status n* photoproduction with clas

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Status N* photoproduction with CLAS Eugene Pasyuk Jefferson Lab CLAS 3 rd Euroworkshop Glasgow, UK, June 20-22, 2013

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CLAS 3 rd Euroworkshop Glasgow, UK, June 20-22, 2013. Status N* photoproduction with CLAS. Eugene Pasyuk Jefferson Lab. Resonance status for N * and Δ *. Nearly half the states have only fair or poor evidence! Most states need more work to learn details Are there missing states?. - PowerPoint PPT Presentation

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Page 1: Status  N*  photoproduction with CLAS

Status N* photoproduction with CLAS

Eugene PasyukJefferson Lab

CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Page 2: Status  N*  photoproduction with CLAS

2E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Resonance status for N* and Δ*

• Nearly half the states have only fair or poor evidence!

• Most states need more work to learn details

• Are there missing states?

Page 3: Status  N*  photoproduction with CLAS

3E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Baryon Resonance Spectrum

Masses, widths, and coupling constants not well known for many resonances

Most models predict more resonance states than observed

N*

S. Capstik and W. Roberts

Lattice QCD

Mass(π) = 396 MeV

R.G. Edwards et al. Phys. Rev. D84 074508 (2011)

Page 4: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 4

From the Experiment to Theory

Experimentcross section,

spin observables

TheoryLQCD,

quark models,QCD sum rules,

Reaction Theorydynamical frameworks

Amplitude analysis→multipole amplitudes

→phase shifts

(single) dσ/dΩ,Σ,P,T(beam-target) E,F,G,H,(beam-recoil) Cx,Cz,Ox,Oz,(target-recoil) Lx,Lz, Tx,Tz,

Page 5: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 5

Polarization observables in pseudoscalar meson production4 Complex amplitudes: 16 real polarization observables.Complete measurement from 8 carefully chosen observables. πN has large cross section but in KY recoil is self-

analysing

I. S. Barker, A. Donnachie, J. K. Storrow, Nucl. Phys. B95 347 (1975).

πN KYrecoil targ

γ γ targ recoil

☻☻☻

linearly polarized photons

☻☻☻☻☻☻

longitudinally polarized target

☻☻☻☻☻☻

circ polarized photons

☻☻☻☻☻☻☻☻☻☻☻☻

transversely polarized target

Complete, andover-determined

Page 6: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 6

CEBAF Large Acceptance Spectrometer 1997-2012

Torus magnet6 superconducting coils

Gas Cherenkov counterse/ separation, 256 PMTs

Time-of-flight countersplastic scintillators, 684 photomultipliers

Drift chambers35,000 cells

target + start counter

Electromagnetic calorimetersLead/scintillator, 1296 photomultipliers

Page 7: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 7

12/18/2012

Page 8: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 8

Page 9: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 9

Polarized pohoton beamC

ircu

lar

pola

riza

tion

Circular polarization from 100% polarized electron beam

Linearly polarized photons: coherent bremsstrahlung on oriented diamond crystal

Circularly polarized beam produced by longitudinally polarized electrons

H. Olsen and L.C. Maximon, Phys. Rev. 114, 887 (1959)

Page 10: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 10

FROST

Page 11: Status  N*  photoproduction with CLAS

11E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

HDIce polarized target Polarized at very high

magnetic field and very low temperature

Transferred to in-beam cryostat

Spin can be moved between H and D with RF transitions

All material can be polarized with small background

Page 12: Status  N*  photoproduction with CLAS

12E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

What we measure with CLAS

γp→π0p, π+n γp→ηp γp→η’p γp→KY (K+Λ, K+Σ0, K0Σ+) γp→π+π-p ωp, ρp, ϕp ….

γn→π-p γn→π+π-n γn→Σ-K+ , ΛK0

…..

Page 13: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 13

Single pion production

Page 14: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 14

Σ for γp → nπ+

60 1200 60 1200

DU12CM12MAIDBbGa

M. Dugger et al.Paper under collaboration review

g8b

Page 15: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 15

Σ for γ p → p π0

M. Dugger et al.

DU12CM12MAIDBbGa

Paper under collaboration review

g8b

Page 16: Status  N*  photoproduction with CLAS

16E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Changes in couplings

Solution A1/2 A3/2

D(1700)3/2- DU12 132 ± 5 108 ± 5CM12 105 ± 5 92 ± 4BnGa 160 ± 20 165 ± 25MD07 226 210PDG12 104 ± 15 85 ± 22

D(1905)5/2+ DU12 20 ± 2 -49 ± 5CM12 19 ± 2 -38 ± 4BnGa 25 ± 5 -49 ± 4MD07 18 -28PDG12 26 ± 11 -45 ± 20

Those are both **** states!

Page 17: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 17

E for γ p → p π0

• Early stage results• Predictions agree

better at lower energies

(new)

M. Dugger et al.

g9a

Page 18: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 18

E for γ p → n π+

S. Strauch

PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARY

PRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY

Predictions worse at higher energies above 1.7 GeV

SAIDSAID (new fit)MAID

Cos(θπc.m.)

W = 1.25 GeV W = 1.27 GeV

W = 1.29 GeV W = 1.31 GeV W = 1.33 GeV W = 1.35 GeV

W = 1.47 GeVW = 1.45 GeV

W = 1.43 GeVW = 1.41 GeVW = 1.39 GeVW = 1.37 GeV

W = 1.49 GeV W = 1.51 GeV W = 1.53 GeV W = 1.55 GeV W = 1.57 GeV W = 1.59 GeV

W = 1.71 GeVW = 1.69 GeVW = 1.67 GeVW = 1.65 GeVW = 1.63 GeVW = 1.61 GeV

W = 1.73 GeVW = 1.75 GeV W = 1.77 GeV W = 1.81 GeV W = 1.83 GeV W = 1.9 GeV

W = 2.19 GeVW = 2.13 GeVW = 2.07 GeV

W = 2.02 GeVW = 1.98 GeVW = 1.94 GeV

W=1.73 GeV

Analysis note is being written

g9a

Page 19: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 19

T for γ p → n π+

(new)

(new)

(new)

M. Dugger et al.

g9b

Page 20: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 20

F for γ p → n π+

• Agreement with predictions get much worse at higher energies

• SAID13 are predictions based on preliminary fits to CLAS pion Σ measurements

(new) (new)

(new)

M. Dugger et al.

g9b

Page 21: Status  N*  photoproduction with CLAS

21E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Σ for γ n → p π-

D. Sokhan

preliminary

Curve - SAIDRed GRAALMagenta and Blue - Erevan 9 out of 40 angular bins are shown

Bins 0.04 in cos and 20 MeV in W

g13

Page 22: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 22

E for γn(p) → pπ-(p) g14

T. Kagea

Page 23: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 23

η photoproduction

Page 24: Status  N*  photoproduction with CLAS

24E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

P. Collins

Σ for γp → pη

SAIDMAID

PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY PRELIMINARY

PRELIMINARY

PRELIMINARYPRELIMINARY

PRELIMINARYPRELIMINARYPRELIMINARYPRELIMINARY

PRELIMINARY

PRELIMINARY

PRELIMINARY PRELIMINARY

PRELIMINARY

PRELIMINARY

preliminary

Analysis under working group review

g8b

Page 25: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 25

E for for γp → pη

I. Senderovich

g9a

Page 26: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 26

G for for γp → pη

I. Senderovich

g9a

Page 27: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 27

T for for γp → pη

R. Tucker

Page 28: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 28

F for for γp → pη

R. Tucker

Page 29: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 29

KY production

Page 30: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 30

D. G. Ireland, K. Livingston, B. McKinnon, C. A. Paterson

Σ , Ox , Oz for γ p → K+ Λ g8b

Page 31: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 31

Σ , Ox , Oz for γ p → K+ Σ0

D. G. Ireland, K. Livingston, B. McKinnon, C. A. Paterson

g8b

Page 32: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 32

T for γ p → K+ Λ and γ p → K+Σ0

D. G. Ireland, K. Livingston, B. McKinnon, C. A. Paterson

Due to the self-analyzing nature of the , determine many observables using only a linearly polarized beam

Direct measurements of TA4 – N. Walford

g8b

Page 33: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 33

W=1725 MeVEγ=1117 MeV

W=2125 MeVEγ=1938 MeV

W=2025 MeVEγ=1717 MeV

W=1975 MeVEγ=1610 MeV

W=1925 MeVEγ=1506 MeV

W=1875 MeVEγ=1405 MeV

W=1825 MeVEγ=1306 MeV

W=1775 MeVEγ=1210 MeV

W=2275 MeVEγ=2290 MeV

W=2225 MeVEγ=2170 MeV

W=2175 MeVEγ=2053 MeV

W=1675 MeVEγ=1027 MeV

T for γp→K+Λ

N. Walford

preliminary

★-CLASBnGakaonMAID

g9b

Page 34: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 34

W=1725 MeVEγ=1117 MeV

W=2125 MeVEγ=1938 MeV

W=2075 MeVEγ=1826 MeV

W=2025 MeVEγ=1717 MeV

W=1975 MeVEγ=1610 MeV

W=1925 MeVEγ=1506 MeV

W=1875 MeVEγ=1405 MeV

W=1825 MeVEγ=1306 MeV

W=1775 MeVEγ=1210 MeV

W=2275 MeVEγ=2290 MeV

W=2225 MeVEγ=2170 MeV

W=2175 MeVEγ=2053 MeV

T for γp → K+Σ0

N. Walford

preliminary

★-CLASBnGakaonMAID

g9b

Page 35: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 35

F for γp→K+Λ

N. Walford

★-CLASBnGakaonMAID

preliminary

g9b

Page 36: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 36

+- photoproduction

Page 37: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 37

Photoproduction of π+π-p states • Dominates photoproduction cross section for W >1.6 GeV • 64 observables• 28 independent relations related to helicity amplitude magnitudes• 21 independent relations related to helicity amplitude phases• Results in 15 independent numbers

Could be used for search of resonances that decay into other resonances

Page 38: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 38

Cross section for γp →pπ+π-

Page 39: Status  N*  photoproduction with CLAS

39E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

IS for pπ+π-

E=1900-1950 MeV W=2120 MeV

One of 20 energy bins Charles Hanretty

Linearly polarized photons, unpolarized target

g8b

Page 40: Status  N*  photoproduction with CLAS

40E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

I for pπ+π-

S. Strauch et al., PRL. 95, 162003 (2005) W. Roberts and T. Oed, PRC 71, 055201 (2005)A. Fix and H. Arenhovel, EPJA 25, 115 (2005) S. Park

g9a

Page 41: Status  N*  photoproduction with CLAS

41E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Pz for pπ+π-

W. Roberts and T. Oed, PRC 71, 055201 (2005)A. Fix and H. Arenhovel, EPJA 25, 115 (2005) S. Park

g9a

Page 42: Status  N*  photoproduction with CLAS

42E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Pz for pπ+π-

W. Roberts and T. Oed, PRC 71, 055201 (2005)A. Fix and H. Arenhovel, EPJA 25, 115 (2005) S. Park

g9a

Page 43: Status  N*  photoproduction with CLAS

43E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Comparison with model: Pcz

preliminary

A. Fix and H. Arenhovel, EPJA 25, 115 (2005)

Y. Mao

g9a

Page 44: Status  N*  photoproduction with CLAS

44

Comparison with model: Psz

preliminary

Y. Mao

A. Fix and H. Arenhovel, EPJA 25, 115 (2005)

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

g9a

Page 45: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 45

Summary of meson photoproduction σ Σ T P E F G H Tx Tz Lx Lz Ox Oz Cx Cz

Proton target

pπ0 ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓

nπ+ ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓

pη ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓

pη’ ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓

K+Λ ✔ ✓ ✓ ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✔ ✔

K+Σ0 ✔ ✓ ✓ ✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✔ ✔

K0*Σ+

✔ ✓ ✓ ✓ ✓ ✓ ✓ ✓

“Neutron” targetpπ- ✔ ✓ ✓ ✓ ✓ ✓ ✓

K+Σ- ✓ ✓ ✓ ✓ ✓ ✓ ✓

K0Λ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓

K0Σ0 ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓ ✓

✔ - published ✔ - acquired

Page 46: Status  N*  photoproduction with CLAS

46E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Summary Data collection with proton and deuteron targets is

complete “complete (or nearly complete) measurement” in

pseudoscalar meson photoproduction is in the can In many cases these are the first measurements. In most cases model predictions do not agree with

the data at higher energies Phenomenological and theoretical analyses will have

to deal with tenths of thousands of data points for various observables in different final states.

Setting up close collaboration with Bonn-Gatchina group.

Page 47: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 47

Extras

Page 48: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 48

Polarization observables in pseudoscalar meson production

Page 49: Status  N*  photoproduction with CLAS

g14 – E06-101: polarized gamma beams on polarized HD

• Circular and Linear polarized photons• flux up to 108 s-1 tagged (low bkg)• Longitudinally polarized solid HD• P(D) ~ 22%; lifetimes ~ 2 yr• Nov/11 – May/12: 14 billion triggers

Page 50: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 50

Page 51: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 51

R Values for the

The appears 100% polarized when created with a fully polarized beam.

2 2 2x zR P C C + +

Page 52: Status  N*  photoproduction with CLAS

52E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Average R values

Energy and angle averages are consistent with unity.

No model predicted this CLAS result.

1 .0 1 0 .0 1R = ±

Page 53: Status  N*  photoproduction with CLAS

53E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Model of effective Lagrangian approach

About the model:•Calculates diff-cross section by using transition amplitudes

•Amplitudes are determined by all the double-pion diagrams

53

• The diagrams above show the decay from N* resonances.

• Include resonances:

Diagrams of N* for the reaction γN → ππN

Other decays:• N-Born terms• Δ-Born terms

Page 54: Status  N*  photoproduction with CLAS

Examples of 2-fold differential g p → p + - cross sections2-fold cross sections within the CLAS acceptance.

Nine one-fold and 18 two-fold differential cross sections have become available for the first time in W-bins of 25 MeV width.

Page 55: Status  N*  photoproduction with CLAS

One-fold differential g p → p + - cross sections Blue dots: experimental data within the CLAS acceptanceBlack dots: accounting for the contributions from inefficient areas employing phase space approximationRed dots: extrapolating cross sections into inefficient areas within the framework of the JM model

Two approaches for cross section extrapolation provided close results

Page 56: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 56

recoil polarization P

excitation function

g11: W=1.7 – 2.8 GeV(unpolarized beam & target)

M.E. McCracken et al., PRC 81, 025201 (2010)

γp→K+Λ: cross section and P

Page 57: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 57

γp→K+Λ: Cx/Cz

Bradford et al. PRC 75, 035205 (2007),

Page 58: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 58

Comparison with other measurements

Experiment

Final State

W range (Gev)

S P T Ox Oz

CLAS g11K 1.62 – 2.84 N Y N N N

KS 1.69 – 2.84 N Y N N N

LEPSK 1.94 – 2.30 Y N N N N

KS 1.94 – 2.30 Y N N N N

GRAALK 1.64 – 1.92 Y Y Y Y Y

KS 1.74 – 1.92 Y Y N N N

CLAS g8K 1.71 – 2.19 Y Y Y Y Y

KS 1.75 – 2.19 Y Y Y Y Y

Page 59: Status  N*  photoproduction with CLAS

59E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Comparison with other measurements

LEPS LEPS

CLAS g8 CLAS g8

GRAAL

GRAAL

Page 60: Status  N*  photoproduction with CLAS

60E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Beam Asymmetry Comparison

Page 61: Status  N*  photoproduction with CLAS

61E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

Beam Asymmetry Comparison

Page 62: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 62

Beam Asymmetry Comparison

Page 63: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 63

Beam-Recoil Comparison

Page 64: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 64

Beam Asymmetry Comparison

Page 65: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 65

Beam Asymmetry

Page 66: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 66

Target Asymmetry

Page 67: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 67

Beam-Recoil, Ox

Page 68: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 68

Beam-Recoil, Oz

Page 69: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 69

Beam Asymmetry

Page 70: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 70

Target Asymmetry

Page 71: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 71

Beam-Recoil, Ox

Page 72: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 72

Beam-Recoil, Oz

Page 73: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 73

Σ for γ p → p π0

DU12CM12MAIDBbGa

M. Dugger et al.

Page 74: Status  N*  photoproduction with CLAS

74E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013

W=1725 MeVEγ=1117 MeV

W=2125 MeVEγ=1938 MeV

W=2075 MeVEγ=1826 MeV

W=2025 MeVEγ=1717 MeV

W=1975 MeVEγ=1610 MeV

W=1925 MeVEγ=1506 MeV

W=1875 MeVEγ=1405 MeV

W=1825 MeVEγ=1306 MeV

W=1775 MeVEγ=1210 MeV

W=2275 MeVEγ=2290 MeV

W=2225 MeVEγ=2170 MeV

W=2175 MeVEγ=2053 MeV

W=1675 MeVEγ=1027 MeV

Page 75: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 75

T for γ p → K+ Λ

N. Walford

Page 76: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 76

Preliminary results: integrated cross section at W from 1.6 to 2.8 GeV

SAPHIR(2005)&ABBHHM(1969)

JLAB g11a within CLAS acceptance

JLAB g11aaccept. corr. applied

Systematic errors from accept. corr. procedure ~8-20%

Integrated cross sections for γp → p π+π -

E .Golovach

Page 77: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 77

Differential cross sections for γp → pπ+π-

Blues dots:Measured cross sections within the CLAS acceptance.

Blue line: JM model* prediction within the CLAS acceptance.Black line: JM model results for 100% acceptance.

Black dots: Estimated cross sections when the contribution from inefficient area was obtained employing phase space approximation.

*Mokeev et al. PRC 80 (2009) 045212

E .Golovach

Page 78: Status  N*  photoproduction with CLAS

E. Pasyuk CLAS 3rd Euroworkshop Glasgow, UK, June 20-22, 2013 78

Differential cross sections for γp → pπ+π-

Blues dots:Measured cross sections within the CLAS acceptance.

Black dots: Estimated cross sections when the contribution from inefficient area was obtained employing phase space approximation.

E .Golovach