The equilibrium of the dense electron-nuclear plasma in the gravitational field. The magnetic fields and masses of stars

B. V. Vasiliev

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The equilibrium of the dense electron-nuclear plasma in the gravitational field. The magnetic fields and masses of stars

B. V. Vasiliev

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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 $10^{25}$ particles per $cm^3$ and temperature about $10^7 K$ 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.

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B. V. Vasiliev. 2003-07-09. The equilibrium of the dense electron-nuclear plasma in the gravitational field. The magnetic fields and masses of stars. https://arxiv.org/abs/astro-ph/0307039

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