Abstract
Spin-polarizabilities are predicted by calculating the cross-section difference from available data for the resonance couplings and and CGLN amplitudes. The forward spin-polarizabilities are predicted to be and in units of fm where the different signs are found to be due to the isospin dependencies of the and the amplitudes. The backward spin-polarizabilities are predicted to be and , to be compared with the experimental values and . Electric and magnetic spin-polarizabilities are introduced and discussed in terms of the and components of the photo-absorption cross section of the nucleon.
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