Bryce Fore is a postdoctoral researcher whose research focuses on nuclear theory especially in relation to dense astrophysical matter such as neutron stars. His previous work has included calculations of the effects of pions on the dense matter nuclear equation of state, neutrino propagation, and axion production. More recently his research has focused on using quantum Monte Carlo techniques with artificial neural network wavefunction ansatz to model nuclear matter.

Education

• Doctor of Philosophy, University of Washington, Seattle (2021)
• Bachelor of Science, University of Illinois at Urbana-Champaign (2015)