2007/01/01 by Vivian de la Incera, Ricardo Alarcón, P. L. Cole +2 · 1 citation
Earth and Planetary Sciences · Physics and Astronomy · #High-pressure geophysics and materials #Pulsars and Gravitational Waves Research #Quantum, superfluid, helium dynamics #astro-ph #hep-ph #nucl-th
paper · pdf · doi:10.1063/1.2813838
published as AIPConf.Proc.947:395-400,2007 · Presented at VII Latin American Symposium on Nuclear Physics and Applications, El Cusco, Peru, June 2007
openalex publication_date 2007/01/01 · arxiv created 2007/08/12 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/29
In this paper I discuss the magnetic phases of the three‐flavor color superconductor. These phases can take place at different field strengths in a highly dense quark system. Given that the best natural candidates for the realization of color superconductivity are the extremely dense cores of neutron stars, which typically have very large magnetic fields, the magnetic phases here discussed could have implications for the physics of these compact objects.