Kerr Black string flow
High Energy Physics - Theory
2015-12-09 v5
Abstract
We give a general theory of a rotated black string stream into a rotational horizon in dimension D=5. It is a configuration about one smooth intersection between these two objects when the spacetime is axisymmetric and in the limit that the thickness of the black hole is much larger than the thickness of the black string. Following this configuration we extend to a more general situation, the rotational charged flows.
Cite
@article{arxiv.1405.6906,
title = {Kerr Black string flow},
author = {Meng Sun and Yong-Chang Huang},
journal= {arXiv preprint arXiv:1405.6906},
year = {2015}
}
Comments
14 pages, 3 figures