Hybrid magnetized stars within the Field Correlator Method

Ignacio F. Ranea-Sandoval; Mauro Mariani; Milva G. Orsaria; Octavio M. Guilera

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Hybrid magnetized stars within the Field Correlator Method

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arxiv 1902.02814 v1 pith:2A6TZS3Q submitted 2019-02-07 astro-ph.HE

Mauro Mariani , Milva G. Orsaria , Ignacio F. Ranea-Sandoval , Octavio M. Guilera This is my paper · ORCID

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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 matter phase, 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.

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