exotic baryon resonances in the chiral dynamics tetsuo hyodo a a rcnp, osaka b ect* c ific, valencia...
DESCRIPTION
Motivations : Two poles? Cloudy bag model (1990) J. Fink et al. PRC41, 2720 Chiral unitary model (2001~) J. A. Oller et al. PLB500, 263 E. Oset et al. PLB527, 99 D. Jido et al. PRC66, T. Hyodo et al. PRC68, There are two poles of the scattering amplitude around nominal (1405) energy region. (1405) : J P =1/2 , I=0 ChU model, T. HyodoTRANSCRIPT
![Page 1: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/1.jpg)
Exotic baryon resonances Exotic baryon resonances in the chiral dynamicsin the chiral dynamics
Tetsuo Hyodoa
a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th
A. Hosakaa, D. Jidob, S.I. Nama, E. Osetc, A. Ramosd and M. J. Vicente Vacasc
![Page 2: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/2.jpg)
1. Structure of (1405)1. Motivation : Two poles?2. Chiral unitary model3. Pole structure of (1405)4. Photo-production of K*(1405)
2. Quantum numbers of
1. Present status of theoretical studies2. Chiral model for K+p -> +KN3. Results4. Polarization test
Contents
![Page 3: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/3.jpg)
Motivations : Two poles?
• Cloudy bag model (1990) J. Fink et al. PRC41, 2720
• Chiral unitary model (2001~) J. A. Oller et al. PLB500, 263 E. Oset et al. PLB527, 99 D. Jido et al. PRC66, 025203 T. Hyodo et al. PRC68, 018201
There are two poles of the scattering amplitudearound nominal (1405) energy region.
(1405) : JP=1/2, I=0
ChU model, T. Hyodo
![Page 4: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/4.jpg)
Chiral unitary model
Unitarity of S-matrixChiral symmetry
Flavor SU(3) meson-baryon scatterings (s-wave)
Resonances
Low energy behavior
Non-perturbativeresummation
(1405), (1670), N(1535),(1620), (1620)
Dynamicalgeneration
![Page 5: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/5.jpg)
Chiral perturbation theory
Unitarization
Framework of the chiral unitary model
Resonances
Generated resonances areexpressed as poles of the scattering amplitude.
![Page 6: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/6.jpg)
Total cross sections of Kp scatterings
T. Hyodo, et al., Phys. Rev. C 68, 018201 (2003)
200
150
100
50
0300200100
K
70
60
50
40
30
20
10
0300200100
0
200
150
100
50
0300200100
−
60
50
40
30
20
10
0300200100
Plab [MeV/c]
K0n
60
50
40
30
20
10
0300200100
Plab [MeV/c]
0080
60
40
20
0300200100
Plab [MeV/c]
−
![Page 7: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/7.jpg)
(1405) in the chiral unitary model
D. Jido, et al., Nucl. Phys. A 723, 205 (2003)
mass distribution
1390 + 66i (
1426 + 16i (KN)
![Page 8: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/8.jpg)
Example : the p -> K0 reaction
Chiralterm
N(1710)
Chiral unitary model
![Page 9: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/9.jpg)
Results for p -> K0
T. Hyodo, et al., nucl-th/0307005, Phys. Rev. C, in press
Total cross sections [mb]Mass distribution
� There are two mechanisms in the initial stage interaction, which filter each one of the resonances.
Good agreement(1385) effect
![Page 10: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/10.jpg)
Photoproduction of K* (1405)
Only Kp channel appears at the initial stage
Higher pole ??
![Page 11: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/11.jpg)
Effective interactions for meson part
1. VP coupling
2. VPP coupling
![Page 12: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/12.jpg)
Effective interaction for (1385)
3. (1385)MB coupling
4. KP -> (1385) -> MB amplitude
SU(6) symmetry
![Page 13: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/13.jpg)
6
5
4
3
2
1
015001450140013501300
MI [MeV]
00 (~I=0 averae of chared 0 (I=1
invariant mass distribution
Plab = 2.5 GeV/csqrt s ~ 2.35 GeV
Preliminary
![Page 14: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/14.jpg)
1.2
1.0
0.8
0.6
0.4
0.2
0.0300028002600240022002000
sqrt s
π0Σ0 (~I=0) average of charged πΣ
π0Λ (I=1)
ΛK*KππΣ
Result : Total cross section
Preliminary
![Page 15: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/15.jpg)
Summary and conclusions
We study the structure of (1405) using the chiral unitary model.
� There are two poles of the scattering amplitude around nominal (1405).
Pole 1 (1426+16i) : strongly couples to KN statePole 2 (1390+66i) : strongly couples to state
� By observing the mass distribution in the p -> K*(1405) reaction, it could be possible to isolate higher energy pole.
![Page 16: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/16.jpg)
Appendix : other processes
p -> K
Kp -> J.C. Nacher, et al., PLB461, 299(1999)
J.C. Nacher, et al., PLB445, 55(1999)
SPring-8
J-PARC?
![Page 17: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/17.jpg)
baryon : Introduction
+ : 5-quark (4 quark + 1 anti-quark)LEPS, T. Nakano et al., Phys. Rev. Lett. 91 (2003) 012002
Quantum numbers are not yet determinedTheory prediction D. Diakonov et al. (chiral quark soliton) Naive quark model S. Capstick et al. (isotensor formulation) A. Hosaka (chiral potential) R. L. Jaffe et al. (qq-qq-q : 10 + 8) J. Sugiyama et al. (QCD sum rule) F. Csikor et al. (Lattice QCD) S. Sasaki (Lattice QCD)
: 1/2+, I=0: 1/2
: 1/2, 3/2, 5/2, I=2: 1/2+ (strong ): 1/2+, I=0: 1/2, I=0: 1/2+ -> 1/2
: 1/2
S = +1, M ~ 1540 MeV, < 25 MeV
![Page 18: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/18.jpg)
Photo-production process
W. Liu et al. nucl-th/0308034S. I. Nam et al. hep-ph/0308313W. Liu et al. nucl-th/0309023Y. Oh et al. hep-ph/0310117
p -> K0, n -> K
Model (mechanism) dependence
Form factor dependence
Unknown parameters
Initial cm energy ~ 2 GeV (pcm ~ 750 MeV) not low energy -> linear or nonlinear?N* resonances, K* exchange, K1 exchange,…
Monopole, dipole… , value of , …
coupling, K*p coupling, …
Assuming the quantum numbers (spin, parity), we can calculate a reaction
![Page 19: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/19.jpg)
Motivation and advantage
K+p -> ++ -> +K+n(K0p) Low energy model is sufficient (pcm ~ 350 MeV) take decay into account -> background estimation -> Width independent Hadronic process : clear mechanism
We propose
to extract a qualitative behavior which dependson the quantum numbers of .
Determination of quantum numbersNew : pp -> , A. W. Thomas, K. Hicks, and A. Hosaka, hep-ph/0312083
![Page 20: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/20.jpg)
A model for Kp -> +K+n
E. Oset and M. J. Vicente Vacas, PLB386, 39(1996)
Vertices are derived from the chiral Lagrangian
Proportional to vanishes
Assume final + is almost at rest
Dominant
![Page 21: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/21.jpg)
Diagrams
Tree level(background)
One loop
![Page 22: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/22.jpg)
Possibilities of spin & parity
1/2 (KN s-wave resonance)1/2 , 3/2 (KN p-wave resonance)
MR = 1540 MeV = 20 MeV
![Page 23: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/23.jpg)
Resonance term
Amplitude of resonance term for K+p -> +K+n :
![Page 24: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/24.jpg)
Angular dependence
total resonance background
10
8
6
4
2
01.00.50.00.51.0
cos θ
10
8
6
4
2
01.00.50.00.51.0
cos θ5
4
3
2
1
01.00.50.00.51.0
cos θ
I,JP=0,1/2 I,JP=0,1/2
I,JP=0,3/2
![Page 25: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/25.jpg)
Mass distributions
8
6
4
2
015801560154015201500
MI
I,JP=0,1/2
I,JP=0,1/2
I,JP=0,3/2kin(ab = 850 MeV/cθ = 90 de
1.4
1.2
1.0
0.8
0.6
0.4
0.2
0.015801560154015201500
MI
![Page 26: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/26.jpg)
Polarization test
# Same result is obtained for final pK0
![Page 27: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/27.jpg)
Angular dependence : polarization test
total resonance background
5
4
3
2
1
01.00.50.00.51.0
cos θ
20
15
10
5
01.00.50.00.51.0
cos θ5
4
3
2
1
01.00.50.00.51.0
cos θ
I,JP=0,1/2 I,JP=0,1/2
I,JP=0,3/2
Polarization test
![Page 28: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/28.jpg)
Mass distributions : polarization test
14
12
10
8
6
4
2
015801560154015201500
MI
I,JP=0,1/2
I,JP=0,1/2
I,JP=0,3/2kin(ab = 850 MeV/cθ = 90 de
1.4
1.2
1.0
0.8
0.6
0.4
0.2
0.015801560154015201500
MI
Polarization test
![Page 29: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/29.jpg)
Incomplete polarization
14
12
10
8
6
4
2
015801560154015201500
MI
I,JP=0,1/2
I,JP=0,1/2 kin(ab = 850 MeV/cθ = 90 de
Polarization
100 %80 % 0 %
![Page 30: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/30.jpg)
Conclusion
We calculate the Kp -> 0KN reaction usinga chiral model, assuming the possible quantum numbers of + baryon. � If we find the resonance with polarization test, the quantum number of + can be determined as I=0, JP=1/2+
T. Hyodo, et al, nucl-th/0307105, Phys. Lett. B, in pressE. Oset, et al, nucl-th/0312014, Hyp03 proceedings
![Page 31: Exotic baryon resonances in the chiral dynamics Tetsuo Hyodo a a RCNP, Osaka b ECT* c IFIC, Valencia d Barcelona Univ. 2003, December 9th A.Hosaka a, D](https://reader035.vdocuments.mx/reader035/viewer/2022062317/5a4d1b577f8b9ab0599a9f1d/html5/thumbnails/31.jpg)
Future work
� Full calculation of the present reaction without approximation of kinematics -> information from + angular dependence� photo-production of K* and V. Kubarovsky et al., hep-ex/0307088