“…It is, however, severely limited by the energy conservation condition S 2n < B( 2 H) + (m n − m p − m e ) c 2 ≈ 3.007 MeV, (1) where S 2n is the two-neutron separation energy of the halo nucleus, B( 2 H) is the binding energy of the deuteron, and m n , m p , and m e are the neutron, proton, and electron masses, respectively. Only a few nuclei have low enough separation energies to allow this decay: 6 He, 8 He, 11 Li, 14 Be, 17 B, 27 F, ....…”