  In this contribution we present a noncanonical phase-space noncommutative
(NC) extension of a Kantowski Sachs (KS) cosmological model to describe the
interior of a Schwarzschild black hole (BH). We evaluate the thermodynamical
quantities inside this NC Schwarzschild BH and compare with the well known
quantities. We find that for a NCBH the temperature and entropy have the same
mass dependence as the Hawking quantities for a Schwarzschild BH.
