Isospin Symmetry along the N=Z line in the sd shell
- DELLA VEDOVA, Francesca
- Lenzi, SILVIA MONICA
- M., IONESCU BUJOR
- N., Marginean
- E., Farnea
- M., Nespolo
- G., DE ANGELIS
- M., Axiotis
- D., Bazzacco
- A., BIZZETI SONA
- P. G., Bizzeti
- Brandolini, Franco
- D., Bucurescu
- A., Iordachescu
- Lunardi, Santo
- R., Menegazzo
- D. R., Napoli
- C., ROSSI ALVAREZ
- C. A., Ur
Publication date
January 2005
DOI Publisher
American Institute of Physics:2 Huntington Quadrangle, Suite 1NO1:Melville, NY 11747:(800)344-6902, (631)576-2287, EMAIL: subs@aip.org, INTERNET: http://www.aip.org, Fax: (516)349-9704. ISSN
0094-243X Citation count (estimate)
1Abstract
Excited states have been studied in sd-shell nuclei following the O-16 (70 MeV) + Mg-24 (400 mu g/cm(2)) fusion-evaporation reaction. The GASP spectrometer in conjunction with the charged-particle detector ISIS and the Neutron ring allowed the detection of the gamma-rays in coincidence with evaporated light particles. New data on the mirror pairs A = 31 and A = 35 have been obtained. In particular, the comparison between the level schemes of Ar-35 and (CI)-C-35 has confirmed the importance of the electromagnetic spin-orbit term, which explains the large Mirror Energy Difference values. Evidence of isospin mixing can be deduced from the E1 transitions
Add to ORKG