Dynamical coupled-channels approach to meson-production reactions in the nucleon resonance region Hiroyuki Kamano (KEK) 2016 2nd HaPhy meeting “Hadron.

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Dynamical coupled-channels approach to meson-production reactions in the nucleon resonance region Hiroyuki Kamano (KEK) 2016 2nd HaPhy meeting “Hadron productions: Theory and Experiment” APCTP, Pohang, Korea, November 25-26, 2016

Outline PART I: Background & motivation for spectroscopic study of N* & Δ* baryon resonances PART II: Recent results from ANL-Osaka Dynamical Coupled-Channels (DCC) analysis

Background & motivation for spectroscopic PART I Background & motivation for spectroscopic study of N* & Δ* baryon resonances

Introduction: N* & Δ* spectroscopy Discovery of the Δ baryon (1952) Behavior of the π+ p & π- p cross sections implies the existence of a new baryon with isospin 3/2 !! π+ p total π- p total

Introduction: N* & Δ* spectroscopy Arndt, Briscoe, Strakovsky, Workman PRC74(2006)045205 N* Δ* ? N* & Δ* spectroscopy remains as central issue in the hadron physics !! Mass, width, spin, parity …? quark-gluon structure (form factors)? How produced in reaction processes? ... meson baryon “molecule-like” state multiquark state 3-quark state PDG(2016): http://pdg.lbl.gov

Static hadron models and reaction dynamics Various static hadron models have been proposed to calculate hadron spectrum and form factors. In reality, excited hadrons are “unstable” and can exist only as resonance states in hadron reactions. Constituent quark models, Dyson-Schwinger Eq. approaches, soliton models,... Excited hadrons are treated as stable particles. Capstick, Roberts, Prog. Part. Nucl. Phys 45(2000)S241 CQM results PDG N* baryon spectrum u d Constituent quark model What is the role of reaction dynamics in interpreting the hadron spectrum, structures, and dynamical origins ??

Light-quark hadron spectroscopy : Physics of broad & overlapping resonances Δ (1232) Width: ~10 keV to ~10 MeV Each resonance peak is clearly separated. ~ 20 resonances Width: a few hundred MeV. Resonances are highly overlapping   in energy except D(1232).

Cooperative efforts between experiments and theoretical analyses ELPH, ELSA, GRAAL, JLab, MAMI, SPring-8, ... Experiments Multichannel unitary condition: ANL-Osaka Argonne-Pittsburgh Bonn-Gatchina Carnegie-Mellon-Berkeley Dubna-Mainz-Taipei EBAC Giessen GWU/VPI Juelich-Bonn Karlsruhe-Helsinki KSU Zagreb … Theoretical analyses with coupled-channels framework Since late 90s e.g.) Meson photoproductions N N*, Δ* . πN ηN ππN KΛ KΣ ωN … γ

Why multichannel unitarity is so important ?? 1) Ensures conservation of probabilities in multichannel reaction processes (exclusive) γp reaction total cross sections Key essential to simultaneous analysis of various inelastic reactions. increasing predictivity of constructed reaction models 2) Defines proper analytic structure (branch points, cuts,…) of scattering amplitudes in the complex energy plane, as required by scattering theory Crucial for extracting resonances “correctly”, and avoiding WRONG resonance signals !! [e.g., Ceci et al, PRC84(2011)015205] Im(W) Re(W) πN ππN ηN πΔ e.g.) N*, Δ case × resonance pole

Approaches for coupled-channels analysis Multichannel unitary condition: Heitler equation: K-matrix: must be hermitian for real E. (on-shell) K-matrix approach: Dynamical-model approach: ANL-Osaka, Dubna-Mainz-Taipei, Juelich-Bonn,... Argonne-Pittsburgh, Bonn-Gatchina, Carnegie Mellon-Berkely, GWU/VPI, Karlsruhe-Helsinki, KSU, ... off-shell rescattering effect Heitler equation can be solved algebraically. Heitler equation becomes identical to Lippmann-Schwinger integral equation. Potential V is derived from a model Hamiltonian.

Why dynamical coupled-channels approach?? (on-shell) K-matrix Dynamical model Numerical cost Cheap - solve on-shell algebraic eq. (Analysis can be done quickly on PC.) (Very) Expensive - solve off-shell integral eq. (Supercomputers are needed.) Data fitting Efficient - K(E) can be parametrized as one likes Not so efficient - Form of V is severely constrained by theoretical input (model Hamiltonian) To understand the physics of reaction dynamics behind formation, structure, etc. of hadron resonances, one needs: Modeling reaction processes appropriately with a model Hamiltonian. ( not a simple “pole + polynomial” parametrization, etc.) Solving proper quantum scattering equation (LS eq.) in which off-shell rescattering effects are also appropriately contained. This can be achieved only by using the dynamical-model approach !!

Dynamical origin of P11 N* resonances (nontrivial feature of multichannel reaction dynamics) Would be related to a baryon state in static hadron models excluding meson-baryon continuums Move of poles by “gradually” strengthening channel couplings Turn on πΔ coupling Double-pole structure of the Roper resonance [Arndt 1985, Cutkosky 1990 Arndt 2006, Doring 2009 Suzuki 2010, Kamano 2010] Corresponding to N(1710)1/2+ Suzuki, Julia-Diaz, HK, Lee, Matsuyama, Sato, PRL104 042302 (2010)

Recent results from ANL-Osaka DCC analysis PART II Recent results from ANL-Osaka DCC analysis

Dynamical coupled-channels (DCC) model for meson production reactions For details see Matsuyama, Sato, Lee, Phys. Rep. 439(2007)193 HK, Nakamura, Lee, Sato, PRC(2013)035209 p, r, s, w,.. N N, D, ... s-channel u-channel t-channel contact Exchange potentials Z-diagrams Bare N* states N*bare D p r, s Partial-wave (LSJ) amplitudes of a  b reaction: Reaction channels: Transition Potentials: core meson cloud meson baryon Physical N*s will be a “mixture” of the two pictures: coupled-channels effect off-shell effect Meson-Baryon Green functions Stable channels Quasi 2-body channels N p D r, s Summing up all possible transitions between reaction channels !! ( satisfies multichannel two- and three-body unitarity) Momentum integral takes into account off-shell rescattering effects in the intermediate processes. + = … V π N η K Λ Δ e.g.)πN scattering Would be related with hadron states of the static hadron models (quark models, DSE, etc.) excluding meson-baryon continuums. Exchange potentials Z-diagrams bare N* states

Strategy for N* and Δ* spectroscopy 1) Construct a model by making χ2-fit of the world data of meson production reactions. Use supercomputers to accomplish coupled-channels analyses: Latest published model (8-channel): Made simultaneous analysis of - πN  πN(SAID amp) (W < 2.3 GeV) - πp  ηN, KΛ, KΣ (W < 2.1 GeV) - γp  πN, ηN, KΛ, KΣ (W < 2.1 GeV) - γ ‘n’  πN (W < 2 GeV) ~27,000 data points of both dσ/dΩ & spin-pol. obs. HK, Nakamura, Lee, Sato, PRC88(2013)035209 [updated in PRC94(2016)015201 ] γp total cross sections in N* region Region our model can cover 2) Search poles of scattering amplitudes by analytic continuation to a complex energy plane. Im(W) Re(W) |T| Branch point unphysical sheet physical Cut rotated from real W axis Pole position  (complex) resonance mass Residues  coupling strengths between resonance and meson-baryon channel 3) Extract resonance parameters defined by poles. Mass spectrum Partial decay widths

Baryon resonances as poles of scattering amplitudes There are attempts to link real energy spectrum of QCD in the finite volume to resonance pole masses. Dudek et al, PRL113(2014)182001 QCD spectrum in finite volume Phase shifts & inelasticity (Luescher’s formula) Extracted resonance poles (K-matrix analysis) (see also an approach based on the HAL QCD method: Inoue et al., NPA881(2012)881; Ikeda et al., arXiv:1602.03465) PROPER definition of Hadron resonance masses (complex)  Pole positions of scattering amplitudes in the lower-half of complex-W plane Transition amplitudes between  ~ Residues1/2 at the pole resonance and scattering states Residue at the pole ~ Energy eigenvalue = pole energy Transition matrix elements between ~ Residues1/2 at the pole resonance and scattering states Resonance theory based on Gamow vectors: [G. Gamow (1928), R. E. Peierls (1959), …] “Quantum resonance state is an (complex-)energy eigenstate of the FULL Hamiltonian of the underlying theory solved under the Purely Outgoing Boundary Condition (POBC).” Im(W) Re(W) physical sheet unphysical Branch point (channel threshold) cut W = MR Resonance pole position ( Im(MR) < 0 )

ANL-Osaka DCC approach to N* and Δ* HK, Nakamura, Lee, Sato, PRC88(2013)035209; 94(2016)015201 γp  π0p dσ/dΩ for W < 2.1 GeV Σ for W < 2.1 GeV Red: Updated model [PRC94(2016)015201] Blue: Original model [PRC88(2013)035209]

Extracted N* & Δ* mass spectrum (pole mass MR) J-PARC E45 experiment [Sako, Hicks et al.] πNππN data would provide crucial information on establishing Roper-like Δ resonance !! Partial decay widths N* & Δ* below Re(MR) ~ 1.7 GeV have been established (with one exception).

Electromagnetic transition form factors: quantitative understanding of N* & Δ* structure virtual g (q2 = -Q2 <0) q Q2: corresponds to “resolution” N-N* e.m. transition form factor “dressed”-quark core obscured by dense meson clouds “Partons” How effective d.o.f.s of baryon constituents changes with Q2 ?? ? Q2:small (low “resolution”) Q2:large (high “resolution”)

Role of reaction dynamics in form factors: Meson-cloud effect N-N* e.m. transition form factor Re[GM(Q2)] for g N  D (1232) M1 transition Most of the available static hadron models INDEED give GM(Q2) close to the “Bare” form factor !! N*, Δ* N virtual g (q2 = -Q2 <0) q Q2: corresponds to “resolution” = “bare” state (core composed of “dressed” quarks) meson cloud Bare + Full dressed Q2 increases Bare Meson cloud Julia-Diaz, Lee, Sato, Smith, PRC75 015205 (2007)

N* program at CLAS12: Find evidence of “dressed quarks” inside N* See, e.g., INT workshop “Spectrum and Structure of Excited Nucleon from Exclusive Electroproduction”, Nov. 14-18, 2016 http://www.int.washington.edu/PROGRAMS/16-62w/ “dressed”-quark core obscured by dense meson clouds Meson clouds become small; “dressed”-quark core dominates “Partons” “dressed”-quark with “running” mass Will be studied as a main N* program at CLAS12@JLab (E12-09-003, E12-06-108A) Q2:small (low “resolution”) Q2:large (high “resolution”) Running dressed quark mass “constituent” quark “current” quark Curves: a model based on Dyson-Schwinger equations (Landau gauge) Points: Lattice QCD e.g.) Cloet, Roberts, Prog.Part.Nucl.Phys.77(2014)1

E.M. transition form factors: Critical input to neutrino physics Neutrino-induced meson production reaction: W+, Z0 N ν N*, Δ* l-, ν V - A Neutrino collaboration@J-PARC Branch, KEK Theory Center http://nuint.kek.jp/index_e.html A review article for the neutrino collaboration (to be published in Rep. Prog. Phys.): Nakamura et al., arXiv:1610.01464 DCC model for neutrino-nucleon reactions: Nakamura, HK, Sato, PRC92(2015)025205 GOAL: Construct a unified model comprehensively describing neutrino-nucleon/nucleus reactions over QE, RES, and DIS regions !! Quasi elastic region QE Deep inelastic scattering DIS Resonance RES CP phase & mass hierarchy studies with atmospheric exp. T2K (long-baseline exp.) Vector part of the weak current matrix elements can be precisely determined with exclusive electroproduction data !! - Data for BOTH proton & deuteron (“neutron”) targets are required to make isospin decomposition of vector current. Key to precise determination of leptonic CP violation & neutrino mass hierarchy from next-generation neutrino-oscillation expt. at T2K and DUNE etc. [see. e.g., Alvarez-Ruso et al., New J. Phys. 16(2014)075015]

e.m. transition form factor: Analysis of electroproduction reactions: Determining N-N* e.m. transition form factors Meson electroproductions: γ* N e N*, Δ* e’ N-N* e.m. transition form factor e.m. transition form factor: Varies model parameters included only in the “bare” transition form factors. (Other parameters are fixed with the values obtained in πN & γN analysis.) N*, Δ* N g* = Bare Meson cloud + Database for 1π electroproduction@CLAS6 (Q2 < 6 GeV2) (W,Q2) region in the current analysis (Q2 < 6 GeV2, W < 1.7 GeV) + K+Λ, K+ Σ0, ππN electro- production data (W,Q2) region in the early analysis: Julia-Diaz, HK, Lee, Matsuyama, Sato, Suzuki, PRC80(2009)025207

Analysis of electroproduction reactions: Determining N-N. e. m Analysis of electroproduction reactions: Determining N-N* e.m. transition form factors Data for structure functions are obtained with the help of K. Joo and L. C. Smith. σT+εσL for ep  eπ0p Q2 = 1.15 GeV2, 1.10 < W < 1.69 GeV Q2 = 5.0 GeV2, 1.11 < W < 1.69 GeV PRELIMINARY PRELIMINARY Q2 = 3.0 GeV2, 1.11 < W < 1.69 GeV Q2 = 6.0 GeV2, 1.11 < W < 1.39 GeV PRELIMINARY PRELIMINARY cosθ cosθ

Extracted e.m. transition form factors N  Δ(1232)3/2+ transition form factor A3/2 [evaluated at Δ pole mass: MR = 1210 –i 50 MeV] meson cloud (current) PRELIMINARY PRELIMINARY - Full π N πN-loop Current = πN, ππN, ηN, KΛ, KΣ; 2 bare states in P33 JLMS = πN, ππN, ηN; 2 bare states in P33 [PRC80(2009)025207; 82(2010)045206] Sato-Lee = πN; 1 bare state in P33 [PRC63(2001)055201; 75(2007)015205]

Summary  Multichannel reaction dynamics in the origin of P11 N* resonances.  Meson-cloud effect on the transition form factors. N* & Δ* spectroscopy as physics of broad & overlapping resonances Cooperative efforts between experiments and theoretical analyses with coupled-channels framework are indispensable to establishing the spectrum. Reaction dynamics is a crucial part of understanding the spectrum, dynamical origin, and structure, ... of N* & Δ*. Dynamical coupled-channels approach is a suitable one to study the role of reaction dynamics. Establishing high-mass N* & Δ* resonances [Re(MR) > 1.7 GeV] Determining Q2 dependence of electromagnetic transition form factors for well-established low-lying N* & Δ* resonances. Major topics in N* & Δ* spectroscopy  “(over-)complete” experiments for photoproduction reactions (CLAS6, ELSA, MAMI,...)  Measurements of electroproduction reactions over wide Q2 range (CLAS6, CLAS12) Electroproduction analysis & extension of our DCC model are underway !!

Summary 2 ANL-Osaka DCC approach N* & Δ* spectroscopy - Early analyses of πN & γN reactions: PRC76(2007)065201; 77(2008)045205; 78(2008)025204 PRC79(2009)025206; 80(2009)065203; 81(2010)065207 PRL104(2010)042302 - Latest analysis of πN & γN reactions: PRC88(2013)035209; 88(2013)045203; 94(2016)015201 - Electroproduction analysis & Form factor extraction: PRC80(2009)025207; 82(2010)045206 Neutrino reactions - Calculation in Q2 = 0 limit: PRD86(2012)097503 - Full DCC-model calculation up to W = 2 GeV, Q2 = 3 GeV2: PRD92(2015)074024 DIS Deep inelastic scattering region QE Quasi elastic Atmospheric exp. T2K RES Resonance Collaboration@J-PARC Branch, KEK Theory Center [arXiv:1303.6032] http://j-parc-th.kek.jp/html/English/e-index.html ANL-Osaka DCC approach Λ* & Σ* spectroscopy - Λ*, Σ* resonance extractions via analysis of K-p & K-d reactions: PRC90(2014)065204; 92(2015)025205; arXiv:1608.03470 Meson spectroscopy - Formulation of 3-body unitary model for decays of mesons: PRD84(2011)114019 - Application to γp  M*N  (3π)N: PRD86(2012)114012

Predicted results for neutrino-induced reactions Nakamura, HK, Sato, arXiv:1506.03403; to appear in PRD The first-time full coupled-channels calculation of n-nucleon reactions beyond the Δ(1232) region !! Single pion production: ν p  μ- π+ p ν n  μ- π0 p ν n  μ- π+ n ν n  ν π- p Double pion production: KΛ production: dσ/dWdQ2 at Eν = 2 GeV ν n  μ- K+ Λ ν p  μ- π+ π0 p ν n  μ- π+ π- p

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Comparison of N* & Δ* spectrum between multichannel analyses HK, Nakamura, Lee, Sato, PRC88 (2013) 035209 Existence and mass spectrum are now well established for most low-lying resonances !! ( Next task: establish high-mass resonances) -2Im(MR) (“width”) Re(MR) MR : Resonance pole mass (complex) JP(L2I 2J) “N” resonance (I=1/2) JP(L2I 2J) “Δ” resonance (I=3/2) Re Im πN  πN P33 (I=3/2, JP=3/2+) amp. ### NOTE: Presented only N* and Δ* with -2Im(MR) < 400 MeV ### J : Juelich [EPJA49(2013)44] BG : Bonn-Gatchina [EPJA48(2012)5] PDG: 4* & 3* states assigned by PDG2012 AO : ANL-Osaka

Predicted results for neutrino-induced reactions Nakamura, HK, Sato, arXiv:1506.03403; to appear in PRD The first-time full coupled-channels calculation of n-nucleon reactions beyond the Δ(1232) region !! Single pion production: ν p  μ- π+ p ν n  μ- π0 p ν n  μ- π+ n ν n  ν π- p dσ/dQ2 for ν p  μ- π+ p (flux averaged for Eν) d2σ/dWdQ2 at Eν = 2 GeV ν p  μ- π+ p ν n  μ- π0 p + μ- π+ n

Predicted results for neutrino-induced reactions Nakamura, HK, Sato, arXiv:1506.03403; to appear in PRD Double pion production: ν p  μ- π+ π0 p ν p  μ- π+ π+ n ν n  μ- π+ π- p dσ/dWdQ2 at Eν = 2 GeV ν p  μ- π+ π0 p ν n  μ- π+ π- p KΛ production: ν n  μ- K+ Λ