L. V. Grigorenko, I. G. Mukha, M. V. Zhukov
The structure and decay of $^{26}$O are studied in a three-body $^{24}$O+$n+n$ model. We have found extremely strong effect of the subbarrier configuration mixing on the width of true $2n$ emitters due to core recoil and neutron-neutron final state interaction. This effect is far exceeding analogous effect in the true $2p$ emitters. Our calculations provide reasonably narrow boundaries for the lifetime vs.\ decay energy dependence for the true $2n$ emission. An upper limit of $\sim 1$ keV for the decay energy of the unbound $^{26}$O is inferred basing on the recent experimental lifetime value.
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http://arxiv.org/abs/1304.4901
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