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Progress of analysis of dissociation of C-10, B-10 and C-12 nuclei in nuclear track emulsion

Author
Artemenkov D.A. JINR
Bradnová Věra, Ing.
et al.  different institutions

Year
2017

Scientific journal
EPJ Web of Conferences, 138, UNSP 01030

Web


Abstract
Proceedings of the 23rd International Baldin Seminar on High Energy Physics Problems - Relativistic Nuclear Physics and Quantum Chromodynamics

Recent findings related with the unstable nuclei Be-8 and B-9. in the coherent dissociation of relativistic nuclei C-10, B-10 and C-12 in nuclear track emulsion ("white" stars) are highlighted. Selection of the C-10 "white" stars accompanied by 8Be ( 9B) leads to appearance of the distinct peak with a maximum at 4.1 +/- 0.3 MeV in the excitation energy distribution of 2 alpha 2p ensembles. The Be-8(g.s.) nucleus is manifested in the coherent dissociation B-10 -> 2He + H with a probability of 25 +/- 5 % including 13 +/- 3 % of B-9 decays. A probability ratio of the mirror channels B-9 + n and Be-9 + p is estimated to be 10 +/- 1. Reanalysis of relativistic C-12 dissociation in lead enriched emulsion revealed 9 3 alpha-events corresponding to the Hoyle state.

Cite article as:
D. Artemenkov, V. Bradnová, . et al., "Progress of analysis of dissociation of C-10, B-10 and C-12 nuclei in nuclear track emulsion", EPJ Web of Conferences, 138, UNSP 01030 (2017)