Properties of massive rotating protoneutron stars with hyperons: structure and universality

In this work, we study the properties and structure of a massive and rapidly rotating protoneutron star (PNS) with hyperon content. We follow several stages of quasi-stationary evolution in an approximate way at four discrete steps. We use a density-dependent relativistic mean field theory model and calculate different quantities such as mass, equatorial radius, moment of inertia, and quadrupole moment to get different rotating configurations up to the mass-shedding limit. We study the effect of the appearance of Lambda, the lightest of all hyperons, on each of the evolutionary stages of the PNS. We also check its sensitivity to the inclusion of phi vector meson as a mediator of Lambda-Lambda interaction in detail. Finally, we investigate the universal relations between moment of inertia and compactness in the context of a hot and young compact object.