2017
DOI: 10.1007/s10773-017-3286-x
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Small-x Behavior of Non-singlet Spin Structure Function and Bjorken Sum Rule with pQCD Correction up to NNLO and Higher Twist Correction

Abstract: A calculation of the non-singlet part of spin dependent structure function, xg N S 1 (x, Q 2 ) and associated sum rule, the Bjorken Sum rule up to next-next-to-leading order(NNLO) is presented. We use a unified approach incorporating Regge theory and the theoretical framework of perturbative Quantum Chromodynamics. Using a Regge behaved model with Q 2 dependent intercept as the initial input, we have solved the Dokshitzer-GribovLipatov-Altarelli-Parisi (DGLAP) evolution equation up to NNLO at small-2 ) and the… Show more

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Cited by 4 publications
(2 citation statements)
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“…In the light-cone operator-product expansion (OPE), the leading-twist (twist τ = 2) contributions correspond to scattering off asymptotically free partons, while the higher-twist contributions emerge due to multiparton correlations. The leading-twist spin-dependent proton and neutron structure functions, g p,n 1 (x, Q 2 ) at NNLO, can be expressed as a linear combination of polarized parton densities and coefficient functions as [13,21,22]…”
Section: A Leading-twist Polarized Dis Structure Functionmentioning
confidence: 99%
“…In the light-cone operator-product expansion (OPE), the leading-twist (twist τ = 2) contributions correspond to scattering off asymptotically free partons, while the higher-twist contributions emerge due to multiparton correlations. The leading-twist spin-dependent proton and neutron structure functions, g p,n 1 (x, Q 2 ) at NNLO, can be expressed as a linear combination of polarized parton densities and coefficient functions as [13,21,22]…”
Section: A Leading-twist Polarized Dis Structure Functionmentioning
confidence: 99%
“…The results are then adjusted to fit the experimental data (mainly at small-x) available for the proton structure function F 2 (x, Q 2 ) measured in DIS, over a large range of values of x and Q 2 by adjusting the parameters in the initial distributions. With much phenomenological success approximate solutions of the linear DGLAP evolution equations have been reported in recent years [21][22][23][24][25][26][27][28][29][30].…”
Section: Introductionmentioning
confidence: 99%