The study of the detector’s efficiency can be very interesting in our experiment: gamma rays are uncharged, so they can travel in the detector for long distances before they interact; for this reason we need a relation between the number of incident photons and the number of detector’s counts. We analized 232Th’s spectra to study the dependence of HpGe detector's efficiency versus Energy.
EFFrel=N/I
Where N is the number of counts obtained by the gaussian peak’s integration and I is the relative intensity of the line (from http://atom.kaeri.re.kr/).
We have fitted 232Th’s datas with the following linear function (Knoll, “Radiation Dectection and Measurement”):
og(eff) = A + B log (E/E0)
(questa formula e la precedente le ho scritte con microsoft equation ma non riesco a copiarle...beh l'importante è che si capiscano)
As we can see from image XXX, (in which we put E0=1Kev), the best efficiency has been obtained for the lowest Energy.
peggio di fiorini....

1 commento:
bella!
io non direi che i fotoni possono percorrere lunghe distanze, solo nel vuoto! i 5cm di germanio se li succhiano quasi tutti!
Posta un commento