Properties of Magnetized Quark-Hybrid Stars
High Energy Astrophysical Phenomena
2015-05-28 v1 High Energy Physics - Phenomenology
Abstract
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).
Keywords
Cite
@article{arxiv.1106.5084,
title = {Properties of Magnetized Quark-Hybrid Stars},
author = {M. Orsaria and Ignacio F. Ranea-Sandoval and H. Vucetich and F. Weber},
journal= {arXiv preprint arXiv:1106.5084},
year = {2015}
}
Comments
5 pages, 2 figures, prepared for the 2nd International Symposium on Strong Electromagnetic Fields and Neutron Stars (SMFNS2011), Varadero, Cuba, 5-7 May 2011