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arXiv · 1106.5084

Properties of Magnetized Quark-Hybrid Stars

M. Orsaria·Ignacio F. Ranea-Sandoval·H. Vucetich·F. Weber
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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).

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M. Orsaria, Ignacio F. Ranea-Sandoval, H. Vucetich, F. Weber. 2011-06-25. Properties of Magnetized Quark-Hybrid Stars. https://doi.org/10.1142/s0218301311040542

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