Deep UV emitting scintillators for alpha and beta particle detection

• Published in: Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Accelerators, spectrometers, detectors and associated equipment, 2011-03, Vol.633 (1), p.31-35
• Main Authors: Zhou, Y., Jia, D.D., Lewis, L.A., Feofilov, S.P., Meltzer, R.S.
• Format: Article
• Language: English
• Subjects: Alpha rays; Deep UV; Detectors; Electron energy; Emittance; Ionization; Light yields; Monitors; Radiation monitoring; Scintillators; Spectrometers
• ISSN: 0168-9002; 1872-9576
• DOI: 10.1016/j.nima.2010.12.238

Several deep UV emitting scintillators, whose emission falls in the solar blind region of the spectrum (200–280 nm), are described and their scintillator properties are characterized. They include LaPO 4:Pr, YPO 4:Pr, YAlO 3:Pr, Pr(PO 3) 3, YPO 4:Bi and ScPO 4. These materials would facilitate the detection of ionizing radiation in open areas, even during the daylight hours, and could be used to support large area surveys that monitor for the presence of ionization radiation due, for example, to system leaks or transfer contamination. These materials can be used in the form of powders, thin films or paints for radiation detection. They are characterized for both beta radiation using electron beams (2-35 keV) and 137Cs and alpha radiations using 241Am sources. Their absolute light yields are estimated and are compared to that of Y 2SiO 5:Ce. Their light yields decrease as a function of electron energy but at 10 keV they approach 8000 ph/MeV.