  The equilibrium configurations of uniformly rotating white dwarfs at finite
temperatures are investigated, exploiting the Chandrasekhar equation of state
for different isothermal cores. The Hartle-Thorne formalism is applied to
construct white dwarf configurations in the framework of Newtonian physics. The
equations of structure are considered in the slow rotation approximation and
all basic parameters of rotating hot white dwarfs are computed to test the
so-called moment of inertia, tidal Love number and quadrupole moment
($I$-Love-$Q$) relations. It is shown that even within the same equation of
state the $I$-Love-$Q$ relations are not universal for white dwarfs at finite
temperatures.
