The compressibility of quark matter under strong magnetic field in the NJL model
arXiv:2111.10008 · doi:10.1103/PhysRevD.104.114010
Abstract
The compressibility of magnetized quark matter is investigated in the SU(2) NJL model. The increases of the chemical potential and the temperature can reduce the compressibility, and lead to the much stiffer equation of state. The variation of the compressibility with the magnetic field will depend on the phase region. Due to the anisotropic structure, the compressibility is different in the directions parallel and perpendicular to the field. The discontinuity of longitudinal compressibility with the chemical potential and the temperature captures the signature of a first-order chiral phase transition and the crossover at high temperature. Moreover, the magnetic-field-and-temperature running coupling would have an important effect on the position of the phase transition. Under the lowest landau level approximation at zero temperature, the longitudinal compressibility has a direct inverse proportional relation to the magnetic field strength and the chemical potential square as .
11 pages, 10 figures
References in corpus (16)
- The Chiral Magnetic Effect
- Quantum field theory in a magnetic field: From quantum chromodynamics to graphene and Dirac semimetals
- Charge separation induced by P-odd bubbles in QCD matter
- Chiral Magnetic conductivity
- Quark matter under strong magnetic fields in the Nambu--Jona-Lasinio Model
- The Importance of Asymptotic Freedom for the Pseudocritical Temperature in Magnetized Quark Matter
- Inverse magnetic catalysis in the (2+1)-flavor Nambu--Jona-Lasinio and Polyakov--Nambu--Jona-Lasinio models
- Chiral transition in a strong magnetic background
- Anisotropic pressure of deconfined QCD matter in presence of strong magnetic field within one-loop approximation
- Inverse magnetic catalysis and regularization in the quark-meson model
- Thermodynamics of Neutrons in a Magnetic Field and its Implications for Neutron Stars
- Magnetized color flavor locked state and compact stars
- Chiral restoration at finite T under the magnetic field with the meson-loop corrections
- The quark mass gap in strong magnetic fields
- Magnetic-Field Induced Critical Endpoint
- Effects of the temperature and magnetic-field dependent coupling on the properties of QCD matter