Status and prospects of GPD extraction from DVCS

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1 Status and prospects of GPD extraction from DVCS Krešimir Kumerički University of Zagreb, Croatia Probing Nucleons and Nuclei in High Energy Collisions October 1 November 16, 18, INT, Seattle

2 Outline 1 Introduction and status of fits to DVCS data Uncertainties? 3 Neural net fits 4 Summary Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 / 7

3 Access to GPDs via DVCS Deeply virtual Compton scattering (DVCS) gold plated process of exclusive physics DVCS is measured via leptoproduction of a photon l l γ γ l γ l γ l γ γ l + + p DVCS p p BH p p BH p Interference with Bethe-Heitler process gives unique access to both real and imaginary part of DVCS amplitude. Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 3 / 7

4 DVCS cross section dσ T = T BH + T DVCS + I. where e. g. interference term is { e l 3 I c I [ + c I P 1 (φ)p (φ) n cos(nφ) + sn I sin(nφ) ] }, where e. g. c1 I [ c1,unpol. I F 1 Re H n=1 harmonic for unpolarized target is t 4M p F Re E + x B x B (F 1 + F ) Re H and at leading order everything depends on four complex Compton form factors (CFFs) H(ξ, t, Q ), E(ξ, t, Q ), H(ξ, t, Q ), Ẽ(ξ, t, Q ) ] Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 4 / 7

5 Factorization of DVCS GPDs γ ( Q ) γ γ ( Q ) γ [Collins et al. 98] DVCS C = + O 1 Q GPD CFFs are convolution: a H(ξ, t, Q ) = p p p p dx C a (x, ξ, Q Q ) H a (x, ξ, t, Q) H a (x, η, t, Q ) Generalized parton distribution (GPD) a=q,g Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 5 / 7

6 Hybrid GPD models for global fits [K.K., Müller 9-15] Sea quarks and gluons modelled using SO(3) partial wave expansion in conformal GPD moment space + Q evolution. Valence quarks model CFFs directly (ignoring Q evolution): [ 4 Im H(ξ, t) = π 9 Hu val (ξ, ξ, t) Hd val (ξ, ξ, t) + ] 9 Hsea (ξ, ξ, t) ( ) x α(t) ( ) 1 x b H(x, x, t) = n r α 1 ( ) 1 + x 1 + x p. 1 1 x t 1+x M Re H determined by dispersion relations 15 free parameters in total for H, H, E, Ẽ. Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 6 / 7

7 Fit examples (1/): H1/ZEUS Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 7 / 7

8 Fit examples (/): JLab s Hall A (15) KM15 global fit is fine. χ /n d.o.f. = 4./75 Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 8 / 7

9 Global fit χ values: KM and PARTONS [K.K., Müller 9-15] [Moutarde, Sznajder, Wagner, 18] Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 9 / 7

10 Including Hall A 17 data in global world fit: fail.6 KM world KM 17 data Hall A KM world KM 17 data Hall A 17.4 d cos, w. sin, w Q = 1.98 E = Q = 1.74 E = Q = 1.51 E = Q = 1.98 E = Q = 1.74 E = Q = 1.51 E = d cos, w. sin, w..1. Q = 1.99 E = 4.46 Q = 1.74 E = 4.46 Q = 1.5 E = Q = 1.74 E = 4.46 Q = 1.5 E = t [GeV ]..3.4 t [GeV ]..3.4 t [GeV ]..3.4 t [GeV ]..3.4 t [GeV ] Global world DVCS data fit before 17 χ /n d.o.f = 4./75 including 17 Hall A χ /n d.o.f =545./337 Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 1 / 7

11 Uncertainties? Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 11 / 7

12 Example: Uncertainty of D-term D-term is a part of GPD that has nice physical interpretation (related to pressure distribution inside nucleon [M. Polyakov 3]), see talk by [P. Schweitzer] tomorrow within some approximations and up to a charge-related prefactor of order one it is equal to subtraction constant in dispersion relation for CFFs H and E [O. Teryaev 5]: D(t) (t) = Re H(ξ, t) 1 1 π P.V. x dx ξ Im H(x, t) x In KM fits [K.K., D. Müller], D(t) = D/(1 t/m D ) and is extracted directly by fits (where Re H is then determined by dispersion relations) Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 1 / 7

13 Extractions of D-term D Q (t) KM15 global fit -.5 JLab data lattice LHPC -3 dispersion relations chiral quark soliton -3.5 Skyrme model bag model t [GeV ] Fit parameter uncertainties of D(t) are %, but systematic uncertainty due to model selection is unknown and presumably much larger! [V. D. Burkert, F.-X. Girod and L. Elouadrhiri 18] use just CLAS dσ and σ DVCS data to extract very precise value of D-term Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 13 / 7

14 Extractions of D-term D Q (t) KM15 global fit -.5 JLab data lattice LHPC -3 dispersion relations chiral quark soliton -3.5 Skyrme model bag model t [GeV ] Fit parameter uncertainties of D(t) are %, but systematic uncertainty due to model selection is unknown and presumably much larger! [V. D. Burkert, F.-X. Girod and L. Elouadrhiri 18] use just CLAS dσ and σ DVCS data to extract very precise value of D-term Data science: total error = bias + variance Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 13 / 7

15 Bias-variance tradeoff: toy example Unknown f (x) = sin(πx) measured at two points. H - rigid (biased) H 1 - flexible [Abu-Mostafa et al. 1] h(x) = a h(x) = ax + b error = bias + variance Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 14 / 7

16 Bias-variance tradeoff: toy example Unknown f (x) = sin(πx) measured at two points. H - rigid (biased) H 1 - flexible [Abu-Mostafa et al. 1] h(x) = a h(x) = ax + b error = bias + variance In DVCS situation is the opposite! We need to decrease bias. Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 14 / 7

17 Bias-variance tradeoff: toy example Unknown f (x) = sin(πx) measured at two points. H - rigid (biased) H 1 - flexible [Abu-Mostafa et al. 1] h(x) = a h(x) = ax + b error = bias + variance In DVCS situation is the opposite! We need to decrease bias. Neural networks are proven to be unbiased Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 14 / 7

18 Neural net fits Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 15 / 7

19 Fitting with neural networks Essentially a least-square fit of a complicated many-parameter function. f (x) = tanh( w i tanh( w j )) no theory bias Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 16 / 7

20 Study A: NN fit to CLAS 15 data We start by fitting just to the CLAS 15 dσ and σ measurements [Jo et al. 15], and just H We utilize dispersion relations (one NNet represents Im H, another represents D(t)) Uncertainty is estimated by averaging over ensemble of neural nets: t =. GeV = xb/( xb) = xb/( xb) t =. GeV NNDR-C = xb/( xb) = xb/( xb) Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 17 / 7

21 Comparison to [Burkert et al. 18] ImH t =. GeV ξ ReH KM15 GK NNet H Burkert et al ξ Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 18 / 7

22 Comparison to [Burkert et al. 18] ImH t =. GeV ξ ReH KM15 GK NNet H Burkert et al ξ But what is the effect of using the limited set of data, and assumption of H dominance? χ /n pts = 175/8 (this NNet), 191/8 (KM15), 3/8 (GK) Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 18 / 7

23 More flexible model: H + H t =. GeV NNDR-C15- NNDR-C15-4t t =. GeV ξ ImH ReH KM15 7 GK NNet H, E, H, Ẽ 8 Burkert et al ξ Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 19 / 7

24 Adding more data points Adding HERMES A LU,I data. (Model now includes H and E) t =. GeV NNDR-C15-6 NNDR-C15_ALUI Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 / 7

25 Adding more data points Adding HERMES A LU,I data. (Model now includes H and E) t =. GeV NNDR-C15-6 NNDR-C15_ALUI D Q (t) t[gev ] KM15 global fit CLAS 15 + HERMES BSA CLAS15 data alone is still consistent with zero D-term. Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 / 7

26 Propagating uncertainties back to d σ and σ d = d + d = d d NNDR-C15-6 NNDR-C15_ALUI-6 CLAS 15 xb =.335, Q =.78, t = -. xb =.335, Q =.78, t = -. xb =.335, Q =.78, t = -.6 xb =.335, Q =.78, t = -.45 xb =.335, Q =.78, t = -.6 xb =.335, Q =.78, t = [deg] [deg] [deg] Small propagated error is due to small sensitivity of these observables to CFFs (and D-term). Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 1 / 7

27 Independent simple way to the same conclusion.35.3 Q = 1.63 xb =.18 Q = 1.64 xb =.1 Q = 1.88 xb =.1 Q = 1.79 xb =.4 Q =.1 xb =.4 sin, w KM9a model with subtraction constant C describes CLAS 15 dσ and σ data correctly χ /n pts = 1746/3 d = d + d = d d KM9a(C->) CLAS 15 xb =.335, Q =.78, t = -. sin, w Q =.35 xb = Q =.58 xb = Q =.78 xb = t [GeV ] xb =.335, Q =.78, t = -.6 xb =.335, Q =.78, t = xb =.335, Q =.78, t = xb =.335, Q xb =.335, Q =.78, t = -.6 =.78, t = [deg] [deg] [deg] Q =.97 xb = Q = 3.18 xb =.4 KM9a(C->) Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 / 7

28 Study B: NN fit to world fixed target data Representative subset of world DVCS fixed target data: npt x obs collab harm. ref x ALUI HERMES -1. arxiv: x AUTDVCS HERMES arxiv: x AUTI HERMES 1. arxiv: x BCA HERMES. arxiv: x BCA HERMES 1. arxiv: x BSDw CLAS -1 arxiv: x BSDw HALLA -1 arxiv: x BSSw CLAS. arxiv: x BSSw CLAS 1. arxiv: x BSSw HALLA. arxiv: x BSSw HALLA 1. arxiv: x BTSA HERMES. arxiv:14.177v1 3 x TSA CLAS -1 arxiv:hep-ex/651 6 x TSA HERMES -1. arxiv:14.177v TOTAL = 18 We now use completely unconstrained neural nets representing Im H, Re H, Im E, Re E,... (do not assume dispersion relations) Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 3 / 7

29 Results (1/) Only Im H, Im H and Re E consistently extracted as different from zero, and, with somewhat smaller significance, Re H and Im E: 3 NN-fix-3L-ReE-ImHt NN-fix-4L-ImHt-ReH NN-fix-4L-ImHt-ImE t =. GeV NN-fix-3L-ReE-ImHt NN-fix-4L-ImHt-ReH NN-fix-4L-ImHt-ImE t =. GeV Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 4 / 7

30 Results (/) Other CFFs come out consistent with zero. Only bounds on their size are obtained. E. g. for Im Ẽ: 3 NN-fix-3L-ReE-ImHt NN-fix-4-ImHt-ImEt t =. GeV NN-fix-3L-ReE-ImHt NN-fix-4-ImHt-ImEt NN-fix-4-ImHt-ReHt t =. GeV Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 5 / 7

31 Summary Neural network method has a unique capability of extraction of Compton form factors (and, later, GPDs) with reliable uncertainties Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 6 / 7

32 GPD/CFF server Plots of all CFFs available; numerical values soon to come... Krešimir Kumerički Status of GPD extraction INT 18-3, Week 1 7 / 7

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