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76 5 Scintilla<strong>to</strong>r <strong>upgrade</strong><br />

Figure 5.11: Energy deposition of about 1.8×10 5 coincident 134 Cs<br />

events in one or two CZT and CsI detec<strong>to</strong>rs, with marked 5σ interval<br />

aro<strong>und</strong> the 1294 keV entry in the CsI detec<strong>to</strong>rs.<br />

The backgro<strong>und</strong> contribution of 134 Cs <strong>for</strong> events with more than two<br />

involved detec<strong>to</strong>rs can be reduced by considering the angle correlation<br />

of the subsequent gamma rays. After a 134 Cs decay, the majority<br />

of gamma rays are emitted at a 4 + → 2 + → 0 + transition<br />

with a correlation of the emitting angle between both pho<strong>to</strong>ns of<br />

W (θ) ∝ 1 + 1<br />

8 cos2 θ + 1<br />

24 cos4 θ. This favours emission in the same or op-<br />

posite directions. Up <strong>to</strong> now, the only in<strong>for</strong>mation of the interaction<br />

position is the involved detec<strong>to</strong>r number. An analysis, considering the<br />

angles between the in one event involved detec<strong>to</strong>rs is, owing <strong>to</strong> the big<br />

dimensions of the CsI crystals in comparison <strong>to</strong> the small distance between<br />

different detec<strong>to</strong>rs, not possible. However, the distribution of<br />

hits in neighbouring and not neighbouring CsI crystals was studied.<br />

It showed, that the regarded double beta decay leads <strong>to</strong> more hits in<br />

neighbouring and next neighbouring CsI crystals (<strong>for</strong> events, involving<br />

one CZT and two CsI crystals) than 134 Cs decays. Four categorisations<br />

are distinguished, being neighbouring crystals, which have a joint<br />

surface (N), next neighbouring crystals with a joint edge (NN), crystals<br />

at opposite sides of the Nest, having joint surfaces with the Nest (O)<br />

and crystals, being not in the <strong>for</strong>mer categorisation (R). The distribu-

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