  We obtain new black hole solutions in a Einstein-Bumblebee-scalar theory. By
starting with a Einstein-Bumblebee theory in D + d dimensions, the scalar
dilaton field and its interaction with the gravitational and bumblebee fields
are obtained by Kaluza-Klein (KK) reduction over the extra dimensions.
Considering the effects of both the bumblebee vacuum expectation value (VEV)
and the fluctuations over the VEV, we obtained new charged solutions in (3 + 1)
dimensions. For a vanishing dilaton, the black hole turned out to be a charged
de Sitter-Reissner-Nordstrom solution, where the transverse mode is the Maxwell
field and the longitudinal mode is the cosmological constant. The stability of
these new solutions is investigated by means of the analysis of the black hole
thermodynamics. The temperature, entropy and heat capacity show that these
modified black holes are thermodynamic stable.
