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Gregory-Laflamme instability of a slowly rotating black string

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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.

fields

gr-qc 1

years

2026 1

verdicts

UNVERDICTED 1

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