科研之友
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摘要
We study the Gregory-Laflamme instability of a five-dimensional slowly rotating black string in which the four-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.
- 出版日期2011-6
