Journal
PHYSICS LETTERS B
Volume 644, Issue 1, Pages 33-37Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/j.physletb.2006.10.066
Keywords
inverse scattering NN interaction; no-core shell model; light nuclei
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Fully-microscopic no-core shell model (NCSM) calculations of all stable s and p shell nuclei are used to determine a realistic NN interaction, JISP16, describing not only the two-nucleon data but the binding energies and spectra of nuclei with A <= 16 as well. The JISP16 interaction, providing rapid convergence of the NCSM calculations, is obtained in an ab exitu approach by phase-equivalent transformations of the JISP6 NN interaction. Published by Elsevier B.V.
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