research

our framework

In our research in nuclear astrophysics, we take a systems approach to understanding how the elements are made in the Cosmos. We begin by identifying the most important nuclear processes that shape the evolution of stars and stellar explosions, using nucleosynthesis calculations based on advanced stellar models. To probe these critical reactions, we carry out experiments with radioactive ion beams at leading facilities around the world. These measurements help reduce uncertainties in the models and sharpen our picture of how the rarest elements are formed. Finally, we compare our predictions with the latest astronomical observations, which both test our theories of nucleosynthesis and guide the direction of future experiments and modeling.

You can explore more in our publications and presentations. If you want to discuss further, don’t hesitate to contact.


  Research Interests

nuclear astrophysics • radiative capture reactions with recoil separators • nuclear reaction networks • large-scale nuclear sensitivity studies • charged–particle spectroscopy • in–beam and activation γ-ray spectroscopy • experimental studies with stable and radioactive ion beams


The origin of the elements

Big Bang nucleosynthesis
Cosmic Ray Spallation
Massive stars
Exploding massive stars
Neutron Star Mergers or ν-driven ejecta
Dying low- and intermediate-mass stars
Exploding white dwarfs
Man-made, artificial (or decay products)
Motivated by Christian Iliadis' (UNC/TUNL) version.