QCD radiative and power corrections and Generalized GDH sum rules
arXiv:hep-ph/0410228 · doi:10.1103/PhysRevD.70.116004
Abstract
We extend the earlier suggested QCD-motivated model for the -dependence of the generalized Gerasimov-Drell-Hearn (GDH) sum rule which assumes the smooth dependence of the structure function , while the sharp dependence is due to the contribution and is described by the elastic part of the Burkhardt-Cottingham sum rule. The model successfully predicts the low crossing point for the proton GDH integral, but is at variance with the recent very accurate JLAB data. We show that, at this level of accuracy, one should include the previously neglected radiative and power QCD corrections, as boundary values for the model. We stress that the GDH integral, when measured with such a high accuracy achieved by the recent JLAB data, is very sensitive to QCD power corrections. We estimate the value of these power corrections from the JLAB data at . The inclusion of all QCD corrections leads to a good description of proton, neutron and deuteron data at all .
10 pages, 4 figures (to be published in Physical Review D)
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- Nucleon spin structure and pQCD frontier on the move
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- Moments of the Spin Structure Functions g_1^p and g_1^d for 0.05 < Q^2 < 3.0 GeV^2
- Bjorken polarized sum rule and infrared-safe QCD couplings
- Analyticity and higher twists
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- Sum Rules and Moments of the Nucleon Spin Structure Functions
- Measurement of the Bjorken Sum at very low
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- Bjorken sum rule in QCD with analytic coupling
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- Highlights and Perspectives of the JLab Spin Physics Program
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- Measurement of the nucleon spin structure functions for 0.01<<1 GeV using CLAS
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