Induced Magnetism in Color-Superconducting Media

Details Induced Magnetism in Color-Superconducting Media Induced Magnetism in Color-Superconducting Media

2009-12-05

arxiv.org/abs/0912.0967v2

Physics

High Energy Physics

High Energy Physics - Phenomenology

To appear in Proceedings for "Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, KIAA at Peking University

Scientific paper

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 $\beta$-equilibrium constraints.

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