Photoproduction of K* for the study of Λ(1405)tetsuo.hyodo/old/... · 1 Photoproduction of K* for...

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1 Photoproduction of K* for the study of Λ(1405) Tetsuo Hyodo a , RCNP, Osaka a Valencia Univ. b A. Hosaka a , E. Oset b , and M. J. Vicente Vacas b 2004, March 29th

Transcript of Photoproduction of K* for the study of Λ(1405)tetsuo.hyodo/old/... · 1 Photoproduction of K* for...

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

Tetsuo Hyodoa,

RCNP, Osakaa Valencia Univ.bA. Hosakaa, E. Osetb, and M. J. Vicente Vacasb

2004, March 29th

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Motivation : Two poles?

ChU model, T. Hyodo

There are two poles of the scattering amplitudearound nominal Λ(1405) energy region.

1360

1380

1400

1420

1440

-20

-40

-60

-80

0.5

1.0

1.5

0.5

1.0

1.5

!(1405)

Re[z]Im[z]

|T|

Λ(1405) : JP = 1/2−, I = 0• Cloudy bag model J. Fink, et al., PRC41, 2720

• Chiral unitary model 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 C. Garcia-Recio, et al., PRD67, 076009 D. Jido, et al., NPA725, 181 T. Hyodo, et al., PRC68, 065203

• Quark model : qq-qq-q A. Zhang, et al., hep-ph/0403210

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Chiral unitary model

Unitarity of S-matrixChiral symmetry

Flavor SU(3) meson-baryon scatterings (s-wave)

Low energy behavior

Non-perturbativeresummation

Dynamicalgeneration

JP = 1/2− resonances

MB

Λ(1405),Λ(1670),

N(1535)Σ(1620),Ξ(1620),

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Framework of the chiral unitary model

LWT =1

4f2Tr(B̄iγµ[(Φ∂µΦ − ∂µΦΦ), B])

T= +

T

Tij(√

s) ∼ gigj√s − MR + iΓR/2

+ TBGij

Chiral perturbation theory

Unitarization

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Λ(1405) in the chiral unitary model

mass distribution

1390 + 66i ( )

1426 + 16i (KN)

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

Re[z]

Im[z]

position of poles

dMI= C|tπΣ→πΣ|2pCM

dMI= |

∑i

Citi→πΣ|2pCM

800

600

400

200

01460144014201400138013601340

Ec.m.

[MeV]

200

150

100

50

0

_

KN -> !"!" #> !"

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Only K p channel appears at the initial stageHigher energy pole ??

Photoproduction of K* and Λ(1405)

K∗+

K !

Λ(1405), Σ(1385)p B

M

K+,K0

π0,π+

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Advantage of this reaction

There is a correlation between polarization of initial photon and final πK angular distribution

Clear mechanism

!

(1)

(2)

K*

(1) "µ (! )//"µ (K*) : JP = natural

"µ (!)#"µ (K*)(2) : JP = unnatural

K

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Effective interaction for meson part

LK∗Kγ = gK∗Kγεµναβ∂µAν(∂αK∗−β K+ + ∂αK̄∗0

β K0) + h.c.

LV PP = − igV PP√2

Tr(V µ[∂µP, P ])

γ

π

γKK* coupling

VPP coupling

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Effective interaction for baryon part

ChU amplitude

(1385) pole termΣ

−itΣ∗i = ci125

D + F

2fS · ki

Ff (k1) =Λ2 − m2

K

Λ2 − (k1)2

Σ(1385)MB coupling

form factor

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Isospin decomposition of πΣ states

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

dσ(π0Σ0)dMI

∝ 13|T (0)|2

• Pure I=0 amplitude

dσ(π±Σ∓)dMI

∝ 13|T (0)|2 +

12|T (1)|2 ± 2√

6Re(T (0)T (1)∗)

Since initial state is KN, we neglect the I=2.

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Invariant mass distributions4

3

2

1

0

d/d

MI[

nb/M

eV

]

15001450140013501300

MI [MeV]

0 0

(I=0)

+ -

- +

(I=1)

( + -

+ - +

) / 2

Plab = 2.5 GeV/csqrt s ~ 2.35 GeV

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Summary

There are two poles of the scattering amplitude around nominal Λ(1405).In the reaction, Charged πΣ states isolate the higher energy pole.Neutral πΣ state gives a clear I=0 distribution.

We study the structure of Λ(1405) using the chiral unitary model.

γp → K∗Λ(1405)

T. H., A. Hosaka, E. Oset, M. J. Vicente Vacas, nucl-th/0401051