Speaker
Description
Neutron stars are excellent laboratories to study the physics of matter at extreme conditions, which are beyond the scope of any terrestrial experiments. Recent multimessenger observations of neutron stars such as the measurements of the tidal deformability from the gravitational wave observation, the simulataneous mass and radius measurements of several pulsars in X-rays by the \textit{Neutron Star Interior Composition Explorer} (NICER) instrument aborad the International Space Station along with the discoveries of massive radio pulsars with $\sim 2 M_\odot$ in the last decade have significant implications towards the understanding the equation of state of dense nuclear matter. In this talk, I will discuss how this information is combined with the nuclear experimental data to constrain the properties and the composition of the interior of the neutron stars. I will also review the correlation between certain nuclear empirical parameters, such as the symmetry energy, and incompressibility with the macroscopic structure parameters, such as the radius and tidal deformability of the star.
