  In an accompanying paper, we have formulated two types of regulariz_ation
methods to calculate the scalar self-force on a particle of charge $q$ moving
around a black hole of mass $M$, one of which is called the ``power expansion
regularization''. In this paper, we analytically evaluate the self-force (which
we also call the reaction force) to the third post-Newtonian (3PN) order on the
scalar particle in circular orbit around a Schwarzschild black hole by using
the power expansion regularization. It is found that the $r$-component of the
self-force arises at the 3PN order, whereas the $t$- and $\phi$-components,
which are due to the radiation reaction, appear at the 2PN and 1.5PN orders,
respectively.
