Reaction theory is fascinating because it sits at the intersection of the experimental world and the theory that explains the internal organization in nuclei themselves. Reaction theory is the essential bridge between these two worlds. In the FRIB few-body reaction group, our goal is to improve the theoretical description of reactions involving exotic nuclei, needed to interpret experimental data, and arrive at a more fundamental understanding of the their dynamical processes. A large part of our focus is on direct reactions, such as capture, breakup, knockout, transfer reactions, many of which are of astrophysical interest. Our research is key to both, unveiling exotic phenomena away from stability, such as halo formation, and improving our understanding of the nucleosynthesis occurring in explosive stellar environments. In addition, our group uses Bayesian analysis to quantify uncertainties and to explore experimental design.
Figure: From ab initio to few-body description of reactions.
When a nucleus impinges on another nucleus, this constitutes a complex many-body problem, where the dynamics of all nucleons need be treated accurately. Typically, this complex problem is untractable and therefore simplified into a few-body problem (illustrated above) where most nucleonic degrees of freedom are frozen into specific clusters. In this few-body picture, simplified potentials are used to simulate the interactions between the clusters. To arrive at a predictive description of reactions we must combine robust few-body methods with potentials grounded on the underlying nuclear structure, as well as have quantified uncertainties. Projects in our group can be broadly grouped into three categories:
Enhancing the connection between microscopic predictions and few-body models;
Developing accurate methods to solve few-body reactions;
Quantifying the theoretical uncertainty in few-body models of reaction observables.