Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

35
Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013

Transcript of Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Page 1: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Kaon Production on the Nucleon

D. G. Ireland

MENU Rome, September 30 – October 4, 2013

Page 2: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

2

Kaon Photoproduction

very high momentum

transfer (pQCD)

Page 3: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

3

Page 4: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Baryon Summary Table (PDG 2008)

4

Page 5: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Baryon Summary Table (PDG 2012)

5

Page 6: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

“Missing” Baryon Resonances

6

Page 7: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

7

Resonances in Quark Models

Page 8: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Baryon Spectrum on the Lattice

8

Excited state baryon spectroscopy from lattice QCD.Edwards, Dudek, Richards, Wallace Phys. Rev. D 84, 074508 (2011)

Page 9: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

9

Resonance Hunting…

Mostly done with pN scatteringMissing resonances may decay through other channels

Total Cross-sections+ differential cross-sections+ Partial Wave Analysis + ...

Page 10: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Meson Photoproduction Cross Sections

10

Page 11: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

11

Jefferson Lab

Page 12: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

CLAS

12

Page 13: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

13

*g p →KY Electroproduction

p

proton

Hyperon is self-analysing

Cross Section:

… with electron polarization…

Page 14: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

14

*g p →KL Separated Structure Functions

D. Carman et al. (CLAS), Phys. Rev. C 87, 025204, 2013

Page 15: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

15

*g p →KS Separated Structure Functions

D. Carman et al. (CLAS), Phys. Rev. C 87, 025204, 2013

Page 16: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

16

*g p →KL Q2 Dependence

D. Carman et al. (CLAS), Phys. Rev. C 87, 025204, 2013

Page 17: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

17

*g p →KS Q2 Dependence

D. Carman et al. (CLAS), Phys. Rev. C 87, 025204, 2013

Page 18: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

gp →KL Photoproduction

proton

zy

x

z

y

x

zy

x

p

. .c m

K

proton

K+

Hyperon is self-analysing

18

Page 19: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

19

CLAS results γp→K+Λ → K+pπ-

Bonn-Gatchina Coupled Channel Analysis, A.V. Anisovich et al, EPJ A48, 15 (2012)

(Includes nearly all new photoproduction data)

M. McCracken et al. (CLAS), Phys. Rev. C 81, 025201, 2010

Page 20: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

20

CLAS results γp→K+Λ → K+pπ-

Bonn-Gatchina Coupled Channel Analysis, A.V. Anisovich et al, EPJ A48, 15 (2012)

(Includes nearly all new photoproduction data)

M. McCracken et al. (CLAS), Phys. Rev. C 81, 025201, 2010 R. Bradford et al. (CLAS), Phys.Rev. C75, 035205, 2007

Page 21: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

21

Fit to K+Λ with PDG2010 states < 2 GeV

EBAC group: Kamano, Nakamura, Lee, Sato (2012) Includes ***, **** states

PDG states insufficient to fit KΛ data

1965 1965

Page 22: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

22

Evidence for new N* states and couplings

StateN((mass)JP

PDG 2010 PDG 2012 KΛ KΣ Nγ

N(1710)1/2+ ***(not seen in

GW analysis)

*** *** ** ***

N(1880)1/2+ ** ** * **

N(1895)1/2- ** ** * ***

N(1900)3/2+ ** *** *** ** ***

N(1875)3/2- *** *** ** ***

N(2150)3/2- ** ** **

N(2000)5/2+ * *** ** * **

N(2060)5/2- *** ** ***

Bonn-Gatchina Analysis – A.V. Anisovich et al., EPJ A48, 15 (2012)(First coupled-channel analysis that includes nearly all new photoproduction data)

Page 23: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Ref: Scaling and Resonances in Elementary K+L Photoproduction [R.A. Schumacher and M.M. Sargsian, Phys. Rev. C 83, 025207 (2011)]

Compute coherent total amplitude:

Fit to observed angular distributions:

Test various resonance sets vs. mass

Free parameters: mass, width, couplings

Spin observables neglected

Sensitive to smaller contributions to reaction

Structure appears when scaling utilised.

N* K+L Amplitude Analysis

Page 24: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

24

Linearly Polarized Photons

Diamond radiator mountedon target ladder

Radiator in goniometer

Alignment checked byobserving symmetric

“Stonehenge Plot”

Polarization determined by fit to coherent bremsstrahlung

spectrum

Page 25: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

25

FROzen Spin Target (FROST)

Target can be longitudinally or transversely polarised[See talk by Barry Ritchie]

Page 26: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Transversity Amplitudes

b1 = < | M | > p

K } p

K } p

K } p

K }

b2 = < | M | >

b3 = < | M | ‖ >

b4 = < | M | ‖>

26

Page 27: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Observables

27

Page 28: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Imaging Multi-dimensional Objects

28

Page 29: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Imaging Multi-dimensional Objects

?

29

Page 30: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Comparison with other measurements

30

Experiment Final State W range (Gev)

S P T Ox Oz

CLAS g11KL 1.62 – 2.84 N Y N N N

KS 1.69 – 2.84 N Y N N N

LEPSKL 1.94 – 2.30 Y N N N N

KS 1.94 – 2.30 Y N N N N

GRAALKL 1.64 – 1.92 Y Y Y Y Y

KS 1.74 – 1.92 Y Y N N N

CLAS g8KL 1.71 – 2.19 Y Y Y Y Y

KS 1.75 – 2.19 Y Y Y Y Y

Page 31: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Comparison with other measurements

31

LEPS LEPS

CLAS g8 CLAS g8

GRAAL

GRAAL

Page 32: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Beam Asymmetry Comparison

32

Preliminary

Page 33: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Beam-Recoil Comparison

33

Preliminary

Page 34: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Beam Asymmetry Comparison

34

Preliminary

Page 35: Kaon Production on the Nucleon D. G. Ireland MENU Rome, September 30 – October 4, 2013.

Summary

• CLAS has measured a large set of data involving Kaon production

• Electroproduction: • Separated structure functions• Q2 dependence – information on form factors• Needs theoretical work

• Photoproduction: • Cross sections and recoil polarizations sensitive to N* physics• Exact interpretation of N* spectrum still ambiguous

• Outlook: • More polarization data to come (electro- and photo-production)• Results from (quasi-free) neutron• Full set of observables in KL and KS in resonance region• Exciting prospect for N* physics (with results from other channels)

35