scholarly journals Collective modes in a saturated lithium-ammonia solution as a probe of the response of the low-density homogeneous electron gas

2011 ◽  
Vol 84 (9) ◽  
Author(s):  
C. Petrillo ◽  
F. Sacchetti ◽  
E. Guarini ◽  
L. E. Bove ◽  
F. Demmel
Keyword(s):  
Electron Gas ◽  
Ammonia Solution ◽  
Collective Modes ◽  
Low Density

scholarly journals Interplay between collective modes in hybrid electron-gas–superconductor structures

2020 ◽  
Vol 101 (16) ◽  
Author(s):  
M. V. Boev ◽  
I. G. Savenko ◽  
V. M. Kovalev
Keyword(s):  
Electron Gas ◽  
Collective Modes

scholarly journals Relaxation of spin-polarized low-density electron gas

2017 ◽  
pp. 1-23
Author(s):  
Igor Vadimovich Fomin ◽  
Pavel Vasilievich Sasorov
Keyword(s):  
Electron Gas ◽  
Low Density ◽  
Spin Polarized

scholarly journals Transparency and stability of low density stellar plasma related to Boltzmann statistics and to thermal bremsstrahlung

2019 ◽  
Vol 9 (1) ◽  
Author(s):  
Y. Ben-Aryeh
Keyword(s):  
Large Volume ◽  
Spherical Symmetry ◽  
Total Mass ◽  
Electron Gas ◽  
Low Density ◽  
Gravitational Forces ◽  
Magnetic Spectrum ◽  
Boltzmann Statistics ◽  
Electro Magnetic ◽  
The Stability

AbstractThe 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.

Low‐density high‐mobility electron gas in wide parabolic GaAs/AlxGa1−xAs wells

1990 ◽  
Vol 57 (26) ◽  
pp. 2823-2825 ◽  
Author(s):  
P. F. Hopkins ◽  
A. J. Rimberg ◽  
E. G. Gwinn ◽  
R. M. Westervelt ◽  
M. Sundaram ◽  
...  
Keyword(s):  
Electron Gas ◽  
High Mobility ◽  
Low Density
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