1. Study of the Involvement of 8Be and 9B Nuclei in the Dissociation of Relativistic 10C, 10B, and 12C Nuclei
- Author
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R. R. Kattabekov, R. Stanoeva, K. Z. Mamatkulov, Maria Haiduc, G. I. Britvich, D. A. Artemenkov, N. K. Kornegrutsa, S. P. Kharlamov, V. A. Kalinin, I. G. Zarubina, V. V. Rusakova, E. Firu, A. A. Zaitsev, M. K. Polkovnikov, V. A. Pikalov, V. Bradnova, Alina Tania Neagu, M. Yu. Kostin, P. I. Zarubin, P. A. Rukoyatkin, V. R. Sarkisyan, A. V. Maksimov, and E. Mitseva
- Subjects
Physics ,Nuclear and High Energy Physics ,010308 nuclear & particles physics ,Branching fraction ,Carbon-12 ,White dwarf ,Isotopes of boron ,01 natural sciences ,Atomic and Molecular Physics, and Optics ,Dissociation (chemistry) ,medicine.anatomical_structure ,0103 physical sciences ,medicine ,Atomic physics ,010306 general physics ,Isotopes of beryllium ,Nucleus ,Isotopes of helium - Abstract
The results obtained by estimating the contribution of 8Be and 9B nuclei to the coherent dissociation of 10C, 10B, and 12C relativistic nuclei in nuclear track emulsions (“white” stars) are presented. The selection of white stars accompanied by 9B leads to a distinct peak appearing in the distribution of the excitation energy of 2α2p ensembles and having a maximum at 4.1 ± 0.3 MeV. A 8Be nucleus manifests itself in the coherent-dissociation reaction 10B → 2He + H with a probability of (25 ± 5)%, (14 ± 3)% of it being due to 9B decays. The ratio of the branching fractions of the 9B + n and 9Be + p mirror channels is estimated at 6 ± 1. An analysis of the relativistic dissociation of 12C nuclei in a nuclear track emulsion revealed nine 3α events corresponding to the Hoyle state.
- Published
- 2017
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