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Overview of JLab Nuclear Program • General Introduction: Why ?

• 10+ years of JLab Experiments: Highlights •The Role of in Nuclear Physics CEBAF‟s Original Mission Statement

and Elastic Form Factors and Transition Form Factors to Nucleon Excited States

• The Strange Content of the

• The Onset of the Quark Parton Model: The Quark- Transition

• Deep Exclusive Reactions: Constraints on Angular Momentum Proton Tomography Cool Facts about QCD and Nuclei Did you know that … ? • If an was the size of a football field, the (atomic) nucleus would be about the size of a marble. • Despite its tiny dimensions, the nucleus accounts for 99.9% of an atom‟s mass. • and swirl in a heavy with speeds of up to some ¾ of c. More commonly, their speed is some ¼ the speed of . The reason is because they are “strong-forced” to reside in a small space. • Quarks (and ) are “confined” to the even smaller space inside protons and neutrons. Because of this, they swirl around with the speed of light. Cool Facts about QCD and Nuclei Did you know that … ? • The strong force is so strong, that you can never find one quark alone (this is called “confinement”). •When pried even a little apart, quarks experience ten tons of force pulling them together again. • Quarks and gluons jiggle around at nearly light- speed, and extra gluons and quark/anti-quark pairs pop into existence one moment to disappear the next. • It is this flurry of activity, fueled by the of the gluons, that generates nearly all the mass of protons and neutrons, and thus ultimately of all the we see. • 99% of your mass is due to this stored energy. • Even the QCD “vacuum” is not truly empty. Long-distance gluonic fluctuations are an integral part. Quarks have small mass themselves, but attain an effective larger mass due to the fact that they attract these gluonic fluctuations around them  M(up) + M(up) + M(down) ~ 10 MeV << M(proton) Cool Facts about QCD and Nuclei Did you know that … ? • Nuclear are trying to answer how basic properties like mass, shape, and come about from the flood of gluons, quark/anti-quark pairs, and a few ever- present quarks • A small fraction of the force between quarks and gluons “leaks out” of protons and neutrons, and binds them together to form tiny nuclei. The long-range part of this process can be well described as if protons and neutrons exchange . • Nuclear physicists are only now starting to understand how this “leakage” occurs, and how it results in the impressive variety of nuclei found in nature. • A nucleus consisting of some 100 protons and 150 neutrons can be the same size as one with 3 protons and 8 neutrons. Elementary

• Protons , neutrons and (p,n,e) build all the . • Proton and neutrons make up 99.9% of the visible mass in the universe. • Dozens of new particles were discovered in the past century. • : strength can be 100 times the electromagnetic one (e,m,n,..): not involved in strong interaction [(p,K,…) and (p,n,…)]: involved in strong interaction

Quarks & Gluons: QCD QCD and Nuclei

Gluons mediate the strong (color) force, just like mediate the electromagnetic force, but … gluons interact with themselves … which gives QCD unique properties

QCD Lagrangian: quarks and gluons Nuclear Physics Model is an effective (but highly successful!) model using free and mesons as degrees of freedom. The Structure of the Proton Naïve : proton = uud (valence quarks) QCD proton = uud + uu + dd + ss + …

The proton is far more than just its up + up + down (valence) quark structure QCD and the Origin of Mass

 99% of the proton‟s mass/energy is due to the self-generating field – Higgs mechanism has almost no role here.

 The similarity of mass between the proton and arises from the fact that the gluon dynamics are the same – Quarks contribute almost nothing. Electron Scattering

Electrons as probe of have some distinct advantages over other probes like hadrons or g-rays: • The interaction between the electron and the nucleus is known; it is the electromagnetic interaction with the charge r and the current J of the nucleus: Vint = rf + J.A, where f and A are the scalar and vector potentials generated by the electron. • The interaction is weak, so that in almost all cases it can be treated in the “one- exchange approximation” (OPEA), i.e., two-step processes (two- photon exchange) are small. The exception is charge of the Coulomb field of a heavy-Z nucleus. • The energy (w) and linear momentum (q) transferred to the nucleus in the scattering process can be varied independently from each other. This is very important, as for a certain |q| one effectively measures a Fourier component of r or J. By varying |q| all Fourier components can be determined and from these the radial dependence of r and J can be reconstructed. • Because the photon has no charge, only the J.A interaction plays a role, leading to magnetic Ml and electric El transitions. In electron scattering, one can also have charge Cl transitions. Electron Scattering Electron scattering has also some disadvantages:

• The interaction is weak, so cross sections are small, but one can use high electron beam currents and thick targets.

• Neutrons are less accessible than protons, since they do not have a net electric charge.

• Because electrons are very light particles, they easily emit (so- called Bremsstrahlung). This gives rise to radiative tails, with often large corrections for these processes. k’ = (E’,k’) Kinematics k = (E,k) Q Virtual photon  off-mass shell m 2 2 qmq = n – q = 0 q = (n,q) Define two invariants: 2 m m m 1) Q = -qmq = -(km – km’)(k -k’ ) 2 m = -2me + 2kmk’ m (me ~ 0) = 2kmk’ (LAB) = 2(EE’ – k.k’) p = (M,0) = 2EE’(1-cos(Q)) = 4EE’sin2(Q/2) Undetected 2 only assumption: neglecting me !! final state X 2) 2M = 2p qm = Q2 + W2 – M2 p’ = (sqrt(p‟2 + M‟2),p’) n m

( p‟2 = M‟2 = W2) !! Elastic scattering  W2 = M2  Q2 = 2M(E-E‟) Electron Scattering at Fixed Q2 d 2σ Elastic Quark dωd (fictitious)

w

Proton Elastic  Deep Inelastic N*

Q 2 Q2  300 MeV w 2m 2m Electron Scattering at Fixed Q2

d 2σ Elastic Nucleus Deep dωd  Inelastic Quasielastic N*

Q 2 Q 2 Q2  300 MeV w 2M 2m 2m

Proton Elastic  Deep Inelastic N*

w Extracting the (e,e’)

-2 NN (cm ) e' Ne

e (e, pe)

Scattering probability or cross section

d3σ Counts  dedpe Ne N N epe Electron-Charge Scattering

Form Factors characterize internal structure of particles History - Charge Distributions

In „70s large data set was acquired on elastic electron scattering (mainly from Saclay) over large Q2-range and for variety of nuclei “Model-independent” analysis provided accurate results on charge distribution well described by mean-field Density-Dependent Hartree-Fock calculations History - Proton Knock-out

pm  Ee  Ee '  p  q  p E  wn  T  T  E  E m p A 1 sep e xc in binding

Visualizing the

in momentum

Missing 20+% in the integral???

 Deep 2

=

In the limit of large Q2, structure functions scale (with logarithmic corrections) MW (ν,Q2 )  F (x) Q2 1 1 x  (Infinite Momentum Frame) 2 νW1(ν,Q )  F2 (x) 2Mν

F2 interpreted in the quark-parton model as the 2 charge-weighted sum over quark distributions: F2 (x)  ei xqi (x) i Empirically, DIS region is where 2 2 2 2 logarithmic scaling is observed Q > 1 GeV , W > 4 GeV Parton Distribution Functions (PDFs) PDF q(x): probability that a quark (or gluon) has fraction x of proton‟s momentum

proton: uud + uū + dđ + … CEBAF’s Original Mission Statement

Key Mission and Principal Focus (1987): The study of the largely unexplored transition between the nucleon- and the quark-gluon descriptions of . The Role of Quarks in Nuclear Physics

Related Areas of Study: • Do individual nucleons change their size, shape, and quark structure in the nuclear medium?

• How do nucleons cluster in the nuclear medium? Pushing the Limits of the of Nuclear Physics

• What are the properties of the force which binds quarks into nucleons and nuclei at distances where this force is strong and the quark confinement mechanism is important? Charge and Magnetization in Nucleons and Pions The Onset of the Parton Model JLab accelerator CEBAF Continuous Electron Beam • Energy 0.4 ─ 6.0 GeV • 200 mA, polarization 85% • 3 x 499 MHz operation • Simultaneous delivery 3 halls

A B C Halls A/B/C Base Equipment

Hall A (2 HRS)

Hall C (SOS/HMS) Hall B (CLAS) Hall B - CLAS (forward carriage and side clamshells retracted)

CLAS has more than 38,000 readout channels Large angle EC

Panel 2 & 3TOF Panel 4 TOF

Panel 1 TOF

Region 3 drift chamber Cerenkov & Forward angle EC

CLAS Overview, B. Mecking & staff, collaborators, NIM A503 (2003) 513 Ancillary Equipment and Experiment-Specific Apparatus

2006 2002-2007

n GE Electron Channel Setup G0 Setup

2004 2005 2005

DVCS Proton Array BONUS RTPC Detector ENGE/HKS Setup CEBAF’s Original Mission Statement

Key Mission and Principal Focus (1987): The study of the largely unexplored transition between the nucleon-meson and the quark-gluon descriptions of nuclear matter. The Role of Quarks in Nuclear Physics

Related Areas of Study: • Do individual nucleons change their size, shape, and quark structure in the nuclear medium?

• How do nucleons cluster in the nuclear medium? Pushing the Limits of the Standard Model of Nuclear Physics

• What are the properties of the force which binds quarks into nucleons and nuclei at distances where this force is strong and the quark confinement mechanism is important? Charge and Magnetization in Nucleons and Pions The Onset of the Parton Model 2H(e,e)2H elastic scattering 2H: spin-1  3 form factors to disentangle Solution: measure tensor polarization in 2H(e,e‟d)

“T20 experiment” used HMS to detect the scattered electrons and a dedicated magnetic spectrometer on the

floor to detect the recoiling deuteron and measure it‟s tensor 1st large installation experiment: 1997 polarization JLab Data Reveal Deuteron’s Size and Shape

Hall A

Combined Data -> Deuteron‟s Intrinsic Shape

The nucleon-based description works down to < 0.5 fm Is there a Limit for Meson-Baryon Models? Not really but …

… there might be a more economical QCD description. Scaling behavior (d/dt  s-11) quark-gluon description sets for PT > 1.2 GeV/c (see ) in at scales below ~0.1 fm? CEBAF’s Original Mission Statement

Key Mission and Principal Focus (1987): The study of the largely unexplored transition between the nucleon-meson and the quark-gluon descriptions of nuclear matter. The Role of Quarks in Nuclear Physics

Related Areas of Study: • Do individual nucleons change their size, shape, and quark structure in the nuclear medium?

• How do nucleons cluster in the nuclear medium? Pushing the Limits of the Standard Model of Nuclear Physics

• What are the properties of the force which binds quarks into nucleons and nuclei at distances where this force is strong and the quark confinement mechanism is important? Charge and Magnetization in Nucleons and Pions The Onset of the Parton Model Quarks in Nuclei - History: the EMC Effect

• Observation that structure functions are altered in nuclei stunned much of the HEP community 23 years ago • ~1000 papers on the topic; the best models explain the curve by change of nucleon structure, BUT more data are needed to uniquely identify the origin What is it that alters the quark momentum in the nucleus?

J. Ashman et al., Z. A Phys. C57, 211 (1993) F2 D J. Gomez et al., Phys. F2 Rev. D49, 4348 (1994)

x Polarization transfer in 4He(e,e’p)3H • E93-049 (Hall A): Measured 4He(e,e‟p)3H in quasi-elastic kinematics for Q2 = 0.5, 1.0, 1.6 and 2.6 (GeV/c)2 using Focal Plane Polarimeter 4 1 • Extracted “Superratio”: (P‟x/P‟z) in He/(P‟x/P‟z) in H At nuclear matter densities of 0.17 nucleons/fm3, nucleon wave functions overlap considerably. RPWIA RDWIA +QMC

Medium Modifications of Nucleon Form Factor? • Compared to calculations by Udias without and with inclusion of medium effects predicted by Thomas et al. (Quark Meson Coupling model). EMC Effect in very light nuclei EMC effect scales with average nuclear density if we ignore Be ? Be = 2 a clusters (4He nuclei) + “extra” neutron

Suggests EMC effect depends on local nuclear environment

dR/dx = slope of line fit to A/D ratio over region x=0.3 to 0.7

Nuclear density extracted from ab initio GFMC calculation – scaled by (A-1)/A to remove contribution to density from “struck” nucleon

C. Seely, A. Daniel, et al, PRL 103, 202301 (2009) CEBAF’s Original Mission Statement

Key Mission and Principal Focus (1987): The study of the largely unexplored transition between the nucleon-meson and the quark-gluon descriptions of nuclear matter. The Role of Quarks in Nuclear Physics

Related Areas of Study: • Do individual nucleons change their size, shape, and quark structure in the nuclear medium?

• How do nucleons cluster in the nuclear medium? Pushing the Limits of the Standard Model of Nuclear Physics

• What are the properties of the force which binds quarks into nucleons and nuclei at distances where this force is strong and the quark confinement mechanism is important? The Onset of the Parton Model Use the Nuclear Arena to Study QCD Proton Momenta in the nucleus

Similar shapes for few- body nuclei and nuclear matter at high k (=pm).

Nuclear Matter

Short-range repulsive core gives rise to high proton momenta 2H 3He p n 4He

0 200 400 600 800 1000 P (MeV/c) Hall B Short Range Correlations in Nuclei CLAS

3 4 12 56 K. Egiyan, et al, (CLAS), PRC 68:014313,2003; A(e,e‟)X, A = He, He, C, Fe PRL 96, 082501,2006.

Measured Composition ( %)

1N state 2N SRC 3N SRC 2H 96 0.7 4.0 0.7 --- 3He 92 ± 1.6 8.0 1.6 0.18 ± 0.06 4He 86 3.3 15.4 ± 3.3 0.42 ± 0.14 12C 80 ± 4.1 19.3 ± 4.1 0.55 ± 0.18 56Fe 76 ± 4.7 23.0 ± 4.7 0.79 ± 0.25

Q2/2Mn Hall A Short Range Correlations in Nuclei

CLAS  two-nucleon correlations contributed ~20% to the 12C wave function. Hall A  two nucleons close together are almost always a p-n pair. Proton-neutron rate is ~20 x the proton-proton rate. Expected to be due to short-range tensor correlations.

calculation CEBAF’s Original Mission Statement

Key Mission and Principal Focus (1987): The study of the largely unexplored transition between the nucleon-meson and the quark-gluon descriptions of nuclear matter. The Role of Quarks in Nuclear Physics

Related Areas of Study: • Do individual nucleons change their size, shape, and quark structure in the nuclear medium?

• How do nucleons cluster in the nuclear medium? Pushing the Limits of the Standard Model of Nuclear Physics

• What are the properties of the force which binds quarks into nucleons and nuclei at distances where this force is strong and the quark confinement mechanism is important? Charge and Magnetization in Nucleons and Pions The Onset of the Parton Model Revolutionized Polarized Beam Experiments! Precise access to (small) charge form factor of proton utilizing polarization transfer technique: e + p  e‟ + p Focal Plane Polarimeter

G P‟ (E + E ) Q __E = - __x _____i f tan __e GM P‟z 2m 2

No error contributions from • analyzing power • beam polarimetry Polarization Measurement

Spin-dependent scattering Focal-Plane Polarimeter

r r r r l  s  0 l  s  0

 

Observed angular distribution Proton charge and magnetism in 2006

2-g exchange Hall A important

1) e + p  e‟ + p G p/G p constant E M smaller distance  2) e + p  e‟ + p p p 2 GE /GM drops with Q charge depletion in interior of proton Orbital motion of quarks play a key role (Belitsky, Ji + Yuan PRL 91 (2003) 092003) Hall A What about the neutron? Neutron has no charge, but does have a charge distributions: n = p + p-, n = ddu. charge and magnetization density Use polarization and 2H(e,e‟n) to access. “Guarantee” that electron hits a neutron AND electron transfers its polarization to this neutron.

(Polarization Experiments only)

Combining proton and neutron: J. J. Kelly, PRC 66 (2002) 065203 has wider distribution. Why? Pion’s charge distribution • At low Q2 (< 0.3 (GeV/c)2): use p + e 2 -2 scattering  Rrms = 0.66 fm • In asymptotic region, Fp  8pas ƒp Q • At higher Q2: use 1H(e,e‟p+)n

• Use a realistic pion electroproduction (Regge-type) model to extract Fp

T. Horn et al., nucl-ex/0607005 V. Tadevosyan, et al., nucl-ex/0607007 First measurements away from region where Fp is simply given by the p radius Hall B Electron Scattering CLAS

p(e,e‟)X p(e,e‟p)X

2

2p thresh.

1.5

1

 Resonances cannot be uniquely separated in inclusive scattering → measure exclusive processes. The gN(1232) Quadrupole Transition

SU(6): E1+=S1+=0 * Hall B Transition amplitudes g p → N3/2+ (1232) CLAS (The N- Transition)

. R = E /M remains small EM 1+ 1+ 1 and negative at –2% to -3% GD = 2 2 from 0 ≤ Q2 ≤ 6 GeV2. (1 + Q /0.71)

. No trend towards sign change and towards asymptotic 2 * behavior. Helicity conservation  At high Q G M requires REM → +100(%). continues to drop faster than the elastic . RSM = S1+/M1+ remains magnetic proton form negative andHall Ccontinues 1999 to increase inCLAS magnitude. 2002 No trend factor. towards asymptoticCLAS 2006 behavior. Helicity conservation requires

RSM → constant. N(1440)P11 helicity amplitudes in 2010 The elusive Roper resonance Nπ Hall B Nππ Nπ, Nππ

LCQM CLAS Q3G

. First sign change of a nucleon form factor. Seen in both the Nπ and Nππ electro-production analysis. . At large Q2 consistent with radial excitation of the nucleon in LCQM. . Excludes hybrid assignment for the state.

I. Aznauryan et al (CLAS), Phys.Rev.C80:055203,2009 I. Aznauryan et al (CLAS), Phys.Rev.C78:045209,2008 The proton’s magnetic moment

Nobel Prize, 1943: "for his contribution to the development of the molecular ray method and his discovery of the magnetic moment of the proton"

mp = 2.5 nuclear magnetons, 10% (1933)

Otto Stern 2002 experiment: mp = 2.792847351(28) mN mn = -1.91304274(45) mN

2006 theory: How do the quark contributions add up? mp ~ 2.8 mN m m n ~ -1.8 N How are charge and magnetism distributed? JLab: Polarized Electrons!!!

Electron retains circular polarization of laser beam

Reverse polarization of beam at rate of 30 Hz

Feedback on laser intensity and position at high rate Hall A Parity Violating Studies on 1H and 4He

The HAPPEx Program: Contributions to the Proton

Open circles: online data Closed circles: final data e JLab polarized beam e G0 forward running beam: HAPPEX-II beam (2005):

• strained GaAs (PB ~ 73%) • superlattice (PB > 85%) • 32 ns pulse spacing • 2 ns pulse spacing • 40 mA beam current • 35 mA beam current

Beam Parameter G0 beam (Hall C) HAPPEx beam (Hall A) Charge -0.14 0.32 ppm -2.6 0.15 ppm

Position difference 4 4 nm -8 3 nm

angle difference 1.5 1 nrad 4 2 nrad

Energy difference 29 4 eV 66 3 eV

Total correction to -0.02 0.01 ppm 0.08 0.03 ppm Asymmetry The spatial distribution of quarks and the proton’s magnetism Hall A p 2 2 u 2 1 d 2 1 s 2 GM (Q )  3 GM (Q )  3 GM (Q )  3 GM (Q ) proton charge/magnetism up neutron charge/magnetism down proton response to Weak force strange ~ 5% 1st Separation using G0, HAPPEx-II & HAPPEx-He, and A4 & SAMPLE data

smaller distance  CEBAF’s Original Mission Statement

Key Mission and Principal Focus (1987): The study of the largely unexplored transition between the nucleon-meson and the quark-gluon descriptions of nuclear matter. The Role of Quarks in Nuclear Physics

Related Areas of Study: • Do individual nucleons change their size, shape, and quark structure in the nuclear medium?

• How do nucleons cluster in the nuclear medium? Pushing the Limits of the Standard Model of Nuclear Physics

• What are the properties of the force which binds quarks into nucleons and nuclei at distances where this force is strong and the quark confinement mechanism is important? Charge and Magnetization in Nucleons and Pions The Onset of the Parton Model The Double-Faced Strong Force

Confinement Constituent Asymptotically Nucleons Quarks Free Quarks Q < L Q > L Q >> L as(Q) > 1 as(Q) large as(Q) small

One parameter, LQCD, ~ Mass Scale or q Inverse Distance Scale where as(Q) =  g “Separates” Confinement q and Perturbative Regions

Mass and Radius of the Proton are (almost) completely governed by

LQCD0.213 GeV

Quark Model Quark Parton Model Nuclear Physics in terms of protons, neutrons and pion exchange is a very good effective model. Momentum transfer Q is negligible

Protons and Neutrons in terms of constituent (valence) quarks is a very decent effective model: the Constituent Quark Model works surprisingly well. Momentum transfer Q is small

Looking deep inside protons and neutrons, they are really balls of energy, with lots of gluons and quark-antiquark pairs popping in and out of existence. Momentum transfer Q is “large” Hall B Electron Scattering CLAS p(e,e‟)X

(GE, GM)

(1620)

(1232)

N(1680)

N(1440)

N(1535) N(1520)

Map “Quark-Hadron Transition” in electron-proton scattering (From Resonance to Deep Inelastic Region / From Quark Model to Parton Model) E94-110 : Separated Structure Functions

Duality works well for F2, 2xF1 (FT), and FL . The resonance region is, on average, well described by NNLO QCD fits. .

2 This implies that Higher-Twist (FSI)

F contributions cancel, and are on average small. “Quark-Hadron Duality” . The result is a smooth transition from Quark Model Excitations to a Parton Model description, or a smooth

1 quark-hadron transition. . This explains the success of the

2xF parton model at relatively low W2 (=4 GeV2) and Q2 (=1 GeV2).

“The successful application of duality to extract known quantities suggests

L that it should also be possible to use F it to extract quantities that are otherwise kinematically inaccessible.” (CERN Courier, December 2004) Quantification: Resonance Region F2 w.r.t. Alekhin NNLO Scaling Curve

• Evidence of resonance (Q2 ~ 1.5 GeV2) transitions is “bumps and valleys” around the expected parton model behavior. • Similar as standard textbook example of e+e-  hadrons

• “Resonances build the parton subprocess cross section because of a separation of “typical” scales between hard  = -0.1 +/- 0.7% and soft processes.” example • Confinement is Local Parton Model Ideas Valid @ 6 GeV Hall A

First measurement in large-x region Allows for Flavor Decomposition: n unambiguously showing that A1 > 0 n n (A1 = 0 in the SU(6) Quark Model) A1 in Parton Model ~

x = fraction of nucleon momentum carried by struck quark 2 Structure function g1 and its G1(Q ) Moment e + p e + X As Q2  , symmetry and G1p current algebra to the Bjorken sum rule, relating the n-p difference to the neutron b-decay coupling constant gA p n G1 – G1 = gA/6 hadron parton As Q2 0, Lorentz invariance, unitarity, and dispersion relations lead to the GDH sum rule, relating it to the anomalous magnetic moment of the nucleon Q2 G1 IGDH Q2  2M2 G Expect rapid change of 1 in “Zoom in” from tiny lenght scales transition from the hadronic (DIS) to large length scales to the partonic regimes. p-n Bjorken Integral G1 (pre-JLab)

Impressive set of data at larger Q2 (not shown) validates Bjorken Sum Rule to ~10-15%. p-n Bjorken Integral G1 (today)

Hall B Hall A

. Operator Product Expansion description works surprisingly well for Q2 > 0.7 GeV2.

. HBcPT compatible for Q2 < 0.2 GeV2 The Spin Structure of the Proton

Proton helicity sum rule:

½ = ½ S + G + Lq + Lg

~ 0.3

Small?

? Large ?

The Impact of Quark and Gluon Motion on the Nucleon Spin

“TMDs and GPDs” Towards a “3D” spin- u (Wigner Function) flavor landscape W (x,k,r)

m m

p p TMD x GPD B

Transverse- u Link to TMD (x,k ) Momentum T GPDu(x,x,t) GeneralizedLink to DependentOrbital OrbitalParton f1,g1,f1T ,g1T ~ ~ MomentumParton Hu, Eu, Hu, Eu MomentumDistributions

Distributions h1, h1T ,h1L ,h1 d

Want PT > dx 2

L but not k too large! T

u f1(x) u(x) F1 (t) u u u g1, h1 u, du F2 ,GA ,GP Parton Distributions Form Factors Beyond form factors and quark distributions – Generalized Parton Distributions (GPDs) X. Ji, D. Mueller, A. Radyushkin (1994-1997)

Proton form Structure functions, factors, transverse quark longitudinal charge & current Correlated quark momentum momentum & helicity densities and helicity distributions in distributions transverse space - GPDs Extend longitudinal quark momentum & helicity distributions 2000‟s to transverse momentum distributions - TMDs What’s the use of GPDs? 1. Allows for a unified description of form factors and parton distributions

2. Describe correlations of quarks/gluons 3. Allows for Transverse Imaging Fourier transform in momentum transfer

x < 0.1 x ~ 0.3 x ~ 0.8 gives transverse spatial distribution of quark (parton) with momentum fraction x 4. Allows access to quark angular momentum (in model-dependent way) Beyond form factors and quark distributions – Generalized Parton Distributions (GPDs) DVCS e Simplest process: e + p  e’ + p + g (DVCS). e BH Unprecedented set of Deeply Virtual Compton Scattering data accumulated in Halls A and B p p

Hall A data agree well with hard-scattering assumption Next Round of DVCS Experiments: Hall B

α = ALU(90) as a function of t

Indeed: t-slope decreases

as xB increases orbital angular momentum carried by quarks : solving the spin puzzle e k' g k q q' g* Jd p p' At one value of x only Ingredients: 1) GPD Modeling 2) HERMES 1H(e,e‟g)p (transverse target spin asymmetry) 3) Hall A n(e,e‟g)n (neutron-DVCS from 2H target) Or independent: Lattice QCD! Ju  Tremendous progress to constrain quark angular momenta  12 GeV will give final answers for quarks 10 Years of Physics Experiments at JLab • Experiments have successfully adressed original Mission Statement: “The study of the largely unexplored transition between the nucleon-meson and the quark-gluon descriptions of nuclear matter” Highlight 1: The Role of Quarks in Nuclear Physics Probing the Limits of the Traditional Model of Nuclei • Emphasis has slowly shifted from Base Equipment Experiments to Experiments with dedicated/additional setups and/or detectors • Emphasis has shifted to third sub-area of intended CEBAF research: “What are the properties of the force which binds quarks into nucleons and nuclei at distances where this force is strong and the quark confinement mechanism is important?” • Highlight 2: Charge and Magnetization in Nucleons and Pions Charge distribution in proton differs from magnetization distribution Elusive charge distribution of neutron well mapped out to high resolution Strange quarks play <5% role in mass of proton  unsolved mysteries… • Highlight 3: The Onset of the Parton Model at Low High hadronic structure function data at JLab at 6 GeV have been accumulated spanning the nucleon resonance and low-W2 deep inelastic region. The data indicate a surprisingly smooth parton-hadron transition at relatively low Q2, allowing, for x > 0.1, an unprecedented access to Parton Model physics with the 12 GeV Upgrade