QUANTUM SPONTANEOUS MAGNETIZATION

Abstract

The problem of spontaneous generation of magnetic fields in plasma is one of the main problems in physics. The idea of this generation by the motion of a conducting fluid is based on the classical instability of the wave type. The amplification of the seed field or the transformation of one field component into another occurs through a dynamo mechanism, for example, toroidal to poloidal in a rotating ball. Superexchange in an ionized gas is considered . In a dense low-temperature plasma, the effects of overlapping of electron shells turn out to be significant even before the overlapping stage. The overlap integrals in the expression for the energy of ions interacting via electronic exchange reduce the latter. The decrease in energy is the greater, the closer to each other the projections of the orbital momenta of active electrons onto a fixed quantization axis. In this case, the orbital moments of the particles, and hence the magnetic moments, are co-directed . For the first time, a mechanism has been developed for the occurrence of magnetic fields in the central regions of planets, stars and on the surface of the Sun.