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Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbe rt Coherent 0 Photoproduction Claire Tarbert, University of Edinburgh

Coherent p 0 Photoproduction

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Coherent p 0 Photoproduction. Claire Tarbert, University of Edinburgh. Coherent p 0 Photoproduction. 208 Pb. CoherentA( g,p 0 )A IncoherentA( g,p 0 )A*. Theoretical Calculations (Kamalov): PWIA (Plane Wave Impulse Approx ) DWIA (Distorted Wave Impulse Approx) - PowerPoint PPT Presentation

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Page 1: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Coherent 0 Photoproduction

Claire Tarbert, University of Edinburgh

Page 2: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Coherent0 Photoproduction

Coherent A(0)A

IncoherentA(0)A*

208Pb

Theoretical Calculations (Kamalov):

PWIA (Plane Wave Impulse Approx ) DWIA (Distorted Wave Impulse Approx) DREN (Delta Resonance Energy Model)

Good agreement with theory.

Page 3: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Coherent0 Photoproduction

Pion Missing EnergyDecay Gammas (16O)

Energy (MeV)

Pion Missing Energy:

E = E(1,2) – E(E)

E(1,2) = pion energy calculated from energy and angle of decay photonsE(E) = pion energy calculated from incident photon assuming a coherent reaction

Page 4: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Crystal Ball Energy Calibration

Traditionally calibration of CB uses 2 body 0 decay kinematics:p p

Instead try using kinematics of 0 decay from 12C: 0

i.e. for each crystal plot M when it is the central element of one of two clusters making a 0

Constraints:

Limit E < 180 MeV i.e. just above threshold ratio of light collection/shower loss remains ~constant low energy 0s i.e. photon opening angle is large

80% of cluster energy in central crystal Correction for cluster ~ correction for central crystal I E1 – E2 I < 0.25( E1 + E2 ) Same correction applies to both 0 photons

M2 = 2E1E2(1 - cos)

Page 5: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Crystal Ball Energy Calibration

Result:

Correction factor for MeV/Chn values for each crystal.

Correction Factor = m / M

Page 6: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Crystal Ball Energy Calibration

p p0 Calibration(January 2005)

Using low E 0s from 12C(March/April 2005)

Page 7: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Linearity of Energy CalibrationSeparate into bins according to E1 and E2 (0 decay photon energies)e.g. 200 < E1 < 210 MeV && 40 < E2 < 60 MeV, 200 < E1 < 210 MeV && 60 < E2 < 80 MeV,

200 < E1 < 210 MeV && 80 < E2 < 100 MeV etc…

Page 8: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Linearity of Crystal Ball Energy Calibration

Tabulated values plotted

Page 9: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Linearity of Crystal Ball Energy Calibration

Page 10: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Linearity of Crystal Ball Energy Calibration

Fit to plots:

aE3 + bE2 + CE + d

(Fit to average of data… will improve fit!!)

i.e. M = aE3 + bE2 + CE + d

To correct photon cluster energy:

Etrue = Edet ( mo / M )2

Page 11: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Linearity of Crystal Ball Energy Calibration

Reran WITHCorrection Factor

Without correction fornon linearity

(Only 1/3 of data)

Page 12: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Low Energy Calibration of Crystal Ball

• Use 4.43MeV decay s from 12C.• Select events where decay fires single crystal.• new MeV/Chn values for low energies.

Page 13: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Low Energy Calibration of Crystal Ball

Comparison to AmBe calibration

Page 14: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Low Energy Walk Correction of Crystal Ball

Page 15: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Low Energy Walk Correction of Crystal Ball

With Low Energy Walk Correction

Page 16: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Preliminary look at Incoherent 0 Photoproduction

12C

•Contains information on overlap of wavefunction between ground and excited state i.e. Matter Transition Form Factor.

•Interesting minimum at high energies?

Cro

ss

se

cti

on

(A

rb.

Un

its

)

Cro

ss

se

cti

on

(A

rb.

Un

its

)

+ Coherent+ Incoherent

Page 17: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Conclusion

• Solid target CB energy calibration almost finalisedCoherent Photoproduction cross

sections hopefully available soon.

• Interesting hints from incoherent channels.

Page 18: Coherent  p 0  Photoproduction

Collaboration Meeting, 28 March 2006, Glasgow Claire Tarbert

Preliminary decay gammas from nucleon knockout

12C(,ppp)9Li

Q value

Low energyclusters from shaded region

2.69 MeV

E=400-500 MeV

i=1

3

• Also look at pp, 4p, 5p … knockout

Missing Energy (MeV) = E–Tpi –Trec

Energy of cluster (MeV)