Indirect study of $^{60}$Fe(n,γ)$^{61}$Fe via the transfer reaction $^{60}$Fe(d,pγ)$^{61}$Fe
Résumé
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.
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