Ralf W. Gothe N STAR 2009 1 Nucleon Transition Form Factors at JLab: Status and Outlook Beijing, April 19 – 22, 2009  Motivation: Why Nucleon Transition.

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Presentation transcript:

Ralf W. Gothe N STAR Nucleon Transition Form Factors at JLab: Status and Outlook Beijing, April 19 – 22, 2009  Motivation: Why Nucleon Transition Form Factors?  Consistency: N  N Roper, and other N N* Transitions  Outlook: Experiment and Theory Ralf W. Gothe University of South Carolina

Ralf W. Gothe N STAR Physics Goals Models Quarks and Gluons as Quasiparticles ChPT Nucleon and Mesons pQCD q, g, qq 1.0 fm <  Determine the electrocouplings of prominent excited nucleon states (N *, Δ * ) in the unexplored Q 2 range of GeV 2 that will allow us to:  Study the structure of the nucleon spectrum in the domain where dressed quarks are the major active degree of freedom.  Explore the formation of excited nucleon states in interactions of dressed quarks and their emergence from QCD. vv N  p   p  ? ! ! ? ? ? ! !

Ralf W. Gothe N STAR quark mass (GeV) Quark mass extrapolated to the chiral limit, where q is the momentum variable of the tree-level quark propagator using the Asquat action.  … resolution low high q e.m. probe LQCD (Bowman et al.) Hadron Structure with Electromagnetic Probes N,N *,  * … 3q-core+MB-cloud 3q-core pQCD LQCD, DSE and …

Ralf W. Gothe N STAR M. Polyakov

Ralf W. Gothe N STAR S 11 Q 3 A 1/2 F 15 Q 5 A 3/2 P 11 Q 3 A 1/2 D 13 Q 5 A 3/2 F 15 Q 3 A 1/2 D 13 Q 3 A 1/2 Constituent Counting Rule  A 1/2  1/Q 3  A 3/2  1/Q 5  G M  1/Q 4 * Quark mass extrapolated to the chiral limit, where q is the momentum variable of the tree-level quark propagator using the Asquat action. Bowman et al. (LQCD) (GeV )

Ralf W. Gothe N STAR N →  Multipole Ratios R EM, R SM  New trend towards pQCD behavior does not show up.  CLAS12 can measure R EM and R SM up to Q² ~ 12 GeV².  R EM +1 M. Ungaro  G M 1/Q 4 * G D = 1 (1+Q 2 /0.71) 2

Ralf W. Gothe N STAR N →  Multipole Ratios R EM, R SM A. Villano very preliminary e p e'p  0 … but the trend that R SM becomes constant in the limit of Q 2 → ∞ seems to show up in the latest MAID 2007 analysis of the high Q 2 data.

Ralf W. Gothe N STAR Progress in Experiment and Phenomenology Dressed quarks (I. Aznauryan, M. Giannini et al., B. Julia-Diaz et al.) Meson-baryon cloud (EBAC) N  NN NN p0p0  (1232)P 33 N(1440)P 11 N(1520)D 13 Recent experimental and phenomenological efforts show that meson- baryon contributions to resonance formations drop faster with Q 2 than contributions from dressed quarks. A 1/2

Ralf W. Gothe N STAR Resonance Electrocouplings in Lattice QCD LQCD calculations of the  (1232)P 33 and N(1440)P 11 transitions have been carried out with large  -masses. By the time of the upgrade LQCD calculations of N* electrocouplings will be extended to Q 2 = 10 GeV 2 near the physical  -mass as part of the commitment of the JLab LQCD and EBAC groups in support of this proposal.  (1232)P 33 N(1440)P 11 see White Paper Sec. II and VIII Huey-Wen Lin

Ralf W. Gothe N STAR LQCD & Light Cone Sum Rule (LCSR) Approach LQCD is used to determine the moments of N* distribution amplitudes (DA) and the N* electrocouplings are determined from the respective DAs within the LCSR framework. Calculations of N(1535)S 11 electrocouplings at Q 2 up to 12 GeV 2 are already available and shown by shadowed bands on the plot. By the time of the upgrade electrocouplings of others N*s will be evaluated. These studies are part of the commitment of the Univ. of Regensburg group in support of this proposal. see White Paper Sec. V N(1535)S 11 CLAS Hall C

Ralf W. Gothe N STAR Dynamical Mass of Light Dressed Quarks DSE and LQCD predict the dynamical generation of the momentum dependent dressed quark mass that comes from the gluon dressing of the current quark propagator. These dynamical contributions account for more than 98% of the dressed light quark mass. The data on N* electrocouplings at 5<Q 2 <12 GeV 2 will allow us to chart the momentum evolution of dressed quark mass, and in particular, to explore the transition from dressed to almost bare current quarks as shown above. per dressed quark Q 2 = 12 GeV 2 = (p times number of quarks) 2 = 12 GeV 2 p = 1.15 GeV DSE: lines and LQCD: triangles

Ralf W. Gothe N STAR Dyson-Schwinger Equation (DSE) Approach DSE provides an avenue to relate N* electrocouplings at high Q 2 to QCD and to test the theory’s capability to describe N* formations based on QCD. DSE approaches provide a link between dressed quark propagators, form factors, scattering amplitudes, and QCD. N* electrocouplings can be determined by applying Bethe-Salpeter / Fadeev equations to 3 dressed quarks while the properties and interactions are derived from QCD. By the time of the upgrade DSE electrocouplings of several excited nucleon states will be available as part of the commitment of the Argonne NL and the University of Washington. see White Paper Sec. III

Ralf W. Gothe N STAR Constituent Quark Models (CQM) Pion Cloud (EBAC) |q 3 +qq  (Li, Riska) 3q Relativistic CQM are currently the only available tool to study the electrocouplings for the majority of excited proton states. This activity represent part of the commitment of the Yerevan Physics Institute, the University of Genova, INFN-Genova, and the Beijing IHEP groups to refine the model further, e.g., by including qq components. see White Paper Sec. VI LC CQM PDG value NN N , N  combined analysis N(1440)P 11 :

Ralf W. Gothe N STAR Phenomenological Analyses  Unitary Isobar Model (UIM) approach in single pseudoscalar meson production  Fixed-t Dispersion Relations (DR)  Isobar Model for Nππ final state (JM)  Coupled-Channel Approach (EBAC) see White Paper Sec. VIII see White Paper Sec. VII

Ralf W. Gothe N STAR Unitary Isobar Model (UIM) Nonresonant amplitudes: gauge invariant Born terms consisting of t-channel exchanges and s- / u-channel nucleon terms, reggeized at high W.  N rescattering processes in the final state are taken into account in a K-matrix approximation. Fixed-t Dispersion Relations (DR) Relates the real and the imaginary parts of the six invariant amplitudes in a model-independent way. The imaginary parts are dominated by resonance contributions. Phenomenological Analyses in Single Meson Production see White Paper Sec. VII

Ralf W. Gothe N STAR Legendre Moments of Unpolarized Structure Functions Q 2 =2.05GeV 2 Two conceptually different approaches DR and UIM are consistent. CLAS data provide rigid constraints for checking validity of the approaches. K. Park et al. (CLAS), Phys. Rev. C77, (2008) I. Aznauryan DR fit w/o P 11 I. Aznauryan DR fit I. Aznauryan UIM fit

Ralf W. Gothe N STAR Energy-Dependence of  + Multipoles for P 11, S 11 imaginary partreal part Q 2 = 0 GeV 2 The study of some baryon resonances becomes easier at higher Q 2. Q 2 = 2.05 GeV 2 preliminary

Ralf W. Gothe N STAR BES/BEPC, Phys. Rev. Lett. 97 (2006) Bing-Song Zou and    ±     ±        -     ±   invariant mass / MC phase space

Ralf W. Gothe N STAR Nucleon Resonances in N  and N  Electroproduction p(e,e')X p(e,e'p)   p(e,e'  + )n p(e,e'p  + )  -   channel is sensitive to N*s heavier than 1.4 GeV  Provides information that is complementary to the N  channel  Many higher-lying N*s decay preferentially into N  final states Q 2 < 4.0 GeV 2 W in GeV

Ralf W. Gothe N STAR    (1232)P 33, N(1520)D 13,  (1600)P 33, N(1680)F 15 JM Model Analysis of the p  +  - Electroproduction see White Paper Sec. VII

Ralf W. Gothe N STAR JM Mechanisms as Determined by the CLAS 2  Data Each production mechanism contributes to all nine single differential cross sections in a unique way. Hence a successful description of all nine observables allows us to check and to establish the dynamics of all essential contributing mechanisms. Full JM calculation  -   ++  + N(1520) D 13  + N(1685) F 15 pp 2  direct

Ralf W. Gothe N STAR Separation of Resonant/Nonresonant Contributions in 2  Cross Sections Due to the marked differences in the contributions of the resonant and nonresonant parts to the cross sections, the nine observables allow us to neatly disentangle these competing processes. resonant part nonresonant part

Ralf W. Gothe N STAR Electrocouplings of N(1440)P 11 from CLAS Data N  (UIM, DR) PDG estimation N , N  combined analysis N  (JM) The good agreement on extracting the N* electrocouplings between the two exclusive channels (1  /2  ) – having fundamentally different mechanisms for the nonresonant background – provides evidence for the reliable extraction of N* electrocouplings.

Ralf W. Gothe N STAR Comparison of MAID 08 and JLab analysis A 1/2 S 1/2 Roper Electro-Coupling Amplitudes A 1/2, S 1/2 L. Tiator MAID 07 and new Maid analysis with Park data MAID 08

Ralf W. Gothe N STAR Electrocouplings of N(1520)D 13 from the CLAS 1  /2  data world data GeV -1/2 N  (UIM, DR) PDG estimation N , N  combined analysis N  (JM) A hel = A 1/2 2 – A 3/2 2 A 1/2 2 + A 3/2 2 A 1/2 A 3/2 L. Tiator

Ralf W. Gothe N STAR N(1520)D 13 Electrocoupling Amplitudes A 3/2, S 1/2 I. Starkovski

Ralf W. Gothe N STAR N(1700)D 33 N(1720)P 13 Combined 1  -2  JM Analysis of CLAS Data  PDG at Q 2 =0  Previous world data  2  analysis  1  -2  combined at //// Q 2 =0.65 GeV 2  Many more examples: //// P 11 (1440), D 13 (1520), S 31 (1650), //// S 11 (1650), F 15 (1685), D 13 (1700), //// … preliminary

Ralf W. Gothe N STAR CLAS12 Detector Base Equipment

Ralf W. Gothe N STAR CLAS 12 Kinematic Coverage and Counting Rates Genova-EG SI-DIS (e',  + ) detected (e', p) detected (e ’,  + ) detected (E,Q 2 )(5.75 GeV, 3 GeV 2 )(11 GeV, 3 GeV 2 )(11 GeV, 12 GeV 2 ) N+N    10 4 NpNp   10 4 NpNp   days L=10 35 cm -2 sec -1, W=1535 GeV,  W= GeV,  Q 2 = 0.5 GeV 2

Ralf W. Gothe N STAR Angular Acceptance of CLAS12  + Acceptance for cos  = 0.01 Full kinematical coverage in W, Q 2, , and 

Ralf W. Gothe N STAR < W < 2 GeV 60 MeV 1.5 < W < 2 GeV 10 MeV W < 2 GeV 33 22 W and Missing Mass Resolutions with CLAS12 W calculated from electron scattering exclusive p  +   final state ep  e'p'  + X Final state selection by Missing Mass M X 2 (GeV 2 ) FWHM

Ralf W. Gothe N STAR Kinematic Coverage of CLAS12 60 days L= cm -2 sec -1,  W = GeV,  Q 2 = 0.5 GeV 2 Genova-EG (e ’, p     ) detected W GeV Q 2 GeV 2 2  limit >1  limit > 2  limit >1  limit > 1  limit >

Ralf W. Gothe N STAR Summary  We will measure and determine the electrocouplings A 1/2, A 3/2, S 1/2 as a function of Q 2 for prominent nucleon and Δ states,  see our Proposal  Comparing our results with LQCD, DSE, LCSR, and rCQM will gain insight into  the strong interaction of dressed quarks and their confinement in baryons,  the dependence of the light quark mass on momentum transfer, thereby shedding light on chiral-symmetry breaking, and  the emergence of bare quark dressing and dressed quark interactions from QCD.  This unique opportunity to understand origin of 98% of nucleon mass is also an experimental and theoretical challenge. A wide international collaboration is needed for the:  theoretical interpretation on N* electrocouplings, see our White Paper and  development of reaction models that will account for hard quark/parton contributions at high Q 2.  Any constructive criticism or direct participation is very welcomed, please contact:  Viktor Mokeev or Ralf Gothe