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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Autor principal: Ben-Aryeh, Y.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2019
Materias:
Article
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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author Ben-Aryeh, Y.
author_facet Ben-Aryeh, Y.
author_sort Ben-Aryeh, Y.
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description 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 results are obtained for the radius and total mass of such star and its gravitational forces are large due to the extreme large volume. The absorption and emission of radiation for extremely low density star plasmas is very small over the entire electro-magnetic spectrum.
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spelling pubmed-69384912020-01-06 Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal bremsstrahlung Ben-Aryeh, Y. Sci Rep Article 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 results are obtained for the radius and total mass of such star and its gravitational forces are large due to the extreme large volume. The absorption and emission of radiation for extremely low density star plasmas is very small over the entire electro-magnetic spectrum. Nature Publishing Group UK 2019-12-31 /pmc/articles/PMC6938491/ /pubmed/31892718 http://dx.doi.org/10.1038/s41598-019-56784-2 Text en © The Author(s) 2019 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.
spellingShingle Article
Ben-Aryeh, Y.
Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal bremsstrahlung
title Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal bremsstrahlung
title_full Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal bremsstrahlung
title_fullStr Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal bremsstrahlung
title_full_unstemmed Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal bremsstrahlung
title_short Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal bremsstrahlung
title_sort transparency and stability of low density stellar plasma related to boltzmann statistics and to thermal bremsstrahlung
topic Article
url 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
work_keys_str_mv AT benaryehy transparencyandstabilityoflowdensitystellarplasmarelatedtoboltzmannstatisticsandtothermalbremsstrahlung

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