Deeply Virtual Compton Scattering at 11GeV with CLAS12

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Presentation transcript:

Deeply Virtual Compton Scattering at 11GeV with CLAS12 Franck Sabatié Saclay JLab PAC30 August 23rd Introduction Experiment E1-DVCS Characteristics of 11 GeV DVCS Experimental setup Analysis procedure Projected results for BSA and TSA e- p g

Deeply Virtual Compton Scattering at 11GeV with CLAS12 Two proposals bundled in one: DVCS Beam Spin Asymmetry 2. DVCS Target Spin Asymmetry

GPDs from Theory to Experiment x+x x-x t GPDs Handbag Diagram g* g 2. The GPDs enter the DVCS amplitude as an integral over x: GPDs appear in the real part through a PP integral over x GPDs appear in the imaginary part but at the line x=x Factorization theorem states: In the suitable asymptotic limit, the handbag diagram is the leading contribution to DVCS. Q2 and n large at xB and t fixed 1. Needs to be checked !!! Experiment g* g Physical process g* g but it’s not so simple… Collins, Freund

Experimental observables linked to GPDs 3. Experimentally, DVCS is indistinguishable with Bethe-Heitler However, we know FF at low t and BH is fully calculable Using a polarized beam on an unpolarized target or an unpolarized beam on a polarized target, one can access 2 observables: At JLab energies, |TDVCS|2 is small… maybe! Kroll, Guichon, Diehl, Pire, …

Into the harmonic structure of DVCS |TBH|2 Interference term e-’ j p e- g* hadronic plane leptonic plane g BH propagators j dependence Belitsky, Mueller, Kirchner

Analysis – Extraction of observables (BSA) Difference of cross-section for polarized beam on unpolarized target: GPD !!!

Analysis – Extraction of observables (TSA) Difference of cross-section for unpolarized beam on polarized target: Mostly sensitive to

Special case of the asymmetry Experimentally advantageous, the asymmetry can be written as: With limited statistics and to give rough estimates, one can consider that the denominator is dominated by c0BH. However, high precision experiment will need to take everything into account to extract twist-2 GPDs without model dependence. This is foreseen to be achieved using a global fit to parametrized GPDs, just like NLO fits to structure functions yield PDFs. X. Ji Workshop in October !

E1-DVCS data and analysis are promising ! Same experimental method as the proposed experiment BSA vs. j + more data in 2008 Analysis by F.X. Girod

EG1 data for TSA PRL 97, 072002 (2006) + more data in 2008

80 days unpolarized target, 120 days polarized target From 6 to 11 GeV ! Goal: To measure BSA, TSA and (beam)-helicity dependent cross-sections for the DVCS process in the full domain allowed by 11 GeV beam with statistical error bars similar or better than foreseen systematic errors: 80 days unpolarized target, 120 days polarized target Within a global analysis of world data including HERMES and Hall A Deep Exclusive data, the impact of JLab 11 GeV data will provide the strongest constraints to a model independent parametrization of GPDs (Mueller et al.). + increase in luminosity by a factor ~5 + improved acceptance

Experimental Setup and proposed experiments at 11 GeV Use of base CLAS12 equipment, including Inner Calorimeter (IC) Detection of the full (e,p,g) final state Perform 2 experiments for the extraction of the BSA and the TSA IC tungsten shielding Distance, target-IC: ~1.75m currently (note: this is NOT optimized for DVCS!)

Longitudinally polarized NH3 target Polarization: 85% Dilution factor: 1/6 Length: up to 100 mm Diameter: up to 30 mm Luminosity: up to 2x10^35 /cm2/s Pol. Meas.: NMR + physics

IC radiation study Current state of optimization of Tungsten shielding for IC Study by L. Elouadrhiri and A. Vlassov

IC radiation study E1-DVCS configuration [compatible with data study] CLAS12 configuration with IC shielding (Lumx10) 10^6 Hz 5.10^5 Hz The IC radiation is not worse with CLAS12 configuration than during E1-DVCS

IC block gain variation during E1-DVCS running Laser calibration method used to check relative gain stability Front View Slight gain decrease of blocks closest to the beam line.

Electron acceptance for DVCS Generated Events Generated Events Accepted Events Accepted Events Effect of solenoidal field Effect of solenoidal field

Proton acceptance for DVCS Generated Events Generated Events Accepted Events Accepted Events Central Detector

Photon acceptance for DVCS Generated Events Generated Events Accepted Events Accepted Events Inner Calorimeter

Selection of events - exclusivity Clean exclusive (e,p,g) final state is selected the usual way. The remaining contribution comes from p° electroproduction asymetric decays (only 1 photon detected), which can be reduced by performing cuts on Emiss and d, the angle between the expected and measured photons. EC+preshower EC+preshower IC IC Reduction in pion contamination by up to a factor 10 !

p° subtraction: removing the remaining contribution p0 subtraction relies on: Determination of 1-g to 2-g photon acceptance ratio from Monte-Carlo Measurement of p0 yield (2-g detected) and asymmetry [Method already used for analysis of EG1 data (PRL 97, 072002 (2006))] Study by. A. Biselli

Statistical error bar estimates – Arbitrary binning choice Events up to Q2=9.5 GeV2 The following graphs only represent this region. Events down to xB=0.1

Acceptance for DVCS events in (x,Q2,t) Enlarged IC would improve acceptance in this region 1 Good acceptance to (e,p,g): roughly between 0.1 and 0.35 overall

Beam Spin Asymmetry to 10% statistical error at high xB IC in standard position – 80 days – 10^35 Lum – VGG model From 1% statistical error on extracted Twist-2 coefficient to 10% statistical error at high xB

Target Spin Asymmetry Study by H. Egiyan IC in standard position – 120 days – 2x10^35 Lum – VGG model Study by H. Egiyan

Sensitivity to GPD models – sample of data points LU BSA <xB> =0.2 <Q2> = 3.3 GeV2 <-t> = 0.45 GeV2 <xB> =0.2 <Q2> = 3.3 GeV2 <Q2> =3.3 GeV2 <-t> = 0.45 GeV2 TSA <xB> =0.36 <Q2> = 4.1 GeV2 <-t> = 0.52 GeV2 <xB> =0.36 <Q2> = 4.1 GeV2 <Q2> =4.1 GeV2 <-t> = 0.52 GeV2

Systematic Errors (all relative) Source BSA Ds s Luminosity - 2% Pe determination p° contamination 1%-5% 3-8% Acceptance 3% 8% Radiative Corr. 1% Total 4%-7% 9%-10% 8%-12% Unpolarized Target Source TSA Nuclear Material 4% Pt determination 3% p° contamination 1%-5% Acceptance Accidentals 1% Radiative Corr. Total 6%-8% Polarized Target

Summary Deeply Virtual Compton Scattering remains the best understood tool in order to access GPDs at moderate energies. Beam and Target spin asymmetries will allow access to observables linked to GPDs (different kinds and combinations). Experimentally, the previous analyses have proven the feasibility of these type of experiments. The potential issue of radiation damage to the IC is under control with proper shielding. An essential aspect of the GPD study for 12 GeV is to collect a large statistical sample in order to give constraints on GPD parametrizations. Precision data is the key to the understanding of the nucleon structure with this study.