PAN is sponsored by the Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements (JINA-CEE) which is a Physics Frontier Center funded by the National Science Foundation.

The school is connected to the International Conference on Nuclear Physics in Astrophysics X and aims at introducing important concepts related to nuclear astrophysics, including experimental and theoretical nuclear physics, astrophysics and astronomical observations.

Please join us at 7:00pm at 1300 Auditorium at the FRIB Laboratory for this performance

The workshop will bring together experts from the four areas hydrodynamic simulations, neutrino-flavor physics, r-process nucleosynthesis, and kilonova modeling. The goal is to identify the main shortcomings of current models and to discuss strategies for how to propagate modeling uncertainties into r-process abundances and kilonova predictions, thereby improving models in a way to maximize the scientific output of future multi-messenger observations of neutron star mergers.