E e’ GPDs NN’ Deeply virtual Compton scattering on the nucleon at 6 and 11 GeV Silvia Niccolai...
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Transcript of E e’ GPDs NN’ Deeply virtual Compton scattering on the nucleon at 6 and 11 GeV Silvia Niccolai...
ee’
GPDsN N’
Deeply virtual Compton scattering on the nucleon at 6
and 11 GeV
Silvia Niccolai
Soutenance HDRIPN Orsay – November 27th 2014
p
p
n
N 'NGPDs
sud
Technical project: polarized target for electron scattering experiments at CLAS
Few-body interactions among nucleons:three-body photodisintegration of 3He at CLAS
Baryon spectroscopy: pentaquark searchin d(3He)→+(p) Phys. Rev. Lett. 97, 032001 (2006)
Nucleon structure: GPDsPAC proposal: DVCS with polarized target at CLAS
Nucleon structure: strange form factors → parity violationRadiative corrections for G0 (Hall C), forward anglesEur. Phys. J. A26, 429 (2005)
GENOVA
9/97-10/98
CV: Experimental hadronic physics at JLab (junior years)
1/99-2/03
3/03-9/03
10/03-9/06
Phys. Rev. C 70, 1 (2004)
CV: Structure of the nucleon at CLAS (senior years)
e1-dvcs experiment (2005):• cross sections for ep→e’p’0
→ sensitivity of this channel to transversity GPDs (chiral-odd)Phys. Rev. Lett. 109, 112001 (2012)Phys. Rev. C 90, 039901 (2014)
• 3 PhD theses at IPN: H.S. Jo (DVCS cross section) B. Moreno (DVCS asymmetry) A. Fradi (ep→e’n+ c. s.)
e1-dvcs2 experiment (2008):• 2 PhD theses: B. Guegan (DVCS c.s.) N. Saylor (DVCS c.s.)
e1-6 experiment (2001):• 1 PhD thesis, underway: B. Garillon (ep→e’p’f0 (f2) c.s.)
3 « encadrements de stagiaires »
Part 1: DVCS on longitudinally polarized
protons at 6 GeV
x
e e’
Xp
(Q2)
Electron-proton scattering: yesterday
e e’
p p’
(t=Q2)
1950: Elastic scattering ep→e’p’ (Hofstadter, Nobel prize 1961)
1967: Deep inelastic scattering (DIS) ep→e’X (Friedman, Kendall, Taylor, Nobel prize 1990)
• Discovery of the quarks (or “partons”)• Measurement of the momentum and spin distributions of the partons: q(x), q(x)
• The proton is not a point-like object• Measurement of charge and current distributions of the proton: form factors (F1(t), F2(t))
LowQ2
HighQ2
x
Electron-proton scattering: today
?Form factors:
transverse quark distribution in
coordinate space
Parton distributions:longitudinal
quark distributionin momentum space
F1(t), F2(t) q(x), (x)
x
Electron-proton scattering: today
GPDs: H, E, H, EFully correlated quark
distributions in both coordinate and momentum space
~ ~
Form factors: transverse quark distribution in
coordinate space
Accessible inhard exclusive processes
Parton distributions:longitudinal
quark distributionin momentum space
q(x), (x)F1(t), F2(t)
pNm
pNtxEpNpNtxH
pypedyP
pNm
ipNtxEpNpNtxH
pypedyP
N
yyqq
yixP
N
yyqq
yixP
2',,
~',,
~
)()0('2
,2
',,',,
)()0('2
55
0
5
0
Deeply Virtual Compton Scattering and GPDse’
t
(Q2)
e*
x+ξ x-ξ
H, H, E, E (x,ξ,t)~~
N(p) N(p’)
« Handbag » factorization validin the Bjorken regime:
high Q2 , (fixed xB), t<<Q2
• Q2= - (e-e’)2
• xB = Q2/2M=Ee-Ee’
• x+ξ, x-ξ longitudinal momentum fractions• t = 2 = (p-p’)2
• xB/(2-xB)
GPDs: Fourier transforms of non-local, non-diagonal QCD operators
P = (p+p’)/2
Light-cone: a± = (a0 ± a3 )/ √2
factorization
Deeply Virtual Compton Scattering and GPDs
Vector: H (x,ξ,t)
Tensor: E (x,ξ,t)
Axial-Vector: H (x,ξ,t)
Pseudoscalar: E (x,ξ,t)
~
~conserve nucleon spin
flip nucleon spin
At leading order QCD, twist 2, chiral-even (quark helicity is conserved), quark sector→ 4 GPDs for each quark flavor
Properties and “virtues” of GPDs
X. Ji, Phy.Rev.Lett.78,610(1997)
tGdxtxE
tGdxtxH
tFdxtxE
tFdxtxH
P
A
,,~
,,~
,,
,,
2
1
)()0,0,(~
)()0,0,(
xqxH
xqxH
Link with FFs Forward limit: PDFs
(not for E, E)~
Nucleon tomography
Nucleon spin: ½ = ½ + L + G JLJtxEtxHxdx 2
1))0,,()0,,((
2
1 1
1
Intrinsic spin of the quarks ≈ 25% Intrinsic spin on the gluons G ≈ 0 (??) Orbital angular
momentum of the quarks L ?
Quark angular momentum (Ji’s sum rule)
M. Burkardt, PRD 62, 71503 (2000)
),0,(~
)2()b,(
~
),0,()2(
)b,(
2b
02
2
2b
02
2
xHed
xH
xHed
xH
i
i
Accessing GPDs through DVCS
1
1
1
1
),,(),,(
~),,(
~ tGPDsidxx
txGPDsPdx
ix
txGPDsT DVCS
Only and tare accessible
experimentally
IDVCSBH
BHDVCSIA
BHDVCSI
TT BHDVCS
22
2
2
~
dxxx
txHtxHPRe qq
1
0
q
11),,(),,(
2
qe H
),,(),,(q tHtHIm qq 2qe H
DVCS allows access to 4 complex GPDs-related quantities:
Compton Form Factors (,t)
Im{Hn, En, En}
= xB/(2-xB) k=-t/4M2)
leptonic planehadronic
planeN’
e’
e
Unpolarized beam, longitudinal target:
sI1,UL ~ sinIm{F1H+(F1+F2)(H + xB/2E) –kF2 E+…}~ Im{Hp, Hp}
~
sI1,unp ~ sin Im{F1H + (F1+F2)H -kF2E}~
Polarized beam, unpolarized target: Im{Hp, Hp, Ep}~
Sensitivity to GPDs of DVCS spin observables
Polarized beam, longitudinal target:
cILP ~ (A+BcosRe{F1H+(F1+F2)(H + xB/2E)…}~ Re{Hp, Hp}
~
Im{Hn, Hn, En}
~
Proton Neutron
~
Re{Hn, En, En}~
Im{Hn}
~
cos)(
cos)(
cos)(
sin
,1,1,0,0
,1,1,0,0
,1,1,0,0
)(,1)(
Iunp
BHunp
Iunp
BHunp
ILP
BHLP
ILP
BHLP
LL
Iunp
BHunp
Iunp
BHunp
IULunp
ULLU
cccc
ccccA
cccc
sA
Unpolarized beam, transverse target:
UT ~ cossinsIm{k(F2H – F1E) +… } Im{Hp, Ep}
Twist 2
sI1,unp ~ sin Im{F1H + (F1+F2)H -kF2E}~
Polarized beam, unpolarized target: Im{Hp, Hp, Ep}~
= xB/(2-xB) k=-t/4M2)
leptonic planehadronic
planeN’
e’
e
Unpolarized beam, longitudinal target:
sI1,UL ~ sinIm{F1H+(F1+F2)(H + xB/2E) –kF2 E+…}~ Im{Hp, Hp}
~
Sensitivity to GPDs of DVCS spin observables
Polarized beam, longitudinal target:
cILP ~ (A+BcosRe{F1H+(F1+F2)(H + xB/2E)…}~ Re{Hp, Hp}
~
Im{Hn, Hn, En}
Proton Neutron
~
~
cos)(
cos)(
cos)(
sin
,1,1,0,0
,1,1,0,0
,1,1,0,0
)(,1)(
Iunp
BHunp
Iunp
BHunp
ILP
BHLP
ILP
BHLP
LL
Iunp
BHunp
Iunp
BHunp
IULunp
ULLU
cccc
ccccA
cccc
sA
Twist 2
DVCS experiments worldwide
Jefferson Lab(Halls A&B)
HERMES
COMPASS
The CLAS eg1-dvcs experiment ep→epγ→→
Analysis team composed of:E. Seder, U Connecticut (CEA Saclay)S. Pisano, INFNFRA. Biselli, Fairfield US. Niccolai
Also: ongoing BSA and TSA for nDVCS(D. Sokhan, Glasgow U)
• Target: longitudinally polarized NH3 (polarization ~80%)
• Experiment approved by PAC28 (2005) with A rating• Data taken from February to end of August 2009• Beam energy ~5.9 GeV• CLAS + IC to detect forward photons
IC (inner calorimeter): 424 lead-tungstate
crystals + APD readout(built at IPNO)
The eg1-dvcs polarized target
Dynamic Nuclear Polarization of NH3
• Free electrons (ṄH2 radicals) are implanted in crystalline beads of ammonia via electron radiation
• Radicals are polarized ( ~100%) at 5 T and 1 K (P=tanh(µB/kT) )
• Microwaves (140 Ghz) drive electron/proton spin-flip transitions and transfer polarization to protons
• Polarization is measured with NMR
Polarized ammonia
Carbon
Empty
Optics
bt
btepbtbt
FC
NBN )1( 0
NNPNNPP
NNPNNPA
ttb
ttLU
UTAttf
UL cNNPNNPD
NNNNA
LTAttbf
LL cNNPNNPPD
NNNNA
Experimental definition of the observablesb: beamt: targetFCbt: charge, from Faraday CupB0: relative 0 contaminationPt: target polarizationPb: beam polarizationDf: dilution factorcAUT, cAUL: transverse corrections
Beam-spin asymmetry
Target-spin asymmetry
Double-spin asymmetry
Im{Hp
}
For each 4-dimensional bin in (Q2, xB, -t,
Charge-normalized DVCS/BH yield
Im{Hp, Hp}~
Re{Hp, Hp}~
« Highlights » of the eg1-dvcs analysis• Selection of the ep final state: exclusivity cuts to reduce nuclear background and ep0→ep() contamination; different strategies to define the cuts for the IC and EC topologies
NH3, before cuts12C, before cuts
NH3, after cuts
12C, after cuts92.01)(
3
12
NH
Cf N
NcepD %10
)90(
0
A
B
Pt : measured during the experiment by NMR.NMR coils surrounded the target → more sensitive to polarization of its outer volume. Risk to overestimate Pt
« Highlights » of the eg1-dvcs analysis
• Extraction of PbPt
theotb A
APP exp
PbPt deduced from elastic BSA (ep→e’p’):
)(exp
NND
NNA
f
Atheo : known function of the kinematics and of the e.m. FFs
Pb measured during the experiment with Moller runs
%74%80 tt PP
Beam-spin asymmetryFit:LUsin/(1+cos) ( constrained: equal for the 3 asymmetries)
Beam-spin asymmetryLU ~ Im{Hp}
Fit:LUsin/(1+cos)
Beam-spin asymmetryLU ~ Im{Hp}
Fit:LUsin/(1+cos)
• VGG: Vanderhaegen, Guidal, Guichon• KMM12: Kumericki, Mueller, Murray• GK: Goloskokov, Kroll • GGL: Gonzalez., Goldstein, Liuti
Target-spin asymmetryUL ~ Im{Hp, Hp}
~Fit:ULsin/(1+cos)
E. Seder et al. arXiv:1410.6615 , submitted to PRL
Target-spin asymmetry
E. Seder et al. arXiv:1410.6615 , submitted to PRL
Fit:ULsin+B sin 2
Agreement with world dataImproved statistics x10 at low -tExtended kinematic coverage
E. Seder et al. arXiv:1410.6615 , submitted to PRL
CLAS: <Q2>= 2.4 (GeV/c)2, <xB>= 0.31HERMES: <Q2>= 2.459 (GeV/c)2, <xB>= 0.096CLAS2006: <Q2>= 1.82 (GeV/c)2, <xB>= 0.28
Target-spin asymmetry
E. Seder et al. arXiv:1410.6615 , submitted to PRLE. Seder et al. arXiv:1410.6615 , submitted to PRL
“This paper presents new data on Generalized Parton Distributions (GPDs) obtained through DVCS. The results obtained are by far (at least one order of magnitude) the most accurate and the most extensive to date on the target-spin asymmetry in DVCS. Together with earlier published data on beam-spin asymmetries they will significantly advance our knowledge about GPDs. As such, this work has indeed significant impact on the field of hadronic structure. The fact that insight in the 3D-structure of the nucleon is pushed forward by experiments and analyses today fully merits the attention of a broader audience than that served by the Physical Review journals, and I support the publication in Physical Review Letters.” PRL referee
Double-spin asymmetryFit:LL+LLcos/(1+cos)
Constant termdominated
by BH
LL~ Re{Hp, Hp}~Fit:LL+LLcos/(1+cos)
cos term small and dominated by BH
Double-spin asymmetry
Extraction of Compton Form Factors from DVCS observables
8 CFF
M. Guidal: Model-independent fit, at fixed Q2, xB and t of DVCS observables8 unknowns (the CFFs), non-linear problem, strong correlations Bounding the domain of variation of the CFFs with model (5xVGG) M. Guidal, Eur. Phys. J. A 37 (2008) 319
Extraction of CFF from DVCS TSA, BSA, DSA
[12] CLAS BSA (Girod et al.)[14] CLAS TSA (Chen et al.)
CFFs fitting code by M. Guidal
ImH has steeper t-slope than ImH : is axial charge more
“concentrated” than the electromagnetic charge?
~
Some sensitivity to ReH, ReEbut with big uncertainties
→ DSA at CLAS12
~~
Slope of ImH decreasing as xB increases: fast quarks
(valence) more concentrated in the nucleon’s center, slow quarks (sea) more spread out
Part 2:DVCS on the neutron at 11 GeV
JLab upgrade and CLAS12
CHL-2CHL-2
Add new hallAdd new hall
CLAS12
CLAS12
H1, ZEUS
Valence region
Sea/gluon region
Emax(A,B,C) = 11 GeV
CLAS12: high luminosity (1035 cm-2s-1) and large acceptance:• Charged particles, 5o<<135o • Photons: 2.5o<< 5o (Forward Tagger) 5o<<40° (E.m. Calorimeter)
12 GeV
Extensive experimental program for p-DVCS planned: • BSA, lTSA, tTSA (CLAS12)• Cross sections, Q2-scaling tests (Halls A and C)
(H,E)p(ξ, ξ, t) = 4/9 (H,E)u(ξ, ξ, t) + 1/9 (H,E)d(ξ, ξ, t)(H,E)n(ξ, ξ, t) = 1/9 (H,E)u(ξ, ξ, t) + 4/9 (H,E)d(ξ, ξ, t)
A combined analysis of DVCS observables on proton and neutron targets is necessary for the flavor separation of the GPDs
(H,E)u(ξ, ξ, t) = 9/15[4(H,E)p(ξ, ξ, t) – (H,E)n(ξ, ξ, t)](H,E)d(ξ, ξ, t) = 9/15[4(H,E)n(ξ, ξ, t) – (H,E)p(ξ, ξ, t)]
DVCS on the neutron: motivation
GPDs depend on the quark’s flavor: Proton and neutron GPDs are linear combinations of quarks GPDs
The BSA for nDVCS is sensitive to the GPD E, That is the least known and the least constrained of the
GPDs and that appears in Ji’s sum rule → Ju, Jd
We will intiate an experimental program at JLab on neutron DVCS at 11 GeV, by measuring the beam-spin asymmetry (BSA)
LU ~ sin Im{F1H + (F1+F2)H -kF2E}d~ Im{Hn, Hn, En}~
First nDVCS measurement: Hall A@6 GeV
deedneenpeepXeeD ),(),(),(),(
Subtraction of the contributions from the proton using H2 data convoluted with Fermi motion
“Impulse approximation” (no FSI)
Active nucleon identified via
MM(e
M. Mazouz et al., PRL 99 (2007) 242501
Model-dependent extraction of Ju et Jd
Q2 = 1.9 GeV2 xB = 0.36
Im(CIn) compatible with zero (→ too high xB?)
Big statistical and systematic uncertainties(mostly due to the H2 subtraction and 0 background)
S. Ahmad et al., PRD75 (2007) 094003
VGG, PRD60 (1999) 094017
= 60°xB = 0.17Q2 = 2 GeV2
t = -0.4 GeV2
The BSA for nDVCS:• is very sensitive to E• depends strongly on the kinematics→ a large acceptance is necessary → CLAS12
VGG model
Ju=.3, Jd=.1
Ju=.1, Jd=.1
Ju=.5, Jd=.1
Ju=.3, Jd=.3
Ju=.3, Jd=-.1
Ee = 11 GeV
BSA for nDVCS at 11 GeV: sensitivity to E
LU
Hall A
Central Detector
nDVCS@CLAS12: detector requirements
More than 80% of the neutrons have >40°→ Neutron detector in the CD
<pn> ~ 0.4 GeV/c <n> ~ 60°
ed→e’n(p)
Detected in forward CLAS12
Detected inEC, FT
Not detected
Detected in CND
In the hypothesis of absence of FSI:pμ
p = pμp’ → kinematics are complete
detecting e’, n (p,,),
pμe + pμ
n + pμp = pμ
e′ + pμn′ + pμ
p′ + pμ
Resolution on MM(en) studied with nDVCS event generator + electron and photon resolutions
obtained from CLAS12 FastMC+ design specs for Forward Tagger
→ dominated by photon resolutions
Resolution on MM(en) studied with nDVCS event generator + electron and photon resolutions
obtained from CLAS12 FastMC+ design specs for Forward Tagger
→ dominated by photon resolutions
The Central Neutron Detector (CND) must ensure:• good neutron/photon separation for 0.2<pn<1 GeV/c → ~150 ps time resolution (obtained from GEANT4 simulations)• momentum resolution below 10%• no stringent requirements for angular resolutions
CTOF can detect neutrons as well (3% efficiency)
Central Tracker (SVT+MM): charged-particles veto
• limited available space (~10 cm radially)
→ limited efficiency
→ no space for light guides in the forward direction (CTOF)
• strong magnetic field (~5 T) → problems for light readout
CND(IPNO)
CTOF
Central Tracker(Micromegas
SPhN)
CND: constraints and early R&D studies
~ 2 years of R&D (IPNO, INFN Genova et Frascati)Three kinds of magnetic-resistant photo-detectors tested
Silicon PMs: too small active surface→ Too few photons → too big Nt 1
APDs:• Too noisy• t ~ 1.5 ns
Micro-channel-plate PMs:• Good resolution t ~ 100 ps• Loss of gain in magnetic field B ~ 1T• Short life time due to radiation damage
Chosen design for the CND
CND design: scintillator barrel3 radial layers, 48 bars per layer
coupled two-by-two by “u-turn” lightguides, light read upstream by
PMTs connected to the bar via 1.5m-long light guides
• Plastic scintillator: compromise between neutron efficiency (~1% /cm) and fast response
• Photon-neutron separation → measurement of β via Time-Of-Flight
cTOF
l
22 hzl
TOF: time from the interaction vertex to the impact point; l: path lenght + PID (m) → momentum
z: hit position along the scintillator bar; h: radial distance of the hit from the vertex → requires radial segmentation
rightlefteff ttvz 2
1 veff : light velocity in the scintillator bar; tleft,right: time measured at the two ends of the bar→ double readoutz → θ
nDVCS@CLAS12 & CND history• Simulations and R&D for detector conception started in 2008 (summer student project…)
• LOI for nDVCS@CLAS12 endorsed by PAC34 (2009)
• Proposal for nDVCS@CLAS12 approved by PAC37 and rated (A) by PAC38 (2011)
• CND project presented at Conseil Scientifique of IN2P3, obtained 300 k€ (fall 2011)
• Partial support also received from the HP3 program of the European 7th Framework
• JLab review of the CND in February 2012
• R&D and choice of all components finalized the same year
• Completion of purchase of all detector components by end of 2013
• Construction started in December 2013, almost complete!
PMT-N
PMT-D
GEANT4 simulations used to evaluate: efficiency PID (neutron/photon separation) momentum and angular resolutions definition of reconstruction algorithms background studiesMeasured t and light loss due to u-turn implemented in the simulation
CND: expected performances
Efficiency ~ 8-9% for a threshold of 3 MeV, TOF<8 nsand pn = 0.2 - 1 GeV/c
pn=0.4 GeV/c
Beam-time requested and obtained: 90 days (80 of production data taking at L = 1035 cm−2s−1/nucleon)• CLAS12 + Forward Calorimeter + Central Neutron Detector (efficiency ~10%)• 85% polarized electron beam• liquid deuterium target
nDVCS: expected accuracy and coverage
ed→ e(p)n
-t0 1.2
BSA
-0.2
0.2
Relative error on the yield: N/N~0.05%-10%
Estimated systematicuncertainties: 8%
Ju=.3, Jd=.1Ju=.1, Jd=.1
Ju=.3, Jd=.3Ju=.3, Jd=-.1
Model predictions (VGG)for different values of
quarks’ angular momentum
JLab PAC: high-impact experiment
E12-11-003
Determination of the detector components
Goal: optimize the time resolution ↔ neutron/photon discrimination
• Components chosen via comparative tests in cosmic rays on prototypes, checking light yield and σt (and costs…)
• Measured σt fed to simulation to verify PID requirements
Shielding PMT Wrapping Scintillator Glue U-turn
- 2.5 mm - R2083 - Mylar Al - BC408 - MBOND 200 - Triangular
- 5 mm - 9954A - VM2000 - EJ200 - BC600 - Semicircular
- R9779 - Al foil
- R10533
Tests on the one-layer prototype
One-layer prototype used to determine:• Wrapping material• PMT• Scintillator
Direct PMT
Trigger detectors
Indirect PMT
Ind PMT
Dir PMTR2083
R9779
(EJ200 scintillator, semicircular U-turn, Al foil wrapping)
• R2083 gives the best σt but is very expensive
• R9779 σt is ~10% worse but a factor 3 less expensive
)( 22)(
2)()2(1)2(1 scSizetriggerTtriggerT
Shape of u-turn (semicircular) was chosen using a preliminary setup (without long light guides)
Ind PMT
Dir PMTR2083
R9779
(EJ200 scintillator, semicircular U-turn, Al foil wrapping)
PMTs choice: test and simulation
Photons: R2083 R9779Neutrons: R2083 R9779
Gemc simulation of the CND:• measured t used to smear timing• vs p for photons and neutrons• Error bars represent 3• R9779 still meets requirements
Final choice R10533: same price and time performances of R9779, higher gain – no amplifier needed
Tests on three-layer prototype confirmed all choices of components
+ choice of CFDs and splitters
• R2083 gives the best σt but is very expensive
• R9779 σt is ~10% worse but a factor 3 less expensive
45°
<B>=230 G @ PMTsRelative angle B-PMT~70°
Final choice is 5 mm of mild-steel shielding
Magnetic field values
without shielding
Magnetic probe
Position of photocathode
Mild steel
µ-metal
Magnetic field tests (LAL, Orsay)
JLab field simulations confirm the B~0 inside our
5mm shieldings
60°ProbeShielding
Magnet
Also done tests checking PMT signal amplitude vs field angle
Detector construction: gluing
U-turn: yes, it works!
144 scintillators, 144 long light guides, 72 u-turn light guides, 144 « fish-tail » guides, 144 « connection » guides
Gluing started in December 2013Polishing before gluing
The gluing room at IPN OrsayFish-tail guide
Detector construction: wrapping
Wrapping:Al foilBlack tape
Measurement of the thickness to verify clearance requirements
One layer is completed
Detector construction and testing
One block of the CND:end of the light guides
Connecting the guideto the shielded PMT
All PMT bases are ready and mounted
One block of the CND in the cosmic-raystest room
Direct light
Indirect light
U turn drop
TOP layer
MIDDLE layer
BOTTOM layer
Raw data: TDC vs ADC
Characterization of the blocksOne week of data taking to characterize each block, right after assembly (same 6 PMTs used):
• Light collection• Effective light velocity in scintillator+light guides• Light attenuation • Time resolution
E.S. Smith et al. NIM A 432 (1999) 265-298Measurement of time resolution with cosmic rays (following the method described by R.T. Giles et al. NIM A 252 (1986) 41-52)
SPMT PMTAPMT PMT
BPMT PMT
Time resolution with cosmic rays, trigger from triple coincidence
Support structure and installation tests
6 stainless steel brackets
6 aluminum arches
Mock up of the solenoid
Mock up of the solenoid support ring
21 blocks constructed: only 3 more to go! Shipping to JLab in April ‘15
We arrived at this stage thanks to (alphabetic order): Julien Bettane, Jean-Luc Cercus, Brice Garillon, Giulia Hull, Miktat Imre, Michael Josselin, Alain Maroni, Gilles Minier, Thi Nguen-Trung, Joel Pouthas, Daria Sokhan, Claude Thèneau.
Conclusions and outlook GPDs are a unique tool to explore the internal landscape of the nucleon:
• 3D quark/gluon imaging of the nucleon• orbital angular momentum carried by quarks
Their extraction from experimental data is very difficult: • there are 4 GPDs for each quark flavor• they depend on 3 variables, only two (, t) experimentally accessible• they appear as integrals in cross sections
Recently-developed fitting methods allow to extract CFFs from DVCS observables•We need to measure several p-DVCS and n-DVCS observables over a wide phase space
Our new measurement of 3 spin observables for p-DVCS allows the extraction of ImHp and ImHp → spatial distribution of electric and axial charge in the proton
The 12-GeV-upgraded JLab will be the only facility to perform DVCS experiments in the valence region, for Q2 up to 11 GeV:
• DVCS experiments on both proton (L/T polarized and unpolarized) and deuteron targets are planned for 3 of the 4 Halls at JLab@12 GeV
• The CND is ready to go! nDVCS@CLAS12 experiment foreseen for the year 2018
• Work ongoing on PAC proposal for nDVCS with a longitudinally-polarized target (TSA and DSA): sensitivity to ImHn and ReHn → flavor separation!
~