Chiral Approach to the Phi Radiative Decays and the Quark Structure of the Scalar Meson Masayasu Harada (Nagoya Univ.) based HEP-Nuclear Physics Cross Over Meeting (May 27, Nara Women's University, Nara, Japan) D.Black, M.H. and J.Schechter, Phys. Rev. Lett. 88, (2002) D.Black, M.H. and J.Schechter, in preparation.
☆ A possible structure of Pentaquarks Jaffe-Wilczek, PRL 91, ; Shuryak-Zahed, hep-ph/ s u d diquarks Θ + ~ ・・・ play an important role It is interesting to study other bound states including diquarks. Diquarks give a new information on forces between 2 quarks in QCD. qq 3 × 3 → 1 Most Atractive Channel q q 3 × 3 → 3 Next MAC ⇒ Important for Color SuperConductivity
☆ Possible bound states including diquarks other than pentaquarks q q baryons ? q ordinary mesons ? q dibaryons ? ordinary mesons X(3872) ?
☆ Light Scalar mesons ◎ Properties interactions with other mesons ・・・ quark structure ・・・ 2-quark or 4-quark ? scalar nonet ◎ Effective Lagrangian study of the properties of the scalar mesons ・ Radiative decays involving scalar mesons Exotic hadron ?
Outline 1. Introduction 2. Quark Structure of Light Scalar Mesons 3. Effective Lagrangian for Scalar Mesons - Masses of scalar mesons and thier couplings to pseudoscalar mesons - 4. Radiative Decays Involving Scalar Mesons 5. Summary
☆ 2-quark picture ◎ “experiment” contradict ? ⇔ ρ, ω ⇔ K*⇔ K* ⇔ φ⇔ φ
☆ 4-quark picture ☆ diquark one-gluon exchange gives atraction in ◎ scalar diquarks ◎ scalar anti-diquarks
☆ Scalar nonet consistent with “experiment” !
- Masses of scalar mesons and their couplings to pseudoscalar mesons -
☆ Scalar meson nonet field cf: vector meson nonet field D.Black, A.H.Fariborz, F.Sannino and J.Schechter, PRD 59, (1999)
☆ Relation to quark structure
☆ Mass terms for scalar nonet - m s d = 2 m s b = 2 c < 0 quark mass
c = d = 0 ; b < 0
D.Black, A.H.Fariborz, F.Sannino and J.Schechter, PRD 59, (1999)
A.H.Fariborz and J.Schechter, PRD 60, (1999) ◎ Fit π-π scattering ☆ An effective Lagrangian for the interactions among one scalar meson and two pseudoscalar mesons from hadronic decays ◎ light pseudoscalar mesons (p, K, h) ・・・ approximate Nambu-Goldstone bosons ☆ Pseudoscalar mesons couple to other mesons with derivative interaction
D.Black, M.H. and J.Schechter, Phys. Rev. Lett. 88, (2002) D.Black, M.H. and J.Schechter, in preparation
scalar → + vector → scalar + scalar → vector + ☆ Radiative decays involving light scalar mesons ◎ Effective Lagrangian ← SU(3) L ×SU(3) R chiral symmetry + vector meson dominance
☆ Vector Meson Dominance (VMD) in (N→ ), (V→N ) and (N→V ) N V = V V N N V V N →γγV → Nγ N → Vγ VMD → NVV vertex determines (N→ ), (V→N ) and (N→V )
☆ SU(3) L ×SU(3) R chiral symmetry + VMD ☆ Effective Lagrangian for NVV vertices ・・・ not contribute
◎ Inputs ・・・ It may be difficult to distinguish two pictures from radiative decays !? ☆ Predictions (GeV -1 ) (keV)
☆ → f 0 decay ◎ prediction from present analysis ・ K-loop effect gives an important contribution N.N.Achasov and V.N.Ivanchenko, NPB315, 465 (1989) F.E.Close, N.Isgur and S.Kumano, NPB389, 513 (1993) ・・・ 1.87±0.11 keV ◎ Inclusion of mixing to f 0 (1370), f 0 (1500), f 0 (1700) helps but not enough (Teshima-Kitamura-Morisita, hep-ph/ ) ◎ Similar contribution for derivative coupling ? → Let us study φ→π 0 ηγ decay
☆ → 0 through 00 poor fit for
☆ → 0 through with K-loop K K Note : Exact Cancellation of divergences ・ good fit for ・ poor fit for
00 K K ☆ → 0 through with and without K-loop Good agreement with experiment !
☆ Analysis on the quark structure of the scalar mesons based on the effective Lagrangian approach hadronic processes ⇒ mass hierarchy ☆ Radiative decays involving scalar mesons Problems in φ→π 0 π 0 γand φ→ηπ 0 γ decays ⇒ Inclusion of K-loop effects gives a good fit to experimental data. Both pictures predict similar values for several radiative decays. ⇒ It may be difficult to distinguish two pictures from radiative decays !?
☆ Future directions Study the φ→π 0 π 0 γ decay Include K-loop into a 0, f 0 propagators Include non-resonant background Study several radiative decays ・・・ Explore the structure of the light scalar nonet