a design study for a cobra upgrade to - Institut für Kern- und ...
a design study for a cobra upgrade to - Institut für Kern- und ...
a design study for a cobra upgrade to - Institut für Kern- und ...
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5.1 Monte Carlo studies <strong>for</strong> the <strong>upgrade</strong> <strong>design</strong> 57<br />
cage is also limited. It is there<strong>for</strong>e favourable <strong>to</strong> build a compact scintillation<br />
detec<strong>to</strong>r.<br />
The advantages and disadvantages of these four different scintilla<strong>to</strong>rs<br />
<strong>for</strong> the planned COBRA <strong>upgrade</strong> are listed in table 5.4. NaI:Tl, although<br />
being a common used scintilla<strong>to</strong>r with a very high light yield<br />
and low radioactive contamination, has <strong>for</strong> this project a <strong>to</strong> low density<br />
and a<strong>to</strong>mic number. Additionally, the required PMT readout and<br />
the difficult handling of this hygroscopic scintilla<strong>to</strong>r is not suitable. An<br />
<strong>upgrade</strong> with BGO can be used with diode readout and is compact in<br />
size, but BGO has a low light yield, leading <strong>to</strong> a low energy resolution<br />
and the contained radioiso<strong>to</strong>pe 207 Bi (Q-value = 2.3 MeV) can be a serious<br />
backgro<strong>und</strong> component <strong>for</strong> the searched signal. CWO is a suitable<br />
scintilla<strong>to</strong>r <strong>for</strong> this <strong>upgrade</strong>, but is nearly twice as expensive as BGO.<br />
CsI:Tl has the highest light yield, a readout with diodes is possible and<br />
the radioactive 137 Cs is not expected <strong>to</strong> be a serious backgro<strong>und</strong> <strong>for</strong> the<br />
2νββ signal of transitions in<strong>to</strong> the excited state. Although it is not as<br />
compact as BGO or CWO, this <strong>upgrade</strong> is also less expensive.<br />
scintilla<strong>to</strong>r light yield size handling diode readout radioactivity<br />
CsI:Tl �� � � �� �<br />
CWO � �� �� � �<br />
BGO - �� �� � -<br />
NaI:Tl �� - - - ��<br />
Table 5.4: Advantages ( �) and disadvantages (-) of different scintilla<strong>to</strong>rs.<br />
Accordingly, 5 cm of CsI:Tl were considered as a compromise between<br />
cost and detection efficiency. Due <strong>to</strong> its much higher light yield than<br />
BGO and CWO and, in comparison <strong>to</strong> NaI:Tl, more easy handling, it<br />
was chosen as the most promising scintilla<strong>to</strong>r material <strong>for</strong> this <strong>upgrade</strong>.<br />
5.1.3 Electronic readout<br />
The Cobra Nest will be surro<strong>und</strong>ed by a layer of 5 cm CsI crystals. For<br />
a high detection efficiency and smaller amounts of needed scintilla<strong>to</strong>r<br />
material, the scintilla<strong>to</strong>r should be placed as close as possible <strong>to</strong> the<br />
Nest with as little material as possible between the CZT and the scintilla<strong>to</strong>rs.<br />
The scintilla<strong>to</strong>r readout device is there<strong>for</strong>e placed at the outer<br />
sides of the scintilla<strong>to</strong>r layer. Additionally, electronic devices nearby<br />
the CZT detec<strong>to</strong>r increase the backgro<strong>und</strong> level. In general, all six outer<br />
sides of the layer could be used <strong>for</strong> placing the readout. The front and