The equilibrium of the dense electron-nuclear plasma in the gravitational field. The magnetic fields and masses of stars
| dc.creator | Vasiliev, B. V. | |
| dc.date | 2003-07-02 | |
| dc.date | 2003-07-09 | |
| dc.date.accessioned | 2026-07-07T02:08:54Z | |
| dc.date.available | 2026-07-07T02:08:54Z | |
| dc.description | 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. | |
| dc.description | 19 pages, 3 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0307039 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0307039 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6236 | |
| dc.subject | Astrophysics | |
| dc.title | The equilibrium of the dense electron-nuclear plasma in the gravitational field. The magnetic fields and masses of stars | |
| dc.type | text |