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Bargmann-Wigner equations are formulated to represent bosonic fields in termsof fermionic fields in curved spacetime. The superradiance phenomena of bosonsand fermions in rotating black hole spacetime are studied in theBargmann-Wigner formulation. As a result of the consistent description betweenscalar bosons and spinor fermions, superradiance phenomena of the type ofpositive frequency $(0<\omega)$ and negative momentum near horizon $(p_{H}<0)$are shown not to occur.

Superradiance Problem of Bosons and Fermions for Rotating Black Holes in Bargmann-Wigner Formulation