The angular distributions for 166 MeV α-particle elastic scattering have been measured and are presented. The differential cross sections obtained are analysed with optical potentials whose real parts are derived from the convolution of nuclear-matter distributions with an effective α-nucleon interaction. This interaction is defined both from an analysis of α-scattering from N = Z light nuclei and from heavy nuclei whose matter distributions are supposedly well known. The imaginary parts of the optical potentials are either taken to be proportional to the real parts or to have a Woods-Saxon form. Using parameters for nuclear charge distributions derived from elastic electron scattering, radii of neutron matter distributions with errors varying between ±0.09 fm and ±0.16 fm are extracted for the following nuclei: 12C, 24Mg, 28Si, 32S, 40, 44, 48Ca, 48Ti, 56Fe, 59Co, 58, 60, 62Ni, 68Zn, 88Sr, 89Y, 90, 94Zr, 92Mo, 116, 118, 120, 124Sn, 140Ce 208Pb. The assumptions made in the present analysis and the resulting uncertainties are presented. Charge and neutron radii are compared in isotope and isotone families and to radii determinations from other sources. In particular, our results agree with those derived from proton-scattering analyses and with Hartree-Fock calculations but are not always in accord with the results obtained from Coulomb energy difference methods.
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