出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要:60Fe nuclei play an important role both in g-ray astronomy and in pre-solar grains study. The interpretation of these observations depends on a reliable 60Fe yield prediction. We report here on the d(60Fe,pg)61Fe experiment performed at GANIL, aiming at studying the 60Fe(n,g)61Fe reaction to reduce nuclear uncertainties surrounding 60Fe nucleosynthesis. Preliminary results concerning excitation energies of 61Fe are presented.