γ*N → N* (1520) form factors in the spacelike region

The covariant spectator quark model is applied to the gamma*N -> N* (1520) reaction in the spacelike region. The spin quark core contributions to the electromagnetic form factors and helicity transition amplitudes are estimated from the covariant structure of the N* (1520) wave function calibrated by the experimental data for large squared momentum transfer Q(2). The difference between the model results and the experimental data is then used to parametrize the low Q(2) behavior, where meson cloud effects are assumed to dominate. This parametrization can be very useful for future studies of the reaction, as well as for the extension of the transition form factors to the timelike region.