Magnetohydrodynamics and Plasma Cosmology

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dc.creatorKleidis, K.
dc.creatorKuiroukidis, A.
dc.creatorPapadopoulos, D. B.
dc.creatorVlahos, L.
dc.date2005-12-22
dc.date.accessioned2026-07-07T11:04:23Z
dc.date.available2026-07-07T11:04:23Z
dc.descriptionWe study the linear magnetohydrodynamic (MHD) equations, both in the Newtonian and the general-relativistic limit, as regards a viscous magnetized fluid of finite conductivity and discuss instability criteria. In addition, we explore the excitation of cosmological perturbations in anisotropic spacetimes, in the presence of an ambient magnetic field. Acoustic, electromagnetic (e/m) and fast-magnetosonic modes, propagating normal to the magnetic field, can be excited, resulting in several implications of cosmological significance.
dc.description9 pages, RevTeX, To appear in the Proceedings of the Peyresq X Meeting, IJTP Conference Series
dc.identifierhttps://arxiv.org/abs/gr-qc/0512131
dc.identifierhttp://arxiv.org/abs/gr-qc/0512131
dc.identifierInt.J.Theor.Phys.46:2283-2298,2007
dc.identifierdoi:10.1007/s10773-007-9346-x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188875
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleMagnetohydrodynamics and Plasma Cosmology
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