Abstract

The role of the relativistic amplitudes for a number of O(k){\cal O}(k) processes usually neglected in potential model calculations of NN--bremsstrahlung is investigated. In particular, we consider the Δ\Delta--excitation pole contributions related to the one--pion and one--rho exchange and in addition include the exchange contributions induced by the radiative ω,ρπγ\omega,\,\rho \to \pi \gamma decays. The contributions are calculated from relativistic Born amplitudes fitted to Δ\Delta--production and absorption data in the energy range up to 1 GeV and then used to supplement potential model and soft photon calculations for nucleon--nucleon bremsstrahlung. The effects on NNγNN\gamma--observables, although moderate in general, are found to be important in some kinematic domains.Comment: 15 pages in LaTex, using Revtex, 6 figures as uufile'd, compressed Postscript file included, TRIUMF preprint TRI-PP-94-9

    Similar works

    Full text

    thumbnail-image

    Available Versions