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arXiv · 0912.0967

Induced Magnetism in Color-Superconducting Media

Efrain J. Ferrer
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Abstract

The dense core of compact stars is the natural medium for the realization of color superconductivity. A common characteristic of such astrophysical objects is their strong magnetic fields, especially those of the so called magnetars. In this talk, I discuss how a color superconducting core can generate or/and enhance the stellar magnetic field independently of a magnetohydrodynamic dynamo mechanism. The magnetic field generator is in this case a gluonic current which circulates to stabilize the color superconductor in the presence of a strong magnetic field or under the pairing stress produced in the medium by the neutrality and $β$-equilibrium constraints.

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Efrain J. Ferrer. 2010-01-22. Induced Magnetism in Color-Superconducting Media. https://arxiv.org/abs/0912.0967

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