Shell-model structure of exotic nuclei beyond 132Sn
Dipartimento di Scienze Fisiche, Università di Napoli Federico II, and Istituto Nazionale di Fisica Nucleare, Complesso Universitario di Monte S. Angelo, via Cintia, 80126 Napoli, Italy
Corresponding author: firstname.lastname@example.org
Published online: 8 December 2007
We report on a study of exotic nuclei around doubly magic 132Sn in terms of the shell model employing a realistic effective interaction derived from the CD-Bonn nucleon-nucleon potential. The short-range repulsion of the bare potential is renormalized by constructing a smooth low-momentum potential, Vlow-k, that is used directly as input for the calculation of the effective interaction. In this paper we focus attention on the nuclei 134Sn and 135Sb which, with an N/Z ratio of 1.68 and 1.65, respectively, are at present the most exotic nuclei beyond 132Sn for which information exists on excited states. Comparison shows that the calculated results for both nuclei are in very good agreement with the experimental data. We present our predictions of the hitherto unknown spectrum of 136Sn.
PACS: 21.60.Cs – Shell model / 21.30.Fe – Forces in hadronic systems and effective interactions / 27.60.+j – 90 ≤A ≤149
© EDP Sciences, Springer-Verlag, 2007