Abstract
It has been shown that non-rotating black holes in three or four dimensions possess a canonical entropy. Recently study showed that thermal fluctuations would give rise to logarithmic corrections to Bekenstein–Hawking entropy in area with a model-dependent uncertain coefficient. In this paper, the thermal fluctuations on Bekenstein–Hawking entropy in three-dimensional AdS black holes, Schwarzschild-de Sitter space and Kerr-de Sitter (KdS) spacetime with J = 0 will be considered based on a uniformly spaced area spectrum approach. Our conclusion shows that there is the same correction form in all cases we considered.
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