Gregory-Laflamme instability of a slowly rotating black string
arXiv:1103.6081 · doi:10.1142/S0218271811019359
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.
26 pages, 1 figure
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