# Toroidal, compressive, and $E1$ properties of low-energy dipole modes in   $^{10}$Be

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

arXiv: 1704.05649 · 2017-06-28

## TL;DR

This study investigates low-energy dipole modes in $^{10}$Be using an advanced molecular dynamics model, identifying distinct toroidal and neutron-skin oscillation modes with specific energy and flow characteristics.

## Contribution

It introduces an extended antisymmetrized molecular dynamics approach capable of describing both 1p-1h excitations and cluster modes, and distinguishes different low-energy dipole modes in $^{10}$Be.

## Key findings

- Identification of two low-energy $1^-$ states with distinct dominant modes.
- The $1^-_1$ state exhibits toroidal neutron flow caused by cluster rotation.
- The $1^-_2$ state shows surface neutron oscillation against the $2	ext{alpha}$ core.

## Abstract

We studied dipole excitations in $^{10}$Be based on an extended version of the antisymmetrized molecular dynamics, which can describe 1p-1h excitations and large amplitude cluster modes. Toroidal and compressive dipole operators are found to be good proves to separate the low-energy and high-energy parts of the isoscalar dipole excitations, respectively. Two low-energy $1^-$ states, the toroidal dominant $1^-_1$ state at $E\sim 8$ MeV and the $E1$ dominant $1^-_2$ state at $E\sim 16$ MeV, were obtained. By analysis of transition current densities, the $1^-_1$ states is understood as a toroidal dipole mode with exotic toroidal neutron flow caused by rotation of a deformed $^6\textrm{He}$ cluster, whereas the $1^-_2$ state is regarded as a neutron-skin oscillation mode, which are characterized by surface neutron flow with inner isoscalar flow caused by the surface neutron oscillation against the $2\alpha$ core.

## Full text

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## Figures

13 figures with captions in the complete paper: https://tomesphere.com/paper/1704.05649/full.md

## References

60 references — full list in the complete paper: https://tomesphere.com/paper/1704.05649/full.md

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Source: https://tomesphere.com/paper/1704.05649