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arXiv · 1103.6081

Gregory-Laflamme instability of a slowly rotating black string

Chul-Moon Yoo·Sugure Tanzawa·Misao Sasaki
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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.

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Chul-Moon Yoo, Sugure Tanzawa, Misao Sasaki. 2011-03-31. Gregory-Laflamme instability of a slowly rotating black string. https://doi.org/10.1142/s0218271811019359

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