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Photoproduction of Photoproduction of K* K* for t for t he study of he study of (1405) (1405) Tetsuo Hyodo a a RCNP, Osaka b IFIC, Valencia 2004, January 30th A.Hosaka a , M. J. Vicente Vacas b and E. Oset ecial thanks to Prof. Morimatsu

Photoproduction of K* for the study of L (1405)

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Photoproduction of K* for the study of L (1405). Tetsuo Hyodo a. Hosaka a , M. J. Vicente Vacas b and E. Oset b. a RCNP , Osaka b IFIC, Valencia. Special thanks to Prof. Morimatsu. 2004, January 30th. Contents. Chiral unitary model Motivation : Two poles? - PowerPoint PPT Presentation

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Page 1: Photoproduction of  K*  for the study of  L (1405)

Photoproduction of Photoproduction of K*K* for the for the study of study of (1405)(1405)

Photoproduction of Photoproduction of K*K* for the for the study of study of (1405)(1405)

Tetsuo Hyodoa

a RCNP, Osaka b IFIC, Valencia

2004, January 30th

A. Hosakaa, M. J. Vicente Vacasb and E. Osetb

Special thanks to Prof. Morimatsu

Page 2: Photoproduction of  K*  for the study of  L (1405)

ContentsContents

1. Chiral unitary model1. Motivation : Two poles?2. Framework of the chiral unitary model3. Example : Kp scatterings4. Pole structure of (1405)

2. K*(1405) production1. Advantage of the reaction2. Effective interactions3. Numerical results4. Summary and conclusions

Page 3: Photoproduction of  K*  for the study of  L (1405)

Motivation : Two poles?Motivation : 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: Photoproduction of  K*  for the study of  L (1405)

Chiral unitary modelChiral 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: Photoproduction of  K*  for the study of  L (1405)

Chiral perturbation theory

Unitarization

Framework of the chiral unitary modelFramework of the chiral unitary model

Resonances

Generated resonances areexpressed as poles of the scattering amplitude.

Page 6: Photoproduction of  K*  for the study of  L (1405)

Total cross sections of Kp scatteringsTotal cross sections of Kp scatterings

T. Hyodo, et al., Phys. Rev. C 68, 018201 (2003)

200

150

100

50

0300200100

K-p

70

60

50

40

30

20

10

0300200100

π0

200

150

100

50

0300200100

π+−

60

50

40

30

20

10

0300200100

Plab [ / ]MeV c

K0n

60

50

40

30

20

10

0300200100

Plab [ / ]MeV c

π0080

60

40

20

0300200100

Plab [ / ]MeV c

π−+

Page 7: Photoproduction of  K*  for the study of  L (1405)

Poles of amplitude in S=1 channelPoles of amplitude in S=1 channel

D. Jido, et al., Nucl. Phys. A 723, 205 (2003)

8×8 ~ 1,8,8,10,10,27attractive repulsive

Page 8: Photoproduction of  K*  for the study of  L (1405)

(1405) in the chiral unitary model(1405) in the chiral unitary model

D. Jido, et al., Nucl. Phys. A 723, 205 (2003)

π mass distribution

1390 + 66i (π

1426 + 16i (KN)

Page 9: Photoproduction of  K*  for the study of  L (1405)

Photoproduction of K* (1405)Photoproduction of K* (1405)

Only Kp channel appears at the initial stage

Higher pole ??

Page 10: Photoproduction of  K*  for the study of  L (1405)

Advantage of this reactionAdvantage of this reaction

With polarized photon beam, the exchangedparticle can be identified.

Clear mechanism

Page 11: Photoproduction of  K*  for the study of  L (1405)

Effective interactions for vector mesonEffective interactions for vector meson

1. VP coupling

2. VPP coupling

Page 12: Photoproduction of  K*  for the study of  L (1405)

3. (1385)MB coupling

4. Form factor

Effective interaction for baryon resonanceEffective interaction for baryon resonance

ChU amplitude

(1385) pole term

Page 13: Photoproduction of  K*  for the study of  L (1405)

0.7

0.6

0.5

0.4

0.3

0.2

0.1

0.0300028002600240022002000

[ ]s MeV

π00 ( =0)I π+-

π-+

π0 ( =1)I

(1405)*KKππ

Total cross sectionTotal cross section

Page 14: Photoproduction of  K*  for the study of  L (1405)

4

3

2

1

015001450140013501300

MI [ ]MeV

π00 ( =0)I π+-

π-+

π0 ( =1)I

nvariant mass distributionnvariant mass distribution

Plab = 2.5 GeV/csqrt s ~ 2.35 GeV

Page 15: Photoproduction of  K*  for the study of  L (1405)

Isospin decomposition of π statesIsospin decomposition of π states

• Difference among charged states -> when summed up, this term vanishes

• No p-wave contribution -> I=1 s-wave amplitude

Page 16: Photoproduction of  K*  for the study of  L (1405)

4

3

2

1

015001450140013501300

MI [ ]MeV

π00 ( =0)I π+-

π-+

π0 ( =1)I

( π+- + π-+ ) / 2

nvariant mass distribution 2nvariant mass distribution 2

Plab = 2.5 GeV/csqrt s ~ 2.35 GeV

Page 17: Photoproduction of  K*  for the study of  L (1405)

I=1, s-wave amplitdueI=1, s-wave amplitdue

-1.5

-1.0

-0.5

0.0

0.5

1.0

1.5

15001450140013501300MI [ ]MeV

π+- − π-+

π ( =1)I

Page 18: Photoproduction of  K*  for the study of  L (1405)

Summary and conclusions 1Summary and conclusions 1

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 π state

� By observing the charged π states in the p -> K*(1405) reaction, it is possible to isolate higher energy pole.

Page 19: Photoproduction of  K*  for the study of  L (1405)

Summary and conclusions 2Summary and conclusions 2

� If we observe neutral π state, clear I=0 distribution is obtained.

� Combining three π states, we can also study the s-wave I=1 amplitude, where the existence of another pole is argued.

T. Hyodo, et al, nucl-th/0401051

http://www.rcnp.osaka-u.ac.jp/~hyodo/

Page 20: Photoproduction of  K*  for the study of  L (1405)

Appendix : other processesAppendix : other processes

p -> Kπ

p -> πJ.C. Nacher, et al., PLB461, 299(1999)

J.C. Nacher, et al., PLB445, 55(1999)