Figure 1
The plot of T given in Eq. (14) versus the radial coordinate r for m=1 and \(r_{f} = 4\). There is a singularity at \(r = r_{f}\) after which the curvature changes sign. The Schwarzschild black hole temperature \(T=\frac{1}{4 \pi r}\) is shown with blue color. In mimetic gravity black hole temperature raises to a maximum value due to evaporation and then decreases. There is a black hole remnant in this mimetic framework as is evident in this figure, see also25.
