Speaker
Description
We study the effect of the isovector-scalar meson
We also include the
We find that, when the chiral invariant mass of nucleon
We then construct the equation of state (EoS) of a neutron star matter to obtain the mass-radius relation of NS.
We find that, in most choices of
We then constrain the chiral invariant mass of nucleon from the observational data of NS, and find that