The equilibrium of the dense electron-nuclear plasma in the gravitational field. The magnetic fields and masses of stars
arXiv:astro-ph/0307039
Abstract
The equilibrium of a hot dense plasma in a gravitational field is considered. From the standard equilibrium equations, the energy minimum at density about particles per and temperature about was found. This effect plays an important role for astrophysics. It enables to explain the mechanism of the star magnetic field generation and to make a prediction for the spectrum of a star mass with a wholly satisfactory agreement for the observation data.
19 pages, 3 figures