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We have investigated the applicability of phosphate glasses as host systems for the formation of rare-earth-activated
gamma- and x-ray scintillators. Glass scintillators have generally suffered from low light yields, usually attributed to
inefficient energy transfer from the glass matrix to the luminescent center. Our research on these phosphate glasses has
shown that their structural properties can be readily varied and controlled by compositional alterations. The melting and
pouring temperature of ~1050°C for these phosphate glasses is significantly lower than the processing temperatures
generally associated with the formation of silicate glass scintillators. The calcium-sodium phosphate glasses will
tolerate relatively high cerium concentrations based on the initial melt compositions, and the light yield for gamma-ray
excitation at 662 keV was determined as a function of cerium concentration up to the saturation level. The rare-earth-activated
Ca-Na phosphate glass primary-component decay time was in the range of 32 to 42 nsec for various Ce
concentrations with the contribution of the light output of the primary component ranging from 80 to 90%. Studies of the
effects of co-doing with both Ce and Gd were also carried out in the case of the Ca-Na phosphate glass hosts. The
effects of post-synthesis thermochemical treatments in a variety of atmospheres and at various processing temperatures
were also investigated for the Ce-activated Ca-Na phosphate scintillators.
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John S. Neal, Lynn A. Boatner, Dariusz Wisniewski, Joanne O. Ramey, "New rare-earth-activated phosphate glass scintillators," Proc. SPIE 6706, Hard X-Ray and Gamma-Ray Detector Physics IX, 670618 (24 September 2007); https://doi.org/10.1117/12.734561