& first nucleon tomographic images Michel Guidal (IPN Orsay)

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Presentation transcript:

& first nucleon tomographic images Michel Guidal (IPN Orsay) ECT Trento, 28/10/2016 Fits of GPDs (CFFs) & first nucleon tomographic images Michel Guidal (IPN Orsay)

JLab Hall A JLab CLAS HERMES DVCS unpol. X-section DVCS B-pol. X-section JLab CLAS DVCS BSA DVCS lTSA DVCS unpol. and B-pol. X-sections HERMES DVCS BSA,lTSA,tTSA,BCA

Hq(x,x,t) but only x and t experimentally accessible

In general, 8 GPD quantities accessible (sub-)Compton Form Factors with

Given the well-established LT-LO DVCS+BH amplitude Bethe-Heitler GPDs Can one recover the 8 CFFs from the DVCS observables? Obs= Amp(DVCS+BH) CFFs Two (quasi-) model-independent approaches to extract, at fixed xB, t and Q2 (« local » fitting), the CFFs from the DVCS observables

1/ Mapping and linearization If enough observables measured, one has a system of 8 equations with 8 unknowns Given reasonable approximations (leading-twist dominance, neglect of some 1/Q2 terms,...), the system can be linear (practical for the error propagation) ~ DsLU ~ sinf Im{F1H + x(F1+F2)H -kF2E}df ~ ~ DsUL ~ sinfIm{F1H+x(F1+F2)(H + xB/2E) –xkF2 E+…}df K. Kumericki, D. Mueller, M. Murray Phys.Part.Nucl. 45 (2014) 4, 723

2/ «Brute force » fitting c2 minimization (with MINUIT + MINOS) of the available DVCS observables at a given xB, t and Q2 point by varying the CFFs within a limited hyper-space (e.g. 5xVGG) The problem can be (largely) underconstrained: JLab Hall A: pol. and unpol. X-sections JLab CLAS: BSA + TSA 2 constraints and 8 parameters ! However, as some observables are largely dominated by a single or a few CFFs, there is a convergence (i.e. a well-defined minimum c2) for these latter CFFs. The contribution of the non-converging CFF enters in the error bar of the converging ones. For instance (naive): If -10<x<10:

2/ «Brute force » fitting c2 minimization (with MINUIT + MINOS) of the available DVCS observables at a given xB, t and Q2 point by varying the CFFs within a limited hyper-space (e.g. 5xVGG) The problem can be (largely) underconstrained: JLab Hall A: pol. and unpol. X-sections JLab CLAS: BSA + TSA 2 constraints and 8 parameters ! However, as some observables are largely dominated by a single or a few CFFs, there is a convergence (i.e. a well-defined minimum c2) for these latter CFFs. The contribution of the non-converging CFF enters in the error bar of the converging ones. M.G. EPJA 37 (2008) 319 M.G. & H. Moutarde EPJA 42 (2009) 71

~ Examples of correlation between HIm and HIm

unpol.sec.eff. + beam pol.sec.eff. c2 minimization Avec « ma » methode, extraction obtenue pour Him en fittant les sec.eff. (pol. et non-pol.) du Hall A c2 minimization

Hall A : s & DsLU , xB=0.36,Q2=2.3,t=.17,.23,.28,.33 c2=1.01 c2=0.92

unpol.sec.eff. + beam pol.sec.eff. beam spin asym. + long. pol. tar. asym Avec « ma » methode, extraction obtenue pour Him en fittant les BSA et les TSA (Shifeng) de CLAS c2 minimization

unpol.sec.eff. + beam pol.sec.eff. beam spin asym. + long. pol. tar. asym beam charge asym. + beam spin asym … Avec la methode de KM et la mienne, extraction obtenue pour Him en fittant les asymetries d’HERMES. c2 minimization linearization

Other approach: Assume a functionnal shape and fit some parameters *D. Mueller & K. Kumericki *H. Moutarde *VGG by the HERMES and n-DVCS Hall A coll. (slide from K. Kumericki)

M.G., H. Moutarde, M. Vanderhaeghen Rept.Prog.Phys. 76 (2013) 066202

New recent data from JLab: CLAS coll. PRL 115 (2015), 212003 Hall A coll. PRC92 (2015), 055202 CLAS coll. PRL 114 (2015), 032001 CLAS coll. PRD91 (2015), 052014

R. Dupré, M.G., M. Vanderhaeghen arXiv:1606.07821 [hep-ph]

If However, this formula involves: While we extract: Need to estimate: (M. Burkhardt) If However, this formula involves: While we extract: Need to estimate: (assuming )

for

« Integrated » radius from elastic form factor F1:

« Integrated » radius from elastic form factor F1:

Resultats pour HtildeIm The axial charge (Him) appears to be more « concentrated » than the electromagnetic charge (Him) ~ Confirmed by new CLAS A_UL and A_LL data: Phys.Rev. D91 (2015) 5, 052014

SUMMARY We have developped a fitting method to extract CFFs from data in which the influence of the subdominant CFFs end up in the uncertainties of the dominant CFFs: uncertainties are thus essentially systematic and will decrease with new measured observables to come. First new insights on nucleon structure already emerging from current data: in particular, the rise of the proton radius (and density) as x decreases

The Bethe-Heitler process

M. Boer, MG J.Phys. G42 (2015) 3, 034023

M. Boer, MG J.Phys. G42 (2015) 3, 034023

M. Boer, MG J.Phys. G42 (2015) 3, 034023

M. Boer, MG J.Phys. G42 (2015) 3, 034023