Transverse Wave Propagation in Relativistic Two-Fluid Plasmas around Schwarzschild-de Sitter Black Hole

被引：16

作者：

Ali, M. Hossain ^{[1
,2
]}

Rahman, M. Atiqur ^{[1
]}

机构：

[1] Rajshahi Univ, Dept Appl Math, Rajshahi 6205, Bangladesh

[2] Abdus Salam Int Ctr Theoret Phys, I-34014 Trieste, Italy

来源：

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2009年 / 48卷 / 06期

关键词：

Two-fluid plasma; Alfven and high frequency electromagnetic waves; Black hole horizon; Cosmological constant; PROBE WMAP OBSERVATIONS; HIGH-REDSHIFT SUPERNOVAE; HUBBLE-SPACE-TELESCOPE; 2 FLUID PLASMAS; ACCELERATING UNIVERSE; COSMOLOGICAL CONSTANT; POWER SPECTRUM; MASS; ELECTRODYNAMICS; DECELERATION;

D O I：

10.1007/s10773-009-9946-8

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We investigate transverse electromagnetic waves propagating in a plasma influenced by the gravitational field of the Schwarzschild-de Sitter black hole. Applying 3+1 spacetime split we derive the relativistic two-fluid equations to take account of gravitational effects due to the event horizon and describe the set of simultaneous linear equations for the perturbations. We use a local approximation to investigate the one-dimensional radial propagation of Alfv,n and high frequency electromagnetic waves. We derive the dispersion relation for these waves and solve it for the wave number k numerically.

引用

页码：1717 / 1735

页数：19