Isothermal plasma waves properties of the Schwarzschild de-sitter black hole in a veselago medium

dc.contributor.authorM. Sharif
dc.contributor.authorIfra Noureen
dc.date.accessioned2011-11-30T13:41:05Z
dc.date.available2011-11-30T13:41:05Z
dc.date.issued2011
dc.description.abstractIn this paper, we study wave properties of isothermal plasma for the Schwarzschild de-Sitter black hole in a Veselago medium. We use ADM 3 + 1 formalism to formulate general relativistic magnetohydrodynamical (GRMHD) equations for the Schwarzschild de-Sitter spacetime in Rindler coordinates. Further, Fourier analysis of the linearly perturbed GRMHD equations for the rotating (non-magnetized and magnetized) background is taken whose determinant leads to a dispersion relation. We investigate wave properties by using graphical representation of the wave vector, the refractive index, change in refractive index, phase and group velocities. Also, the modes of wave dispersion are explored. The results indicate the existence of the Veselago medium.en_US
dc.identifier.citationAstrophysics Space Science,Vol 331 No 1, Pages 151-162, 2011en_US
dc.identifier.urihttps://escholar.umt.edu.pk/handle/123456789/349
dc.language.isoenen_US
dc.publisherAstrophysics Space Scienceen_US
dc.subject3 + 1 formalismen_US
dc.subjectSdS Black Holeen_US
dc.subjectVeselago Mediumen_US
dc.subjectGRMHD equationsen_US
dc.subjectDispersion relationsen_US
dc.titleIsothermal plasma waves properties of the Schwarzschild de-sitter black hole in a veselago mediumen_US
dc.typeArticleen_US
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