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On the near-threshold incoherent photoproduction on the deuteron: Any trace of a resonance? MIN16, Kyoto University July 2016 Alvin Stanza Kiswandhi 1 , 2 In collaboration with: Shin Nan Yang 2 and Yu Bing Dong 3 1 Surya School of Education,


  1. On the near-threshold incoherent φ photoproduction on the deuteron: Any trace of a resonance? MIN16, Kyoto University July 2016 Alvin Stanza Kiswandhi 1 , 2 In collaboration with: Shin Nan Yang 2 and Yu Bing Dong 3 1 Surya School of Education, Tangerang 15810, Indonesia 2 Center for Theoretical Sciences and Department of Physics, National Taiwan University, Taipei 10617, Taiwan 3 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  2. Motivation • Presence of a local peak near threshold at E γ ∼ 2 . 0 GeV in the differential cross-section (DCS) of γp → φp at forward angle by Mibe and Chang, et al. [PRL 95 182001 (2005)] from the LEPS Collaboration . → Observed also recently by JLAB : B. Dey et al. [PRC − 89 055208 (2014)], and Seraydaryan et al. [PRC 89 055206 (2014)]. • Conventional model of Pomeron plus π and η ex- changes usually can only give rise to a monotonically- increasing behavior. • We would like to see whether this local peak can be explained as a resonance . • In order to check this assumption, we apply the results on γp → φp to γd → φpn to see if we can describe the latter . 1 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  3. Reaction model for γp → φp • Here are the tree-level diagrams calculated in our model in an effective Lagrangian approach. γ γ φ φ γ γ φ φ π,η Pomeron N* N* p p p p p p p p (a) (b) (c) (d) N ∗ is the postulated resonance. – p i is the 4-momentum of the proton in the initial state, – k is the 4-momentum of the photon in the initial state, – p f is the 4-momentum of the proton in the final state, – q is the 4-momentum of the φ in the final state. 2 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  4. • Pomeron exchange We follow the work of Donnachie, Landshoff, and Nacht- mann → Pomeron-isoscalar-photon analogy − • π and η exchanges For t -channel exchange involving π and η , we use effec- tive Lagrangian approach . • Resonances Only spin 1 / 2 or 3 / 2 because the resonance is close to the threshold . → Effective Lagrangian approach for the vertices , and − Breit-Wigner form for the propagators . 3 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  5. Fitting to γp → φp experimental data • We include only one resonance at a time . • We fit only masses , widths , and coupling constants of the resonances to the experimental data, while other parameters are fixed during fitting. • Experimental data to fit – Differential cross sections (DCS) at forward angle – DCS as a function of t at eight incoming photon energy bins – Nine spin-density matrix elements (SDME) at three incoming photon energy bins 4 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  6. Results for γp → φp • Both J P = 1 / 2 ± resonances cannot fit the data . • DCS at forward angle and as a function of t are markedly improved by the inclusion of the J P = 3 / 2 ± reso- nances. • In general, SDME are also improved by both J P = 3 / 2 ± resonances. • Decay angular distributions , not used in the fitting proce- dure, can also be explained well. • We study the effect of the resonance to the DCS of γp → ωp . → The resonance seems to have a considerable amount of − strangeness content . 5 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  7. J P = 3 / 2 + J P = 3 / 2 − M N ∗ (GeV) 2.08 ± 0.04 2.08 ± 0.04 Γ N ∗ (GeV) 0.501 ± 0.117 0.570 ± 0.159 eg (1) γNN ∗ g (1) 0.003 ± 0.009 − 0.205 ± 0.083 φNN ∗ eg (1) γNN ∗ g (2) − 0.084 ± 0.057 − 0.025 ± 0.017 φNN ∗ eg (1) γNN ∗ g (3) 0.025 ± 0.076 − 0.033 ± 0.017 φNN ∗ eg (2) γNN ∗ g (1) 0.002 ± 0.006 − 0.266 ± 0.127 φNN ∗ eg (2) γNN ∗ g (2) − 0.048 ± 0.047 − 0.033 ± 0.032 φNN ∗ eg (2) γNN ∗ g (3) 0.014 ± 0.040 − 0.043 ± 0.032 φNN ∗ χ 2 /N 0.891 0.821 • The ratio A 1 / 2 /A 3 / 2 = 1 . 05 for the J P = 3 / 2 − resonance. • The ratio A 1 / 2 /A 3 / 2 = 0 . 89 for the J P = 3 / 2 + resonance. 6 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  8. Reaction model for γd → φpn N N N N N φ φ φ N N N φ N N N φ N N N M M M N + + + + N N N N N N N N N γ γ γ γ γ d d d d d (a) (b) (c) (d) (e) • We calculate only (a) and (b) , as (c), (d), and (e) are estimated to be small . • We want to know if the resonance would manifest itself in dif- ferent reaction . 7 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  9. p n p n φ p p p n φ q p p p n p + + pn interchange n q p’ 1 p 2 p γ p 2 p γ p 1 p 1 k p d k p d d d • Fermi motion of the proton and neutron inside the deuteron is included using deuteron wave function calculated by Machleidt in PRC 63 024001 (2001). • Final-state interactions (FSI) of pn system is included using Nijmegen pn scattering amplitude. • On- and off-shell parts of the pn propagator are included. 1 P 1 − E 2 − iπδ ( E p + E n − E ′ 1 − E 2 + iǫ = 1 − E 2 ) − → E p + E n − E ′ E p + E n − E ′ 8 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  10. • The same model for the amplitude of γp → φp . → Realistic model − → Correct spin structure is maintained − • A J P = 3 / 2 − resonance is also present in the γn → φn amplitude – For φnn ∗ vertex , φp and φn cases are the same since φ is an I = 0 particle . – For γnn ∗ vertex , we assume that the resonance would have the same properties, including its coupling to γn , as a CQM state with the same isospin, J P , and similar value of A 1 / 2 /A 3 / 2 for the γp decay − (2095)[ D 13 ] 5 in Capstick’s work in PRD 46 , 2864 → N 3 − 2 (1992), the only one with positive value of A 1 / 2 /A 3 / 2 for γp in the energy region . 9 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  11. Results for γd → φpn • Notice that no fitting is performed to the LEPS data on DCS [PLB 684 6-10 (2010)] and SDME [PRC 82 015205 (2010)] of γd → φpn from Chang et al. . → We use directly the parameters resulting from − γp → φp . • We found a fair agreement with the LEPS experimental data on both observables. • Resonance , Fermi motion , and pn FSI effects are found to be large . → Without them , the DCS data cannot be described. − 10 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  12. DCS of γd → φpn Not fitted 1.8 1.8 1.57<E γ <1.67 GeV 1.67<E γ <1.77 GeV LEPS data 1.2 1.2 FSI -2 ) No FSI No FSI - NR d σ d /dt φ ( µ b GeV 0.6 0.6 No FSI - R 0 0 1.77<E γ <1.87 GeV 1.87<E γ <1.97 GeV 1.2 1.2 0.6 0.6 0 0 -0.6 -0.4 -0.2 0 -0.6 -0.4 -0.2 0 2 ) t φ -t max (proton) (GeV 11 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  13. DCS of γd → φpn Not fitted 1.8 1.8 2.07<E γ <2.17 GeV 1.97<E γ <2.07 GeV 1.2 1.2 -2 ) d σ d /dt φ ( µ b GeV 0.6 0.6 0 0 2.17<E γ <2.27 GeV 2.27<E γ <2.37 GeV 1.2 1.2 0.6 0.6 0 0 -0.6 -0.4 -0.2 0 -0.6 -0.4 -0.2 0 2 ) t φ -t max (proton) (GeV 12 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  14. DCS of γd → φpn Not fitted 1.8 1.8 1.57<E γ <1.67 GeV 1.67<E γ <1.77 GeV LEPS data Only FSI 1.2 1.2 free p and n Only FSI on-shell -2 ) FSI FSI on-shell d σ d /dt φ ( µ b GeV 0.6 0.6 No FSI 0 0 1.77<E γ <1.87 GeV 1.87<E γ <1.97 GeV 1.2 1.2 0.6 0.6 0 0 -0.6 -0.4 -0.2 0 -0.6 -0.4 -0.2 0 2 ) t φ -t max (proton) (GeV 13 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  15. DCS of γd → φpn Not fitted 1.8 1.8 2.07<E γ <2.17 GeV 1.97<E γ <2.07 GeV 1.2 1.2 -2 ) d σ d /dt φ ( µ b GeV 0.6 0.6 0 0 2.17<E γ <2.27 GeV 2.27<E γ <2.37 GeV 1.2 1.2 0.6 0.6 0 0 -0.6 -0.4 -0.2 0 -0.6 -0.4 -0.2 0 2 ) t φ -t max (proton) (GeV 14 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  16. DCS of γd → φpn Not fitted 0.5 1.65<E γ <1.75 GeV 0.4 -2 ) d σ d /dt φ ( µ b GeV 0.3 0.2 0.1 0 -1 -0.9 -0.8 -0.7 -0.6 -0.5 -0.4 2 ) t φ -t max (proton) (GeV 15 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  17. DCS of γd → φpn and its ratio to twice DCS of γp → φp at forward angle Not fitted t φ = t max (proton) 2 -2 ) (a) FSI d σ d /dt φ ( µ b GeV 1.5 no FSI 1 0.5 0 1.5 1.6 1.7 1.8 1.9 2 2.1 2.2 2.3 2.4 1 (d σ d /dt φ )/(2 d σ p /dt φ ) (b) 0.8 0.6 0.4 0.2 0 1.7 1.8 1.9 2 2.1 2.2 2.3 2.4 1.5 1.6 E γ (GeV) 16 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

  18. SDME of γd → φpn as a function of t Not fitted 1.77 < E γ < 1.97 GeV 0.2 0 0 0 ρ ρ ρ 00 10 1-1 0.1 Spin-density matrix elements 0 1 1 1 ρ 0.2 ρ ρ 00 11 10 0 -0.2 0.5 2 Im ρ 1-1 0 1 2 ρ Im ρ 1-1 10 -0.5 0 0.05 0.1 0.15 0.05 0.1 0.15 0.05 0.1 0.15 2 ) |t φ - t max (proton)| (GeV 17 • First • Prev • Next • Last • Go Back • Full Screen • Close • Quit

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