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Evidence of nonstatistical neutron emission following $$beta$$ decay near doubly magic $$^{132}$$Sn

二重魔法$$^{132}$$Snの近く、$$beta$$崩壊後の非統計的中性子放出の証拠

Heideman, J.*; Grzywacz, R.*; Xu, Z. Y.*; Madurga, M.*; Escher, J. E.*; 河野 俊彦*; Algora, A.*; Andreyev, A. N.; 他41名*

Heideman, J.*; Grzywacz, R.*; Xu, Z. Y.*; Madurga, M.*; Escher, J. E.*; Kawano, Toshihiko*; Algora, A.*; Andreyev, A. N.; 41 of others*

$$beta$$-delayed neutron emission was observed in the study of the $$beta$$ decay of $$^{134}$$In at ISOLDE CERN. Neutron emission probabilities from the unbound states in $$^{134}$$Sn to known low-lying, single-particle states in $$^{133}$$Sn were measured. The neutron energies were determined using the time-of-flight technique and the decay from excited states in $$^{133}$$Sn was studied by detecting its $$gamma$$ rays. Individual $$beta$$-delayed neutron emission probabilities were determined by correlating the relative intensities and energies of neutrons and $$gamma$$ rays. The new results suggest the violation of the assumption that neutrons are emitted statistically via the intermediate compound nucleus. This impacts the neutron-emission probabilities and other properties of nuclei participating in the $$r$$-process. A model of neutron emission, which links the observed neutron emission probabilities to nuclear shell effects, is proposed.

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パーセンタイル:40.52

分野:Physics, Nuclear

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