Structure of the nucleon and spin-polarizabilities

preprint2011arXivOpen access

Abstract

Spin-polarizabilities are predicted by calculating the cross-section difference σ3/2−σ1/2σ_{3/2}-σ_{1/2} from available data for the resonance couplings A3/2A_{3/2} and A1/2A_{1/2} and CGLN amplitudes. The forward spin-polarizabilities are predicted to be γ0(p)=−0.58±0.20γ^{(p)}_0=-0.58\pm 0.20 and γ0(n)=+0.38±0.22γ^{(n)}_0=+0.38\pm 0.22 in units of 10−410^{-4}fm4^4 where the different signs are found to be due to the isospin dependencies of the E0+E_{0+} and the (M,E)1+(1/2)(M,E)^{(1/2)}_{1+} amplitudes. The backward spin-polarizabilities are predicted to be γπ(p)=−36.6γ^{(p)}_π=-36.6 and γπ(n)=+58.3γ^{(n)}_π=+58.3, to be compared with the experimental values γ(p)=−36.4±1.5γ^{(p)}=-36.4\pm 1.5 and γπ(n)=+58.6±4.0γ^{(n)}_π=+58.6\pm 4.0. Electric γEγ_E and magnetic γMγ_M spin-polarizabilities are introduced and discussed in terms of the E1E1 and M1/E2M1/E2 components of the photo-absorption cross section of the nucleon.

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