Black hole radiation and volume statistical entropy

The simplest possible equation for Hawking radiation P-SH = G(rho h)/90, and other black hole radiated power is derived in terms of black hole density,rho. Black hole density also leads to the simplest possible model of a gas of elementary constituents confined inside a gravitational bottle of Schwarzchild radius at tremendous pressure, which yields identically the same functional dependence as the traditional black hole entropy S-bh proportional to ( kAc(3))/hG. Variations of S-bh can be obtained which depend on the occupancy of phase space cells. A relation is derived between the constituent momenta and the black hole radius R-H, p = ( 3/2 pi) h/R-H, which is similar to the Compton wavelength relation.