It is demonstrated that in simple soliton models essential features of the electro-magnetic nucleon form factors observed over three orders of magnitude in momentum transfer t are naturally reproduced. The analysis shows that three basic ingredients are required: an extended object, partial coupling to vector mesons, and relativistic recoil corrections. We use for the extended object the standard skyrmion, one vector meson propagator for both isospin channels, and the relativistic boost to the Breit frame. Continuation to timelike t leads to quite stable results for the spectral functions in the regime from the 2-or 3-pion threshold to about two rho masses. Especially the onset of the continuous part of the spectral functions at threshold can be reliably determined and there are strong analogies to the results imposed on dispersion theoretic approaches by the unitarity constraint. PACS: 12.39.Dc; 12.39.Fe; 13.40.Gp
I IntroductionTopological soliton models for structure and dynamics of baryons are based on effective nonlinear lagrangians for selected mesonic degrees of freedom. These usually comprise the pseudoscalar Goldstone boson octet of spontaneously broken chiral symmetry, but also the light vector and axial vector mesons have been included.A decisive advantage of the soliton concept as compared to models where explicit pointlike fermion fields are coupled to meson and gauge fields is the fact that already in leading classical approximation the spatial structure of the baryon as an extended object is obtained from the underlying effective action. Therefore all types of form factors can readily be extracted from the models, and comparison with the experimentally observed dependence on momentum transfer presents a stringent test for the resulting spatial profiles.Specifically, the electro-magnetic form factors of the nucleon for which we expect a wealth of precise data in the few (GeV/c) region from the new generation of electron accelerators pose a severe challenge for chiral soliton models.Shortly after the initial work of [1] the e.m. nucleon form factors have been evaluated for various versions of effective meson models [2, 3, 4] and various sets of parameters, mainly for momentum transfers Q < 1 GeV/c. The conclusion was that the resulting Q 2 -dependence follows roughly the standard dipole form, and that reasonable values for radii require the presence of explicit vector mesons. Unfortunately, in cases where these results have been included in more detailed comparisons with new data (e.g. in [9, 10]), they have left the prejudice that soliton form factors are not satisfactory. However, for momentum transfers Q > 1 GeV/c it is important to incorporate relativistic kinematical corrections into the form factors. This is crucial for quark bag or cluster models [5,6,7,8,9,10] as well as for soliton models [11]. The implementation of these corrections is fairly easy for solitonic nucleons due to the Lorentz covariance of the underlying field equations.The proton magnetic form factor is quite accurately known u...