Articulo
Properties of Magnetized Quark-Hybrid Stars
Registro en:
issn:0218-3013
issn:1793-6608
Autor
Orsaria, Milva Gabriela
Ranea Sandoval, Ignacio Francisco
Vucetich, Héctor
Weber, Fridolin
Institución
Resumen
The structure of a magnetized quark-hybrid stars (QHS) is modeled using a standard relativistic mean-field equation of state (EoS) for the description of hadronic matter. For quark matter we consider a bag model EoS which is modified perturbatively to account for the presence of a uniform magnetic field. The mass-radius (M-R) relationship, gravitational redshift and rotational Kepler periods of such stars are compared with those of standard neutron stars (NS). Facultad de Ciencias Astronómicas y Geofísicas