02.12.2012 Views

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 ...

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

50 4 Scintillation detec<strong>to</strong>rs<br />

pho<strong>to</strong>cathode, fabricated by Electron Tubes Ltd.. The energy resolution<br />

at 662 keV was aro<strong>und</strong> 4.2 % (RMS) and the resolution curve was<br />

parametrised by σ = 0.58 · � E (keV ) + 0.0191 · E (keV ). The relative<br />

standard derivation was evaluated with radioactive sources like 55 Fe,<br />

241 Am, 57 Co, 137 Cs, 22 Na and 60 Co positioned in the centre of the crystal<br />

and a 60 Co source with collima<strong>to</strong>r positioned in 5 cm distances. In<br />

this way the energy dependent and also position depending resolution<br />

due <strong>to</strong> doping nonuni<strong>for</strong>mity and different collection efficiency was regarded<br />

[43].<br />

The announced standard derivation σ determines the FWHM of any<br />

Gaussian through the relation FWHM= 2 √ 2ln2σ ≈ 2.35σ.<br />

The requirements <strong>for</strong> the COBRA <strong>upgrade</strong> are, as is discussed in the<br />

previous chapter 3, a low radioactive contamination, a high energy resolution,<br />

a moderate price and a high detection efficiency at compact<br />

size.<br />

The four scintilla<strong>to</strong>rs NaI:Tl, CsI:Tl, BGO and CWO can provide some<br />

of these properties.<br />

All four scintilla<strong>to</strong>rs can have low radioactive contamination, depending<br />

on the used scintilla<strong>to</strong>r powder and crystal production process.<br />

CWO contains the intrinsic 113 Cd, which has a low Q-value, BGO can<br />

contain 207 Bi, which has a problematically high Q-value and CsI:Tl contains<br />

the anthropogenic radioiso<strong>to</strong>pe 137 Cs. CWO and BGO have high<br />

density and high Z, but a lower light yield than NaI:Tl and CsI:Tl. Especially<br />

NaI:Tl has low density and Z, whereas the level of radioactive<br />

contamination can be very small. The drawback of NaI:Tl is also the<br />

emission spectrum, matching well with bialkali PMTs. CWO, BGO and<br />

CsI:Tl can be read out with semiconduc<strong>to</strong>r readouts. The reached energy<br />

resolution depends, beside the light yield of the scintilla<strong>to</strong>r and<br />

the matching of the scintillation emission spectrum with the quantum<br />

efficiency of the readout, also on the crystal and readout dimensions.<br />

It is not possible <strong>to</strong> deduce the reachable energy resolution of a scintilla<strong>to</strong>r<br />

of several h<strong>und</strong>red cm 3 from the resolution obtained with a<br />

small scintilla<strong>to</strong>r. The required compact size of the planned COBRA <strong>upgrade</strong><br />

favours the scintilla<strong>to</strong>r readout with semiconduc<strong>to</strong>rs, providing,<br />

the detection efficiency and energy resolution are high enough and the<br />

backgro<strong>und</strong> contamination is small enough. The consideration, which<br />

of these scintilla<strong>to</strong>rs is most suitable, requires studies, which are presented<br />

in the following chapter.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!