Pure Lovelock black holes emit much less Hawking radiation than Schwarzschild-Tangherlini black holes at equal horizon radius, with integrated powers reduced by roughly 10^{-3} for scalars and 10^{-5} for electromagnetism in six dimensions, and the radiation becomes increasingly scalar-dominated as
Second-order transport, quasinormal modes and zero-viscosity limit in the Gauss-Bonnet holographic fluid
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Hawking Radiation and Greybody Factors of Test Scalar and Electromagnetic Fields on Asymptotically Flat Pure Lovelock Black Holes
Pure Lovelock black holes emit much less Hawking radiation than Schwarzschild-Tangherlini black holes at equal horizon radius, with integrated powers reduced by roughly 10^{-3} for scalars and 10^{-5} for electromagnetism in six dimensions, and the radiation becomes increasingly scalar-dominated as