General relativistic plasma in higher dimensional space time
D. Panigrahi, S. Chatterjee

TL;DR
This paper generalizes Einstein-Maxwell and plasma equations to higher-dimensional spacetimes, analyzing wave propagation, redshift, and Faraday rotation effects in an expanding universe with implications for cosmology.
Contribution
It extends plasma physics and electromagnetic wave analysis to higher dimensions within a cosmological context, providing new dispersion relations and insights into wave behavior.
Findings
Maximum redshift for photons varies with dimension.
Wave propagation restricted to specific frequency ranges depending on dimensions.
Dielectric constant remains constant despite universe expansion.
Abstract
The well known (3+1) decomposition of Thorne and Macdonald is invoked to write down the Einstein-Maxwell equations generalised to (d+1) dimensions and also to formulate the plasma equations in a flat FRW like spacetime in higher dimensions (HD). Assuming an equation of state for the background metric we find solutions as also dispersion relations in different regimes of the universe in a unified manner both for magnetised(un) cold plasma. We find that for a free photon in expanding background we get maximum redshift in 4D spacetime, while for a particular dimension it is so in pre recombination era. Further wave propagation in magnetised plasma is possible for a restricted frequency range only, depending on the number of dimensions. Relevant to point out that unlike the special relativistic result this allowed range evolves with time. Interestingly the dielectric constant of the plasma…
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