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General introduction to GPDs From data to GPDs General introduction to GPDs From data to GPDs.

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Presentation on theme: "General introduction to GPDs From data to GPDs General introduction to GPDs From data to GPDs."— Presentation transcript:

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2 General introduction to GPDs From data to GPDs

3 General introduction to GPDs From data to GPDs

4 Operator in Operator in space coordinates Structure function in Structure function in momentum coordinates ep  eX ep  ep ep  ep  Diagramme Diagramme Process Process (restricting myself to LT-LO, chiral even, quark sector)

5 H, H, E, E (x,ξ,t) ~~ Standard Parton Distributions H(x,0,0) = q(x), H(x,0,0) = Δq(x) ~ x Elastic Form Factors  H(x,ξ,t)dx = F(t) (  ξ) x Ji’s sum rule 2J q =  x(H+E)(x,ξ,0)dx (nucleon spin) x+ξx-ξ t γ, π, ρ, ω… -2ξ : don’t appear in DIS : NEW INFORMATION

6 0 t=0 1 DDs « D-term » x,b GPDs Pion cloud Long.mom./trans.pos. correlations F (t), G (t) 1,2 A,PS q(x),  q(x) R (t),R  (t) A V J q  (z)

7  p p’  H,E,H,E ~~ x t Deconvolution needed ! x : mute variable xx H q (x, ,t) but only  and t accessible experimentally dd d  dt B ~A H (x, ,t) q x-ix-i dxdx +B E (x, ,t) q x-ix-i dx +…. 1 1 2 == x B 1-x /2 B t=(p-p ’) 2 x = x B ! /2

8 GPD and DVCS Cross-section measurement and beam charge asymmetry (ReT) integrate GPDs over x Beam or target spin asymmetry contain only ImT, therefore GPDs at x =  and  (at leading order:)

9 General introduction to GPDs From data to GPDs

10 The experimental actors p-DVCS BSAs,lTSAs p-DVCS X-sec Hall BHall A JLab CERN COMPASS Vector mesons DVCS p-DVCS X-sec,BCA p-DVCS BSA,BCA, tTSA,lTSA H1/ZEUSHERMES DESY

11 In general, 8 GPD quantities accessible (Compton Form Factors) DVCS : golden Channel Anticipated Leading Twist dominance already at low Q 2

12 Model-independent fit, at fixed x B, t and Q 2, of DVCS observables with MINUIT + MINOS Given the well-established LT-LO DVCS+BH amplitude DVCSBethe-Heitler GPDs 7 unknowns (the CFFs), non-linear problem, strong correlations M.G. EPJA 37 (2008) 319M.G. & H. Moutarde, EPJA 42 (2009) 71) M.G. PLB 689 (2010) 156M.G. arXiv:1005.4922 [hep-ph] (acc.PLB) Only 3 CFFs come out from the fit with finite error bars: H Im, H Im and H Re ~

13 * « Shrinkage » of H Im * H Im >H Re As energy increases: JLab x B =0.36,Q 2 =2.3 *Different t-behavior for H Im &H Re (model dependent Fit of D. Muller, K. Kumericki Hep-ph 0904.0458 HERMES H Im H Re H Im H Re x B =0.09,Q 2 =2.5

14 x B dependence at fixed t of H Im VGG prediction

15 x B -dependence at fixed t lTSAs Fitting the CLAS & HERMES lTSAs: of H Im ~ VGG prediction Fit with 7 CFFs (boundaries 5xVGG CFFs) Fit with 7 CFFs (boundaries 3xVGG CFFs) JLab HERMES

16 VGG prediction Fit with 7 CFFs (boundaries 5xVGG CFFs) Fit with 7 CFFs (boundaries 3xVGG CFFs) Fit with ONLY H and H ~ t-dependence at fixed x B of H Im & H Im ~ Axial charge more concentrated than electromagnetic charge ?

17 First CFFs model independent fits (leading-twist/leading order approximation); “Minimal theoretical input” Procedure tested by Monte-Carlo Procedure is working on real data; extraction of H Im and H Re at JLab (cross sections) and HERMES (asymmetries) energies Relatively large uncertainties on extracted CFFs (due to lack of observables -and precision on data-) Introducing more theoretical input will reduce uncertainties (but model dependency) Large flow of new observables and data expected soon; will bring much more experimental constraints to extract CFFs with minimum theoretical input


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