# [RIBF-ULIC-Symposium-007] E(U)RICA International Workshop

23-24 May 2011
RIKEN Nishina Center
Asia/Tokyo timezone

## Study of the N=34 subshell gap (and abstract Ids 12,13,16)

23 May 2011, 14:30
40m
RIBF Building 2F Conference Room (RIKEN Nishina Center)

### RIBF Building 2F Conference Room

#### RIKEN Nishina Center

2-1 Hirosawa, Wako, Saitama 351-0198, Japan

### Speaker

Jose Javier Valiente Dobon (LNL-INFN)

### Description

Shell closures are a fundamental concept in nuclear physics and most of our knowledge of effective nucleon-nucleon interactions comes from the study of nuclei with few valence particles around doubly-magic cores. There are by now a wealth of data coming from the study of exotic nuclei showing that the relative energies of the shell-model orbitals are not immutable but can change and evolve as a function of neutron number. This leads to the disappearance of well established magic numbers or to the appearance of new ones. For example, the presence of a $N=32$ subshell closure has been recently derived from various experiments on neutron-rich nuclei from Ca to Cr. The existence of this energy gap at N=32 around Z=20 arises from a large energy spacing between the neutron p3/2 orbital and the higher lying p1/2 and f5/2 orbitals. Otsuka and collaborators have also predicted that the N=34 isotones around Z=20 could exhibit characteristics of a shell closure due to the proton f7/2 - neutron f5/2 monopole tensor interaction. This effect could be revealed by measuring the first excited states involving the f5/2 neutron single particle orbital in the 55Sc nucleus. The most direct evidence of the subshell at N=34 would be the high energy of the first \$+ state in 54Ca, not accessible today. However, the low-lying excited states of 55Sc, populated via the beta decay of 55Ca (g.s. 5/2-), involving the f5/2 neutron single particle orbital will help to elucidate the gap at N=34 and this will represent a crucial test for theoretical calculations predicting a new shell clousure at N=34 around Z=20. This nucleus will be produced in a fragmentation reaction at relativistic energies, using a 86Kr primary beam at 350MeV.A. The BigRIPS fragment separator in combination with some of the Euroball Cluster detectors will be used for this study. Probably a total of 7 days of beam time would be enough to perform this experiment with final relevant results.

### Primary authors

Eda Sahin (INFN-LNL) Giacomo de Angelis (INFN Laboratori Nazionali di Legnaro) Jose Javier Valiente Dobon (LNL-INFN)

 Slides