The authors measured the two-neutron separation energy to be 1.35 ( 10 ) MeV, in good agreement with shell model calculations, using standard interactions for this mass region.
2.
Clark, David D .; McElroy, Robert D .; Gill, R . L .; Piotrowski, A . Level densities near the neutron separation energy in strontium-93 to-97.
3.
Those excited states that lie below the separation energy for protons ( Sp ) decay by ? emission towards the groundstate of daughter B . For the higher excited states a competitive decay channel of proton emission to the granddaughter C exists, called ?-delayed proton emission.
4.
Thus, the only type of nuclei that are longer lived and undergo proton or neutron emission are in the class of beta-delayed decays, where first the isospin of one nucleon is reversed ( proton to neutron or vice versa ) via beta-decay, and then if the particle separation energy is non-positive, the daughter nucleus will undergo particle decay.
Meaning
the energy required to separate particles from a molecule or atom or nucleus; equals the mass defect Synonyms: binding energy,
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