Defining a finite universe from a holographic horizon.

By combining Carl Schwarzschild's solution for BH mass and radius with Hawking's solution for the BH mass and temperature one can define both the initial and final condition of a finite Universe, (U); which conserves Mass, (M$_{u})$, Energy (E$_{u})$ and Quantum Information, (I$_{u})$ measured from a holographic horizon that contains the entire universe at some time (t) where (c$^{2}$t$^{2}) \quad =$ (R$^{2})$. Since (c) is a constant then (t$^{2})$ $=$ (R$^{2}) \quad =$ (M$_{u})$/(T). I will derive 4 equations that prove this.