Gregory-Laflamme instability of a slowly rotating black string
High Energy Physics - Theory
2011-06-07 v1 General Relativity and Quantum Cosmology
Abstract
We study the Gregory-Laflamme instability of a 5-dimensional slowly rotating black string in which the 4-dimensional section is described by the Kerr black hole. We treat the rotation in a perturbative way introducing a small parameter for the rotation. It is found that rotation makes the Gregory-Laflamme instability stronger. Both the critical wavelength at the onset of instability and the growth time-scale are found to decrease as the rotation increases.
Cite
@article{arxiv.1103.6081,
title = {Gregory-Laflamme instability of a slowly rotating black string},
author = {Chul-Moon Yoo and Sugure Tanzawa and Misao Sasaki},
journal= {arXiv preprint arXiv:1103.6081},
year = {2011}
}
Comments
26 pages, 1 figure