Материал портала ядерных знаний BelNET
статья/документ по запросу ресурса "4238"
DOI: 10.1134/S1063778817060047 7 P. Physics of Atomic Nuclei, 2017, Vol. 80, No. 6, pp. 1126–1132. The results obtained by estimating the contribution of  and  nuclei to the coherent
dissociation of  ,  , and 
relativistic nuclei in nuclear track emulsions (“white” stars) are presented.
The selection of white stars accompanied by leads to a distinct peak appearing in the distribution of the
excitation energy of  ensembles and having a maximum at  MeV.
A nucleus manifests
itself in the coherent-dissociation reaction 
with a probability of  %,  % of
it being due to decays. The ratio of the branching fractions of the 
and  mirror channels
is estimated at  . An analysis of the relativistic dissociation of nuclei in a nuclear track emulsion
revealed nine  events corresponding to the Hoyle state.
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