newport beach, ca 25 october 2012

Download Newport Beach, CA  25 October 2012

If you can't read please download the document

Upload: cybele

Post on 09-Jan-2016

25 views

Category:

Documents


0 download

DESCRIPTION

Overview of Medium Energy Physics (“Cold QCD”): Presentation to the Hadron Physics Town Meeting (Presentation to the 2007 NSAC Long Range Plan Implementation Subcommittee) Roy J. Holt. Newport Beach, CA 25 October 2012. Key questions in hadron physics. - PowerPoint PPT Presentation

TRANSCRIPT

  • Overview of Medium Energy Physics (Cold QCD): Presentation to the Hadron Physics Town Meeting

    (Presentation to the 2007 NSAC Long Range Plan Implementation Subcommittee)

    Roy J. Holt

    Newport Beach, CA 25 October 2012

    Argonne National Laboratory

  • Key questions in hadron physicsWhat is confinement and how is it connected with dynamical chiral symmetry breaking, the origin of more than 98% of visible mass in the Universe?What are the dynamics underlying elastic and transition form factors and structure functions of hadrons? How does valence quark structure affect the sea?Where is the missing spin in the nucleon? Are there significant contributions from gluons or valence quark orbital angular momentum?Can we reveal a novel landscape of nucleon substructure through measurements of new multidimensional distribution functions?Do gluonic excitations have a role in the spectroscopy of light mesons and baryons?

    How do nuclei emerge from QCD?What is the relation between short-range N-N correlations and the partonic structure of nuclei?

    Argonne National Laboratory*

    Argonne National Laboratory

  • Elastic electron scattering from a nucleonArgonne National Laboratory*Cross section for scattering from a point-like objectj=J=Nucleon vertex:Dirac Pauli1990 Nobel Prize1961 Nobel PrizeDeep inelastic scattering

    Argonne National Laboratory

  • Tremendous advances in electron scatteringArgonne National Laboratory*Unprecedented capabilities: High Intensity High Duty Factor High Polarization- M. Poelker (2012 Lawrence Award) Large acceptance detectors State-of-the-art polarimetry, polarized targetsFocal plane polarimeter Jefferson LabPolarized 3He target

    Argonne National Laboratory

  • Argonne National Laboratory*The proton form factor: Re-wrote the textbooksPolarization measurements ) Revolutionized our knowledgeNP2010

    Two-photon experiments: OLYMPUS (DESY), JLab, Novosibirsk

    Argonne National Laboratory

  • Flavor separation of proton form factors

    Very different behavior for u & d quarks Evidence for diquark correlations axial diquark -> soft f.f.

    Thanks to Craig Roberts*Cates, de Jager, Riordan, Wojtsekhowski, PRL 106 (2011) 252003Q4 F1qNSAC milestone HP4 (2010) completedQ4F2q/k

    Thanks to Craig Roberts

  • Only JLab 12 GeV can access these form factors to ~10 GeV2

    Argonne National Laboratory*Locations of the zeroes depend on the relative probability of finding scalar & axial diquarks in proton

    Requires SBS

    Six 12-GeV experimentsPlot credit: JLab whitepaper

    Argonne National Laboratory

  • Proton Radius PuzzleArgonne National Laboratory*rp0.8768(69)fm (ep atom)rp0.8772(46)fm (ep scattering)rp=0.84184(67)fm (p atom)Future sub 1% measurements: (1) ep elastic scattering at JLab (2) p elastic scattering at PSI - 16 U.S. institutions!(~$2 M, no contingency)PSAS 2012 Symposium

    ECT* Workshop - Nov. 2012

    7 sX. Zhan et al, PLB 705 (2011) 59Thanks to R. Gilman, H. Gao

    Argonne National Laboratory

  • Hadron polarizabilities Compton scatteringHigh Intensity Gamma Source (HIgS)Proton, neutron polarized H target Polarized 3He target(9 U.S. institutions)MAMI (3 U.S. institutions)Polarized hydrogen target + Crystal BallComplete proton in 2014, begin neutron

    Argonne National Laboratory*Thanks to H. Gao, H. Griesshammer, D. Phillips, W. Briscoe, R. Miskimen, B. Norum D. Shukla, A. Nogga, D. Phillips, PRL (2007)HIgS projectionLattice calculationsChiral perturbation theoryInterplay of pion cloud and shorter distance effects

    Pion polarizabilityCOMPASS II (CERN)(UIUC)Faraday effect

    Argonne National Laboratory

  • Argonne National Laboratory*Partonic structure of the nucleonThree longitudinal structure functions:EIC whitepaper

    Argonne National Laboratory

  • The Neutron Structure FunctionProton structure function:

    Neutron structure function (isospin symmetry):

    Ratio:

    Focus on high x:

    Three 12-GeV experimentsProton : PVDIS and SoLID (K. Paschke)Deuteron: radial TPC and CLAS123H/3He: 3H target and existing spectrometers

    Argonne National Laboratory*DSENSAC milestone HP14 (2018)Thanks to C. Keppel, K. Kumar, G. Petratos

    Argonne National Laboratory

  • Spin Structure of the neutron valence regionCourtesy of Z.-E. Meziani, K. Griffioen, S. Kuhn, G. PetratosNSAC milestone HP14 (2018)Polarized electron scattering from a polarized nucleonThanks to N. Makins, Z.-E. MezianiThree 12-GeV experiments(benefits from SoLID)

  • Tensor charge from transversity measurements at JLabArgonne National Laboratory*Thanks to A. Prokudin and Z.-E. MezianiTensor Charge

    Collins fragmentation function from KEK-B/Belle - M. Grosse-Perdekamp (UIUC)dd benefits from SoLIDTwo 12-GeV experimentsDistribution of transversely polarized quarks inside a transversely polarized proton

    Argonne National Laboratory

  • Drell-Yan is the best way to measure anti-quark distributionsArgonne National Laboratory*What is the A dependence of antiquarks?No model predicts dbar/ubar
  • HERMES Surprise!Strange quark distribution Future: COMPASS-II at CERN (2015), JLab with12 GeV (RICH)A. Airapetian et al, PLB 666 (2008) 446Deep inelastic scattering with flavor tagging

    Serious discrepancy with decades of neutrino data

    Thanks to H. Jackson, J.-C. Peng Intrinsic sea?

  • Strange sea and LHCArgonne National Laboratory*rs = ( s + sbar)/dbarSea appears to be flavor symmetric at low x, consistent with HERMESATLAS Collaboration,ArXiV:1203.4051 [hep-ex]Parton distribution uncertainties at high x feed into benchmark LHC processesThanks to T. LeCompte

    Argonne National Laboratory

  • Worldwide quest: spin structure of the nucleonFrom DIS measurementsDS 0.3DG = 1.01.2

    quark polarization Dq(x)first 5-flavor separation from HERMES: Dq 0RHIC-spin: future charge- current measurements

    gluon polarizationG(x)RHIC-spin, HERMES, COMPASS

    orbital angular momentum L GPDs and TMDsFar future: EICSpin budget of the proton30%70%What is the origin of the proton spin?Jets, pions, ALL

  • Measurement of the gluon polarization DG at RHICD. de Florian et al,Prog. in Part. Nucl. Phys.67 (2012) 251Dominates at high pTDominates at low pTdxDg(x,Q2=10GeV2) = 0.13 (error?)0.050.2RHIC whitepaperSee E. Aschenauers talk for impact of 2013-14 experiments.

  • W production expected from RHIC runs 12+13Argonne National Laboratory*B. Jacak, N. Xu, RHIC PAC 2012NSAC milestone HP8 (2013)Provides an important check of SIDIS method

    No fragmentation function

    Q2=MW2 (no high twist effects)http://www.bnl.gov/npp/pac0612.aspThanks to E. AschenaurSee E. Aschenauers talk for impact on

    Argonne National Laboratory

  • Is there a flavor asymmetry in the sea quark helicity distributions?Sea quark polarization at high xJLab 12 GeV (Hall B)Kaon detection - RICH

    Argonne National Laboratory*Plot credit: K. Hafidi

    Argonne National Laboratory

  • Multidimensional parton distribution functionsArgonne National Laboratory*JLab whitepaperGeneralized parton distribution functionsTransverse momentum distribution functionseg., Sivers distributioneighteen 12-GeV experiments! Separate talk: M. Guidal

    Argonne National Laboratory

  • Transverse Momentum Distributions: The Sivers effectNSAC Milestone HP13 (2015) Test unique QCD predictions for relations between single-transverse spin phenomena in p-p scattering and those observed in deep-inelastic scattering.COMPASS-II, RHIC-spin, polarized FNAL

    HERMESThanks to H. Jackson, M. Burkhardt

  • Polarized Drell-Yan and W production (2014+)Argonne National Laboratory*COMPASS-II (2014, if upgraded)1 U. S. institution~ $0.9M NSF (large area trackers)FNAL Polarized SeaQuest (>2017)8 U.S. institutions, 4 off-shore institutions~$10.5M including 50% contingency

    PHENIXThanks to E. Aschenauer, W. Lorenzon, M. Liu, M. Grosse-PerdekamppolarizedDelivered 500 pb-1Forward upgrades -> transverse spin asymmetriesSTAR

    Argonne National Laboratory

  • Generalized parton distributions and DVCSVector: H (x,,t)Tensor: E (x,,t)Hq(x,0,0) = q(x) Forward limit (t 0, x0) Sum rulesA. Radyushkin,PRD 56 (1996) 5524

    C. Munoz Comacho et al,PRL 97 (2006) 262002 ;F. X. Girod et al, PRL 100 (2008)162002.

  • Extraction of quark total angular momentum NSAC milestones HP11 (2012), HP9 (2014)DVCS is the golden channel:g* + N -> g + NLattice + experiment provides a much greater constraint on GPDs than from either alone. - J. Negele

    Major program for JLab 12 GeV, COMPASS-II, EICPlot credit: JLab whitepaper

  • DVCS measurements and imagingArgonne National Laboratory*Thanks to Z.-E. Meziani, JLab whitepaper

    Argonne National Laboratory

  • A new form of matter: Matter formed from the force field (gluons): meson spin

    intrinsic parity

    charge conjugationConventional mesons:K. Juge et al, nucl-th:030711 separate talk: J. DudekThanks to C. Meyer, C. D. Roberts

  • Search for exotic hybrid mesons at the 12-GeV JLabArgonne National Laboratory*Hybrids are predicted by modern QCD treatments: DSE, latticeNSAC milestone HP15 (2018)Complementary work: GSI (PANDA) : antiproton-proton annihilation in charmonium region (2017-) (Northwestern U.)

    BES-III: electron-positron annihilation in charmonium region also decays to light quark bound states(Indiana U.)Plot credit: NP2010 Two 12-GeV JLab experimentsThanks to K. Seth, M. Shepherd, J. Dudek

    Argonne National Laboratory

  • Baryon resonances JLab Physics Analysis CenterArgonne National Laboratory*Kamano, Nakamura, Lee et al., 2012NSAC milestones HP3 (2009) completed, HP7 (2012)Future: J-PARC, Mainz 6 U. S. institutionsThanks to K. Hicks, W. Briscoe, M. Pennington, T.-S. H. LeePrevious (p,2p) data in the N* mass range are all from 1970s bubble chambers!New Lattice calculations: arXiv:1201.2349 N* resonances and exotic baryons.

    Coupled channels dynamics are essential!

    Argonne National Laboratory

  • A look at quarks in the nucleus: the EMC effectEMC effect discovered 1982 (H. Montgomery et al.), remains a mystery todayScattering from quarks in a nucleus is not just a superposition of scattering from quarks in nucleonsDependence on nuclear density, short range correlations, flavor, spin, isospin?

    Argonne National Laboratory*SLAC E-139, 1984, J. Gomez et al.J. Seeley et al, PRL 103 (2009)

    Argonne National Laboratory

  • EMC effect and short range N-N interaction*EMC effect is correlated with short range N-N interaction L. Weinstein et al, PRL 106, 052301 (2011) , J. Arrington et al, arXiv:1206.6343

    Flavor, isospin and spin dependence of EMC effect? JLab@12, Drell-Yan, MINERvA

    Plot credit: JLab whitepaperN. Fomin et al, PRL 108, 092502 (2012)

    SRC Scaling factors xB 1.5Four JLab 12 GeV experiments

  • MINERnA Main Injector ExpeRiment -A*MINERvA is studying A dependence of neutrino interactions in unprecedented detail, with He, C, Scintillator (CH), H2O, Fe, Pb targets.Uses high intensity NuMI Beamline at FNAL with MINOS near detector as muon spectrometer

    Nuclear physics goalsHigh precision measurement of the axial form factor to high Q2 and search for A dependence of form factorStudies of quark-hadron duality in neutrino interactions, complementing JlabStudying partonic nuclear effects with neutrino interactionsPrecision cross section measurements and studies of final states ScheduleLow E and anti- (average E ~4 GeV) 11/09-4/12~1.7 Million CC interactions and 250 K anti- CC interactions on scintillator, ~300 K CC interactions on Fe and PbMedium E (avg E ~8 GeV) spring 2013 to about 2019MEP ParticipationHampton, Rutgers PMT detector construction and testing, scintillator plane construction. He target funded by MEP

    Slide credit: R. Ransome

  • Hadronization and quark propagation in nuclear matterProduction lengthParton energy lossFormation lengthColor transparencyHadron multiplicitypT broadening

    CEBAF @ 12 GeV + CLAS12: ideal facility to study light quark hadronization: What governs the transition of quarks and gluons into pions and nucleons? NSAC 2007W. Brooks, K. Hafidi, K. Joo et al.

  • The EIC (>2020)Argonne National Laboratory*Source: EIC whitepaperGluon saturationGluon and sea quark polarizationGluon imagingQuark propagationSea quark imaging

    Argonne National Laboratory

  • 2020 and beyond: Electron Ion Collider

    We recommend the allocation of resources to develop accelerator and detector technology necessary to lay the foundation for a polarized Electron-Ion Collider. NSAC LRP 2007Brookhaven National LabJefferson LabUnique: high-luminosity with polarized electrons, nuclear and polarized ion beams

  • Non-JLab, non-RHIC cold-QCD experimentsArgonne National Laboratory**ExpectedThanks to C. Howell

    ProgramContactStatusLab# U.S. MEPInstitutionsEducation # U.S. MEP postdocs, grad. students, undergradsn polarizability, GDH, few-bodyH. GaoOngoingHIgS92, 5, 3Drell-YanD. Geesaman, P. ReimerOngoingFNAL87, 7, 4COMPASS-IIM. Grosse-PerdekampOngoingCERN11, 2, 4N polarizabilityR. MiskimenOngoingMainz32, 3, 1Baryon resonancesW. BriscoeOngoingMainz61, 3, 6MINERvAR. RansomeOngoingFNAL22, 2, 2N polarizability, GDH, few-body, Bethe-HeitlerB. NorumOngoingHigS42, 1, 2OLYMPUSR. MilnerOngoingDESY43, 6, 6HERMESH. JacksonOngoingDESY31, 4, 1BES-IIIM. ShepherdOngoingBES11 ,2, 0Threshold pion photoproductionA. BernsteinOngoingMainz31, 0, 0Radiative pion productionB. NorumNewMainz20.2, 0, 0Polarized Drell-YanW. LorenzonNewFNAL80.5, 0.5, 3N polarizabilityR. MiskimenNewHIgS40, 0, 1Proton radiusR. GilmanNewPSI161, 0, 0Baryon resonancesK. HicksNewJ-PARC62, 5, 0*Charmed mesonsK. SethNewGSI11, 2, 0

    Argonne National Laboratory

  • Concluding statement

    Understanding hadrons will be one of nuclear physics greatest contributions to science

    New 21st century tools have positioned us well for the next decade: JLab 12 GeV, RHIC - Major U.S. facilities lead the worldFNAL MI, CERN COMPASS-II, HIgS, Mainz, J-PARC, FAIR provide targeted experiments that complement the central programFar future: EIC

    We are camped on one of the most interesting frontiers in science

    Argonne National Laboratory*

    Argonne National Laboratory

  • Many thanks toArgonne National Laboratory*M. AhmedE. AschenauerJ. ArringtonT. BarnesD. BeckW. BriscoeM. BurkhardtG. CatesA. DesphandeC. DjalaliE. DownieR. EntC. GagliardiH. GaoD. GeesamanR. GilmanH. GriesshammerM. Grosse-PerdekampK. HafidiK. HicksC. HowellB. Jacak

    Helpful documents:

    NP2010 Report

    NSAC 2007 Long Range Plan

    Whitepaper drafts:JLab 12 GeVThe Case for Continuing RHIC OperationsElectron Ion Collider

    JLab12, RHIC, COMPASS-II proposals

    STAR and PHENIX decadal plans

    NSAC Performance Measures 2008

    J.-C. PengM. PenningtonD. PhillipsG. PetratosJ. QiuR. RansomeP. ReimerC. RobertsJ. RubinK. SethM. ShepherdM. StratmannB. SurrowS. VigdorW. VogelsangH. WellerR. WiringaB. WojtsekhowskiN. XuH. JacksonK. JooB. KeisterC. KeppelW. KorschK. KumarT.-S. H. LeeM. LiuW. LorenzonT. LeCompteN. MakinsC. MeyerZ.-E. MezianiR. McKeownR. MilnerR. MiskimenH. MontgomeryJ. NagleB. NorumK. OrginosK. Paschke

    Argonne National Laboratory

    Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"*Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"*Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"*Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"**Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"*Test*Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"Took data through the end of April 2012. Assume medium energy run is for 6 years (NOvA plans to take 3 years of neutrinos and 3 years of anti-neutrinos, what they really end up wanting to take may change, of course. Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"*Go to "View | Header and Footer" to add your organization, sponsor, meeting name here; then, click "Apply to All"