Abstract
We give an introduction to the phase structure of QCD matter under rotation based on effective four-fermion models. The effects of the magnetic field on the rotating QCD matter are also explored. Recent developments along these directions are overviewed, with special emphasis on the chiral phase transition. The rotational effects on pion condensation and color superconductivity are also discussed.
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Notes
- 1.
To specify the terminology, any non-Minkowski metric with either zero or nonzero Riemann curvature is referred to as a “curved spacetime”.
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Acknowledgements
We thank Kenji Fukushima, Defu Hou, Kazuya Mameda, Kentaro Nishimura, Yin Jiang, Naoki Yamamoti, and Hui Zhang for collaborations. This work is supported in part by the NSFC Grants No. 11535012 and No. 11675041, as well as by the NSF Grant No. PHY-1913729 and by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, within the framework of the Beam Energy Scan Theory (BEST) Topical Collaboration.
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Chen, HL., Huang, XG., Liao, J. (2021). QCD Phase Structure Under Rotation. In: Becattini, F., Liao, J., Lisa, M. (eds) Strongly Interacting Matter under Rotation. Lecture Notes in Physics, vol 987. Springer, Cham. https://doi.org/10.1007/978-3-030-71427-7_11
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