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Updated: Dec 31, 2025

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
Published on: August 1, 2017
Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal
1Technion-Israel Institute of Technology, Physic Department, Haifa, 32000, Israel. phr65yb@physics.technion.ac.il.
Abstract:
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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