2014
DOI: 10.1140/epjc/s10052-014-2751-4
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Nonlinear GLR-MQ evolution equation and $$Q^2$$ Q 2 -evolution of gluon distribution function

Abstract: In this paper we have solved the nonlinear Gribov-Levin-Ryskin-Mueller-Qiu (GLR-MQ) evolution equation for gluon distribution function G(x, Q 2 ) and studied the effects of the nonlinear GLR-MQ corrections to the Leading Order (LO) Dokshitzer-Gribov-Lipatov-Altarelli-Parisi (DGLAP) evolution equations. Here we incorporate a Regge like behaviour of gluon distribution function to obtain the solution of GLR-MQ evolution equation. We have also investigated the Q 2dependence of gluon distribution function from the … Show more

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Cited by 26 publications
(16 citation statements)
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“…Here ρ = xg(x,Q 2 ) πR 2 , where R is the correlation radius between two interacting gluons, πR 2 is the target area. The factor γ is evaluated by Muller and Quie that is found to be γ = 81 16 for N c = 3 [7]. Now in terms of gluon distribution function G (x, Q 2 )= xg (x, Q 2 ) the GLR-MQ equation can be written in standard form [23] ∂G (x, Q 2 )…”
Section: Glr-mq Equation Deals With the Number Of Partons Increased Tmentioning
confidence: 99%
“…Here ρ = xg(x,Q 2 ) πR 2 , where R is the correlation radius between two interacting gluons, πR 2 is the target area. The factor γ is evaluated by Muller and Quie that is found to be γ = 81 16 for N c = 3 [7]. Now in terms of gluon distribution function G (x, Q 2 )= xg (x, Q 2 ) the GLR-MQ equation can be written in standard form [23] ∂G (x, Q 2 )…”
Section: Glr-mq Equation Deals With the Number Of Partons Increased Tmentioning
confidence: 99%
“…This shadowing term, which is quadractic in gluon density is coming from gluon recombinations inside the hadrons. In our previous work, we have studied extensively the gluon distribution functions by obtaining the solutions of GLR-MQ equation at leading order(LO) [14,15], next-to-leading order(NLO) [16] and next-to-next-to-leading order(NNLO) [17,18]. We observed the taming of gluon distribution function towards small- [19].…”
Section: Introductionmentioning
confidence: 99%
“…Here, we consider the range x ≥ 10 −3 . We expect that at low initial scale the DGLAP evolution with a leading twist is not sufficient at low x [93,94] and one needs to consider the higher twist corrections in the DGLAP equation [95][96][97][98][99][100][101]. It should be mentioned here that there is also uncertainty from the longitudinal basis resolution within the initial scale PDFs.…”
Section: B Qcd Evolution Of Heavy Meson Pdfsmentioning
confidence: 98%