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JLab: Probing Hadronic Physics with Electrons and Photons Elton S. Smith Jefferson Lab V Latinamerican Symposium on Nuclear Physics Santos, Brazil, September 2003 Introduction to JLab The shape of the proton Pentaquarks 1 Elton S. Smith

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  • JLab: Probing Hadronic Physics with Electrons and Photons

    Elton S. SmithJefferson Lab

    V Latinamerican Symposium on Nuclear Physics

    Santos, Brazil, September 2003

    Introduction to JLabThe shape of the protonPentaquarks

    1Elton S. Smith

  • 2Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Why use electron and photon probes?

    Electromagnetic interaction is well-known

    e e’

    p p

    F(Q2)

    Elastic Form Factors Inelastic transitions

    Size probed ~ 1/√Q2

  • 3Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    CEBAF @ JLab TodayMain physics programs─ nucleon electromagnetic form factors (including strange form factors)─ N → N* electromagnetic transition form factors─ spin structure functions of the nucleon─ form factors and structure of light nuclei

    Superconducting recirculating electron accelerator─ max. energy 5.7 GeV─ max current 200 µA─ e polarization 80%

    Simultaneous operation in 3 halls L[cm-2s-1]─ A: Two High Resolution Spectrometers (pmax=4 GeV/c 10

    39

    ─ B: Large Acceptance Spectrometer for e and γ induced reactions 1034

    ─ C: Two spectrometers (pmax= 7 and 1.8 GeV/c) + special equipment 1039

  • 4Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    CEBAF accelerator site

  • 5Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Three Experimental End-Stations

    High Resolution SpectrometersElectron or Hadron Arm

    Detector

    Q2Q1Dipole

    Q3

    53 m

    30 m

    HALL C

    46 m

    HALL B

    HALL A

    High MomentumSpectrometer

    Short OrbitSpectrometer

    Pair of identical High ResolutionSpectrometers (HRS2)

    CEBAF's Large Acceptance Spectrometer(CLAS) and Bremsstrahlung Photon Tagger

    High Momentum Spectrometer (HMS)and Short Orbit Spectrometer (SOS)

  • 6Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    GEp: Electric form factor of the proton

    Goal: Determine the charge and current distributions inside the proton

    NY Times “Is a proton round?”

    from G.A. Miller

    u

    u d

    Naïve expectation is that the charge and currents are determined from the spatial distribution of quark charges and spins.

  • 7Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Charge distribution and Form Factors

    0 0.2 0.4 0.6 0.8 10.01

    0.1

    1

    0 2 4 60.01

    0.1

    1

    ∫ ⋅−= rqieqFqdrrr

    )()( 23ρρ(r) F(Q2)

    2

    222

    /11)( ⎟⎟

    ⎞⎜⎜⎝

    ⎛Λ+

    =Q

    QF

    Λ=0.94 GeVΛ=0.84 GeVΛ=0.74 GeV

    rρ =)(re Λ−Λ

    π8

    3

    Radius (fm) Q2 (GeV2/c2)

  • 8Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Charge Distributions and Form Factors

    1)( 2 =QF

    rrf e Λ−Λ=π8

    )(3 2

    222

    /11)( ⎟⎟

    ⎞⎜⎜⎝

    ⎛Λ+

    =Q

    QF

    )()( orrrf −= δ

    rr

    rf e Λ−Λ=π4

    )(2

    222

    /11)(

    Λ+=

    QQF

    ⎟⎠⎞

    ⎜⎝⎛ Λ−

    ⎟⎟⎠

    ⎞⎜⎜⎝

    ⎛ Λ=

    2221

    2)(

    2 rrf e

    π

    unitypoint

    exponential dipole

    Yukawa pole

    ⎟⎟⎟

    ⎜⎜⎜

    ⎛Λ−

    =

    2/221

    )( 2Q

    QF eGaussian Gaussian

  • 9Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Decomposition of the elastic cross section

    )( )2/(tan21

    2222

    eMpMpEp

    ns GGG

    dd ϑτ

    ττ

    σσ +++

    =Ω

    2

    2

    4 pMQ

    =τEE

    E ee

    ns′

    =)2/(sin4)2/(cos

    42

    22

    ϑϑασ

    )()()1( 2222 QGQGdd

    MpEpns

    R +=+

    Ω=

    τε

    τσετσσ

    12 })2/(tan)1(21{ −++= eϑτε

  • 10Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Proton Form Factors pre-1998

    DMp

    Ep GG

    G ~~µ

    271.0

    1

    1

    )( 2QGD

    +=

  • 11Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Spin transfer reaction e p → e p

    e

    e’

    p

    p’

    T̂ L̂θ

    )2/tan(2

    ' ϑM

    EEPP

    GG ee

    l

    t

    Mp

    Ep +−= e

  • 12Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Transport through magnet

  • 13Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Azimuthal asymmetry in the polarimeter

  • 14Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    GEp from polarization transfer

    E93-027, E99-007 Perdrisat, Punjabi, Jones, Brash

  • 15Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    World data for GEp

  • 16Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Interpretation of new data

    F2(Q2) is a spin-flip transition

    )(2

    )'()(~' 22 PuMqiPuQFPJP ↓↑↓↑

    αµν

    µ σ

    In the absence of quark angular momentum

    0~ 01

    22 ⎯⎯ →⎯ →qmq MmFFQ

    Quark orbital angular momentum essential to describe data

    constQQF

    FQ ~log1~ 22

    2

    1

    2⎟⎟⎠

    ⎞⎜⎜⎝

    ⎛Λ

  • 17Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Pentaquark: Baryon with five quarks

    Goal: Determine quark content of colorless hadrons

    Expectation from the quark model is that the properties of baryons are determined by three valence quarks (qqq)

  • 18Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Hadron multiplets

    Mesons qq1833 ⊕=⊗

    Baryons qqq

    18810333 ⊕⊕⊕=⊗⊗

    18810102788 ⊕⊕⊕⊕⊕=⊗

    Baryons built from meson-baryon basis Ω─

    Θ+

    N

    Σ

    Ξ

  • 19Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Production and decay of Ω─→ Ξο π─

  • 20Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    What are pentaquarks?Minimum quark content is 5-quarks.Anti-quark has different flavor than any of 4-quarks ( ).Quantum numbers can not be defined by 3-quarks.

    General idea of a five-quark states has been around since late 60’s.However, searches did not give any conclusive results.PDG dropped the discussion on pentaquarksearches after 1988.

    Qqqqq

  • 21Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    The Anti-decuplet predicted by Diakonov et al.

    ( )uud dd ss+

    ( )uus dd ss+

    ( )udd uu ss+

    ( )dds uu ss+

    ( )dss uu dd+ ( )uss uu dd+

    ( )uds uu dd ss+ +

  • 22Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Reactions on deuterium

    n

    γK─

    K+

    nΘ+

    p p

    p

    γK+

    K─

    pΛ∗

    n npK

    nKnp

    nKΘ+pΘ+pn

    +

    +

    K−

    →Λ

    Λ→

    )1520()()1520()(

    )()(

    *

    γ

    γN → φ(1020) N → K+K- N

  • 23Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    CEBAF Large Acceptance Spectrometer

    Liquid D2 (H2)target +γ start counter; e minitorus

    Torus magnet6 superconducting coils

    Drift chambersargon/CO2 gas, 35,000 cells

    Time-of-flight countersplastic scintillators, 684 photomultipliers

    Gas Cherenkov counterse/π separation, 256 PMTs

    Electromagnetic calorimetersLead/scintillator, 1296 photomultipliers

  • 24Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Exclusive measurement using γd reactions

    CLAS Collaboration (S. Stepanyan, K. Hicks, et al.), hep-ex/0307018Requires FSI – both nucleons involved─ No Fermi motion

    correction necessary─ FSI puts K- at larger lab

    angles: better CLAS acceptance

    ─ FSI not rare: in ~50% of Λ∗(1520) events both nucleons detected with p > 0.15 GeV/c

  • 25Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    γd → p K+K─ (n) in CLASK- K+

    p

  • 26Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Kaon times relative to proton

    ppπ- pπ+π-

    22;

    Kc

    cK

    mpp

    cRtt

    +=

    ⋅−=∆ β

    β

    ∆t (p-K─)(ns)

    ∆t (p-K+) (ns)

    pK+K─

  • 27Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Reaction γd→pK+K-(n)

    Clear peak at neutron mass.

    15% non pKK events within ±3σ of the peak.

    Almost no background under the neutron peak after event selection with tight timing cut.

    MM(pK+K-) [ GeV/c2 ]

    Eve

    nts

    MM(pK+K-) [ GeV/c2 ]

    Eve

    nts

    |∆tpK| ≤ 0.75 ns

    0

    100

    200

    300

    400

    500

    0.8 0.85 0.9 0.95 1 1.05 1.1 1.15 1.2 1.25

    0

    50

    100

    150

    200

    250

    300

    350

    0.8 0.9 1 1.1

    Reconstructed Neutrons

  • 28Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Identification of known resonances

    Remove events with IM(K+K−) φ(1020) by IM > 1.07 GeVRemove events with IM(pK−) Λ(1520)Limit K+ momentum due to γ d p K− Θ + phase space pK+ < 1.0GeV/cC. Meyer (CLAS note 03-009): checked narrow structure impossible inγd K+Y*N K+(K-N)N,+ KN rescattering

  • 29Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    nK+ invariant mass distribution

    MM(nK+) [ GeV/c2 ]

    Eve

    nts

    NΘ = 43

    MΘ = 1.542 GeV

    σΘ = 0.009 GeVNΘ/√NBg = 5.8σ

    0

    5

    10

    15

    20

    25

    30

    35

    1.5 1.6 1.7 1.8 1.9

    0)( PGGMF Bg ++= +Θ

    Distribution of Λ(1520) events

    Θ+

  • 30Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Θ+: experimental statusExperimental evidence for Θ+ have been reported at four laboratories.

    ─ LEPS collaboration at Spring-8 (Japan), January 2003 - peak in the invariant mass of the nK+ at 1.54 GeV with statistical significance of 4.6σ.

    ─ DIANA collaboration at ITEP (Moscow), April 2003 – peak in the invariant mass of pK0 at 1.538 GeV, statistical significance 4.4σ.

    ─ CLAS collaboration at JLAB, July 2003 – peak in the invariant mass of the nK+ at 1.542 GeV, statistical significance 5.3σ.

    ─ SAPHIR collaboration at ELSA (Bonn), August 2003 – peak in the invariant mass of the nK+ at 1.54 GeV, statistical significance 4.8σ.

    All experiments observe a narrow width.Spin, isospin and parity not yet established.Subject of intense interest and research.

    ─ Penta-Quark 2003 Workshop at JLab in November.

  • 31Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    SummaryWe have presented two examples which highlight the physics program at Jefferson Lab.The electromagnetic interaction can be used to probe deep into the structure of nucleons.─ From measurements of GEp up to a Q2 = 5.6 GeV2 we

    have gained new insights into the shape of the proton.─ Orbital angular momentum of quarks is a key ingredient in

    our understanding of proton structure.A key question in non-perturbative QCD is the structure of hadrons─ We have presented evidence for an exotic baryon with

    S = +1, which would have a minimal quark content of five quarks (uudds).

    ─ This baryon represents a new class of colorless hadrons.

  • 32Elton S. Smith V Latinamerican Symposium, Sep 1-5, 2003

    Scaled F2/F1 ratio

    JLab: Probing Hadronic Physics with Electrons and PhotonsWhy use electron and photon probes?CEBAF @ JLab TodayCEBAF accelerator siteThree Experimental End-StationsGEp: Electric form factor of the protonCharge distribution and Form FactorsCharge Distributions and Form FactorsDecomposition of the elastic cross sectionProton Form Factors pre-1998Spin transfer reaction e p → e pTransport through magnetAzimuthal asymmetry in the polarimeterGEp from polarization transferWorld data for GEpInterpretation of new dataPentaquark: Baryon with five quarksHadron multipletsProduction and decay of W─ → Xo p─What are pentaquarks?The Anti-decuplet predicted by Diakonov et al.Reactions on deuteriumCEBAF Large Acceptance SpectrometerExclusive measurement using gd reactionsgd → p K+K─ (n) in CLASKaon times relative to protonReaction gd→pK+K-(n)Identification of known resonancesnK+ invariant mass distributionQ+: experimental statusSummaryScaled F2/F1 ratio