Abstract
Using the solutions of the gap equations of the magnetic-color-flavor- locked (MCFL) phase of paired quark matter in a magnetic field, and taking into consideration the separation between the longitudinal and transverse pressures due to the field-induced breaking of the spatial rotational symmetry, the equation of state (EoS) of the MCFL phase is self-consistently determined. Implications for stellar models of magnetized (self-bound) strange stars and hybrid (MCFL core) stars are discussed. © 2013 International Astronomical Union.
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Paulucci, L., Ferrer, E. J., De La Incera, V., & Horvath, J. E. (2012). Magnetic color-flavor-locked stars. In Proceedings of the International Astronomical Union (Vol. 8, pp. 465–467). Cambridge University Press. https://doi.org/10.1017/S1743921312024532
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