Volume 414, Number 1, January IV 2004
|Page(s)||1 - 6|
|Section||Cosmology (including clusters of galaxies)|
|Published online||12 January 2004|
Magnetized cosmic walls
Astronomical Observatory, Jagellonian University, Faculty of Mathematics, Physics and Computer Science, ul. Orla 171, 30–244 Kraków, Poland
Corresponding author: G. Siemieniec-Oziębło, email@example.com
Accepted: 19 September 2003
Nonlinear growth of one-dimensional density structures with a frozen-in magnetic field is investigated in Newtonian cosmology. A mechanism of magnetic field amplification is discussed. We discuss the relation between the initial conditions for the velocity field and the basic time-scales determining the growth of the magnetized structure.
Key words: cosmology: theory / cosmology: miscellaneous
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.