accounts for 5	ext% of the energy-weighted sum rule, matching experimental observations.

## Abstract

Isoscalar (IS) monopole and dipole excitations in $^{16}$O were investigated by the method of shifted basis antisymmetrized molecular dynamics combined with the generator coordinate method. Significant strengths of the IS monopole and dipole transitions were obtained in the low-energy region below the giant resonances. In addition to the compressive mode, which mainly contributes to the high-energy strengths for the IS dipole giant resonance, we obtained a variety of low-energy dipole modes such as the vortical dipole mode in the $1^-_1$ state of the vibrating tetrahedral $4\alpha$ and the $^{12}$C+$\alpha$ cluster structure in the $1^-_2$ state. The $1^-_1$ state contributes to the significant low-energy strength of the IS dipole transition as 5\% of the energy-weighted sum rule, which describes well the experimental data observed by the $\alpha$ inelastic scattering.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1903.01075/full.md

## References

54 references — full list in the complete paper: https://tomesphere.com/paper/1903.01075/full.md

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Source: https://tomesphere.com/paper/1903.01075