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Results of Nucleon Resonance Extraction via Dynamical Coupled-Channels Analysis from Collaboration @ EBAC Hiroyuki Kamano (RCNP, Osaka U.) QNP2012, Palaiseau, France, April 16-20, 2012

Hiroyuki Kamano (RCNP, Osaka U.)

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Results of Nucleon Resonance Extraction via Dynamical Coupled-Channels Analysis from Collaboration @ EBAC. Hiroyuki Kamano (RCNP, Osaka U.). QNP2012, Palaiseau , France, April 16-20, 2012. Outline. 1. Background and motivation for N* spectroscopy - PowerPoint PPT Presentation

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Page 1: Hiroyuki Kamano (RCNP, Osaka U.)

Results of Nucleon Resonance Extraction via Dynamical Coupled-Channels Analysis from

Collaboration @ EBAC

Hiroyuki Kamano(RCNP, Osaka U.)

QNP2012, Palaiseau, France, April 16-20, 2012

Page 2: Hiroyuki Kamano (RCNP, Osaka U.)

Outline1. Background and motivation for N* spectroscopy

2. Results of nucleon resonance extraction from Collaboration@EBAC

3. Summary and future works

Description of Dynamical Coupled-Channels (DCC) model Results of DCC analysis (2006-2009) Results of DCC analysis (2010-2012)

Page 3: Hiroyuki Kamano (RCNP, Osaka U.)

N* spectroscopy : Physics of broad & overlapping resonances

Δ (1232)

Width: a few hundred MeV. Resonances are highly overlapping   in energy except D(1232).

Width: ~10 keV to ~10 MeV Each resonance peak is clearly separated.

N* : 1440, 1520, 1535, 1650, 1675, 1680, ...D : 1600, 1620, 1700, 1750, 1900, …

Page 4: Hiroyuki Kamano (RCNP, Osaka U.)

N* states and PDG *s

?

?

?

?

?

Arndt, Briscoe, Strakovsky, Workman PRC 74 045205 (2006)

Most of the N*s were extracted from

Need comprehensive analysis of

channels !!

Page 5: Hiroyuki Kamano (RCNP, Osaka U.)

Hadron spectrum 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.

Quark models, Bag models, Dyson-Schwinger approaches, Holographic QCD,… Excited hadrons are treated as stable particles. The resulting masses are real.

What is the role of reaction dynamics in interpretingthe hadron spectrum, structures, and dynamical origins ??

“Mass” becomes complex !! “pole mass” u

u d

Constituent quark modelN*

bare state

meson cloud

“molecule-like” states

core (bare state) + meson cloud

Page 6: Hiroyuki Kamano (RCNP, Osaka U.)

Objectives and goals:

Through the comprehensive analysis of world data of pN, gN, N(e,e’) reactions,

Determine N* spectrum (pole masses)

Extract N* form factors

(e.g., N-N* e.m. transition form factors)

Provide reaction mechanism information necessary for interpreting N* spectrum, structures and dynamical origins

Collaboration at Excited Baryon Analysis Center (EBAC) of Jefferson Lab

http://ebac-theory.jlab.org/

Spectrum, structure,…of N* states

QCD

Lattice QCDHadron Models

Analysis Based on Reaction Theory

Reaction Data

“Dynamical coupled-channels model of meson production reactions”

A. Matsuyama, T. Sato, T.-S.H. Lee Phys. Rep. 439 (2007) 193

Founded in January 2006

Page 7: Hiroyuki Kamano (RCNP, Osaka U.)

Partial wave (LSJ) amplitudes of a b reaction:

Reaction channels:

Transition Potentials:

coupled-channels effect

Exchange potentials bare N* states

For details see Matsuyama, Sato, Lee, Phys. Rep. 439,193 (2007)

Z-diagrams

Dynamical coupled-channels (DCC) model for meson production reactions

Meson-Baryon Green functions

Stable channels Quasi 2-body channels

N pD

p

D

ppp

r, s r, s

N N

p, r, s, w,..

N N, D

s-channel u-channel t-channel contact

Exchange potentials

Z-diagrams

Bare N* statesN*bare

Dp

N p

p

DDNp

r, s

Can be related to hadron states of the static hadron models (quark models, DSE, etc.)excluding meson-baryon continuum.

core

meson cloud

meson

baryon

Physical N*s will be a “mixture” of the two pictures:

Page 8: Hiroyuki Kamano (RCNP, Osaka U.)

DCC analysis @ EBAC (2006-2009)

p N p N : Analyzed to construct a hadronic part of the model up to W = 2 GeVJulia-Diaz, Lee, Matsuyama, Sato, PRC76 065201 (2007)

p N h N : Analyzed to construct a hadronic part of the model up to W = 2 GeVDurand, Julia-Diaz, Lee, Saghai, Sato, PRC78 025204 (2008)

p N p p N : Fully dynamical coupled-channels calculation up to W = 2 GeVKamano, Julia-Diaz, Lee, Matsuyama, Sato, PRC79 025206 (2009)

g(*) N p N : Analyzed to construct a E.M. part of the model up to W = 1.6 GeV and Q2 = 1.5 GeV2

(photoproduction) Julia-Diaz, Lee, Matsuyama, Sato, Smith, PRC77 045205 (2008) (electroproduction) Julia-Diaz, Kamano, Lee, Matsuyama, Sato, Suzuki, PRC80 025207 (2009)

g N p p N : Fully dynamical coupled-channels calculation up to W = 1.5 GeV Kamano, Julia-Diaz, Lee, Matsuyama, Sato, PRC80 065203 (2009)

Extraction of N* pole positions & new interpretation on the dynamical origin of P11 resonancesSuzuki, Julia-Diaz, Kamano, Lee, Matsuyama, Sato, PRL104 065203 (2010)

Stability and model dependence of P11 resonance poles extracted from pi N pi N dataKamano, Nakamura, Lee, Sato, PRC81 065207 (2010)

Extraction of gN N* electromagnetic transition form factorsSuzuki, Sato, Lee, PRC79 025205 (2009); PRC82 045206 (2010)

Hadronic part

Electromagnetic part

Extraction of N* parameters

gN, pN, hN, pD, rN, sN coupled-channelscalculations were performed.

Page 9: Hiroyuki Kamano (RCNP, Osaka U.)

Dynamical origin of nucleon resonances

Pole positions and dynamical origin of P11 resonances

Suzuki, Julia-Diaz, Kamano, Lee, Matsuyama, Sato, PRL104 065203 (2010)

pole A: pD unphys. sheetpole B: pD phys. sheet Two-pole nature of the Roper is found

also from completely different approaches:

Eden, Taylor, Phys. Rev. 133 B1575 (1964)

Multi-channel reactions can generate many resonance poles from a single bare state !!

For evidences in hadron and nuclear physics, see e.g., in Morgan and Pennington, PRL59 2818 (1987)

Page 10: Hiroyuki Kamano (RCNP, Osaka U.)

N-N* transition form factors at resonance poles

Julia-Diaz, Kamano, Lee, Matsuyama, Sato, Suzuki PRC80 025207 (2009)Suzuki, Sato, Lee, PRC82 045206 (2010)

Real part Imaginary part

Nucleon - 1st D13 e.m. transition form factors

Coupling to meson-baryon continuum states makes N* form factors complex !!

Fundamental nature of resonant particles (decaying states)

Extracted from analyzing the p(e,e’p)N data (~ 20000) from CLAS

Page 11: Hiroyuki Kamano (RCNP, Osaka U.)

Dynamical coupled-channels (DCC) analysis

pp pN

gp pN

pp hN

gp hp

pp KL, KS

gp K+L, KS

2006 - 2009

6 channels (gN,pN,hN,pD,rN,sN)

< 2 GeV

< 1.6 GeV

< 2 GeV

2010 - 2012

8 channels (gN,pN,hN,pD,rN,sN,KL,KS)

< 2.1 GeV

< 2 GeV

< 2 GeV

< 2 GeV

< 2.1 GeV

< 2.2 GeV

# of coupled channels

Fully combined analysis of pN , gN pN , hN , KL, KS reactions !!

Kamano, Nakamura, Lee, Sato(2012)

(~ 28,000 data points to fit)

Page 12: Hiroyuki Kamano (RCNP, Osaka U.)

Partial wave amplitudes of pi N scattering

8ch DCC-analysis(Kamano, Nakamura, Lee, Sato2012)

6ch DCC-analysis(fitted to pN pN data only)[PRC76 065201 (2007)]

Real part

Imaginary part

Page 13: Hiroyuki Kamano (RCNP, Osaka U.)

Single pion photoproduction

6ch DCC-analysis [PRC77 045205 (2008)](fitted to gN pN data up to 1.6 GeV)

Angular distribution Photon asymmetry

1137 MeV 1232 MeV

1334 MeV

1462 MeV 1527 MeV 1617 MeV

1729 MeV 1834 MeV 1958 MeV

1137 MeV 1232 MeV 1334 MeV

1462 MeV 1527 MeV 1617 MeV

1729 MeV 1834 MeV 1958 MeV

8ch DCC-analysisKamano, Nakamura, Lee, Sato 2012

Page 14: Hiroyuki Kamano (RCNP, Osaka U.)

1535 MeV

1674 MeV

1811 MeV

1930 MeV

1549 MeV

1657 MeV

1787 MeV

1896 MeV

Eta production reactions

Analyzed data up to W = 2 GeV. p- p h n data are selected following Durand et al. PRC78 025204.

Photon asymmetry

Kamano, Nakamura, Lee, Sato, 2012

Page 15: Hiroyuki Kamano (RCNP, Osaka U.)

KY production reactions

1732 MeV

1845 MeV

1985 MeV

2031 MeV

1757 MeV

1879 MeV

1966 MeV

2059 MeV

1792 MeV

1879 MeV

1966 MeV

2059 MeV

Kamano, Nakamura, Lee, Sato, 2012

1781 MeV 1785 MeV

Polarizations are calculated using the formulae in Sandorfi, Hoblit, Kamano, Lee, J. Phys. G 38, 053001 (2011)

Page 16: Hiroyuki Kamano (RCNP, Osaka U.)

Spectrum of N* resonances(Current status)

Real parts of N* pole values

L2I 2J

PDG Ours

N* with 3*, 4* 1816

N* with 1*, 2* 5PDG 4*

PDG 3*

Ours

Kamano, Nakamura, Lee, Sato, 2012

Page 17: Hiroyuki Kamano (RCNP, Osaka U.)

Note: Some freedom exists on the definition of partial width from the residue of the amplitudes.

Width of N* resonances(Current status)

Kamano, Nakamura, Lee, Sato, 2012

Page 18: Hiroyuki Kamano (RCNP, Osaka U.)

Summary and future works (1/2)

;

pp pN

gp pN

pp hN

gp hp

pp KL, KS

gp K+L, KS

2006 - 2009

6 channels (gN,pN,hN,pD,rN,sN)

< 2 GeV

< 1.6 GeV

< 2 GeV

2010 - 2012

8 channels (gN,pN,hN,pD,rN,sN,KL,KS)

< 2.1 GeV

< 2 GeV

< 2 GeV

< 2 GeV

< 2.1 GeV

< 2.2 GeV

# of coupled channels

Summary

Two-pole structure of the Roper resonance. One-to-multi correspondence between bare N*s (= static hadrons) and physical resonances. Reaction dynamics can produce sizable mass shift for N*s.

May be a key to understanding the issues in the static hadron models. Complex nature of the resonance form factors.

Mass spectrum, decay widths, and N-N* e.m. transition form factors, etc.have been determined for N* resonances in W < 2 GeV.

Multi-channel reaction dynamics plays a crucial role for understanding the N* parameters (spectrum, formfactors etc) !!

Page 19: Hiroyuki Kamano (RCNP, Osaka U.)

Collaborators @ EBACJ. Durand (Saclay)

B. Julia-Diaz (Barcelona U.)

H. Kamano (RCNP, Osaka U.)

T.-S. H. Lee (Argonne Nat’l Lab.)

A. Matsuyama (Shizuoka U.)

S. Nakamura (JLab)

B. Saghai (Saclay)

T. Sato (Osaka U./KEK)

C. Smith (Virginia, JLab)

N. Suzuki (Osaka U.)

K. Tsushima (Adelaide U.)

Page 20: Hiroyuki Kamano (RCNP, Osaka U.)

Add wN channel and complete the 9 coupled-channels analysis of the pp, gp pN, hN, KY, wN data. (Kamano, Nakamura, Lee, Sato)

Applications to p(n, mp), p(n, mh) reactions beyond the D region (W > 1.3 GeV) and study axial form factors of N*.

A part of the new collaboration “Toward unified description of lepton-nucleus reactions from MeV to GeV region” at J-PARC branch of KEK theory center:(Y. Hayato, M. Hirai, H. Kamano, S. Kumano, S. Nakamura, K. Saito, M. Sakuda, T. Sato)

Summary and future works (2/2)Future works

Applications to strangeness production reactions (Kamano, Nakamura, Lee, Oh, Sato)

Y* spectroscopy, YN & YY interactions, hypernucleus, .. (related to J-PARC physics)

Applications to meson spectroscopy via heavy-meson decaysKamano, Nakamura, Lee, Sato, PRD84 114019 (2011)

p p

g X Exotic hybrids?

GlueX experiment at HallD@JLabf0, r, ..

J/Y

Heavy meson decays

g

X Details are given in S. Nakamura’s talk(Today’s session B

16:35-16:55)

gN, pN, hN, pD, rN, sN, KL, KS, wN

Page 21: Hiroyuki Kamano (RCNP, Osaka U.)

back up

Page 22: Hiroyuki Kamano (RCNP, Osaka U.)

Since the late 90s, huge amount of high precision data of meson photo-production reactions on the nucleon target has been reported from electron/photon beam facilities.

JLab, MAMI, ELSA, GRAAL, LEPS/SPring-8, …

Experimental developments

E. Pasyuk’s talk at Hall-B/EBAC meeting

Opens a great opportunity to make quantitative study of the N* states !!

Page 23: Hiroyuki Kamano (RCNP, Osaka U.)

Kamano, Nakamura, Lee, Sato, 2012

Page 24: Hiroyuki Kamano (RCNP, Osaka U.)

Kamano, Nakamura, Lee, Sato 2012

Page 25: Hiroyuki Kamano (RCNP, Osaka U.)

Kamano, Nakamura, Lee, Sato2012

Page 26: Hiroyuki Kamano (RCNP, Osaka U.)

Kamano, Nakamura, Lee, Sato, 2012

Page 27: Hiroyuki Kamano (RCNP, Osaka U.)

Single pion electroproduction (Q2 > 0)

Fit to the structure function data (~ 20000) from CLAS

Julia-Diaz, Kamano, Lee, Matsuyama, Sato, Suzuki, PRC80 025207 (2009)

p (e,e’ p0) p

W < 1.6 GeVQ2 < 1.5 (GeV/c)2

is determinedat each Q2.

N*N

g (q2 = -Q2)q

N-N* e.m. transitionform factor

Page 28: Hiroyuki Kamano (RCNP, Osaka U.)

Single pion electroproduction (Q2 > 0)Julia-Diaz, Kamano, Lee, Matsuyama, Sato, Suzuki, PRC80 025207 (2009)

p (e,e’ p0) p

p (e,e’ p+) n

Five-fold differential cross sections at Q2 = 0.4 (GeV/c)2

Page 29: Hiroyuki Kamano (RCNP, Osaka U.)

Data handled with the help of R. Arndt

pi N pi pi N reaction

Parameters used in the calculation are from pN pN analysis.

Kamano, Julia-Diaz, Lee, Matsuyama, Sato, PRC79 025206 (2009)

Full result

Phase spaceFull result

W (GeV)

s (m

b)

C. C. effect off

Page 30: Hiroyuki Kamano (RCNP, Osaka U.)

Double pion photoproductionKamano, Julia-Diaz, Lee, Matsuyama, Sato, PRC80 065203 (2009)

Parameters used in the calculation are from pN pN & gN pN analyses.

Good description near threshold

Reasonable shape of invariant mass distributions

Above 1.5 GeV, the total cross sections of pp0p0 and pp+p-

overestimate the data.

Page 31: Hiroyuki Kamano (RCNP, Osaka U.)

Definition of N* parametersDefinitions of

N* masses (spectrum) Pole positions of the amplitudes

N* MB, gN decay vertices Residues1/2 of the pole

N* pole position ( Im(E0) < 0 )

N* b decay vertex

Page 32: Hiroyuki Kamano (RCNP, Osaka U.)

Scattering amplitude is a double-valued function of complex E !!

Essentially, same analytic structure as square-root function: f(E) = (E – Eth)1/2

e.g.) single-channel two-body scattering

unphysical sheet

physical sheet

Multi-layer structure of the scattering amplitudes

physical sheet

Re (E)

Im (E

)

0 0

Im (E

)

Re (E)

unphysical sheet

Re(E) + iε =“ physical world”

Eth(branch point)

Eth(branch point)× ×××

N-channels Need 2N Riemann sheets

2-channel case (4 sheets):(channel 1, channel 2) = (p, p), (u, p) ,(p, u), (u, u)

p = physical sheetu = unphysical sheet

Page 33: Hiroyuki Kamano (RCNP, Osaka U.)

N, N*

Meson cloud effect in gamma N N* form factors

GM(Q2) for g N D (1232) transition

Note:Most of the available static hadron models give GM(Q2) close to “Bare” form factor.

Full

Bare

Page 34: Hiroyuki Kamano (RCNP, Osaka U.)

“Static” form factor fromDSE-model calculation.(C. Roberts et al)

A clue how to connect with static hadron models

“Bare” form factor determined fromour DCC analysis.

g p Roper e.m. transition

Page 35: Hiroyuki Kamano (RCNP, Osaka U.)

Delta(1232) : The 1st P33 resonance

pN unphysical & pD unphysical sheet

pN physical & pD physical sheet

p N

p DpN unphysical & pD physical sheet

Real energy axis“physical world”

Complex E-plane

Suzuki, Julia-Diaz, Kamano, Lee, Matsuyama, Sato, PRL104 042302 (2010)

Im (E

)

Re (E)

Re (T) Im (T)

P33

1211-50i

Riemann-sheet for other channels: (hN,rN,sN) = (-, p, -)

pole 1211 , 50

BW 1232 , 118/2=59

In this case, BW mass & width can be a good approximation of the pole position.

Small background Isolated pole Simple analytic structure of the complex E-plane

Page 36: Hiroyuki Kamano (RCNP, Osaka U.)

Two-pole structure of the Roper P11(1440)

pN unphysical & pD unphysical sheet

pN physical & pD physical sheet

p N

p DpN unphysical & pD physical sheet

Real energy axis“physical world”

Complex E-plane

Suzuki, Julia-Diaz, Kamano, Lee, Matsuyama, Sato, PRL104 042302 (2010)

Im (E

)

Re (E)

Pole A cannot generate a resonance shape on“physical” real E axis.

Re (T)

Im (T)

B

A

P11

pD branch point prevents pole B from generating a resonance shape on “physical” real E axis.

1356-78i1364-105i

Riemann-sheet for other channels: (hN,rN,sN) = (p,p,p)BW 1440 , 300/2 = 150

Two 1356 , 78poles 1364 , 105

In this case, BW mass & width has NO clear relation with the resonance poles:

?