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Preponderant Orbital Polarization in Relativistic Magnetovortical Matter
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We establish thermodynamic stability and gauge invariance in the magnetovortical matter of Dirac fermions under the coexistent rotation and strong magnetic field. The corresponding partition function reveals that the orbital contribution to bulk thermodynamics preponderates over the conventional contribution from anomaly-related spin effects. This orbital preponderance macroscopically manifests itself in the sign inversion of the induced charge and current in the magnetovortical matter, and can be tested experimentally as the flip of the angular momentum polarization of magnetovortical matter when the magnetic field strength is increased.
Forward citations
Cited by 3 Pith papers
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Bose-Einstein condensation in a rigidly rotating relativistic boson gas
In a slowly rotating ideal Bose gas, the BEC critical temperature scales as (density x angular velocity)^{2/5} in the nonrelativistic limit, and the heat capacity acquires a jump at the transition.
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Weak Bose-Einstein condensation in a rigidly rotating magnetized charged Bose gas
Rigid rotation does not restore a sharp BEC transition in a magnetized charged Bose gas; it only changes thermodynamics, and can flip the magnetic response toward paramagnetism.
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1+1 dimensional relativistic viscous non-resistive magnetohydrodynamics with longitudinal boost invariance
New analytic and numerical solutions for 1+1D viscous magnetohydrodynamics show that viscosity and a decaying magnetic field heat the fluid and produce an early temperature peak.
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