PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
Quaternary compound semiconductor Cd0.9Zn0.1Te1-xSex (CZTS) is emerging as the next generation room-temperature detector for radiation spectroscopy and imaging. CZTS is grown by inclusion of Se in small amount (2-3 at. %) in the CdZnTe (CZT) matrix during the crystal growth. Travelling heater method (THM) and Bridgman method (BM) grown CZTS ingots have shown high degree of axial and radial compositional homogeneity leading to crystal growth yield higher than 90% unforeseen in CZT. While the conventional growth methods produce large volume detector grade crystals, the achievable growth rate is typically low – 1-2 mm/day for THM and 1-2 mm/hr for BM. Vertical gradient freeze (VGF) method is an alternative growth method that can deliver much higher growth rates while maintaining the electronic quality of the crystals. We report an electron drift mobility of 1245 cm^2/V/s, measured in a VGF-grown Cd0.9Zn0.1Te0.97Se0.03 (CZTS) single crystal using a time-of-flight alpha spectroscopic method, which is 1.5 times higher than that reported for state-of-the-art CZTS crystals. A mobility-lifetime (μτ) product of ~1x10^-3 cm^2/V was calculated using a single polarity Hecht plot. Photo-induced deep level transient spectroscopy (PICTS) revealed the presence of several charge trapping centers in the temperature scan range 80 - 450 K. The study correlates the effect of the trap parameters on the performance of room-temperature gamma-ray detectors grown using the VGF method.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The alert did not successfully save. Please try again later.
Ritwik Nag, Sandeep K. Chaudhuri, Krishna C. Mandal, "Correlation of transport properties with charge trapping parameters in Cd0.9Zn0.1Te1-xSex room temperature gamma-ray detectors," Proc. SPIE PC12696, Hard X-Ray, Gamma-Ray, and Neutron Detector Physics XXV, PC1269604 (4 October 2023); https://doi.org/10.1117/12.2682618