Abstract

Despite the large interest in the application of LaBr <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sub> :Ce <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3+</sup> , little is known yet about its optical properties, as measurements are hampered by the hygroscopicity of LaBr <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sub> :Ce <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3+</sup> and because it is not trivial to produce crystals with optically polished surfaces. Here, the absorption and scattering lengths as well as the refractive index of LaBr <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sub> :5%Ce <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3+</sup> are determined experimentally for the first time. The refractive index is found to vary from 2.25 to 2.40 in the Ce <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3+</sup> emission wavelength region depending on crystal orientation. Furthermore, a model of the Ce <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3+</sup> absorption and emission probability as a function of wavelength, Ce <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3+</sup> concentration, and scintillation photon traveling distance is developed. This model is used in combination with the measured absorption and scattering lengths to obtain the intrinsic emission spectrum of LaBr <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sub> :Ce <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3+</sup> from measured emission spectra. Additionally, the model is used to illustrate the importance of the investigated crystal properties for scintillation detector design. It is demonstrated that for crystals with dimensions in the order of a few centimeters, the fraction of scintillation photons undergoing scattering and/or absorption before reaching the photosensor can be several tens of percents depending on the Ce <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3+</sup> concentration. Finally, it is shown that self-absorption and re-emission of the scintillation photons can have a non-negligible effect on the timing resolution of LaBr <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sub> :Ce <sup xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3+</sup> scintillator detectors.

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