1975
DOI: 10.1016/0370-2693(75)90687-5
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The (9Be, 8B) reaction and the unbound nuclide 10Li

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Cited by 79 publications
(52 citation statements)
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“…The unbound nature of 10 Li was determined in 1966 by Poskanzer, Cosper, and Hyde [7]. Almost ten years later, Wilcox and collaborators made the first measurement of the unbound nucleus, using a ( 9 Be, 8 B) reaction to measure a mass excess of 33.83 ± 0.25 MeV [8]. This placed the first measured unbound state at 0.8 ± 0.25 MeV decay energy [8].…”
mentioning
confidence: 98%
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“…The unbound nature of 10 Li was determined in 1966 by Poskanzer, Cosper, and Hyde [7]. Almost ten years later, Wilcox and collaborators made the first measurement of the unbound nucleus, using a ( 9 Be, 8 B) reaction to measure a mass excess of 33.83 ± 0.25 MeV [8]. This placed the first measured unbound state at 0.8 ± 0.25 MeV decay energy [8].…”
mentioning
confidence: 98%
“…Almost ten years later, Wilcox and collaborators made the first measurement of the unbound nucleus, using a ( 9 Be, 8 B) reaction to measure a mass excess of 33.83 ± 0.25 MeV [8]. This placed the first measured unbound state at 0.8 ± 0.25 MeV decay energy [8]. The next measurement was made 15 years later [9] and since then, there have been many measurements of energies of the continuum structure of 10 Li [4,5,[10][11][12][13][14][15][16][17][18][19][20][21][22][23][24][25][26][27][28][29]34].…”
mentioning
confidence: 99%
“…In these models, the 9 Li-n interaction is chosen so as to reproduce the experimental p-wave resonance energy of 10 Li at E r ∼ 0.5 MeV. However, despite the success of this model in explaining the halo structure of 11 Li, the binding energy of 11 Li is not reproduced. For example, in the cluster orbital shell model (COSM), 3) which is one of the pioneering 9 Li+n+n models, the binding energy is too weak at least 1-2 MeV.…”
Section: §1 Introductionmentioning
confidence: 97%
“…1) The first motivation for studying neutron-rich nuclei was provided by the observation of the large interaction cross-section of 11 Li. 2) It has been discussed in many works that the large interaction cross-section can be explained in terms of the so-called halo structure, which is a cloud of valence neutrons around the core nucleus.…”
Section: §1 Introductionmentioning
confidence: 99%
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