Quark mass dependence of the QCD temperature transition in magnetic fields
arXiv:1312.4178 · doi:10.1103/PhysRevD.89.074034
Abstract
Vacuum energy of quarks participates in the pressure balance at the temperature transition T_c and defines the dependence of T_c on m_q. We first check this dependence in absence of magnetic fields eB vs known lattice data, and then take into account the known strong dependence of the quark condensate on eB. The resulting function T_c(eB, m_q) is valid for all eB, m_q< \sqrtσand explains the corresponding lattice data.
14 pages, 2 figures
References in corpus (9)
- The QCD transition temperature: results with physical masses in the continuum limit
- Quark-hadron phase transition in a magnetic field
- Can a strong magnetic background modify the nature of the chiral transition in QCD?
- Vacuum phase transition at nonzero baryon density
- The phase diagram of quantum chromodynamics
- Nonperturbative equation of state of quark-gluon plasma. Applications
- The quark-hadron thermodynamics in magnetic field
- Review of recent highlights in lattice calculations at finite temperature and finite density
- Thermodynamic properties of QCD in external magnetic fields
Cited by in corpus (9)
- QCD phase diagram in a magnetic background for different values of the pion mass
- Nonperturbative SU(3) thermodynamics and the phase transition
- Nonperturbative QCD thermodynamics in the external magnetic field
- Magnetic susceptibility at zero and nonzero chemical potential in QCD and QED
- Chiral Perturbation Theory Analysis of the Quark Condensate in a Magnetic Field
- QCD Equation of State and Cosmological Parameters in Early Universe
- Dense Quark-Gluon Plasma in strong magnetic fields
- Quark Condensate in a Weak Magnetic Field
- Pion Pressure in a Magnetic Field