Hybrid magnetized stars in the context of multi-messenger astronomy
Abstract
The most recent detections of LIGO/Virgo and NICER have placed strong constraints on neutron stars' properties. In this work, we study neutron stars modeling them as hybrid stars, compact objects with a quark matter core surrounded by layers of hadronic matter. In addition, we consider the presence of strong magnetic fields, motivated by magnetars detection, like the recently discovered Swift J1818.0-1607. We incorporate the effects of the anomalous magnetic moment of the constituent particles into the equation of state of dense matter and analyze the implications of different hadron-quark phase transitions on the dynamic stability of these compact objects. This study shows that the constraints on the mass, radius, and tidal deformability, imposed by observations of massive pulsars and gravitational waves can be satisfied within the framework of our model.
Keywords
Cite
@article{arxiv.2203.15673,
title = {Hybrid magnetized stars in the context of multi-messenger astronomy},
author = {Mauro Mariani and Daniela Curin and Milva G. Orsaria and Ignacio F. Ranea-Sandoval},
journal= {arXiv preprint arXiv:2203.15673},
year = {2022}
}
Comments
Proceeding accepted for publication in the 63 Bolet\'in de la Asociaci\'on Argentina de Astronom\'ia, in Spanish language