Thermodynamics of magnetized BPS baryonic layers
Thermodynamics of magnetized BPS baryonic layers
Through the Hamilton-Jacobi equation of classical mechanics, BPS magnetized Baryonic layers (possessing both baryonic charge and magnetic flux) have been constructed in the gauged non-linear sigma model (G-NLSM), which is one of the most relevant effective theories for Quantum Chromodynamics (QCD) in the strongly interacting low-energy limit. Since the topological charge that naturally appears on the right hand side of the BPS bound is a non-linear function of the baryonic charge, the thermodynamics of these magnetized Baryonic layers is highly non-trivial. In this work, using tools from the theory of Casimir effect, we derive analytical relationship between baryonic charge, topological charge, magnetic flux and relevant thermodynamical quantities (such as pressure, specific heat and magnetic susceptibility) of these layers. The critical Baryonic chemical potential is identified. Quite interestingly, the grand canonical partition function can be related with the Riemann zeta function. On the technical side, it is quite a remarkable result to derive explicit expressions for all these thermodynamics quantities of a strongly interacting magnetized system at finite Baryon density. On the physical side, such expressions allow a direct physical interpretation which we discuss.
Sergio Luigi Cacciatori、Fabrizio Canfora、Evangelo Delgado、Federica Muscolino、Luigi Rosa
物理学
Sergio Luigi Cacciatori,Fabrizio Canfora,Evangelo Delgado,Federica Muscolino,Luigi Rosa.Thermodynamics of magnetized BPS baryonic layers[EB/OL].(2025-05-23)[2025-07-16].https://arxiv.org/abs/2505.18007.点此复制
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