Magnetic susceptibility of hot hadronic medium and quark degrees of freedom near the QCD cross-over point
Rupam Samanta, Wojciech Broniowski
TL;DR
This paper addresses the mismatch between lattice QCD results for the magnetic susceptibility $\\chi_B$ near the QCD crossover and Hadron Resonance Gas (HRG) predictions. It shows that HRG fails to capture the observed near-$T_c$ paramagnetism unless a light paramagnetic sector is present, and it then develops a non-interacting quark–meson model with temperature-dependent quark masses fitted to lattice susceptibilities $\\chi_{BB}$ and $\\chi_{BS}$, including vacuum contributions and quark anomalous magnetic moments. The results demonstrate that the vacuum quark contribution, the thermal quark sector, and the meson sector together can reproduce the lattice behavior of $\\chi_B(T)-\\chi_B(0)$ around $T_c$, while hadronic polarizabilities are negligible and pion–vector-meson loops provide only modest corrections. The findings underscore the necessity of light, paramagnetic degrees of freedom and vacuum effects below $T_c$ to correctly describe the magnetic response of hot QCD matter, with implications for modeling the hadronic phase in strong magnetic fields.
Abstract
We argue that the lattice QCD results for the temperature-dependent magnetic susceptibility of the medium below the cross-over temperature are difficult to reconcile with the available hadronic models. In particular, in the widely used Hadron Resonance Gas model, reproducing well numerous other features of the medium, one observes a substantially too strong diamagnetism compared to the lattice simulations. One thus needs a significant source of paramagnetism below the QCD cross-over temperature, possible to achieve with sufficiently light fermions. We thus consider a quark-meson model, where the temperature-dependent quark masses are fixed from the baryon-baryon and baryon-strangeness susceptibility data from the lattice at zero magnetic field. We show that in such a framework one can describe the magnetic susceptibility, with the vacuum contributions duly incorporated. In the hadronic picture, we also evaluate the contribution of the pion--vector-meson loops to the magnetic susceptibility evaluated via the photon polarization, showing it is small and paramagnetic.
