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Andro Kacharava Spin Physics at COSY 1 Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen 16 th SPIN Symposium, Trieste, October 10_16, 2004

Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

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Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen 16 th SPIN Symposium, Trieste, October 10_16, 2004. Outline. Experiments at COSY NN Interaction Selected Results • NN Elastic • Meson Production • YN Interaction New Equipment Conclusion. - PowerPoint PPT Presentation

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Page 1: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Andro Kacharava Spin Physics at COSY 1

Spin Physics of NN Interactions

at COSY

Andro Kacharava Universität Erlangen

16th SPIN Symposium, Trieste, October 10_16, 2004

Page 2: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 2

Outline

• Experiments at COSY

• NN Interaction

• Selected Results

• NN Elastic

• Meson Production

• YN Interaction

• New Equipment

• Conclusion

Page 3: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 3

Experiments: COSY Accelerator

COoler SYnchrotron:

Ions: (pol. + unpol.) p and d

Momentum: 300 to 3700 MeV/c

... unique possibilities:

- Spin Manipulation

- Electron Cooling at Injection

- Stochastic Cooling >1.5 GeV/c

Targets:

- Internal: Solid, Cluster,

Polarized Atomic

- External: Solid, Liquid

Page 4: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 4

Cooler Synchrotron (COSY) & Detector systems

COSY

ANKE

EDDA

Experiments: Current Facilities

TOF

COSY-11

Page 5: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 5

NN Interaction

• Fundamental for strong interaction.

• Characterization requires precise data for PSA.

• pp system: up to 2.5 GeV well-known (…, PINTEX, EDDA).

• np system: ANKE-COSY will provide high-quality data.

• Current experimental status:

R.Arndt: Gross misconception within the community that

np amplitudes are known to a couple of GeV.

J.Bystricky: Measurements of ANY observables at small

angle are highly desirable to improve PSAs.

Page 6: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 6

NN Interaction: Observables

N = yS = xL = z

dσ/d = I0 ·[1+AN·(PN+QN)

+ ANN·PN·QN

+ ASS·PS·QS

+ ASL (PL·QS+PS·QL)

+ ALL·PL·QL]

AN and Aik sensitive only

to spins in initial state: easily accessable

Storage rings - unique environment for double-polarized experiments.

Page 7: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 7

Selected Results: pp elastic at EDDA

Characterization of NN-interaction

•Large kinematical range: 1.0-3.3 GeV/c, 30°-90° [c.m.]

•High precision data- Unpolarized, single, double polarized.- Large impact on pp PSA >500 MeV.

•Further Results:•No Evidence for dibaryons•Polarimetry for the pp system

T=2.1 GeV

F. Bauer et al., PRL 90 (2003)

Page 8: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 8

Cooler Synchrotron (COSY) & Detector systems

COSY

ANKE

Experiment: EDDA

TOF

COSY-11EDDA

Page 9: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 9

Selected Results: pp elastic at EDDA

Characterization of NN-interaction

•Large kinematical range: 1.0-3.3 GeV/c, 30°-90° [c.m.]

•High precision data- Unpolarized, single, double polarized.- Large impact on pp PSA >500 MeV.

•Further Results:•No Evidence for dibaryons•Polarimetry for the pp system

T=2.1 GeV

F. Bauer et al., PRL 90 (2003)

Page 10: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 10

Selected Results: NN Modeling above 1 GeV

> 1 GeV: Modified model

original + optical potential + Reggezied vector meson

Total

Elastic

Modified model

Original model R.Machleidt (workshop in Tbilisi, Sep’04)

< 1 GeV: Original model – OBE + Δ

Page 11: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 11

Selected Results: NN Modeling above 1 GeV

R. Machleidt & EDDA data (arXiv:nucl-th/0311002,2003)

PSA (VPI)originalmodified

Page 12: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 12

Selected Results: Status of NN models >1 GeV

• SATURNE and EDDA: Transition region (few GeV). • NN model for transition region:

- σ reproduced, Spin observables > 1 GeV wrong!- Between 1 and 10 GeV serious problems!

R.Machleidt: Defeat of Theory, Triumph of Experiment.We need new ideas !

Page 13: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 13

Selected Results: np elastic at ANKE

• Spin structure of np→pn reaction amplitudes

• Method: Spin filter

• Next Step: Measurement of spin observables for pn system up to 3 GeV

• Method: Spectator technique

→ →pd→psp (pn)

dp→(pp)1S0 n

→→

Page 14: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 14

Cooler Synchrotron (COSY) & Detector systems

COSY

EDDA

Experiment: ANKE

TOF

COSY-11

ANKE

Page 15: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 15

Selected Results: np elastic at ANKE

• Spin structure of np→pn reaction amplitudes

• Method: Spin filter

• Next Step: Measurement of spin observables for pn system up to 3 GeV

• Method: Spectator technique

→ →pd→psp (pn)

dp→(pp)1S0 n

→→

Page 16: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 16

NN Interaction: np Amplitudes

In collinearkinematics

over a range in t

;2/,31 2

3

4

qkSIkdtd

d qkS 2,

;

qkSR

2,

2[ ] ;21 22222

20 RIT ;23 2222

22 RIT

R.IC zz *, 2 IC xx *, ;2 RIC yy *, ;2

2222

2220 ,,,, TTdtd

,2;222

20

22 ITI

cos3;2 *,

*, yxzyy ICIC

dp→(pp)1S0 n

,RδεβΙ 2222 2

Page 17: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 17

Selected Results: Test measurement of CE

Spin ModeTheoretical maximum

Intensity[I]Pz Pzz

0 0 0 1

1 -2/3 0 1

2 +1/3 +1 1

3 -1/3 -1 1

4 +1/2 -1/2 2/3

5 -1 +1 2/3

6 +1 +1 2/3

7 -1 -1/2 2/3

COSY Deuteron Beam I = 3 109 fr Acceptance

Page 18: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 18

Selected Results: dp Reactions

• dp elastic• dp→3He0

• dp→pspd0

• Polarimetry, Luminosity

dp→(pp)n

Page 19: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 19

Selected Results: Spin dependent amplitudes

)(79.10

0

)(15.086.10

0

SAID

ANKE

22

22

20002

002

T

APTDSG 142(0)

DTAPTDSG 2142 (0)

DSG, DT, APT from SAID

27.0

Value from SAID WI00Error from R. Arndt SE-Solution

T20 = 0.39 ± 0.04 (ANKE)

dp→(pp)1S0 n

Method W

orks !

!!

Method W

orks !

!!Bugg, Wilkin, NP A467(1987) 575

Page 20: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 20

Selected Results: NN program at ANKE

Future polarized ANKE Experiments:

1. Charge-Exchange breakup

2. np Elastic scattering

3. Deuteron breakup

dp→(pp)1S0 n

→ →

pd→psp(pn)→ →

pd →(pp)1S0 n

→ →

Strategy: Begin commissioning of PIT using high rate reactions that can be easily identified (e.g. CE).

Talk S. Yaschenko

Page 21: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 21

Selected Results: Meson Production

•η production at COSY-11

pp→ppη near threshold

Single Polarization: Ay

distinguish different models...... dominant ρ exchange___ π and η exchange

Double Polarization: Cxx (Cyy)

model independent extractionof amplitudes:

P. Winter et al., PLB, 544 (2002)

dashed: 1S0s final state

dash-dotted: 1S0s + 3P0

s

dotted: 1S0s +

3P0s+3P2

s

K. Nakayama et al., PRC, 68 (2003)

Page 22: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 22

Cooler Synchrotron (COSY) & Detector systems

COSY

ANKE

EDDA

Experiments: Current Facilities

TOF

COSY-11

Page 23: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 23

Selected Results: Meson Production

•η production at COSY-11

pp→ppη near threshold

Single Polarization: Ay

distinguish different models...... dominant ρ exchange___ π and η exchange

Double Polarization: Cxx (Cyy)

model independent extractionof amplitudes:

P. Winter et al., PLB, 544 (2002)

dashed: 1S0s final state

dash-dotted: 1S0s + 3P0

s

dotted: 1S0s +

3P0s+3P2

s

K. Nakayama et al., PRC, 68 (2003)

Page 24: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 24

Selected Results: YN Interaction

• Strangeness production at COSY-11

• Comparison of Λ - and Σ0 – production via pp p K+Λ/Σ0 close to threshold

• Parameterisation includes:• Individual Λ and Σ0 excitation

functions• p-Y final state interactions

• Hyperon production in pp pK+:• Production mechanism• Next: Double polarization

spin-dependence of p (ANKE, TOF)

Page 25: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 25

New Equipment : WASA@COSY

• Symmetry and –breaking (ISB, …)

• Hadronic states spectroscopy (, …)

• Baryon-baryon interaction (np, YN)

• Hadronic medium effects (Kaon mass)

Page 26: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 26

New Equipment: PIT & Spectator Telescope

PIT: Polarized Internal Target::- ABS

- Lamb-Shift Polarimeter

- Storage Cell

Spectator: Silicon telescope array

Talk K. Grigoriev, Sec 8, Oct’15

beam

Page 27: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 27

New Equipment: Polarized Target for TOF

PT @ COSY-TOF

(H. Dutz et al.,)

PS185/3 @ LEAR set-up Target material test by

Bochum PT-group Components installation

Bonn PT-lab Test of complete system in

spring 2005 Installation at TOF

Status and Outlook

Page 28: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 28

Cooler Synchrotron (COSY) & Detector systems

COSY

ANKE

EDDA

Experiments: Current Facilities

COSY-11

TOF

Page 29: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 29

New Equipment: Polarized Target for TOF

PT @ COSY-TOF

(H. Dutz et al.,)

PS185/3 @ LEAR set-up Target material test by

Bochum PT-group Components installation

Bonn PT-lab Test of complete system in

spring 2005 Installation at TOF

Status and Outlook

Page 30: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 30

Future Experiments: Parity of θ+ (1540)

COSY is perfectly suited to determine the parity free of any model!

Spin-correlation coefficient Axx in pp θ++

+1

-1

50 Q [MeV]0

neg. Parity

pos. ParityA

xx

PLB,590

,(2004),

39-44

Talk Y. Uzikov, Sec 4, Oct’14

Page 31: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 31

Existing Facilities ANKE, EDDA, COSY11 and TOF

pursue a strong spin physics program

Conclusion

Single and Double Polarization Experiments•NN Interaction (pn)•YN Interaction•pd Dynamics•Meson Production in pp and pn Collisions•Parity of Θ+ Pentaquark

Page 32: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 32

Observables: np SAID data

APT (KLL) 600 MeV

APT (KLL) 800 MeV

APT (KLL) 900 MeV

DT (KNN) 600 MeV

DT (KNN) 800 MeV

DT (KNN) 800 MeV

DSG 900 MeV

DSG 800 MeV

DSG 600 MeV

Page 33: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 33

np SAID data: Error analysis

Page 34: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 34

New Equipment: Spectator Detector

Features:– Three layers (double sided)

1st: 60 m2nd: 300 m3rd: 5 mm

– Ekin~2 MeV (60 MeV/c)

– 800 Channels– Self-triggering– On-board electronics

– UHV compatible– Large Acceptance

• 10% per telescope• 30 mm from the beam

Page 35: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 35

New Equipment: Polarized Internal Target

• Development for ANKE Atomic BeamSource

Lamb-Shift Polarimeter

Atomic Beam Intensity

7.4·1016 atoms/s (2 HFS)

Lyman- Spectrum

Talk K. Grigoriev, Sec 8, Oct’15

Page 36: Spin Physics of NN Interactions at COSY Andro Kacharava Universität Erlangen

Spin Physics at COSY 36

Luminosity of ANKE PIT

ANKE Luminosity (double polarized)Target density: (2.5 – 7.1)·1013 cm-2

Beam intensity: 5·109 particlesLuminosity: (2.0 - 5.7)·1029 cm-2s-1

L

dbeam

I

ddt t ~ I~ ILL22dd-3-3TT--

½½

Storage cell target requires a small -function at the interaction point: beam~β½

I=7.51016 H/s

T=300 KL=350 mma=15 mmb=20 mm

dt =2.5·1013 cm-2

a=10 mmb=12 mmdt =7.1·1013 cm-2