neutrino-induced meson productions satoshi nakamura osaka university, japan collaborators : h....

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Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan borators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka U T.-S.H. Lee (Argonne Nat’l Lab)

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Page 1: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Neutrino-induced meson productions

Satoshi Nakamura

Osaka University, Japan

Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H. Lee (Argonne Nat’l Lab)

Page 2: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Contents

★ Introduction nN scattering in resonance region

★ Dynamical coupled-channels (DCC) model

Analysis of g , N pN , , , pN hN KL KS data

Extension to nN l-X ( X= , , , , pN ppN hN KL

KS )

★ Results for nN l-X

Page 3: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Introduction

Page 4: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Neutrino-nucleus scattering for n-oscillation experiments

n

Neutrino-nucleus interactions neutrino detectors (16O, 12C, 36Ar, … )

Neutrino-nucleus interactions need to be known for neutrino flux measurement

Page 5: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

DISregion

QEregion

RESregion

Next-generation exp. leptonic CP, mass hierarchy

-n nucleus scattering needs to be understood more precisely

Wide kinematical region with different characteristic

Combination of different expertise is necessary

Collaboration at J-PARC Branch of KEK Theory Center

http://j-parc-th.kek.jp/html/English/e-index.html

T2K

Neutrino-nucleus scattering for n-oscillation experiments

Atmospheric n

Page 6: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Resonance region (single nucleon)

D

2nd 3rd

Multi-channel reaction

2p production is comparable to 1p

h, K productions (n case: background of proton decay exp.)

(MeV)

(Data)

gN X

Page 7: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

GOAL : Develop nN-interaction model in resonance region

We develop a Unitary coupled-channels model

(multi-channel) Unitarity is missing Important 2 p production model is missing

Problems in previous models

★ Dynamical coupled-channels (DCC) model for , gN pN , , , , pN ppN hN KL

KS

★ Extension to nN l-X ( X= , , , , pN ppN hN KL KS )

Our strategy to overcome the problems…

Page 8: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Dynamical Coupled-Channels model

for meson productions

Page 9: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

,

Coupled-channel unitarity is fully taken into account

Kamano et al., PRC 88, 035209 (2013)

In addition, , gN W±N, ZN channels are included perturbatively

Page 10: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

DCC analysis of meson production data

Fully combined analysis of , gN pN , , , pN hN KL KSdata

and polarization observables (W ≤ 2.1 GeV)

~380 parameters (N* mass, N* MB couplings, cutoffs)

to fit ~ 20,000 data points

Kamano, Nakamura, Lee, Sato, PRC 88 (2013)

Page 11: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Partial wave amplitudes of p N scattering

Kamano, Nakamura, Lee, Sato,

PRC 88 (2013)

Previous model (fitted to pN pN data only)[PRC76 065201 (2007)]

Real part

Imaginary partData: SAID pN amplitude

Constraint on axial current through PCAC

Page 12: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Kamano, Nakamura, Lee, Sato, 2012

Vector current (Q2=0) for 1 p

Production is well-tested by data

Kamano, Nakamura, Lee, Sato, PRC 88 (2013)

Page 13: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Model for vector & axial currents is necessary

Extension to full kinematical region Q2≠0

DCC model for neutrino interaction

n

Forward limit Q2=0

Kamano, Nakamura, Lee, Sato, PRD 86 (2012)

spNX snNX via PCAC

Page 14: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Vector current

Q2=0

gp MB

gn pN isospin separation

necessary for calculating n-interaction

Q2≠0 (electromagnetic form factors for VNN* couplings)

obtainable from (e,e’ p), (e,e’ X) data analysis

We’ve done first analysis of all these reactions VNN*(Q2) fixed neutrino reactions

DCC model for neutrino interaction

Page 15: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Q2=0

non-resonant mechanisms

resonant mechanisms

Interference among resonances and background can be made under control within DCC model

Axial current

DCC model for neutrino interaction

Caveat : phenomenological axial currents are added to maintain PCAC relation

to be improved in future

Page 16: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Axial current

Q2≠0

non-resonant mechanisms

resonant mechanisms

DCC model for neutrino interaction

MA=1.02 GeV

: axial form factors

More neutrino data are necessary to fix axial form factors for ANN*

Sato et al. PRC 67 (2003)

Neutrino cross sections will be predicted with this axial current for this presentation

Page 17: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Analysis of electron scattering data

Page 18: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

• p(e,e’p0)p• p(e,e’p+)n• both

Analysis of electron-proton scattering data

Purpose : Determine Q2 –dependence of vector coupling of p-N* : VpN*(Q2)

Data : * 1 p electroproduction

Database

* Empirical inclusive inelastic structure functions s T , sL Christy et al, PRC 81 (2010)

region where inclusives T & sL are fitted

Page 19: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Analysis resultQ2=0.40 (GeV/c)2

s T + e sL for W=1.1 – 1.68 GeV

p(e,e’p0)p p(e,e’p+)n

Page 20: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Analysis resultQ2=0.40 (GeV/c)2

s T & sL (inclusive inelastic)

DCC

Christy et al PRC 81 s T

sL

region where inclusives T & sL are fitted

Page 21: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

For application to neutrino interactions

Analysis of electron scattering data

VpN*(Q2) & VnN*(Q2) fixed for several Q2 values

Parameterize VpN*(Q2) & VnN*(Q2) with simple analytic function of Q2

I=3/2 : VpN*(Q2) = VnN*(Q2) CC, NC

I=1/2 isovector part : ( VpN*(Q2) - VnN*(Q2) ) / 2 CC, NC

I=1/2 isoscalar part : ( VpN*(Q2) + VnN*(Q2) ) / 2 NC

DCC vector currents has been tested by data for whole kinematical region

relevant to neutrino interactions of En ≤ 2 GeV

Page 22: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Neutrino Results

Page 23: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Caveat

• Results presented here are still preliminary

• Careful examination needs to be made to obtain a final result

Page 24: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Cross section for nm N m- X

• pN & ppN are main channels in few-GeV region

• , hN KY cross sections are 10-1 – 10-2 smaller

nm n m- X nm p m- X

Page 25: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Comparison with nm N m- p N data

ANL Data : PRD 19, 2521 (1979)BNL Data : PRD 34, 2554 (1986)

DCC model prediction slightly undershoots data

• DCC model has flexibility to fit data (ANN*(Q2))• Data should be analyzed with nuclear effects

nm n m- p N nm p m-p+ p

Page 26: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Mechanisms for nm N m- p N

• (1232)D dominates for nm p m- p+ p (I=3/2) for En ≤ 2 GeV

• Non-resonant mechanisms contribute significantly

• Higher N*s becomes important towards En ≈ 2 GeV for nm n m- p N

nm n m- p N nm p m-p+ p

(1232)D (1232)D

Page 27: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

d / s dW dQ2 ( ×10-38 cm2 / GeV2)

nm n m- p N nm n m- pp N nm p m-p+ p nm p m-pp N

En = 2 GeV

Page 28: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Conclusion

Page 29: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Development of DCC model for nN interaction in resonance region

• pN & ppN are main channels in few-GeV region

• DCC model prediction slightly undershoots data

• , D N*s, non-resonant are all important in few-GeV region (for nm n m- X )

essential to understand interference pattern among them

DCC model can do this; consistency between p interaction and axial current  

Start with DCC model for , gN pN , , , , pN ppN hN KL KS

extension of vector current to Q2≠0 region, isospin separation

through analysis of e—- p & e—-’n’ data for W ≤ 2 GeV , Q2≤ 3 (GeV/c)2

Development of axial current for nN interaction; PCAC is maintained

Conclusion

Page 30: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Future development

• Axial form factor more neutrino data is ideal p N r N (t-ch p) (possible at J-PARC)

• ppN channel p N pp N experiment (J-PARC, K. Hicks et al.) g N pp N experiment (ELPH, JLab)

Page 31: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

BACKUP

Page 32: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Physics at J-PARC: Charm, Neutrino, Strangeness, and Spin

T2K (Tokai to Kamioka) experiment for neutrino oscillation measurement

Far Detector (Super Kamiokande)

T2K measures neutrino fluxes at near and far detectors

J-PARC produces neutrino beam directed to Super Kamiokande by

Proton + nucleus p - (p + ) + ….

nm + m - (nm + m + )_

Page 33: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Neutrino oscillation

Expected nm fluxes in T2K

Near detectorFar detector

En (GeV)

n m survival probability (two-flavor case)

q : mixing angle

Dm2 (eV2) = m12 – m2

2

L (km) : distance between J-PARC and SK

E n (GeV) : neutrino energy

Comparing data to oscillation formula, mixing parameters (q , Dm2 ) can be determined

Comparing n data with n data leptonic CP violation ( dCP ) _

Page 34: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

T2K

• Quasi-elastic (QE) is dominant

n-flux is measured by detecting QE

• 1 p production via -D excitation is major background

p can be absorbed QE is contaminated

nm

m-

𝜋nm

m-

D

LBNE and other planned experiments ( higher energy n-beam)

• DIS and higher nucleon resonances are main mechanisms

In this work, we focus on resonance region, single nucleon processes

basic ingredient for neutrino-nucleus interaction model

Page 35: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

DCC model for neutrino interaction

n

spNX is from our DCC model

via PCAC

nN l X ( X = , , , , pN ppN hN KL KS )

at forward limit Q2=0

Kamano, Nakamura, Lee, Sato, PRD 86 (2012)

pN

ppN KS

Page 36: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Formalism

Cross section for nN l X ( X = , , , , pN ppN hN KL KS )

q 0

Q20

CVC & PCAC

LSZ & smoothness

Finally spNX is from our DCC model

Page 37: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Results

SLpN

ppN KShN

KL

Prediction based on model well tested by data (first nN ppN)

pN dominates for W ≤ 1.5 GeV

ppN becomes comparable to pN for W ≥ 1.5 GeV

Smaller contribution from hN and KY O(10-1) - O(10-2)

Agreement with SL (no PCAC) in D region

Page 38: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Comparison with Rein-Sehgal model

• Lower D peak of RS model

RS overestimate in higher energy regions (DCC model is tested by data) Similar findings by Leitner et al., PoS NUFACT08 (2008) 009

Graczyk et al., Phys.Rev. D77 (2008) 053001

Comparison in whole kinematical region will be done

after axial current model is developed

Page 39: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

F2 from RS model

Page 40: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

SL model applied to -n nucleus scattering

1 p production

Szczerbinska et al. (2007)

Page 41: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

SL model applied to -n nucleus scattering

coherent p production

g + 12C p0 + 12C nm + 12C m- + p0 + 12C

Nakamura et al. (2010)

Page 42: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H
Page 43: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Previous models for n-induced 1p production in resonance region

Rein et al. (1981), (1987) ; Lalalulich et al. (2005), (2006)

Hernandez et al. (2007), (2010) ; Lalakulich et al. (2010)

Sato, Lee (2003), (2005)

resonant only

+ non-resonant (tree-level)

+ rescattering ( p N unitarity)

Page 44: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Eta production reactions

Kamano, Nakamura, Lee, Sato, 2012

Page 45: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

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

Page 46: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H
Page 47: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Kamano, Nakamura, Lee, Sato, arXiv:1305.4351

Vector current (Q2=0) for h

Production is well-tested by data

Page 48: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Vector current (Q2=0) for K

Production is well-tested by data

Kamano, Nakamura, Lee, Sato, arXiv:1305.4351

Page 49: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H
Page 50: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Kamano, Nakamura, Lee, Sato, PRC 88 (2013)“N” resonances (I=1/2)

JP(L2I 2J)

Re(MR)

“Δ” resonances (I=3/2)

PDG: 4* & 3* states assigned by PDG2012AO : ANL-OsakaJ : Juelich (DCC) [EPJA49(2013)44, Model A]BG : Bonn-Gatchina (K-matrix) [EPJA48(2012)5]

-2Im(MR)(“width”)

Page 51: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Analysis resultQ2=0.16 (GeV/c)2

s T + e sL for W=1.1 - 1.32 GeV

p(e,e’p0)p p(e,e’p+)n

Page 52: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Analysis resultQ2=0.16 (GeV/c)2

s T & sL (inclusive inelastic)

DCC

Christy et al PRC 81 s T

sL

region where inclusives T & sL are fitted

Page 53: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Analysis resultQ2=2.95 (GeV/c)2

s T + e sL for W=1.11 – 1.69 GeV

p(e,e’p0)p p(e,e’p+)n

Page 54: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Analysis resultQ2=2.95 (GeV/c)2

s T & sL (inclusive inelastic)

DCC

Christy et al PRC 81 s T

sL

region where inclusives T & sL are fitted

Page 55: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Purpose : Vector coupling of neutron-N* and its Q2 –dependence : VnN*(Q2) (I=1/2)

I=3/2 part has been fixed by proton target data

Analysis of electron-’neutron’ scattering data

Data : * 1 p photoproduction (Q2=0)

* Empirical inclusive inelastic structure functions s T , sL (Q2≠0)

Christy and Bosted, PRC 77 (2010), 81 (2010)

Page 56: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Analysis resultQ2=0

ds / d W ( g n p-p) for W=1.1 – 2.0 GeV

Page 57: Neutrino-induced meson productions Satoshi Nakamura Osaka University, Japan Collaborators : H. Kamano (RCNP, Osaka Univ.), T. Sato (Osaka Univ.) T.-S.H

Analysis result

Q2=1 (GeV/c)2

s T & sL (inclusive inelastic e—-’n’ ) DCC

Christy and Bosted PRC 77; 81

s T

sL

Q2=2 (GeV/c)2

sL

s T

Q2≠0