QCD vacuum structure in strong magnetic fields
arXiv:hep-ph/0204120 · doi:10.1103/PhysRevD.66.014004
Abstract
We study the response of the QCD vacuum to strong magnetic fields, using a potential model for the quark-antiquark interaction. We find that production of spin-polarized u-ubar pairs is energetically favorable for fields B > B_crit \sim 10 GeV^2. We contrast the resulting u-ubar condensate with the quark condensate which is present at zero magnetic field, and we estimate the corresponding magnetization as a function of B.
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