Subsonic Potentials in Ultradense Plasmas

2019 ◽  
Vol 74 (3) ◽  
pp. 207-212 ◽  
Author(s):  
Arroj A. Khan ◽  
I. Zeba ◽  
M. Jamil

AbstractThe existence of the subsonic dynamic potential for a test charge in extremely dense quantum plasmas is pointed out for the first time. The dispersion equation of ion acoustic wave in relativistic plasmas is derived by using the quantum hydrodynamic model. The relativistic electrons obey Fermi statistics, whereas the ions are taken classically. The standard model of wake potential is hereafter applied for the derivation of dynamic potential of the test particle. A usual supersonic potential is found suppressed. However, the oscillatory subsonic wake potential does exist in small length scales. The analytical results are applied in different regions by taking the range of magnetic field as well as the electron number density. It is found that the dynamic potential exists only when vt < Cs, showing the presence of subsonic wake potential contrary to the usual supersonic condition vt > Cs. Here vt is the test particle speed and Cs is the acoustic speed defined by the Fermi temperature of the electrons. This work is significant in order to describe the structure formation in the astrophysical environment and laboratory dense plasmas.

2018 ◽  
Vol 2 (2) ◽  
pp. 11-21
Author(s):  
Abdul Rauf ◽  
I. Zeba ◽  
Muhammad Saqlain

Dust-lower-hybrid waves in quantum plasma have been studied. The dispersion relation of the dust-lower-hybrid wave has been examined using the quantum hydrodynamic model of plasma in an ultra-cold Fermi dusty plasma in the presence of a uniform external magnetic field. Graphical analysis shows that the electron Fermi temperature effect and the quantum corrections give rise to significant effects on the dust-lower-hybrid wave of the magnetized quantum dusty plasma.


2020 ◽  
Vol 75 (2) ◽  
pp. 113-118 ◽  
Author(s):  
M. Shahid ◽  
A. Rasheed ◽  
Misbah Kanwal ◽  
M. Jamil

AbstractEffects of Landau quantisation and exchange-correlation potential on Rayleigh–Taylor instability (RTI)/gravitational instability are investigated in inhomogeneous dense plasmas. Quantum hydrodynamic model is used for the electrons, while the ions are assumed to be cold and classical. RTI is modified with the inclusion of Landau quantisation related to plasma density, ambient magnetic field, exchange speed, and modified Fermi speed. Owing to the exchange-correlation effects, gravitational instability increases, whereas the Landau quantisation effects contribute in the opposite way for quantisation factor η < 1. Since the exchange-correlation potential is a function of density, by controlling the number density and magnetic field one can control RTI.


1979 ◽  
Vol 22 (3) ◽  
pp. 443-451 ◽  
Author(s):  
M. Nambu ◽  
K. H. Spatschek ◽  
H. Akama

Using a test particle approach, the potential of a trapped electron is calculated outside the Debye sphere in the electrostatic limit. The potential strongly depends on some characteristic parameters, such as bounce frequencies of the test and background trapped particles, the total number of trapped particles, etc. In some cases, the potential falls off as the inverse of the distance r. The model is limited to the single-wave case; possible generalizations to the many-wave situation in a turbulent plasma are discussed.


2014 ◽  
Vol 351 (2) ◽  
pp. 427-434 ◽  
Author(s):  
Zhonglei Gao ◽  
Hui Zhu ◽  
Lewei Zhang ◽  
Qinghua Zhou ◽  
Chang Yang ◽  
...  

2021 ◽  
Vol 35 (04) ◽  
pp. 2150049
Author(s):  
Zahid Mir ◽  
A. Rasheed ◽  
Arroj A. Khan ◽  
M. Asif ◽  
M. Jamil

The propagation of dust-ion acoustic (DIA) wave is studied with the streaming effects of ion particles in a quantum dusty plasmas. The quantum effects arising from Landau magnetization, Fermi degenerate pressure, tunneling potential and exchange-correlation potential are considered for the electrons. Linear dispersion relation is derived using Quantum Hydrodynamic Model and the results are graphically presented showing the propagation and growth rate of the electrostatic mode in the dense plasma environment.


2020 ◽  
pp. 50-54
Author(s):  
I. Marushchenko ◽  
N.A. Azarenkov

In the paper, the Braginskii equations for relativistic electrons in hot plasmas with slow macroscopic fluxes are derived. This consideration is suitable for description of the typical fusion plasma with the temperatures of about several tens of kiloelectronvolt, when the plasma rotation and the longitudinal currents should be taken into account. Contrary to other papers devoted to classical description of transport processes in fusion devices, as well as to fully relativistic description of the astrophysical objects, we propose the mixed approach with fully relativistic kinetics for the hot electrons and non-relativistic macroscopic fluxes. The obtained form of the Braginskii equations includes all important features of relativistic hydrodynamics, has the same form as the classical representation, which is currently implemented into modern transport codes, and can easily replace the latter.


Laser Physics ◽  
2006 ◽  
Vol 16 (7) ◽  
pp. 1111-1115 ◽  
Author(s):  
T. Yokota ◽  
Y. Nakao ◽  
T. Johzaki ◽  
K. Mima

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