  The $(3+1)$-dimensional Einstein-Gauss-Bonnet theory of gravity which breaks
the Lorentz invariance in a theoretically consistent and observationally viable
way has been recently suggested by Aoki, Gorji and Mukohyama
[arXiv:2005.03859]. Here we calculate grey-body factor for Dirac,
electromagnetic and gravitational fields and estimate the intensity of Hawking
radiation and lifetime for asymptotically flat black holes in this theory.
Positive coupling constant leads to much smaller evaporation rate and longer
life-time of a black hole, while the negative one enhances Hawking radiation.
The grey-body factors for electromagnetic and Dirac fields are smaller for
larger values of the coupling constant.
