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The general solution of the gravitational field equations for a full causalbulk viscous stiff cosmological fluid, with bulk viscosity coefficientproportional to the energy density to the power 1/4, is obtained in the flatFriedmann-Robertson-Walker geometry. The solution describes a non-inflationaryUniverse, which starts its evolution from a singular state. The time variationof the scale factor, deceleration parameter, viscous pressure, viscouspressure-thermodynamic pressure ratio, comoving entropy and Ricci andKretschmann invariants is considered in detail.Comment: 6 pages, 6 figures, to appear in Int. J. Mod. Phys.

FULL CAUSAL DISSIPATIVE COSMOLOGIES WITH STIFF MATTER