  In this paper, we propose a new Analogue Gravity example - a spinning (or
Kerr) Black Hole in an extended fluid model. The fluid model receives Berry
curvature contributions and applies to electron dynamics in Condensed Matter
lattice systems in the hydrodynamic limit. We construct the acoustic metric for
sonic fluctuations that obey a structurally relativistic wave equation in an
effective curved background. In a novel approach of dimensional analysis, we
have derived explicit expressions for effective mass and angular momentum per
unit mass in the acoustic metric (in terms of fluid parameters), to identify
with corresponding parameters of the Kerr metric. The spin is a manifestation
of the Berry curvature-induced effective noncommutative structure in the fluid.
Finally we put the Kerr Black Hole analogy in a robust setting by revealing
explicitly the presence of horizon and ergo-region for a specific background
fluid velocity profile. We also show that near horizon behavior of the
phase-space trajectory of a probe particle agrees with Kerr Black Hole analogy.
In fluid dynamics perspective, presence of a horizon signifies the wave
blocking phenomenon.
