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PEPPo Collaboration Meeting November 8-9, 2010, Newport News Status Status and and Performances Performances of the of the E166 Modified Calorimeter E166 Modified Calorimeter (i) E166 configuration (ii) PEPPo configuration (iii) PMT read-out (iv) Calorimeter operation (v) Workplan Maud Baylac ǂ , Germain Bosson ǂ , Jonathan Dumas ǂ* , Marc Marton ǂ , Jean-François Muraz ǂ , Jean-Sébastien Réal ǂ , Eric Voutier ǂ ǂ Laboratoire de Physique Subatomique et de Cosmologie Grenoble, France * Thomas Jefferson National Accelerator Facility Newport-News, Virginia, USA

PEPPo Collaboration Meeting

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Status and Performances of the E166 Modified Calorimeter. Maud Baylac ǂ , Germain Bosson ǂ , Jonathan Dumas ǂ* , Marc Marton ǂ , Jean-François Muraz ǂ , Jean-Sébastien Réal ǂ , Eric Voutier ǂ. ǂ Laboratoire de Physique Subatomique et de Cosmologie Grenoble, France - PowerPoint PPT Presentation

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Page 1: PEPPo Collaboration Meeting

PEPPo Collaboration Meeting November 8-9, 2010, Newport News

StatusStatus and and PerformancesPerformancesof theof the

E166 Modified CalorimeterE166 Modified Calorimeter

(i) E166 configuration(ii) PEPPo configuration(iii) PMT read-out(iv) Calorimeter operation(v) Workplan

Maud Baylacǂ, Germain Bossonǂ, Jonathan Dumasǂ*, Marc Martonǂ,

Jean-François Murazǂ, Jean-Sébastien Réalǂ, Eric Voutierǂ ǂ Laboratoire de Physique Subatomique et de Cosmologie

Grenoble, France* Thomas Jefferson National Accelerator Facility

Newport-News, Virginia, USA

Page 2: PEPPo Collaboration Meeting

Eric VoutierE166 Configuration

Newport News, November 8-9, 2010

Principle of Operation

G. Alexander et al, PRL 100 (2008) 210801 G. Alexander et al, NIM A 610 (2009) 451

The E166 experiment operated with high incident particle flux, integrating the energy deposited in the crystal per beam pulse and per target polarization orientation.

The signal read-out was realized with BaBar inspired electronics, relying on Hamamatsu S2744-08 photodiodes, a set of amplifiers, and ADCs.

Small experimental asymmetries and large polarization transfer from circularly polarized photons to longitudinally polarized positrons have been reported.

Experimental proof of the undulator based polarized

positron source for ILC.2/14

Page 3: PEPPo Collaboration Meeting

Eric VoutierE166 Configuration

K. Laihem, PhD Thesis, Humboldt Universität zu Berlin (2008)

Cosmics

The high energy response of the crystals is quite good and well understood.

Electronics noise is a matter of concern for small energy deposit.

Energy resolution at small energy deposit does not look impressive.

2.8 MeV

Newport News, November 8-9, 2010 3/14

Page 4: PEPPo Collaboration Meeting

Eric VoutierPEPPo Configuration

Principle of Operation

PEPPo will investigate the longitudinal polarization transfert from polarized electrons to polarized positrons.

Experimental asymmetry will be measured with respect to the electron beam helicity for a given target polarization orientation.

We aim at three different analysis schemes of the experimental signal: integrated (similar to E166), semi-integrated (energy distributed asymmetry and built-in pulse shape analysis), and event-by-event (energy distributed asymmetry and off-line pulse shape analysis).

The PMT read-out is expected to improve the signal-to-noise ratio and the resolution at small photon

energies.

Newport News, November 8-9, 2010 4/14

Page 5: PEPPo Collaboration Meeting

Eric Voutier

Top cosmic triggerVME DAQ

Wiener VME VM-USB controlerCAEN ADC V792 NCCAEN TDC V 775 AC

CAEN DFC

PMT Read-Out

Calorimeter box

Newport News, November 8-9, 2010 5/14

Page 6: PEPPo Collaboration Meeting

Eric VoutierPMT Read-Out

PMT Base

Typical PMT cosmic signal at 1000 V high voltage with a standard Hamamatsu base.

Expected high particle flux and large operational high voltage reduce the PMT life-time.

Custom PMT bases are designed for PMT gain reduction and output signal amplification.

Newport News, November 8-9, 2010 6/14

Page 7: PEPPo Collaboration Meeting

Eric VoutierPMT Read-Out

16 db 16 db 16 db

Top trigger

Bottom trigger

Cosmic Test

The trigger scintillator strips overlap longitudinally the CsI crystal and define a transverse location close to the PMT side.

HV = 1200 V t = 2.5 µs

After 4 data taking days…

About 50 MeV energy deposit for perpendicular minimum ionizing particles.

Crystal

Newport News, November 8-9, 2010 7/14

Page 8: PEPPo Collaboration Meeting

Eric VoutierPMT Read-Out

Signal Characterization

22Na ( 0.511 MeV, 1.275 MeV)

HV = 1400 V t = 2.0 µs Th. = 15 mV

Crystal box

22Na source

1.275 MeV

The test is performed with the same light collection surface as E166 configuration.

Newport News, November 8-9, 2010 8/14

Page 9: PEPPo Collaboration Meeting

Eric VoutierPMT Read-Out

The effective efficient duration of the signal is about 2 µs.

Newport News, November 8-9, 2010 9/14

Page 10: PEPPo Collaboration Meeting

Eric VoutierPMT Read-Out

Improved light collection surface together with a direct coupling of the PMT to the crystal using an optical gel.

20 x 20 → 54 x 54 (surface factor = 7.3)

Optical fiber for LED

monitoring of the

experimental chain

Newport News, November 8-9, 2010 10/14

Page 11: PEPPo Collaboration Meeting

Eric VoutierPMT Read-Out

The improvement of the surface collection and PMT-crystal optical coupling leads to a 100 V gain on the operational high voltage.

Unexpected behaviours appear… DAQ issues… On-going investigations…

22Na (2 mn DataK) Background (860 mn DataK)

1.275 MeV

0.511 MeV

Pedestal

0.511 MeV

1.275 MeV

HV = 1300 V t = 2.0 µs Th. = 7 mV

Newport News, November 8-9, 2010 11/14

Page 12: PEPPo Collaboration Meeting

Eric VoutierCalorimeter Operation

Compton Transmission Polarimetry

LμPPtanhNN

NNA 1tγT

)(Aρμ C

02

e1

dd

ddd

et

Te AP

A P

Polarized e± convert into circularly polarized photons into a tungsten target.The photon polarization is analyzed via Compton scattering off a magnetized iron target.

T = 7.5 MeVP = 85%tw = 1 mmI = 1 pA

t = 100 s

The analyzing power Ae is obtained from electron beam calibration data and simulations.

High DAQ rates capabilities will be obtained with the flash ADC FADC 250 developped at JLab.

Pe = ±0.03

Newport News, November 8-9, 2010 12/14

Page 13: PEPPo Collaboration Meeting

Eric VoutierCalorimeter Operation

Experimental Issues

Newport News, November 8-9, 2010

IMIntegrated Method

SIMSemi Integrated Method

EVEMEvent-by-Event Method

ADC samples are summed over the time duration of the helicity gate.

The total energy deposited in a crystal per helicity state is registered (2 x 9 values).

The DAQ trigger is the helicity gate.

Small asymmetries are expected.

No threshold, pile-up or dead-time concerns.

Potential helicity correlated background issues.

ADC samples per event are summed for a fixed time window and tagged by helicity state.

The energy deposit per crystal, helicity state, and event is registered (2 x 9 x nb of energy bins values).

The DAQ trigger should be external (positron counter ?).

Sizeable asymmetries are expected.

Threshold or pile-up issues but no dead-time concerns.

No helicity correlated background concerns.

ADC samples for a fixed time window (2-3µs) are tagged by helicity state.

Each ADC sample per crystal, helicity state, and event is registered (9 x 750 values).

The DAQ trigger should be external (positron counter ?).

Sizeable asymetries are expected.

Threshold, pile-up, and dead-time issues.

No helicity correlated background concerns.

13/14

Page 14: PEPPo Collaboration Meeting

Eric VoutierWorkplan

14/14Newport News, November 8-9, 2010

Technical Issues

Calorimeter Construction

- Operation of the local electronics and DAQ system- Development of an improved cosmic trigger (scintillator hodoscope, lead absorber for MIPs selection… ); possible use at JLab ?

- Selection of the wrapping material (tyvek, aluminized mylar, millipore…)- Quality tests of the crystals (signal-to-noise ratio, resolution…)- Test of the LED monitoring system- Test of the modified calorimeter before shipment to JLab (mechanics, PMT bases…)

Calorimeter Operation

- Operation of the calorimeter with the FADC 250- Development of solutions and practices for each experimental issues- Exhaustive simulations (analyzing power, transverse polarization effects, misalignement effects, positron distribution sensitivity… )