Hybrid magnetized stars within the Field Correlator Method

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

Congreso; Segunda Reunión Binacional AAA-SOCHIAS 2018; 2018

We study the effects of intense magnetic fields on hybrid stars. For the description of the hadronic phase, we use the mean field approximation. For the quark matter, we use the formalism of the Field Correlator Method. Once the the equation of state (EoS) is built, we discuss the pressure anisotropy due to the presence of the magnetic field and the effects of magnetization. Finally, we calculate the structure of the compact stars using the magnetized hybrid EoSes and analyse their oscillation modes and the corresponding emission of gravitational waves.