Key research themes
1. How do neutron-induced cross section measurements advance our understanding of stellar nucleosynthesis processes?
This research theme focuses on precise experimental determination and evaluation of neutron-induced reaction cross sections, crucial for modeling the slow neutron capture process (s-process) and other nucleosynthesis pathways in different stellar environments. Accurate cross sections enable improved predictions of elemental abundances observed in stars and nucleosynthesis yields of heavy elements.
2. What innovative detection and measurement techniques improve nuclear reaction characterization in nuclear physics experiments?
This theme highlights advanced instrumental and methodological developments in nuclear measurement technologies, such as cryogenic detectors, nuclear emulsions, digital signal processing, and high-resolution spectrometry. Such developments aim to enhance detection sensitivity, accuracy, and resolution for studying nuclear reactions, decay processes, and particle identification in various applications including astrophysics, nonproliferation, and hadron therapy.
3. How do integrated nuclear data assimilation and simulation methodologies enhance nuclear data evaluation and modeling accuracy?
This research area examines the application of data assimilation (DA) techniques to combine theoretical nuclear reaction modeling and experimental measurements. DA enables optimization and uncertainty quantification of nuclear data inputs, supporting nuclear data calibration, validation, and optimization tailored for specific applications, including reactor design and astrophysical simulations. The integration of DA improves reliability and provides evidence-based validation of nuclear data libraries.