The quark mass gap in strong magnetic fields
arXiv:1407.7925 · doi:10.1016/j.nuclphysa.2014.08.004
Abstract
Quarks in strong magnetic fields (|eB|>>Lambda_QCD^2 ~ 0.04 GeV^2) acquire enhanced infrared phase space proportional to |eB|. Accordingly they provide larger chiral condensates and stronger backreactions to the gluon dynamics. Confronting theories with lattice data at various values of |eB|, one can test theoretical ideas as well as validity of various approximations, domain of applicability of the effective models, and so on. The particularly interesting findings on the lattice are inverse magnetic catalysis and linear growth of the chiral condensate as a function of |eB|, which pose theoretical challenges. In this talk we propose a scenario to explain both phenomena, claiming that the quark mass gap should stay at around ~ Lambda_QCD, instead of ~|eB|^{1/2} which has been supposed from dimensional arguments and/or effective model calculations. The contrast between infrared and ultraviolet behaviors of the interaction is a key ingredient to obtain the mass gap of ~Lambda_QCD.
arXiv comment4 pages, proceedings of the XXIV Quark Matter conference, May 19-24 2014, Darmstadt (Germany)
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- Magnetic-Field Induced Critical Endpoint
- Chiral phase transition of three flavor QCD with nonzero magnetic field using standard staggered fermions
- Effects of the temperature and magnetic-field dependent coupling on the properties of QCD matter
- Landau levels of cold dense quark matter in a strong magnetic field
- The compressibility of quark matter under strong magnetic field in the NJL model