Positron sound waves and nonlinear Landau damping of intense transverse EM waves in an isotropic EPI plasma

2013 ◽  
Vol 79 (5) ◽  
pp. 587-596 ◽  
Author(s):  
N. L. TSINTSADZE ◽  
R. CHAUDHARY ◽  
A. RASHEED

AbstractRelativistically hot electron–positron–ion (EPI) plasmas in the presence of relativistic intense electromagnetic (EM) radiation that are not in thermal equilibrium are studied by following a modified plasma particle distribution function. By means of a kinetic description, soliton solution is obtained for a small amplitude EM wave, whereas for large amplitude EM waves a cusp soliton solution is obtained. A general expression of positron density oscillations is obtained for long wavelength in comparison with the Debye length of electrons, and is discussed for special cases. Dispersion relations for a new type of longitudinal waves with slow damping is formulated as a consequence of resonant wave–particle interaction, and the necessary conditions for the existence of positron sound waves are obtained. Furthermore, for ultrarelativistic electrons and non-relativistic positrons, quasi positron sound waves dispersion relation in the intermediate wave range is obtained. It is shown that the modulation of amplitude of relativistic EM waves leads to instability for the rare plasma. Finally, we have obtained the relativistic kinetic nonlinear Schrödinger equation (KNLS) with local and non-local nonlinearities. The KNLS equation depicts nonlinear Landau damping rates for intense EM waves, and these damping rates are also examined.

2010 ◽  
Vol 76 (6) ◽  
pp. 875-886 ◽  
Author(s):  
ROZINA CHAUDHARY ◽  
NODAR L. TSINTSADZE ◽  
P. K. SHUKLA

AbstractThe creation and annihilation of relativistically hot electron–positron (EP) pair plasmas in the presence of intense electromagnetic (EM) waves, which are not in thermal equilibrium, are studied by formulating a new plasma particle distribution functions, which are valid for both relativistic temperatures and relativistic amplitudes of the EM waves. It is found that intense EM waves in a collisionless EP plasma damp via nonlinear Landau damping. Accounting for the latter, we have obtained relativistic kinetic nonlinear Schrödinger equation (NLSE) with local and non-local nonlinearities. The NLSE depicts nonlinear Landau damping rates for intense EM waves. The damping rates are examined for dense and tenuous pair plasmas. Furthermore, we have studied the modulational instabilities of intense EM waves in the presence of nonlinear Landau damping. Our results reveal a new class of the modulational instability that is triggered by the inverse Landau damping in a relativistically hot EP plasma. Finally, we discuss localization of intense EM waves due to relativistic electron and positron mass increase in a hot pair plasma.


1971 ◽  
Vol 105 (12) ◽  
pp. 774-775 ◽  
Author(s):  
Yu.M. Gal'perin ◽  
P.E. Zil'berman ◽  
Sergey N. Ivanov ◽  
V.D. Kagan ◽  
Georgii D. Mansfel'd

1972 ◽  
Vol 14 (6) ◽  
pp. 808-808
Author(s):  
Yu M Gal'perin ◽  
Petr E Zil'berman ◽  
Sergey N Ivanov ◽  
V D Kagan ◽  
Georgii D Mansfel'd

2005 ◽  
Vol 34 (1-2) ◽  
pp. 89-101 ◽  
Author(s):  
Francesco Valentini ◽  
Vincenzo Carbone ◽  
Pierluigi Veltri ◽  
André Mangeney

2018 ◽  
Vol 84 (2) ◽  
Author(s):  
Alexey Mishchenko ◽  
Gabriel G. Plunk ◽  
Per Helander

The electrostatic stability of electron–positron plasmas is investigated in the point-dipole and Z-pinch limits of dipole geometry. The kinetic dispersion relation for sub-bounce-frequency instabilities is derived and solved. For the zero-Debye-length case, the stability diagram is found to exhibit singular behaviour. However, when the Debye length is non-zero, a fluid mode appears, which resolves the observed singularity, and also demonstrates that both the temperature and density gradients can drive instability. It is concluded that a finite Debye length is necessary to determine the stability boundaries in parameter space. Landau damping is investigated at scales sufficiently smaller than the Debye length, where instability is absent.


1997 ◽  
Vol 78 (7) ◽  
pp. 1263-1266 ◽  
Author(s):  
G. Brodin

1999 ◽  
Vol 62 (1) ◽  
pp. 65-86 ◽  
Author(s):  
MAXIM LYUTIKOV

Beam instabilities in the strongly magnetized electron–positron plasma of a pulsar magnetosphere are considered. We analyse the resonance conditions and estimate the growth rates of the Cherenkov and cyclotron instabilities of the ordinary (O), extraordinary (X) and Alfvén modes in two limiting regimes: kinetic and hydrodynamic. The importance of the different instabilities as a source of coherent pulsar radiation generation is then estimated, taking into account the angular dependence of the growth rates and the limitations on the length of the coherent wave–particle interaction imposed by the curvature of the magnetic field lines. We conclude that in the pulsar magnetosphere, Cherenkov-type instabilities occur in the hydrodynamic regime, while cyclotron-type instabilities occur in the kinetic regime. We argue that electromagnetic cyclotron-type instabilities on the X, O and probably Alfvén waves are more likely to develop in the pulsar magnetosphere.


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