Speaker
Prof.
José Arbañil
(Universidad Privada del Norte and Universidad Nacional Mayor de San Marcos)
Description
In this work, we investigate the influence of the phase transition and a stiffer fluid in neutron stars core on the static equilibrium configuration, dynamical stability, and tidal deformability. For this aim, it is taken into account that the fluid on the core and the envelope follow the relativistic polytropic equation of state. We find that phase transition and a stiffer fluid in the core will reflect in the total mass, radius, radial stability with a slow and rapid conversion at the interface, and tidal deformability.
Primary authors
Prof.
César Lenzi
(Instituto Tecnológico de Aeronáutica)
Prof.
José Arbañil
(Universidad Privada del Norte and Universidad Nacional Mayor de San Marcos)
