Hawking radiation from a five-dimensional Lovelock black hole
  We investigate Hawking radiation from a five-dimensional Lovelock black hole
using the Hamilton-Jacobi method. The behavior of the rate of radiation is
plotted for various values of the ultraviolet correction parameter and the
cosmological constant. The results show that, owing to the ultraviolet
correction and the presence of dark energy represented by the cosmological
constant, the black hole radiates at a slower rate in comparison to the case
without ultraviolet correction or cosmological constant. Moreover, the presence
of the cosmological constant makes the effect of the ultraviolet correction on
the black hole radiation negligible.
