Unstable nuclei in dissociation of light stable and radioactive nuclei in nuclear track emulsion
D. A. Artemenkov, A. A. Zaitsev, P. I. Zarubin

TL;DR
This study investigates the role of unstable nuclei like ${}^{6}$Be, ${}^{8}$Be, and ${}^{9}$B in the dissociation of relativistic light nuclei using nuclear track emulsion, revealing detailed configurations and decay pathways.
Contribution
It provides new quantitative insights into the configurations and decay modes of unstable nuclei in relativistic dissociation processes, using nuclear track emulsion techniques.
Findings
${}^{6}$Be + n contributes 8% to ${}^{7}$Be structure.
Simultaneous presence of ${}^{8}$Be ground and excited states in ${}^{9}$Be and ${}^{10}$C.
${}^{8}$Be$_{g.s.}$ appears in 24-27% of certain dissociation events.
Abstract
A role of the unstable nuclei Be, Be and B in the dissociation of relativistic nuclei Be, B and C is under study on the basis of nuclear track emulsion exposed to secondary beams of the JINR Nuclotron. Contribution of the configuration Be + to the Be nucleus structure is 8 1% which is near the value for the configuration Li + . Distributions over the opening angle of -particle pairs indicate to a simultaneous presence of virtual Be and Be states in the ground states of the Be and C nuclei. The core B is manifested in the {C} nucleus with a probability of 30 4%. Selection of the C "white" stars accompanied by Be (B) leads to appearance in the excitation energy distribution…
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