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Crystal Ball Experiment at MAMI Recent Results W.J. Briscoe for the A2 Collaboration (thanks for the sabbatical support) MESONS 2010 SFB443
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Overview of MAMI and the Crystal Ball experimental setup Technical capabilities: pion production, strangeness production from the proton and neutron Selected physics topics: Coherent pion photoproduction Eta photoproduction Complete measurements: Transverse spin observables in pion and eta photoproduction Conclusions & Outlook Overview
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MAMI
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Maximum Energy 1604 MeV, ΔE = 100 KeV 100 % duty cycle Current ≤ 100 μA Electron Polarization ~ 85% ~7000 hours beam / year
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Photon Tagging Facility Detection of radiating electrons: E γ = E e – E e ' Energy resolution 2-4 MeV Tagger Microscope ~6x better E res. Circularly pol. γ from e - pol, upto 85% Linearly pol. γ from crystalline rad., upto 70% Collimation upgrade will give +5% pol. End Point Tagger awaiting funding P e- →P γcirc.
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CB@MAMI Detector System Large solid angle detection: CB & TAPS ~97% 4π Angular discrimination: 672 NaI, 386 / 512 BaF 2 Particle discrimination: PID, VETOS Charged tracking: MWPC Crystal Ball TAPS PID Detector MWPCs Target
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First report of σ(γ,π 0 ) for a specific excited state Simultaneous detection of π 0 and 4.4 MeV decay γ in CB Important first step in isolation of coherent process PRL 100, 132301 (2008) Technical Capabilities: Incoherent π 0 photoproduction on 12 C Decay γ spectrum in coinc. with π 0 4.4 MeV 2+ state γ 12 C→ 12 C* π 0 ↓ 12 C γ(4.4 MeV)
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Technical Capabilities: Kaon Photoproduction No time left to discuss: Recoil polarimetry: γN→πN', γN→ηN', determination of η mass, GDH integral on the neutron, in-medium modification of mesons, threshold hyperon production, double pion production and so much more... Decay sub-cluster energy Incident and decay sub- cluster time difference K + missing mass Incident subcluster from K + ~3ns Decay sub-cluster from K + →μ + ν μ decay ~ 20ns Tom Jude Edinburgh University
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Coherent π 0 photoproduction on 208 Pb Eγ = 160 - 170 MeVEγ = 190 - 200 MeVEγ = 170 - 180 MeVEγ = 180 - 190 MeV Do heavy stable nuclei have a neutron skin? Size of skin gives direct information on equation of state of n-rich matter Skin size gives important new insights into neutron star physics! Measurements planned on Sn, Ca isotope chains Accuracy ~0.05 fm D. P. Watts and C. Tarbert, Edinburgh Preliminary
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Many resonances: broad and overlapping Accurate separation of final states → good detector resolution Sensitivity to small σ processes → 4π detector acceptance, large γ flux Access to polarization observables → polarized beam, target, recoil Excitations of the Nucleon Δ(1232)
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η photoproduction: γp→ηp S 11 (1535) dominant resonance in η production “Dip” in cross section due to interference with less dominant resonances Need polarization observables to extract full resonance composition TAPS at MAMI CB at ELSA CB@MAMI preliminary TAPS/MAMI GRAAL/ESRF CLAS/JLAB CB/ELSA
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S 11 (1535) dominant resonance in η production “Dip” in cross section due to interference with less dominant resonances Need polarization observables to extract full resonance composition JLAB ELSA CB@MAMI preliminary (S. Prakhov) S 11 (1535) J P = 1/2 - J P = 3/2 - D 13 (1520) η photoproduction: γp→ηp
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Complete Experiment 16 possible unpolarised, single & double polarization observables in pseudoscalar meson photoproduction Need 8 carefully selected observables to fully constrain partial wave analyses These have to include single & double polarization observables All polarization degrees of freedom now uniquely accessible in Mainz!
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Recoil Polarimetry π 0 / η decays & is detected as normal Reconstruct π 0 / η Recoiling proton then tagged P reconstructed = γ beam + p target – π 0 Large scattering angle → nucl. interaction Asymmetry gives pol. transfer Data G4 total G4 no nuclear int Proton scattering angle in graphite D. P. Watts, Edinburgh D. Glazier, Edinburgh M. Sikora, Edinburgh. D, Howdle, Glasgow
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Recoil Polarimetry – π 0 Photoproduction No time left to discuss: Recoil polarimetry: γN→πN', γN→ηN', determination of η mass, GDH integral on the neutron, in-medium modification of mesons, threshold hyperon production, double pion production and so much more... Photon Energy Degree of Polarisation Transfer C x ' p(γ,π 0 )p polarisation transfer: circ. polarised beam to recoil proton D. P. Watts, Edinburgh D. Glazier, Edinburgh M. Sikora, Edinburgh D, Howdle, Glasgow
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Polarized Frozen Spin Target H. Ortega Spina Uses DNP to achieve ~ 90 % proton, 80 % deuteron Needs: Horiz. Dilution cryostat, polarizing magnet, microwave, NMR Two holding coils: solenoid → longitudinal, saddle coil → transverse
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Uses DNP to achieve ~ 90 % proton, 80 % deuteron Needs: Horiz. Dilution cryostat, polarizing magnet, microwave, NMR Two holding coils: solenoid → longitudinal, saddle coil → transverse Polarised Frozen Spin Target
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Frozen spin target fully functioning – Polarization > 90% ~1000 hours relaxation time & low He usage – long measurement time! Running with transverse polarized target! N. Froemmgen P=P 0 exp(t/τ)
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First measurement of transverse spin observable F in γp→π 0 p F asymmetry: circ. polarised photons, transverse pol. Target Need to seperate out contribution from 12 C and 16 O and 3/4 He Requiring proton removes coherent contributions Other kinematic cuts and remaining underground fitted & subtracted Data shown from 39 hours minus, 39 hours plus pol. test data, no TAPS Test beamtime ended 07:00 08.03.10, results first shown 10:00 10.03.10 VERY PRELIMINARY! N. Froemmgen
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Asymmetry calculated for each bin (above) Normalized to sin(φ) (target polarization angle corr.) Weighted average for points with |sin(φ)|>0.3 Background Subtraction on MM(π 0 ) E γ = 500 – 600 MeV E γ = 400 – 500 MeV E γ = 400 – 500 MeV E γ = 500 – 600 MeV E γ = 300 – 400 MeV cos(φ π -90) = sin (φ π ) 0 First measurement of transverse spin observable F in γp→π 0 p
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World first measurement of F – VERY PRELIMINARY! Need more work on P γ (currently standard conditions assumed) Need to extend to full solid angle coverage (measure with TAPS) P targ from average over time – need event-by-event normalisation However – everything works! PRELIMINARY F First measurement of transverse spin observable F in γp→π 0 p SAID MAID V. Kashevarov
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Conclusions & Outlook F PRELIMINARY SAID MAID F The CB@MAMI experimental setup is a highly flexible 4π detector system Complete measurements of π and η production within next five years Allow full investigation of: P 33 (1232), P 11 (1440), S 11 (1535) Double meson production (ππ, πη) → other resonance studies e.g. D 33 (1700) Compton scattering: access to nucleon vector polarisabilities Strangeness photoproduction, coherent π 0 studies of isotope chains η/η' decays & more... The CB@MAMI experimental setup is a highly flexible 4π detector system Complete measurements of π and η production within next five years Allow full investigation of:P 33 (1232), P 11 (1440), S 11 (1535), Double meson production ( π → broad range of new resonance studies P 33 (1232), S 11 (1535), D 33 (1700)! V. Kashevarov
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Polarized Target 2 cm Uses DNP to achieve ~ 90 % proton, 80 % deuteron Needs: Horiz. Dilution cryostat, polarising magnet, microwave, NMR Two holding coils: solenoid → longitudinal, saddle coil → transverse Detectors have to move
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Polarized Target Uses DNP to achieve ~ 90 % proton, 80 % deuteron Needs: Horiz. Dilution cryostat, polarising magnet, microwave, NMR Two holding coils: solenoid → longitudinal, saddle coil → transverse Detectors have to move
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Polarized Target
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Polarised Target Uses DNP to achieve ~ 90 % proton, 80 % deuteron Needs: Horiz. Dilution cryostat, polarising magnet, microwave, NMR Two holding coils: solenoid → longitudinal, saddle coil → transverse Detectors have to move
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Conclusions We are running a full program of Transverse proton and neutron (deuteron) polarized target measurements. (Longitudinal will follow.) Circularly and linearly polarized tagged photons. Have preliminary results for F. MAMI B and MAMI C experiments are being analyzed and prepared for publication by a large group of students. Expect at least a 5 year program with CB and TAPS at MAMI!
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