F. Hammache

Indirect study of the C 13 ( α , n ) O 16 reaction via the C 13 ( Li 7 , t ) O 17 transfer reaction

The

Low-energy states of 31 81 Ga 50 : Proton structure of the nuclei close to Ni 78

^{13}mathrm{C}

Recent results in nuclear astrophysics

(

Study of the N=50 shell closure close to 78Ni

ensuremath{alpha},n

Indirect measurement of 17O(p,α)14N cross section at ultra-low energies

)

Coulomb dissociation of 8B: determination of the E2 component

^{16}mathrm{O}

Fusion Cross Sections of Astrophysics Interest Within the STELLA Project.

reaction is considered the main neutron source for the s process in low mass asymptotic giant branch (AGB) stars. In the Gamow peak, the cross section sensitively depends on the

Study of 60Fe(n,γ)61Fe reaction of astrophysical interest via d(60Fe,pγ) indirect reaction

1/{2}^{+}

Indirect study of 12C(α,γ)16O reaction

subthreshold state of

Study of the 26Al(n,p)26Mg and 26Al(n,α)23Na reactions using the 27Al(p,p')27Al inelastic scattering reaction

^{17}mathrm{O}