Radio‐frequency plasmas in CF4: Self‐consistent modeling of the plasma physics and chemistry

1995 ◽  
Vol 77 (12) ◽  
pp. 6169-6180 ◽  
Author(s):  
Nikolaos V. Mantzaris ◽  
Andreas Boudouvis ◽  
Evangelos Gogolides
Keyword(s):  
Radio Frequency ◽  
Plasma Physics ◽  
Self Consistent

A self-consistent fluid model for radio-frequency discharges in SiH4–H2 compared to experiments

1997 ◽  
Vol 82 (5) ◽  
pp. 2060-2071 ◽  
Author(s):  
G. J. Nienhuis ◽  
W. J. Goedheer ◽  
E. A. G. Hamers ◽  
W. G. J. H. M. van Sark ◽  
J. Bezemer
Keyword(s):  
Radio Frequency ◽  
Fluid Model ◽  
Self Consistent ◽  
Radio Frequency Discharges

Radio-frequency sheaths physics: Experimental characterization on Tore Supra and related self-consistent modeling

2014 ◽  
Vol 21 (6) ◽  
pp. 061509 ◽  
Author(s):  
Jonathan Jacquot ◽  
Daniele Milanesio ◽  
Laurent Colas ◽  
Yann Corre ◽  
Marc Goniche ◽  
...  
Keyword(s):  
Radio Frequency ◽  
Experimental Characterization ◽  
Self Consistent

scholarly journals Modelling the solar wind interaction with Mercury by a quasi-neutral hybrid model

2003 ◽  
Vol 21 (11) ◽  
pp. 2133-2145 ◽  
Author(s):  
E. Kallio ◽  
P. Janhunen
Keyword(s):  
Solar Wind ◽  
Plasma Physics ◽  
Hybrid Model ◽  
Space Plasma ◽  
Physical Processes ◽  
Space Plasma Physics ◽  
Solar Wind Interaction ◽  
Plasma Parameters ◽  
Advantages And Disadvantages ◽  
Self Consistent

Abstract. Quasi-neutral hybrid model is a self-consistent modelling approach that includes positively charged particles and an electron fluid. The approach has received an increasing interest in space plasma physics research because it makes it possible to study several plasma physical processes that are difficult or impossible to model by self-consistent fluid models, such as the effects associated with the ions’ finite gyroradius, the velocity difference between different ion species, or the non-Maxwellian velocity distribution function. By now quasi-neutral hybrid models have been used to study the solar wind interaction with the non-magnetised Solar System bodies of Mars, Venus, Titan and comets. Localized, two-dimensional hybrid model runs have also been made to study terrestrial dayside magnetosheath. However, the Hermean plasma environment has not yet been analysed by a global quasi-neutral hybrid model. In this paper we present a new quasi-neutral hybrid model developed to study various processes associated with the Mercury-solar wind interaction. Emphasis is placed on addressing advantages and disadvantages of the approach to study different plasma physical processes near the planet. The basic assumptions of the approach and the algorithms used in the new model are thoroughly presented. Finally, some of the first three-dimensional hybrid model runs made for Mercury are presented. The resulting macroscopic plasma parameters and the morphology of the magnetic field demonstrate the applicability of the new approach to study the Mercury-solar wind interaction globally. In addition, the real advantage of the kinetic hybrid model approach is to study the property of individual ions, and the study clearly demonstrates the large potential of the approach to address these more detailed issues by a quasi-neutral hybrid model in the future.Key words. Magnetospheric physics (planetary magnetospheres; solar wind-magnetosphere interactions) – Space plasma physics (numerical simulation studies)

Radio-frequency sheaths physics: Experimental characterization on Tore Supra and related self-consistent modeling

2014 ◽  
Author(s):  
Jonathan Jacquot ◽  
Daniele Milanesio ◽  
Laurent Colas ◽  
Yann Corre ◽  
Marc Goniche ◽  
...  
Keyword(s):  
Radio Frequency ◽  
Experimental Characterization ◽  
Self Consistent

High-frequency tail of the radio-frequency spectrum in a unitary Fermi gas with particle–hole fluctuation

2018 ◽  
Vol 32 (24) ◽  
pp. 1850280
Author(s):  
Xiao-Xia Ruan ◽  
Fei Wang ◽  
Hao Gong ◽  
Zheng-Ling Wang ◽  
Hong-Shi Zong
Keyword(s):  
Radio Frequency ◽  
Frequency Spectrum ◽  
High Frequency ◽  
Ultracold Atoms ◽  
Fermi Gas ◽  
Normal Phase ◽  
Matrix Approximation ◽  
Self Consistent ◽  
Radio Frequency Spectrum ◽  
Unitary Fermi Gas

The contact plays an important role in the study of ultracold atoms. We determine the contact from the high-frequency asymptotic behavior of radio-frequency spectrum for a homogeneous Fermi gas at unitarity in the normal phase. The contact is obtained within the framework of the non-self-consistent T-matrix approximation with particle–hole fluctuation.

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