Speaker
Alvaro Alejandro Siesquén Abad
(Universidad Nacional Mayor de San Marcos)
Description
We investigate the effects of both the phase transition and a smoother fluid in hybrid stars’ envelopes on the static spherically symmetric configurations. For this purpose, we assume that the fluid in the core and in the envelope follows the MIT-bag-model-equation of state and the polytropic equation of state, respectively. We find the phase transition and a smoother fluid matter on the star's envelope affect the total mass and star radius.
Primary authors
Alvaro Alejandro Siesquén Abad
(Universidad Nacional Mayor de San Marcos)
José Arbañil
(Universidad Privada del Norte)
