Equation of State Development for Neutron Star Merger Simulations

Learn about a groundbreaking research project focused on developing an Equation of State (EoS) for neutron star merger simulations in this physics lecture. Explore the collaborative effort between the University of Caen and the University of Milano-Bicocca to construct a reliable EoS up to twice the nuclear saturation density. Examine the limitations of current nuclear physics models in simultaneously describing electric nuclear dipole polarizability and parity violating asymmetry in different nuclei. Discover the crucial connections between these observables and specific properties of the neutron matter EoS, while understanding why advancing theoretical nuclear physics is essential for both nuclear structure studies and astrophysical applications. Delve into detailed discussions of nuclear models, laboratory observations, neutral skin thickness, resonances, and the challenges faced at low densities, supported by recent research findings published in Physical Review Letters.