  Attempts to find black hole microstates using the Hamiltonian phase space
approach have been made on the Schwarzschild spacetime. Since the Schwarzschild
spacetime is also in the larger family of the Kerr spacetimes, and both are
asymptotically flat, the Kerr black hole is a good option for the method
development. The Kerr black hole is a spinning one. We perform this analysis on
the Kerr spacetime and we obtain promising results using the covariant phase
space analysis. Although we have forced ourselves to use the Bondi fall-off
conditions, we find the gauge degrees of freedom that could be good candidates
for the black hole microstates. The charge algebra on the boundary could be a
Virasoro algebra that has a different central term than the Schwarzschild black
hole. The two dimensional theory on the black hole boundary is conjectured to
be conformally invariant.
