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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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Detalles Bibliográficos
Autor principal: Ben-Aryeh, Y.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2019
Materias:
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

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