2012/12/12 by Tsintsadze, Nodar L., Tsintsadze, Levan N.
#Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences #Plasma Physics (physics.plasm-ph) #Quantum Gases (cond-mat.quant-gas)
paper · doi:10.48550/arxiv.1212.2830
To study the relativistic thermodynamic properties of a Fermi gas in a strong magnetic field, we construct the relativistic thermodynamic potential by the relativistic Fermi distribution function taking into account that the motion of particles in a plane perpendicular to the magnetic field is quantized. With this general potential at hand, we investigate all the thermodynamic quantities as a function of densities, temperatures and the magnetic field. We obtain a novel set of adiabatic equations. Having the expression of the pressure and adiabatic state equations, we determine the sound velocity for several cases revealing a new type of sound velocity. Finally, we disclose the magnetic cooling in the quantized electron Fermi gas, which is based on an adiabatic magnetization in contrast to the known adiabatic demagnetization.