  For the relationship of the limit $y$ of the incident particle under the
superradiance of the preset boundary (${\mu} = {y}{\omega}$),we find the
relationship between black hole thermodynamics and superradiation, and use
boundary conditions to establish the relationship between y and R. One of the
modes under f(R) gravity,there is a possible solution.When r tends to infinity,
as a coordinate transformation, y tends to 0. At that time, there is a
potential barrier near the event horizon, that is, the Schwarzschild black hole
under f(R) gravitation has superradiation at that time.
