E. M. Fiore

An optical model analysis of neutron scattering

Proton scattering on the unstable38Snucleus: Isovector contribution to the21+state

Proton elastic scattering on light nuclei. I. Energy dependence

Energy levels of A = 21–44 nuclei (VII)

Terrestrial in situ cosmogenic nuclides: theory and application

A Skyrme parametrization from subnuclear to neutron star densities Part II. Nuclei far from stabilities

Local and global nucleon optical models from 1 keV to 200 MeV

Intercalibration of standards, absolute ages and uncertainties in 40Ar/39Ar dating

Two-step effects in 15-35 MeV proton scattering fromMg24low-lying states

Energy dependence of optical-model parameters for the p+32S system between 15 and 35 MeV