We present a class of new black hole solutions in D-dimensional Lovelock gravity theory. The solutions have a form of direct product Mᵐ×Hⁿ, where $D=m+n$, Hⁿ is a negative constant curvature space, and the solutions are characterized by two integration constants. When $m=3$ and 4, these solutions reduce to the exact black hole solutions recently found by Maeda and Dadhich in Gauss-Bonnet gravity theory. We study thermodynamics of these black hole solutions. Although these black holes have a nonvanishing Hawking temperature, surprisingly, the mass of these solutions always vanishes. While the entropy also vanishes when m is odd, it is a constant determined by an Euler characteristic of (m-2)-dimensional cross section of black hole horizon when m is even. We argue that the constant in the entropy should be thrown away. Namely, when m is even, the entropy of these black holes also should vanish. We discuss the implications of these results.
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Cai et al. (2010) studied this question.
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