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Proceedings of The 26th International Nuclear Physics Conference — PoS(INPC2016)
Discovery of huge magnetic field in magnetars has stimulated a renewed interest about the magnetic field and physics of compact stars, where microphysics such as QED or QCD may play active parts. Here we discuss the equation of state (EOS) of quark matter in the core of compact stars by taking into account the strong magnetic field. We show that quark EOS becomes very stiff in the presence of the strong magnetic field, and becomes stiffest under the causality condition beyond the thresholddoi:10.22323/1.281.0146 fatcat:3zzhfbt24belrmxeo462tqwedu