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4.1 Refinements to the GEANT Simulation

In a reliable simulation all detector module materials, intrinsic properties of the calorimeter, as well as details pertaining the trigger and readout have to be accurately described. This includes for example electronic noise, photoelectron statistics and the individual crystal non-uniformities. The electronic noise was included after fitting a Gaussian distribution to the pedestal of all channels under consideration. After fitting, the averaged position and width was implemented into the simulation code. To this end a randomly generated number - within the parameters of the obtained Gaussian - becomes added to the energy deposited in a crystal volume.

As reported in sect. 3.2.4, the optical non-uniformity as well as the light output of each crystal was measured. The photoelectron statistics is taken into account in the simulation in the following way. The measured number of photoelectrons per MeV for each crystal is used to generate a normalized Poisson distribution in the simulation code for the detector module. The calculated energy deposited in the crystal is then multiplied for each step with the corresponding Poisson distribution.

The optical non-uniformity that maps the average energy deposition of minimum ionizing particle per volume unit cells of each crystal resulted in a characteristic response function reflecting the measured axial and transverse non-uniformities. This function is convolved with the GEANT shower energy distributions of positrons and photons in the PiBeta detector. This requires some adaptation for the simulation, since the light output per MeV now depends on the shower depths inside the crystal. Although most of the crystals show positive non-uniformity, which indicates an increase of luminosity towards the readout device, some have a negative coefficient. A CsI crystal with a positive non-uniformity would `gain' energy, while a crystal with negative non-uniformity would lose energy. The gains of the 240 CsI modules have to be unified, therefore.

The gain matching procedure requires two sets of simulations. In one set perfect scintillators are assumed, while in the other non-uniformity is included in the simulations. 240 sum spectra are created for the comparison of both cases. A `sum' histogram corresponding to a given crystal is incremented only for those events in which this crystal receives at least 50% of the total energy deposited in the calorimeter. The histogrammed variable is the summed energy of all crystals that received more than 0.5 MeV of energy above the noise threshold. The use of single spectra was not practical due to the great lineshape differences for different crystals. The resulting individual sum spectra show scaleable differences in their peak position. Software gain factors are obtained through repetitive comparison of the ideal and `real' spectra. Both Kolmogorov-[18] and c 2-test were applied for comparison. After about four passes a final set of software gains was found. Table 4-1 is showing a sample of 37 out of 44 crystals that were used during the 1996 beamtime. Here 70 MeV positrons were emitted uniformly onto an array of 44 crystals. This table indicates that both methods result in similar values.

Channel #
Zero Non-uniformity
Unmatched
Kolmogorov-Test
c 2-Method

Peak Position
FWHM
Peak Position
FWHM
Peak Position
FWHM
Peak Position
FWHM
1
67.02
3.94
64.99
4.86
66.34
4.86
66.29
4.43
2
67.21
3.50
65.63
3.79
66.86
3.85
66.81
3.65
3
67.43
3.30
65.80
3.66
66.76
3.93
66.76
3.89
4
67.20
3.60
64.67
4.53
66.86
3.83
66.10
4.46
5
66.97
4.35
63.95
5.31
66.62
5.50
65.94
5.40
6
67.18
3.73
66.92
4.32
67.11
4.01
67.04
4.08
7
66.44
4.63
62.53
5.56
66.16
5.90
64.86
5.79
8, 9








10
66.30
4.46
67.01
4.33
65.88
4.45
66.40
4.56
11
67.82
3.54
65.27
3.92
67.68
3.93
67.28
3.76
12
68.02
3.10
67.45
3.32
67.48
3.52
67.95
3.32
13
67.97
3.16
67.69
3.03
67.85
3.13
67.87
3.27
14
67.90
3.22
67.93
3.30
67.46
3.25
68.10
3.18
15
67.84
3.35
69.75
4.04
67.19
4.00
67.82
3.87
16
67.46
3.65
66.56
4.01
67.47
3.65
67.18
3.68
17
67.61
3.24
67.41
3.42
67.19
3.26
67.30
3.09
18, 19








20
66.55
3.99
67.37
4.35
66.53
3.95
66.77
4.36
21
67.44
3.44
68.35
3.29
67.13
3.52
67.65
3.30
22
67.82
3.29
67.76
3.13
67.81
3.04
68.16
2.99
23
67.84
3.04
68.48
2.99
67.64
2.69
67.97
2.95
24
67.97
2.71
68.30
2.76
68.09
2.69
67.37
3.29
25
67.79
3.10
67.17
3.36
67.85
3.02
67.51
3.56
26
68.02
2.90
67.06
3.21
67.74
2.99
67.56
2.90
27
66.89
3.72
66.78
3.51
66.78
3.44
66.87
3.63
28, 29








30
66.97
3.57
68.06
3.65
67.09
3.29
67.24
3.27
31
67.67
3.15
67.90
2.91
67.40
2.94
67.75
2.98
32
67.83
3.06
67.52
2.92
67.78
2.79
67.81
2.80
33
67.37
3.17
67.43
3.21
67.25
3.24
67.37
2.99
34
66.91
3.82
67.21
3.75
66.88
3.63
67.04
3.70
35








36
64.03
6.89
62.43
9.28
64.56
6.47
64.30
7.46
37
66.65
4.46
64.06
5.78
65.80
4.93
65.13
5.25
38
67.50
2.95
66.36
3.35
67.54
3.12
67.11
3.29
39
66.81
3.99
67.82
5.90
66.52
4.71
67.29
4.78
40
64.77
5.64
57.94
9.69
64.30
5.55
63.00
6.80
41
68.88
2.94


68.98
3.11
69.03
3.23
42
60.57
4.01


59.39
4.01
58.70
4.02
43
60.82
3.96


60.96
4.08
60.67

44
67.49
3.50


67.46
3.32
67.50
3.56
Average
67.19±0.9
3.69±0.8
66.41±2.3
4.20±1.6
66.96±0.9
3.85± 1.0
66.90±1.2
3.96±1.1
Inner Six
67.86±0.1
3.08± 0.2
68.19±0.9
3.23±0.5
67.67±0.3
3.07± 0.5
67.76±0.3
3.28± 0.4
Table 4-1 Table demonstrating the influence of crystal non-uniformity to peak position and resolution The first two rows refer two a simulation run without compensation for the non-uniformity of the individual crystals. The others include a gain correction factor obtained by comparing single spectra without non-uniformity and with non-uniformity.

The gain matching has been repeated with several energies in order to check consistency. Thus it was carried out for 129 MeV photons and for both 70 MeV positrons and photons. Following the gain matching routine as described above one settles with a set of software gain factors. Beside the consistency among those three simulated energies the accuracy of the final set of software gains can be cross checked by looking at the energy resolution.


[18] For a description see [Hbo95]


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