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Coherent -meson Photo-production from Deuterons Near Threshold. Wen-Chen Chang for LEPS collaboration Institute of Physics, Academia Sinica, Taiwan. Outline. Features of photo-production of -mesons from protons.
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Coherent -meson Photo-production from Deuterons Near Threshold Wen-Chen Chang for LEPS collaboration Institute of Physics, Academia Sinica, Taiwan
Outline • Features of photo-production of -mesons from protons. • What we learned from the results of photo-production of -mesons from protons. • Features of coherent production from deuterons. • Measurement of differential cross section and decay asymmetry of DD in the forward direction near threshold. • Summary
Pomeron exchanges0.08 g r, w,f g r, w Pomeron Meson exchanges-0.45 p,h,s・・・ p uud p Vector Meson Photoproduction from Protons
This fact makes the -photoproduction a unique process to determine Pomeron contribution and possible new processes near threshold! Diffractive Photoproduction of (ss) Mesons • Pseudo-scalar particle: • Negative power-law scaling of s. • Showing up at small energy. • Un-natural parity (= –1). • Exchange particles like ,, quark exchange. • OZI suppressed • Pomeron: • Positive power-law scaling of s. • Dominating at large energy. • Natural parity (=+1). • Exchange particles unknown; likely to be gluonic degree of freedom.
Glueball Hunt in PhotoproductionT. Nakano and H. Toki (1997) P1: Pomerons0.08 ; P2: daughter Pomeron s-1.73 , inspired by (0+ glueball, M23 GeV2) P1+P2 P1
f →K+K- K+ eg Decay Plane // g natural parity exchange (-1)J (Pomeron, 0+ glueball, scalar mesons) K- Photon Polarization K+ eg Decay Planeg unnatural parity exchange -(-1)J (Pseudoscalar mesons p,h) K- Polarization Observables with Linearly Polarized Photon
Decay Asymmetry 11-1 - Im 21-1 • Azimuthal angle distribution of : • For spin-conserving processes: • Pomeron exchange: 11-1= –Im 21-1 = +0.5, 11-1-Im 21-1 = +1 • , exchanges: 11-1= –Im 21-1 = – 0.5, 11-1-Im 21-1 = 1
d/dt at t=tmin of pp Peak Off Peak LEPS(2005)
Decay Angular Distributions of pp Forward angles; -0.2 < t+|t|min <0. GeV2 Curves: fit to the data. Peak 11-1=0.197 ±0.030 Off Peak 11-1=0.189 ±0.024 • W ∝ sin2qhelicity-conserving processesare dominating. • 11-10.2N/(N+UN) ~70%
Natural-parity exchange Coherent Photo-production from Deuteron DD • Beside the smallness of coupling constants g andgNN, can we further suppress the unnatural-parity exchange processes? Study coherent production from deuterons, iso-scalar target, where iso-vector -exchange is forbidden. Unnatural-parity exchange We expect a strong dominance of natural-parity exchange processes in diffractive DD.
LEPS Run Summary Experimental detail is referred to the talk by M. Sumihama in this session.
Measurement of Photo-production from Deuterons via K+K Decay Mode DX
LD2 LH2 Disentangle Coherent and Incoherent Interactions in Missing Mass Spectra MMd(,KK) DX MX
Differential Cross Section of Coherent Interactions • The fitted b becomes smaller as we move to the large |t-tmind| region. • At |t-tmind|<0.1 GeV2, • b=20.52.1 GeV-2 Consistent with: b=b(F) + b(gp→ fp) =18.6+3.4=22 GeV-2
Intercept: d/dt at t=tmind Consistency between SLH2 and LLH2. Preliminary
Stronger asymmetry Decay Angular Distributions at |t-tmind|<0.1 GeV2 with MMd Cuts
Pure natural-parity exchange Preliminary Decay Asymmetry of Coherent Interactions Coherent interaction DD is mostly contributed by natural-parity exchanges.
Energy Dependence of Optical Points of DD P1: Pomerons0.08 ; P2: daughter Pomeron s-1.73 , inspired by (0+, M23 GeV2) Preliminary
Summary • The first measurement differential cross section and decay asymmetry of DD in the forward direction near threshold. Disentanglement of coherent and incoherent events is done by the fit in the missing mass spectra. • Large exponential slope about 20. • The intercept of d/dt at t=tmind increases with beam energy. • Close-to-one decay asymmetry for the coherent interaction with LD2 target: significant dominance of natural-parity exchange processes. Consistent with theoretical prediction based on the elimination of unnatural-parity -exchange. • Combining with the measurements at higher energies, the optical points of DD near threshold is consistent with the standard Pomeron exchange near the threshold assuming the same energy dependence.
Consistent with the scenario: • not due to unnatural-parity processes ONLY. • possible presence of additional natural parity exchange • signature of 0+ glueball trajectory?? Peak and Off Peak
Coherent Photoproduction from Deuteron Titov et al., PRC 66, 022202 (2002) • Deuteron form factor leads to a steeper exponential slope in t distribution. • In scattering amplitude, the unnatural-parity iso-vector exchange is completely eliminated due to Tn= Tp. Decay asymmetrygets closer to +1.
Isospin Effect of Quasi-free Photoproduction from Nucleons Due to isospin factor 3: • gpp and gpp are of the same sign: constructive interference between -exchange and -exchange. • gnn (= gpp )and gnn (=gpp ) are of opposite sign: destructiveinterference between -exchange and -exchange. • Value of decay symmetry gets closer to +1 in nn, compared with pp. Titov et al., PRC 59, R2993 (1999)
Stronger asymmetry LD2 |I0U|2=0 LH2 Preliminary Missing Mass Spectra MMd(,KK) and Decay Asymmetry DX MX