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“Before the Big Bang? A new perspective on the Weyl curvature hypothesis” This is the original lecture by Roger Penrose on his fascinating new model of the universe, its origin and future, and of the “Big Bang”; held at the Isaac Newton Institute for Mathematical Sciences (November 7th 2005). Originally published at www.newton.ac.uk See also www.youtube.com and www.perimeterinstitute.ca for other lectures by Penrose on this theory. See also www.youtube.com for an interview with Roger Penrose on his new model. See also accelconf.web.cern.ch for Penrose’s academic article about his theory. See also arxiv.org for an article about Penrose’s “Before the Big Bang” idea, verifying that some of Penrose’s basic predictions are mathematically correct. ... SUMMARY: There is now a great deal of evidence confirming the existence of a very hot and dense early stage of the universe. Much of this data comes from a detailed study of the cosmic microwave background (CMB)—radiation from the early universe that was most recently measured by NASA’s WMAP satellite. But the information presents new puzzles for scientists. One of the most blatant examples is an apparent paradox related to the second law of thermodynamics. Although some have argued that the hypothesis of inflationary cosmology solves some of the puzzles, profound issues remain. In this talk …" http://www.genetibase.com/blog/

My future hologram theory solves the second law of thermodynamics arrow of time problem simply because the universe at the moment of inflation has only one BIT of event horizon entropy and then approaches the asymptote 10^122 BITS the max entropy of our observable universe sandwiched between our 2D past particle horizon and our 2D future event horizon hologram computer screen. We are its retrocausal 3D hologram images.

Figs 1.1c and 5.1 adapted from Tamara Davis's 2004 Ph.D. University of New South Wales (see middle thin solid line on lower figure for the asymptote at ~ 10^122 BITS).