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A&A 471, 409-417 (2007)
DOI: 10.1051/0004-6361:20077109
Excitation of MHD waves in magnetized anisotropic cosmologies
A. Kuiroukidis1, 2, K. Kleidis1, 3, D. B. Papadopoulos1, and L. Vlahos11 Department of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
e-mail: kleidis@astro.auth.gr
2 Department of Informatics, Technological Education Institute of Serres, 64124 Serres, Greece
3 Department of Civil Engineering, Technological Education Institute of Serres, 64124 Serres, Greece
(Received 16 January 2007 / Accepted 16 April 2007 )
Abstract
The excitation of cosmological perturbations in an
anisotropic cosmological model and in the presence of a
homogeneous magnetic field was studied, using the resistive
magnetohydrodynamic (MHD) equations. We have shown that
fast-magnetosonic modes, propagating normal to the magnetic field,
grow exponentially and saturate at high values, due to the
resistivity. We also demonstrate that Jeans-like instabilities
can be enhanced inside a resistive fluid and that the formation of
condensations influence the growing magnetosonic waves.
Key words: magnetic fields -- magnetohydrodynamics (MHD) -- instabilities -- waves -- cosmology: early Universe -- relativity
© ESO 2007
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