Neutron Star Mass and Radius Constraints and Correlations to Dense Matter Equation of State
Offered By: Galileo Galilei Institute via YouTube
Course Description
Overview
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.
Syllabus
J. Lattimer: "Neutron star mass and radius constraints, and correlations connecting them to the ..."
Taught by
Galileo Galilei Institute
Related Courses
Inflationary CosmologyMassachusetts Institute of Technology via World Science U Gravity! The Big Bang, Black Holes and Gravitational Waves
Paris Diderot University via FutureLearn Gravité! Du Big Bang aux Trous Noirs
Paris Diderot University via France Université Numerique Einstein's Astrophysical Messengers
Louisiana State University via World Science U Introduction into General Theory of Relativity
Higher School of Economics via Coursera