Screening length in plasma winds
Abstract
We study the screening length L_s of a heavy quark-antiquark pair in strongly coupled gauge theory plasmas flowing at velocity v. Using the AdS/CFT correspondence we investigate, analytically, the screening length in the ultra-relativistic limit. We develop a procedure that allows us to find the scaling exponent for a large class of backgrounds. We find that for conformal theories the screening length is (boosted energy density)^{-1/d}. As examples of conformal backgrounds we study R-charged black holes and Schwarzschild-anti-deSitter black holes in (d+1)-dimensions. For non-conformal theories, we find that the exponent deviates from -1/d and as examples we study the non-extremal Klebanov-Tseytlin and Dp-brane geometries. We find an interesting relation between the deviation of the scaling exponent from the conformal value and the speed of sound.
Cite
@article{arxiv.hep-th/0607233,
title = {Screening length in plasma winds},
author = {Elena Caceres and Makoto Natsuume and Takashi Okamura},
journal= {arXiv preprint arXiv:hep-th/0607233},
year = {2009}
}
Comments
21 pages, 1 figure, JHEP3; v3&v4: minor improvements & corrections