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We examine the near collapse dynamics of a self-gravitating magnetizedelectron gas at finite temperature, taken as the source of a Bianchi-Ispacetime described by the Kasner metric. The set of Einstein-Maxwell fieldequations reduces to a complete and self-consistent system of non-linearautonomous ODE's. By considering a representative set of initial conditions,the numerical solutions of this system show the gas collapsing into both,isotropic ("point--like") and anisotropic ("cigar-like") singularities,depending on the intensity of the magnetic field. We also examined the behaviorduring the collapse stage of all relevant state and kinematic variables: thetemperature, the expansion scalar, the magnetic field, the magnetization andenergy density. We notice a significant qualitative difference in the behaviorof the gas for a range of temperatures between the values$\hbox{T}\sim10^{3}\hbox{K}$ and $\hbox{T}\sim 10^{7}\hbox{K}$.

Gravity induced evolution of a magnetized fermion gas with finite temperature