Neutron Star Mass and Radius Constraints and Correlations to Dense Matter Equation of State

Neutron Star Mass and Radius Constraints and Correlations to Dense Matter Equation of State

Explore the intricacies of neutron star physics in this 57-minute lecture by J. Lattimer at the Galileo Galilei Institute. Delve into the constraints on neutron star mass and radius, and uncover the correlations that link these properties to the dense matter equation of state. Gain insights into cutting-edge research in astrophysics and nuclear physics as the speaker presents the latest findings and theoretical developments in this fascinating field of study.