Hybrid magnetized stars within the Field Correlator Method

MILVA G. ORSARIA; IGNACIO FRANCISCO RANEA SANDOVAL; MAURO MARIANI; OCTAVIO MIGUEL GUILERA

La Serena

Congreso; 61 reunión anual de la AAA; 2018

We present preliminary results of the study of intense magnetic fields effects on hybrid stars. For the description of the hadronic phase, we use the relativistic mean field approximation. For the quark matterphase, we employ the Field Correlator Method formalism. Once the the equation of state is built, we discuss the pressure anisotropy due the presence of the strong magnetic field. Finally, we calculate the structure of the compact stars using magnetized hybrid equations of state and their oscillation modes related with the emission of gravitational waves