Abstract
In this chapter, we discuss several aspects of the theory of strong interactions in presence of a strong magnetic background. In particular, we summarize our results on the effect of the magnetic background on chiral symmetry restoration and deconfinement at finite temperature. Moreover, we compute the magnetic susceptibility of the chiral condensate and the quark polarization at zero temperature. Our theoretical framework is given by chiral models: the Nambu-Jona-Lasinio (NJL), the Polyakov improved NJL (or PNJL) and the Quark-Meson (QM) models. We also compare our results with the ones obtained by other groups.
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Notes
- 1.
If the vacuum corrections are neglected, the deconfinement and chiral crossovers are found to be coincident even in very strong magnetic fields [71], but the critical temperature decreases as a function of eB; this scenario is very interesting theoretically, but it seems excluded from the recent Lattice simulations [44].
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Acknowledgements
We are pleased to acknowledge the editors of this volume of Lecture Notes in Physics for their interest in our work and their kind invitation to contribute to the book. We also acknowledge K. Fukushima and M. Frasca for scientific collaborations which led to some of the results presented here. Finally we also acknowledge many clarifying discussions with M. D’Elia and G. Endrodi about the topics discussed in this chapter, with particular reference to the ones related to Lattice simulations.
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Gatto, R., Ruggieri, M. (2013). Quark Matter in a Strong Magnetic Background. In: Kharzeev, D., Landsteiner, K., Schmitt, A., Yee, HU. (eds) Strongly Interacting Matter in Magnetic Fields. Lecture Notes in Physics, vol 871. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-37305-3_4
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