39: Optimizing Gamma Detector Geometries for Astrophysics and Planetary Science

Presenter(s)

Charlie Fallon

Abstract or Description

Gamma radiation, characterized by its high energy, holds immense significance in nuclear astrophysics and planetary science. Emitted from distant astronomical entities like blazars and quasars, gamma rays not only provide a lens to observe these objects but also reveal the elemental composition of celestial bodies by detecting gamma-emitting elements hidden beneath surfaces. Consequently, the efficacy of gamma detectors, instrumental in capturing and interpreting this radiation, becomes paramount. This research seeks to enhance current detector capabilities, posing the question: How can we optimize these detectors for a deeper understanding of gamma radiation sources? Through the use of computer simulations, we've explored various detector geometries under diverse scenarios and gamma sources. Preliminary findings indicate a favorable alignment between simulated outcomes and in-lab measurements. While these early results are promising, the research is ongoing. Future endeavors will leverage simulations to evaluate prototype detectors, marking a significant stride towards refined tools for astrophysical studies.