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Magnetic Color-flavor-locked Stars

Published online by Cambridge University Press:  20 March 2013

Laura Paulucci ,
Efrain J. Ferrer ,
Vivian de la Incera  and
Jorge E. Horvath
Laura Paulucci
Affiliation:
Universidade Federal do ABC, Brazil email: laura.paulucci@ufabc.edu.br
Efrain J. Ferrer
Affiliation:
University of Texas at El Paso, USA
Vivian de la Incera
Affiliation:
University of Texas at El Paso, USA
Jorge E. Horvath
Affiliation:
Universidade de São Paulo, Brazil
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Abstract

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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.

Keywords

stars: neutronmagnetic fieldsdense matterequation of state
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 465 - 467
Copyright
Copyright © International Astronomical Union 2013

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