  We analyze the effect of the generalized uncertainty (GUP) principle on the
Hawking radiation from the hairy black hole in U(1) gauge-invariant
scalar-vector-tensor theory by utilizing the semiclassical Hamilton-Jacobi
method. To do so, we evaluate the tunneling probabilities and Hawking
temperature for scalar and fermion particles for the given spacetime of the
black holes with cubic and quartic interactions. For this purpose, we utilize
the modified Klein-Gordon equation for the Boson particles and then Dirac
equations for the fermion particles, respectively. Next, we examine that the
Hawking temperature of the black holes do not depend on the properties of
tunneling particles. Moreover, we present the corrected Hawking temperature of
scalar and fermion particles looks similar in both interactions, but there are
different mass and momentum relationships for scalar and fermion particles in
cubic and quartic interactions.
