# Formation and decay of resonance state in $^{9}$Be and $^{9}$B nuclei.   Microscopic three-cluster model investigations

**Authors:** V. S. Vasilevsky, K. Kat\=o, N. Zh. Takibayev

arXiv: 1706.05514 · 2017-10-11

## TL;DR

This paper investigates the formation and decay of low-lying resonance states in $^{9}$Be and $^{9}$B using a microscopic three-cluster model with hyperspherical harmonics, focusing on decay channels, Coulomb effects, and potential Hoyle-analogue states.

## Contribution

It introduces a detailed three-cluster model analysis of resonance states in $^{9}$Be and $^{9}$B, including Coulomb effects and the search for Hoyle-analogue states.

## Key findings

- Identification of dominant decay channels for resonance states.
- Analysis of Coulomb interaction effects on resonance energies and widths.
-  Exploration of the existence of Hoyle-analogue states in $^{9}$Be and $^{9}$B.

## Abstract

We study nature of the low-lying resonance states in mirror nuclei $^{9}$Be and $^{9}$B. Investigations are performed within a three-cluster model. The model makes use of the hyperspherical harmonics, which provides convenient description of three-cluster continuum. The dominant three-cluster configurations $\alpha+\alpha+n$ and $\alpha+\alpha+p$ in $^{9}$Be and $^{9}$B, respectively, are taken into account. Dominant decay channels for all resonance states in $^{9}$Be and $^{9}$B are explored. Much attention is paid to the controversial $1/2^{+}$ resonance states in both nuclei. We study effects of the Coulomb interaction on energy and width of three-cluster resonances in the mirror nuclei $^{9}$Be and $^{9}$B. We also search for the Hoyle-analogue state which is a key step for alternative way of $^{9}$Be and $^{9}$B syntheses in a triple collision of clusters in a stellar environment.

## Full text

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## Figures

16 figures with captions in the complete paper: https://tomesphere.com/paper/1706.05514/full.md

## References

44 references — full list in the complete paper: https://tomesphere.com/paper/1706.05514/full.md

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Source: https://tomesphere.com/paper/1706.05514