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Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal bremsstrahlung
The stability of low density stellar plasma is analyzed for a star with a spherical symmetry which is in equilibrium between the gravitational attractive forces and the repulsive pressure forces of an ideal electron gas where the analysis is developed by the use of Boltzmann statistics. Fundamental...
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Nature Publishing Group UK
2019
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6938491/ https://www.ncbi.nlm.nih.gov/pubmed/31892718 http://dx.doi.org/10.1038/s41598-019-56784-2 |