Stability and evolution of wave packets in strongly coupled degenerate plasmas

被引:30
作者
Misra, A. P. [1 ,3 ]
Shukla, P. K. [2 ]
机构
[1] Umea Univ, Dept Phys, SE-90187 Umea, Sweden
[2] Ruhr Univ Bochum, Fac Phys & Astron, Int Ctr Adv Studies Phys Sci, D-44780 Bochum, Germany
[3] Visva Bharati Univ, Dept Math, Santini Ketan 731235, W Bengal, India
来源
PHYSICAL REVIEW E | 2012年 / 85卷 / 02期
关键词
Collisional plasmas - Plasma diagnostics - Nonlinear equations - Plasma stability - Viscoelasticity - Modulation;
D O I
10.1103/PhysRevE.85.026409
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We study the nonlinear propagation of electrostatic wave packets in a collisional plasma composed of strongly coupled ions and relativistically degenerate electrons. The equilibrium of ions is maintained by an effective temperature associated with their strong coupling, whereas that of electrons is provided by the relativistic degeneracy pressure. Using a multiple-scale technique, a (3 + 1)-dimensional coupled set of nonlinear Schrodinger-like equations with nonlocal nonlinearity is derived from a generalized viscoelastic hydrodynamic model. These coupled equations, which govern the dynamics of wave packets, are used to study the oblique modulational instability of a Stoke's wave train to a small plane-wave perturbation. We show that the wave packets, though stable to the parallel modulation, become unstable against oblique modulations. In contrast to the long-wavelength carrier modes, the wave packets with short wavelengths are shown to be stable in the weakly relativistic case, whereas they can be stable or unstable in the ultrarelativistic limit. Numerical simulation of the coupled equations reveals that a steady-state solution of the wave amplitude exists together with the formation of a localized structure in (2 + 1) dimensions. However, in the (3 + 1)-dimensional evolution, a Gaussian wave beam self-focuses after interaction and blows up in a finite time. The latter is, however, arrested when the dispersion predominates over the nonlinearities. This occurs when the Coulomb coupling strength is higher or a choice of obliqueness of modulation, or a wavelength of excitation is different. Possible application of our results to the interior as well as in an outer mantle of white dwarfs are discussed.
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页数:15
相关论文
共 24 条
[1]   VISCOUS DISSIPATION OF SOUND IN STRONGLY COMPRESSED PLASMAS [J].
ATRAZHEV, VM ;
IAKUBOV, IT .
PHYSICS OF PLASMAS, 1995, 2 (07) :2624-2629
[2]  
Chandrasekhar S, 1935, MON NOT R ASTRON SOC, V96, P0021
[3]  
Chandrasekhar S, 1931, PHILOS MAG, V11, P592
[4]   The maximum mass of ideal white dwarfs [J].
Chandrasekhar, S .
ASTROPHYSICAL JOURNAL, 1931, 74 (01) :81-82
[5]   White dwarf stars with carbon atmospheres [J].
Dufour, P. ;
Liebert, J. ;
Fontaine, G. ;
Behara, N. .
NATURE, 2007, 450 (7169) :522-524
[6]   THERMAL-ENERGY OF THE CRYSTALLINE ONE-COMPONENT PLASMA FROM DYNAMICAL SIMULATIONS [J].
FAROUKI, RT ;
HAMAGUCHI, S .
PHYSICAL REVIEW E, 1993, 47 (06) :4330-4336
[7]   Nonlinear wave propagation in a strongly coupled collisional dusty plasma [J].
Ghosh, Samiran ;
Gupta, Mithil Ranjan ;
Chakrabarti, Nikhil ;
Chaudhuri, Manis .
PHYSICAL REVIEW E, 2011, 83 (06)
[8]   A fluid model for colloidal plasmas under microgravity conditions [J].
Gozadinos, G ;
Ivlev, AV ;
Boeuf, JP .
NEW JOURNAL OF PHYSICS, 2003, 5 :32.1-32.9
[9]  
Horn H. M. V., 1968, ASTROPHYS J, V151, P227
[10]   Low frequency modes in strongly coupled dusty plasmas [J].
Kaw, PK ;
Sen, A .
PHYSICS OF PLASMAS, 1998, 5 (10) :3552-3559