Talk abstract details

If we assume the fundamental character of the Holographic Principle as a primary principle guiding the behaviour of our universe it would be reasonable a saturation of the holographic limit. On the other hand the Fischler-Susskind holographic prescription seems to be incompatible with spatially closed cosmological models due to the apparently unavoidable recontraction of the particle horizon area. However we will show that the saturation of the Fischler-Susskind holographic prescription over a spatially closed (although almost flat) cosmological model enforces a cosmological evolution very similar to the observed universe.