Separation energies of light nuclei with atomic number from 1 to 20

P. Mandal, R. L. Nayak, T. Sahoo, Anjana Acharya

Abstract


The 1n and 1p halo nuclei from atomic number 1 to 20 are discussed here to calculate the variation of separation energy with mass defect and binding energy. Semi-empirical mass formula and shell model are the methods applied here. The appearances of p- and r-branches satisfying the selection rules for different isotopes of nuclides are discussed.


Keywords


shell model, halo nuclei, separation energy, r- and p- processes

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References


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M. T. Yamashita, R. S. Marques de Carvalho, T. Frederico, Lauro Tomio, “Constraints on 2n separation energy in Borromean 22C nucleus”, Physics Letter B, 697, 90 (2011)


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