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a design study for a cobra upgrade to - Institut für Kern- und ...

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4.2 Detec<strong>to</strong>r assembly 43<br />

secondary electrons are accelerated <strong>to</strong> the second dynode and so on.<br />

PMTs have typically 9 <strong>to</strong> 16 dynodes and an overall multiplication fac<strong>to</strong>r<br />

(gain) of 10 6 up <strong>to</strong> 10 9 . The final electron pulse is collected at the<br />

anode and has a time delay of 20-50 ns and a width of a few nanoseconds.<br />

The detection of single pho<strong>to</strong>ns is possible. The Hamamatsu<br />

PMT R669 shows a temperature coefficient of -0.3 %/K at 550 nm [39].<br />

The time resolution of a PMT is mainly determined by the escape velocity<br />

of the pho<strong>to</strong>electron and the distance between the emission point<br />

and the hitting point at the first dynode. It is typically below one ns<br />

[28, 29, 30].<br />

PIN diodes consist of a p-doped primary material that is heavily<br />

n-doped on one surface. A controlled diffusion of the dona<strong>to</strong>r a<strong>to</strong>ms<br />

leads <strong>to</strong> a n-doped layer at the surface and an internal i-region, with<br />

nearly intrinsic properties. There the number of accep<strong>to</strong>r and dona<strong>to</strong>r<br />

a<strong>to</strong>ms is identical and the specific resistance of 10 5 Ωcm corresponds<br />

<strong>to</strong> the intrinsic resistance of silicon. The depletion zone must be thick<br />

enough so that incident particles can create enough ionisation in the<br />

sensitive region <strong>to</strong> <strong>for</strong>m a larger signal than the noise level. The<br />

thickness of the depletion zone is limited <strong>to</strong> 10 <strong>to</strong> 15 mm and is much<br />

bigger than that of diodes with pn-junction. This is suitable <strong>for</strong> beta<br />

or low-energy pho<strong>to</strong>n detection. The small p-layer of the diode is the<br />

entrance window. The incident ionising particles can produce direct<br />

or indirect electron hole pairs. Those are produced in the i-region and<br />

the induced charge is processed <strong>to</strong> an attached preamplifier <strong>to</strong> produce<br />

the output signal at the anode. With a required energy <strong>for</strong> excitation of<br />

3.6 eV in Silicon and 2.8 eV in Germanium, they are able <strong>to</strong> detect the<br />

typical scintillation light of 3-4 eV with a high quantum efficiency of<br />

60-80 %. Only in the best case, as much electron hole pairs as incident<br />

scintillation pho<strong>to</strong>ns are produces. These are typically just a few<br />

h<strong>und</strong>red. Without any multiplication process the signal is 8 orders of<br />

magnitude lower than that of PMTs. Electronic noise is a problem due<br />

<strong>to</strong> this very small signal. PIN diodes have a fac<strong>to</strong>r 2 worse resolution<br />

than PMTs and can compete only <strong>for</strong> high energetic particles [29]<br />

The temperature dependence of pho<strong>to</strong>diodes (Hamamatsu S2744-08)<br />

is very small with 0.01 %/K at 550 nm [39].<br />

The greater sensitive region leads <strong>to</strong> a greater thermal noise than normal<br />

diodes. Thus cooling is necessary <strong>to</strong> gain a high resolution. The<br />

dark noise can also be reduced by using materials with a larger band<br />

gap than silicon, like mercury iodide crystals. Such PIN diodes are superior<br />

<strong>to</strong> PMTs and achieve energy resolutions of 4.58 % with CsI:Tl<br />

scintilla<strong>to</strong>rs [28, 29, 30, 41].

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