Résumé
Stellar evolution models taking into account atomic diffusion including radiative accelerations of 28 species have been calculated for Pop II stars of 0.5 to 1.2 solar mass with [Fe/H] from -4.31 to -0.71. Overabundances are expected in some turnoff stars with effective temperatures larger than 5900 K. They depend strongly on the metallicity of the cluster. At the metallicity of M92 they reach a factor of 10 for many species at 12 Gyr but a factor of at most 2 at 13.5 Gyr. Series of models were also calculated with turbulence to determine to what extent turbulence reduces predicted abundance anomalies. The level of abundance anomalies observed in turnoff stars may then determine a level of turbulence. Even in the presence of turbulence however allowance for diffusive processes leads to a 10%-12% reduction in age at a given turnoff luminosity. For M 92 an age of 13.5 Gyr is determined which is about 1.5 Gyr younger than obtained in the absence of diffusion. In clusters atomic diffusion is now known to play a role in white dwarfs HB stars for age determination and for abundance anomalies in some turnoff stars.