Microscopic calculations of neutron matter based on nuclear interactions de-rived from chiral effective field theory, combined with the recent observation of a 1.97 ± 0.04M neutron star, constrain the equation of state of neutron-rich matter at sub- and supranuclear densities. We discuss in detail t...
Research Assistant
AI chat, annotations, notes & similar papers
No comments yet
Be the first to share your thoughts!